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Complex Systems - Jean-Philippe Bouchaud -Lecture 9: Choice Theory, Ising paradigm & Schelling model — Transcript

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  1. 0:00this conference will now be recorded
  2. 0:08okay so it's uh unfortunately on our
  3. 0:11last lecture went very quickly this year
  4. 0:14I thought
  5. 0:15and it's a little sad not to see you I
  6. 0:17have four people in the room though
  7. 0:19which is a change
  8. 0:21um so
  9. 0:24today that there's one lecture and then
  10. 0:27the pity as usual
  11. 0:30and then next week I guess that uh you
  12. 0:33don't have anything so you're supposed
  13. 0:34to work on your
  14. 0:37on your revisions but the the problem is
  15. 0:41that we don't know yet exactly the
  16. 0:43circumstances in which the exam will
  17. 0:45take place
  18. 0:46we hope to know that soon
  19. 0:49in any case what I usually do in the in
  20. 0:51this last week is I propose a kind of
  21. 0:53Open Session
  22. 0:55um so if you want I'll send the link
  23. 0:57I'll see that with Valentina I'll send
  24. 1:00the link and for next Wednesday uh nine
  25. 1:03o'clock the usual time
  26. 1:05and then you can connect and we can chat
  27. 1:07about anything really if you have
  28. 1:09questions
  29. 1:10about the lectures or whatever it helps
  30. 1:15you I mean there's no obligation but I
  31. 1:17usually do that in
  32. 1:19in real so we can do that also
  33. 1:23through go to meeting or Zoom or
  34. 1:25whatever
  35. 1:27okay so
  36. 1:29um last time it was always already two
  37. 1:30weeks ago sorry for uh
  38. 1:33the slides changed last week true
  39. 1:38um so I'm in the last chapter chapter
  40. 1:40four interactions and Collective texts
  41. 1:42of course I had talked about Collective
  42. 1:44effects in the random field icing model
  43. 1:46example but here I want to I wanted to
  44. 1:50dwell more on this so I told you about
  45. 1:53Choice Theory and detailed balance I'm
  46. 1:55going to recall a little bit uh what I
  47. 1:57said because it's very important for
  48. 1:59today
  49. 2:00then I
  50. 2:02told you about the the icing Paradigm so
  51. 2:05the fact that
  52. 2:07you can have spontaneous appearance of a
  53. 2:10collective choice if uh interaction is
  54. 2:13strong enough or if
  55. 2:15temperature or irrationality is low
  56. 2:19enough
  57. 2:21and today I want to generalize The
  58. 2:25Simple Choice theory that I gave you
  59. 2:28last time to the case of multi-agents
  60. 2:32interacting multi-agents
  61. 2:34and this will allow me to speak about a
  62. 2:37very well-known model in economics or
  63. 2:41sociology I don't know how you want to
  64. 2:43call it but anyway uh shelling how much
  65. 2:46selling goods and over five in economics
  66. 2:49so I guess uh must be thought of as
  67. 2:51economics propose the model to
  68. 2:54understand
  69. 2:55segregation effects in cities
  70. 2:58and you'll see that this is amenable to
  71. 3:00kind of statistical mechanics type of
  72. 3:03treatment and it shows a very
  73. 3:06counter-intuitive uh effect
  74. 3:08and then you know I of course this is
  75. 3:11going to be very quick uh this session
  76. 3:14is only an hour and a half a little more
  77. 3:17so I won't have time to speak a lot
  78. 3:19about spin glasses but I want to tell
  79. 3:21you uh very few things about the general
  80. 3:24phenomenology of what's called in
  81. 3:26physics spin glasses which has many uh
  82. 3:29incarnations also in economics and
  83. 3:32social sciences and to show you that
  84. 3:35some of the things that I told you about
  85. 3:37optimization I maybe you remember this
  86. 3:40idea of fragile optimization as soon as
  87. 3:42you change a little bit some of the
  88. 3:44parameters you can completely change the
  89. 3:46solution that this actually occurs in
  90. 3:49skin glasses in a very paradigmatic
  91. 3:52manner
  92. 3:54okay so that's the outline for today
  93. 3:57so let me recall what I said last time I
  94. 3:59I was considering a single agent and
  95. 4:03this single agent had a certain number
  96. 4:05of possible choices Alpha Gamma and so
  97. 4:08on
  98. 4:09to which is associated the certain
  99. 4:11utility function U of alpha
  100. 4:15and then the rule of the game in
  101. 4:19decision theory is that agents can
  102. 4:21revise their decision and change their
  103. 4:23mind
  104. 4:24and go from one choice to another
  105. 4:27and this is with a sudden rate w
  106. 4:31Alpha to gamma
  107. 4:33which is
  108. 4:35the probability to change your mind from
  109. 4:38alpha to gamma between t and t plus DT
  110. 4:41and this is equal to a certain
  111. 4:44base rate gamma
  112. 4:46Capital gamma divided by one plus
  113. 4:50exponential of beta and there's always a
  114. 4:55sign here to get right U Alpha minus U
  115. 4:58gamma
  116. 4:59foreign
  117. 5:00[Music]
  118. 5:04it's in physics it's the inverse
  119. 5:06temperature in economics it's a measure
  120. 5:10of irrationality or sometimes it's it's
  121. 5:13thought of as a measure of the
  122. 5:16uncertainty you have on your own utility
  123. 5:19you don't exactly know what you want
  124. 5:20this is well known in life
  125. 5:23and uh and the sign so let's run through
  126. 5:26it again so if you gamma is larger than
  127. 5:29U Alpha so you're more happy with Choice
  128. 5:31uh gamma then this is negative
  129. 5:35and exponential of beta times the
  130. 5:37negative number uh when beta is large is
  131. 5:41very small and so you you actually
  132. 5:44change
  133. 5:46nearly deterministically once you've
  134. 5:48decided to change your mind with with
  135. 5:50raid gamma then you do go for the better
  136. 5:54alternative
  137. 5:56so that explains the sign here okay and
  138. 5:59uh what we've seen is that this
  139. 6:02particular choice which again is a
  140. 6:05choice that can be justified from first
  141. 6:07principles in physics
  142. 6:09where U is the analog of the energy
  143. 6:13in social sciences it's it's really more
  144. 6:16uh a convenient Choice it's something
  145. 6:19that you know goes in the right
  146. 6:21direction of course you make choices
  147. 6:23that are on average favorable
  148. 6:25but the detailed shape of this hopping
  149. 6:29rate of the rate of change is very
  150. 6:32arbitrary and is only motivated by
  151. 6:35mathematical convenience so that that's
  152. 6:38that's really a problem in a sense
  153. 6:39because one doesn't know whether the
  154. 6:42results that one gets from this
  155. 6:44particular choice uh are generic or not
  156. 6:48and I'll give you a little bit uh more
  157. 6:51discussion on that later on but in any
  158. 6:54case what makes everything
  159. 6:56work is that these hopping rates or
  160. 7:00these
  161. 7:01transfer rate obey
  162. 7:05what's called again in physics detail
  163. 7:07balance
  164. 7:09which is that there exists a sudden
  165. 7:11function
  166. 7:13h of alpha
  167. 7:20such that
  168. 7:23the ratio of the rate to go from alpha
  169. 7:26to gamma over the inverse rate is given
  170. 7:30by such a
  171. 7:33a form for any Alpha and gamma
  172. 7:38and in this particular case it's very uh
  173. 7:42it's very easy to show that this is the
  174. 7:45case when u h is is minus U but we'll
  175. 7:48see that this is not necessarily the
  176. 7:50case and it's going to be one of the
  177. 7:53main points of today but then whenever
  178. 7:57this is true when I have a detailed
  179. 7:59balance Falls then we know what's going
  180. 8:02to happen at long times at long times
  181. 8:04this x this random exploration of choice
  182. 8:07of the possible choices is going to lead
  183. 8:10to an invariant probability measure an
  184. 8:13invariant distribution which is that
  185. 8:15this the probability to find agent
  186. 8:19um in Choice Alpha probability to find
  187. 8:22that an agent has made Choice Alpha in
  188. 8:24equilibrium or stationary state is uh
  189. 8:28one over some normalization exponential
  190. 8:31of minus
  191. 8:34beta h of alpha okay
  192. 8:36and this is of course the traditional
  193. 8:38boltzmann Gibbs weight
  194. 8:42in physics
  195. 8:44so again in physics we have a pretty
  196. 8:46pretty detailed understanding of why
  197. 8:48detailed balance holds and of course
  198. 8:51detail balance is is a way to recover
  199. 8:54uh the Bolson Lake
  200. 8:56okay now I want to
  201. 8:59put this in a slightly more General
  202. 9:01context
  203. 9:03which is a
  204. 9:05a context where there's not only one
  205. 9:07agent making choices but many agents
  206. 9:10making choices
  207. 9:12and the utility function of each agent
  208. 9:14depends on the choice of others
  209. 9:16possibly
  210. 9:18so there are many agents many choices
  211. 9:20and
  212. 9:22um
  213. 9:25and they are possibly interacting or not
  214. 9:27we'll see so I'm going to now
  215. 9:32right away use my camera
  216. 9:35don't forget okay
  217. 9:52okay so now I'm considering
  218. 9:55as I said many ages I equal one to n say
  219. 10:01and each of these agents has a certain
  220. 10:03set of choices
  221. 10:05and the configuration of all these
  222. 10:07people together
  223. 10:09is described by the set of all the
  224. 10:12choices they've made so she currently C
  225. 10:15is going to be a configuration a
  226. 10:18configuration of choice so
  227. 10:21Alpha One is the choice made by agent
  228. 10:24one which can be anything in his set of
  229. 10:28choices or her set of choices
  230. 10:30Alpha 2
  231. 10:32Alpha I
  232. 10:34alpha n okay
  233. 10:37so it's a pretty big thing
  234. 10:39uh
  235. 10:40in the simplest case where which I
  236. 10:43talked about last time and also within
  237. 10:46the random field icing model
  238. 10:48each agent has the binary choice
  239. 10:51and and so this is a space of Dimension
  240. 10:53I mean there are two to the end
  241. 10:55configuration in that case but if Alpha
  242. 10:59is something different and we'll see an
  243. 11:01example in the sharing model then the
  244. 11:03space can be even larger Alpha can even
  245. 11:06be continuous variable whatever
  246. 11:10so this is one configuration and
  247. 11:14we'll assume that at each time Step
  248. 11:18One agent changes uh his or her decision
  249. 11:23uh to something else
  250. 11:26and this is not this is done one at a
  251. 11:28time so uh in the in the analog of of
  252. 11:33this rate here we're only going to
  253. 11:35consider cases where only one agent
  254. 11:38changes between t and t plus DT and so
  255. 11:42I'm going to call this agent I
  256. 11:46foreign
  257. 11:50the target configuration
  258. 11:53is going to be C Prime which is the same
  259. 11:56as C except that one of the agent has
  260. 11:59changed to from alpha to gamma okay
  261. 12:04of course this is again this is a
  262. 12:05notation that is not necessarily very
  263. 12:08explicit Alpha One doesn't Alpha One
  264. 12:10Alpha 2 doesn't mean that all agents
  265. 12:12take the same decision alpha alpha one
  266. 12:15is the label of the of the decision made
  267. 12:18by one but it's not necessarily the same
  268. 12:20as the decision made by two in in most
  269. 12:22General generality these Alphas don't
  270. 12:25necessarily need to live in the same
  271. 12:27space anyway they can describe
  272. 12:29completely different things anyway so
  273. 12:32it's a maybe a slightly confusing
  274. 12:35notation
  275. 12:36so what I'm going to assume is that each
  276. 12:39agent does it does this change of uh
  277. 12:42decision based on his or her own utility
  278. 12:46function only so I'm going to assume
  279. 12:49that the probability that the system
  280. 12:51goes from C to C Prime
  281. 12:54is given by something very similar to
  282. 12:56what I wrote here which is one plus one
  283. 13:01over I mean gamma gamma
  284. 13:03over one plus exponential beta and here
  285. 13:08I'm only taking into account the change
  286. 13:10of utility of agent I so UI of
  287. 13:16uh well
  288. 13:18uh so UI of e Prime
  289. 13:26yes UI same notation is here uift minus
  290. 13:31Qi of C Prime
  291. 13:36okay so this looks very similar to that
  292. 13:39okay
  293. 13:42so each agent looks at at its own or her
  294. 13:47own I mean I don't know what to use his
  295. 13:50or it's
  296. 13:52um so agent I look at its current uh
  297. 13:56satisfaction uifc looks at the
  298. 13:59satisfaction you would have in the next
  299. 14:01configuration where he changes from
  300. 14:04alpha to gamma and then this depending
  301. 14:06on this difference he decides or he
  302. 14:09decides to do it or not okay
  303. 14:12so now what's maybe unexpected is that I
  304. 14:17cannot assume right away that these WCS
  305. 14:22T to C Prime although they're written
  306. 14:24exactly the same way as here
  307. 14:27I cannot assume right away that detailed
  308. 14:30balance will hold
  309. 14:33it will hold in a trivial manner if
  310. 14:37the choices the utility functions are
  311. 14:40independent that is if the choice of
  312. 14:43agent I doesn't affect at all the choice
  313. 14:45of other agents but in in the case where
  314. 14:49agents interact it's not at all obvious
  315. 14:52that in general these this Choice allows
  316. 14:58detailed balance to hold and I'm going
  317. 14:59to show this explicitly on an example
  318. 15:03yes so there's a question
  319. 15:11yeah every time you took an agent
  320. 15:13randomly but you you just take one at a
  321. 15:16time
  322. 15:17so here it's I but yeah I haven't
  323. 15:19specified that you right but it can be
  324. 15:22any agent can change his mind also her
  325. 15:24mind but at each time step it's taken
  326. 15:26random B and then you you compute this
  327. 15:28to know whether you're going to go to
  328. 15:30the next consideration
  329. 15:33okay so the question I'm asking now is
  330. 15:37can I find a sudden function H now of of
  331. 15:41the whole configuration
  332. 15:47stats the WC to C Prime obey detailed
  333. 15:51balance which is that WC to C Prime will
  334. 15:54follow something analog to this except
  335. 15:57that instead of having a single choice
  336. 15:59of a single agent I have here a function
  337. 16:02of the whole configuration H okay and so
  338. 16:06what I'm saying is that in some cases
  339. 16:09so in Easy cases
  340. 16:12it will be when h of C
  341. 16:15is simply so there's a spine difference
  342. 16:18uh
  343. 16:19just to keep the fact that in physics
  344. 16:22we're used to boltzmann gives uh having
  345. 16:24an exponential of minus beta H and think
  346. 16:27of H as an energy whereas in economics
  347. 16:30it's more a utility so people tend to
  348. 16:32maximize their utility whereas physical
  349. 16:34systems tend to minimize their energy
  350. 16:36but that's uh that's that's just a
  351. 16:39detail so in the easy case we would have
  352. 16:43that h of
  353. 16:44T is that the sum over I of u i of
  354. 16:49of of of Alpha I
  355. 16:53okay so in this case where the use only
  356. 16:57depends on uh your own choice
  357. 17:01then uh you have this easy rule that
  358. 17:04detailed balance is obeyed just by
  359. 17:07summing individual utility functions and
  360. 17:10then people evolve independently from
  361. 17:12one another and so it's not surprising
  362. 17:14that the whole system the whole problem
  363. 17:16goes back to the uh single agent case
  364. 17:21and you see that if H is the sum of UI
  365. 17:24then the probability the stationary
  366. 17:28probability is the product of
  367. 17:30exponential of UI that is it's a product
  368. 17:32of independent uh individual probability
  369. 17:35so this is this is the easy case
  370. 17:41but let me give you an example which
  371. 17:43already is not that trivial which is
  372. 17:46again uh the case where there are two
  373. 17:52possible decisions for each agent
  374. 17:56so
  375. 17:59back to the I think model back to the
  376. 18:02binary Choice decision imagine that
  377. 18:04Alpha I is s i equal plus or minus one
  378. 18:10and that UI
  379. 18:14of the whole configuration is
  380. 18:19h
  381. 18:21Plus
  382. 18:22h i
  383. 18:25s i
  384. 18:27and here I'm using exactly the same
  385. 18:29notation as in the random field icing
  386. 18:31model Plus
  387. 18:33some
  388. 18:37over J different from i j i j s j
  389. 18:41times s i
  390. 18:44okay
  391. 18:46and so if you want to maximize your
  392. 18:50utility then it means that s i your
  393. 18:54choice must be in the direction of
  394. 18:58the sum of the external field which we
  395. 19:01we call the the common news the
  396. 19:04endosyncratic yield and the influence of
  397. 19:06others okay
  398. 19:10so
  399. 19:11um
  400. 19:12so this is the individual utility
  401. 19:14function which we are going to use
  402. 19:17in this uh hopping rate in in this
  403. 19:21transfer rate from T to C Prime but what
  404. 19:24you can show is that
  405. 19:26and we'll we're going to show it is that
  406. 19:29h
  407. 19:30is function of the configuration that
  408. 19:33we're looking for
  409. 19:35is equal actually to minus
  410. 19:39sum over I of H
  411. 19:42as h i s i
  412. 19:45so this system which is of course the
  413. 19:48independent contribution the what you
  414. 19:51see independence of what others do this
  415. 19:54you just sum over I as as usual but then
  416. 19:57the next term is not the sum over I of
  417. 20:01this one it's one half of that
  418. 20:03so plus one half
  419. 20:06of sum over I and J of s i g i g
  420. 20:12s j
  421. 20:14okay and so in general this is not equal
  422. 20:19to minus the sum
  423. 20:22over I of u i
  424. 20:25of of S5
  425. 20:30there's a one-half here
  426. 20:33so where does it come from well we just
  427. 20:35have to check what's going on
  428. 20:39uh we're going to check that
  429. 20:41um
  430. 20:42h of C Prime minus h of C
  431. 20:45as the correct form in order to ensure
  432. 20:48that this obeys detail balance so let me
  433. 20:53do it uh quietly so first of all let's
  434. 20:56notice that in this notation here
  435. 21:00it means that each jij appears only once
  436. 21:05okay each
  437. 21:07appears
  438. 21:11only one
  439. 21:15because of course you know for example
  440. 21:18one say J12 I can be equal to one and J
  441. 21:22equal to two but
  442. 21:25um but it can be the other way around so
  443. 21:27they are actually in this sum there's uh
  444. 21:30there's twice
  445. 21:31the contribution of gij but because of
  446. 21:33the one half here
  447. 21:35it's it's uh it should actually say
  448. 21:37appear I should just contribute
  449. 21:41foreign
  450. 21:48so let me compute h of C Prime
  451. 21:52minus h of t
  452. 21:58so h of T Prime minus h of C so what is
  453. 22:02e Prime and what is C here C Prime
  454. 22:06is the same as D so it's
  455. 22:09S1
  456. 22:11S2
  457. 22:13minus f i
  458. 22:16s n
  459. 22:19okay so this is what I mean
  460. 22:21in this General uh
  461. 22:26formalism here when Alpha can only take
  462. 22:30two two values then changing your
  463. 22:34decision is going from s i to minus s i
  464. 22:38Okay so
  465. 22:40you see that
  466. 22:43in this sum here the only term that will
  467. 22:46contribute is
  468. 22:49okay so maybe I should
  469. 22:53change my notation
  470. 22:56not to have either everywhere
  471. 23:00I'm changing the index of the sum to K
  472. 23:06and then I'm picking an I here so among
  473. 23:10all these K there's one I that
  474. 23:12corresponds there's one k that
  475. 23:14corresponds to I and for this one I need
  476. 23:17to change SSI into minus this I whereas
  477. 23:21all the other ones will be the same so
  478. 23:23when I take the difference here all the
  479. 23:26terms that are not equal to I in this
  480. 23:28term don't change and they cancel out
  481. 23:32and what I get in the end is twice
  482. 23:37h plus h i
  483. 23:40times s i
  484. 23:44okay
  485. 23:45twice because
  486. 23:47I went from s i to minus s i so the
  487. 23:50difference is 2si
  488. 23:52or minus 2si but there's a minus sign
  489. 23:55in front of that okay so the all the
  490. 23:58signs and the these details uh you
  491. 24:01should you know
  492. 24:02sit down and think about them but I hope
  493. 24:05I haven't made a sign mistake here and
  494. 24:07then in this sum here I should look at
  495. 24:11all the terms where one s i appears okay
  496. 24:15so uh s i k can be equal to I or J can
  497. 24:20be equal to 2i
  498. 24:22and but in any case as I said each
  499. 24:26link here appears only once and so
  500. 24:29because of that what you find is that
  501. 24:32the change of this interaction term when
  502. 24:35I change SI to minus SI is also twice
  503. 24:41um the sum over J
  504. 24:44of 3 i j s j s i
  505. 24:52okay each gij occurs wants so there's I
  506. 24:56mean again contributes once but because
  507. 24:59I change f i to minus s i the country
  508. 25:02the associated contribution changes by a
  509. 25:05factor 2 times s i
  510. 25:08so that's what we get
  511. 25:14and what I'm claiming is that and this
  512. 25:17is really obvious that this is also
  513. 25:19equal
  514. 25:20to minus
  515. 25:24UI of C Prime
  516. 25:27minus q i of C
  517. 25:31and this is Trivial because if you just
  518. 25:34look at at this term
  519. 25:36and you change S5 to minus s i you
  520. 25:38immediately find find this okay so what
  521. 25:42I'm saying is that if I choose H to be
  522. 25:45this function of spins with again a
  523. 25:48factor of one-half which is not the sum
  524. 25:50over I of UI then I'm make sure that if
  525. 25:55I take the ratio
  526. 25:58so
  527. 26:01I make sure because I can identify
  528. 26:04this UI C minus UIC Prime that this WC
  529. 26:08to C Prime is also equal to x amount 1
  530. 26:13over 1 or gamma sorry again one plus
  531. 26:16exponential of beta
  532. 26:19h of C
  533. 26:22Prime
  534. 26:24minus h
  535. 26:30okay and this is true whatever I I take
  536. 26:35so I have a function that is such that I
  537. 26:39obey Global balance at the level of the
  538. 26:41whole configuration space the
  539. 26:44configuration space being
  540. 26:46the set of all choices
  541. 26:50Okay so
  542. 26:51this example is very easy in a sense
  543. 26:54because I can explicitly construct
  544. 26:57the HSC that makes the choice of a scale
  545. 27:01balance but what I insist on is that you
  546. 27:04see that the interaction term
  547. 27:06makes the problem non-trivial makes the
  548. 27:09problem normative and of course this is
  549. 27:12expected because we know that in the
  550. 27:13presence of interaction the stationary
  551. 27:16State cannot be a product of individual
  552. 27:19choices because otherwise it would mean
  553. 27:22that people are not interacting
  554. 27:24so there's an interaction term and this
  555. 27:26interaction term can completely change
  556. 27:29uh the outcome
  557. 27:31and that's what I want to show now
  558. 27:35so this is
  559. 27:36this formalism that I just told you is a
  560. 27:39way to generalize the random field icing
  561. 27:42model uh to uh to non-zero temperature
  562. 27:46or to uh
  563. 27:48non-infinite values of beta you we we
  564. 27:52know how we would make the whole thing
  565. 27:54work because of course it's very similar
  566. 27:56to spins in physics
  567. 27:59but now I want to change a little bit
  568. 28:04the framework and tell you about
  569. 28:07the sharing model
  570. 28:10and read the setting model within this
  571. 28:12General formalism
  572. 28:21and so the the aim will be start to
  573. 28:24define the model and second will be to
  574. 28:29find this famous function HST that
  575. 28:33allows
  576. 28:34the tools of statistical mechanics to
  577. 28:37describe the equilibrium state of the
  578. 28:39system
  579. 28:44okay so as I said the shelling model
  580. 28:48was invented uh by Thomas shelling in
  581. 28:52the 70s
  582. 28:59and if you want to read more there's a
  583. 29:03literature that has developed in the
  584. 29:05physics
  585. 29:07Community recently but Thomas Jenning
  586. 29:10himself has a very nice book called uh
  587. 29:12from micromotives to macro Behavior
  588. 29:16where he's interested exactly in this
  589. 29:19transition from single agents to uh
  590. 29:23Collective effects and so what he what
  591. 29:26he was trying to understand was
  592. 29:28the fact that in U.S cities in
  593. 29:32particular there's a very strong racial
  594. 29:34segregation
  595. 29:36and and what he was puzzled by is that
  596. 29:39if you make surveys at the level of
  597. 29:41individual people
  598. 29:44um
  599. 29:44you know of course you know not all
  600. 29:47states are equivalent but in many states
  601. 29:50where there's a strong segregation
  602. 29:51people individually don't feel
  603. 29:54intolerant they don't feel that they
  604. 29:57want to live in their own Community uh
  605. 30:00their own uh in a community made by the
  606. 30:04same race
  607. 30:06so there's a kind of contradiction
  608. 30:08between individual preferences where
  609. 30:11people are not necessarily opposed to
  610. 30:13living in a mixed neighborhood and the
  611. 30:16actual observation that that he is tend
  612. 30:18to be extremely segregated
  613. 30:22and so he came up with a a very simple
  614. 30:24model and what I'm going to tell you
  615. 30:27about is the model that's inspired by
  616. 30:30the initial model is not exactly the
  617. 30:32same but it has the same uh flavor
  618. 30:36so what I'm going to imagine
  619. 30:39is a city made of
  620. 30:42neighborhoods
  621. 30:45so each Square here
  622. 30:48is going to be a neighborhood and the
  623. 30:51neighborhood is going to be
  624. 30:53labeled by the position of the center of
  625. 30:56the neighborhood for example
  626. 30:58and each neighborhood is going to be
  627. 31:01occupied by a certain number of people
  628. 31:05and there will be a number of vacancies
  629. 31:08or empty spaces or unconstructed sites
  630. 31:11the way you want to think of it and so
  631. 31:14I'm going to describe each neighborhood
  632. 31:16by the density of people in that
  633. 31:18neighborhood
  634. 31:20so row of R is equal to so if I if I
  635. 31:25want to be really
  636. 31:26physical
  637. 31:28each neighborhood is going to be used to
  638. 31:30assume to be assumed to have a square
  639. 31:34shape with a linear size L and so row of
  640. 31:37R is the number of people living in
  641. 31:40neighborhood r divided by L squared okay
  642. 31:47and what I'm saying is that uh here
  643. 31:50there's no question of race there's just
  644. 31:53a question of occupancy of density of
  645. 31:57population
  646. 31:58and what I'm going to assume is that
  647. 32:01people don't like to live in crowded
  648. 32:04neighborhoods because everything I mean
  649. 32:07you know I can tell you the story but
  650. 32:08you can imagine that you should live in
  651. 32:10an overcrowded neighborhood everything
  652. 32:11is difficult parking your car noise blah
  653. 32:15blah but people don't want to live
  654. 32:17either in uh discounted neighborhoods if
  655. 32:21you live in a neighborhood where there's
  656. 32:24no nobody and then there's no coffee
  657. 32:27houses there's no Cinemas blah blah so
  658. 32:30you don't want that either so we're
  659. 32:32going to assume that people have a
  660. 32:35preference
  661. 32:36for living in a kind of half filled the
  662. 32:41happy middle of half filled
  663. 32:43neighborhoods so I'm going to assume
  664. 32:45that row of r that you know this is
  665. 32:48normalized in such a way that this is
  666. 32:51something that belongs to zero one zero
  667. 32:53means there's nobody of course and one
  668. 32:55means that it's fully occupied
  669. 33:00so
  670. 33:02um what is the utility of agent I
  671. 33:05living in neighborhood r
  672. 33:09so here you see the choice of Agents
  673. 33:12will be the neighborhood so it's not a
  674. 33:15binary Choice it's a it's a choice that
  675. 33:18you know can have the infinite values if
  676. 33:21the city expands forever uh but it's uh
  677. 33:25it's a location here so this is the
  678. 33:27equivalent of the choices that I talked
  679. 33:30about before
  680. 33:32uh U of r
  681. 33:35is going to be equal to
  682. 33:38uh
  683. 33:39to you star
  684. 33:42times row of r
  685. 33:45if
  686. 33:47row is less or equal to a half
  687. 33:51and a two U star
  688. 33:54one minus row of r
  689. 33:59is uh row is placed or equal to
  690. 34:05so what what does it mean it means that
  691. 34:07if I plot
  692. 34:09U as a function of rho
  693. 34:13I have a tent shape
  694. 34:15function
  695. 34:18that Peaks
  696. 34:19around one half
  697. 34:21one half
  698. 34:24n is maximum is U star
  699. 34:29okay so that's that's what this function
  700. 34:31encodes and the choice here of a tent
  701. 34:34shape is just to make the calculation uh
  702. 34:37easier but what I'm going to tell you
  703. 34:39about does not depend on this particular
  704. 34:42choice I mean you can choose other
  705. 34:44functions so for example you might not
  706. 34:46like this
  707. 34:48discussed at one half so I could have
  708. 34:51chosen a function that does like this
  709. 34:57it doesn't really matter I mean the this
  710. 34:59function tent shape function is just
  711. 35:02there to illustrate the point is not a
  712. 35:04major uh aspect of the modeling
  713. 35:07Choice following procedure
  714. 35:11but so what I'm heading at here is that
  715. 35:15people in sheddings uh
  716. 35:19analog are you know they don't want to
  717. 35:22live in other in either extreme so it's
  718. 35:25like in the racial problem of shedding
  719. 35:27people don't want
  720. 35:29actually people are tolerant they they
  721. 35:31they actually prefer living in half uh
  722. 35:34filled neighborhoods so they're they're
  723. 35:36happy to be uh in in a mixed
  724. 35:39neighborhood in that sense
  725. 35:46so that's the setup of the model and
  726. 35:48what I'm going to look at is a case
  727. 35:51where the average
  728. 35:54density which I'm going to call rho Bar
  729. 35:57which is the total number of people
  730. 36:00divided by the total area of the city if
  731. 36:03you want the average density is exactly
  732. 36:06equal to one half
  733. 36:08so that's the choice that I'm going to
  734. 36:09make in order to amplify
  735. 36:13uh the point that's going to get out of
  736. 36:15the calculation is that on average
  737. 36:19there's enough people and even enough
  738. 36:22spaces such that all neighbors all
  739. 36:26neighborhoods could be filled at exactly
  740. 36:28one half okay so in in principle
  741. 36:32everything everybody can be happy in
  742. 36:34this model because
  743. 36:36there's exactly the right size of the
  744. 36:39city if you want to accommodate
  745. 36:40everybody in half space a half-filled
  746. 36:43neighborhood okay
  747. 36:45and in principle because everybody wants
  748. 36:47that this naturally should be what you
  749. 36:50find right
  750. 36:52so let's see what happens in the model
  751. 36:55and in order to understand what happens
  752. 36:57I need to give a rule for
  753. 37:00uh what people do
  754. 37:03and so I'm going to choose the choice
  755. 37:06theory that I've exposed earlier
  756. 37:09so what I'm going to assume is that the
  757. 37:12probability for an agent to go from r to
  758. 37:16R Prime
  759. 37:18okay
  760. 37:19is
  761. 37:21gamma divided one by one plus
  762. 37:24exponential of beta
  763. 37:28you
  764. 37:31I of
  765. 37:33uh rho of r
  766. 37:36minus u i of rho
  767. 37:40of our Prime
  768. 37:46Okay so
  769. 37:48if you want
  770. 37:49this is
  771. 37:51index I means that it's agent I who is
  772. 37:54moving is moving from R to R Prime and
  773. 37:57what he wants to see is whether the
  774. 37:59neighborhood at which he decides I mean
  775. 38:02that he you know visits to know whether
  776. 38:05he's going to move
  777. 38:08is the better suited than the current
  778. 38:11neighborhood
  779. 38:13so he looks at this function here and if
  780. 38:16he if he see the neighborhood where U is
  781. 38:18the higher he goes there
  782. 38:21with higher probability if if not he
  783. 38:24still may go there but with lower
  784. 38:25probability
  785. 38:27so if beta goes to Infinity he really
  786. 38:30systematically goes to neighborhoods
  787. 38:32that are better from his point of view
  788. 38:37but you see that again his decision or
  789. 38:40her decision is made based on only what
  790. 38:44happens to his or her utility function
  791. 38:49the choice doesn't take into account the
  792. 38:52fact that when you leave a neighborhood
  793. 38:55you're going to lower the popular the
  794. 38:57density obviously and therefore you're
  795. 39:00going to change the utility function of
  796. 39:02others because suddenly people will find
  797. 39:04themselves in a less populated
  798. 39:07environment but that you don't care you
  799. 39:10do it whatever
  800. 39:11and so people here uh you know take
  801. 39:15selfish decisions in that sense is that
  802. 39:17they only care about their own utility
  803. 39:19but they don't care about what they
  804. 39:21leave behind
  805. 39:22and we'll see how we could take that
  806. 39:25into account to uh obtain a better
  807. 39:28social outcome
  808. 39:29so clearly you know what I'm going to
  809. 39:33show you you've guessed because this is
  810. 39:35the whole uh Knack of the shedding model
  811. 39:38is the fact that although we've put
  812. 39:40everything in the model apparently to
  813. 39:43get the right social outcome so the
  814. 39:46right social outcome would be that
  815. 39:47everybody lives in half-based
  816. 39:49neighborhood then the dynamic this
  817. 39:52stochastic Dynamic here is going to lead
  818. 39:55to completely different outcome and it's
  819. 39:57going to lead to neighborhoods that are
  820. 39:59completely empty and neighborhoods that
  821. 40:02are more crowded than one half which is
  822. 40:06very surprising
  823. 40:08but in order to show this we have now
  824. 40:12the tools that we need which is quite
  825. 40:14remarkable because we're going to be
  826. 40:15able to map the problem in a sense to a
  827. 40:19problem of the liquid gas transition
  828. 40:24okay
  829. 40:27so
  830. 40:29now let's look
  831. 40:32at how the general framework that I've
  832. 40:35tried to tell you about is construction
  833. 40:37of the H function how does this work
  834. 40:41in the in the current situation
  835. 40:56I think that one microphone is on
  836. 41:00I think yes thank you
  837. 41:08okay so let me again try to understand
  838. 41:12what's going on so if I have One agent
  839. 41:18moving
  840. 41:21from
  841. 41:23R to R Prime
  842. 41:26how does it change the densities
  843. 41:29well clearly
  844. 41:31C Prime C is is
  845. 41:35the set of all the row of
  846. 41:39of
  847. 41:41Texas
  848. 41:43okay
  849. 41:45this is the what
  850. 41:48uh
  851. 41:49describes a configuration it's the it's
  852. 41:52the that's what I'm going to choose to
  853. 41:54describe your configuration I'm not I
  854. 41:56could choose to describe the
  855. 41:57configuration by the position of all the
  856. 41:59agents but actually the only thing that
  857. 42:01is going to matter is the density okay
  858. 42:05so if one agent goes from R to R Prime
  859. 42:08then uh C Prime
  860. 42:12will be the same density
  861. 42:15rho of x
  862. 42:18when X is different
  863. 42:20from R and R Prime
  864. 42:24okay and then
  865. 42:27row of r
  866. 42:30will have decreased a little bit by one
  867. 42:34unit so by 1 over L squared
  868. 42:39and R Prime on the contrary will have
  869. 42:42increased by a little bit
  870. 42:44which is 1
  871. 42:46over alphabet
  872. 42:49okay
  873. 42:52so that's my new configuration
  874. 42:55and what I want what I need to construct
  875. 42:57is
  876. 42:59what is the what is it that I want
  877. 43:02exactly as in the ising case I want to
  878. 43:04construct h of t
  879. 43:08such that
  880. 43:12HSC Prime
  881. 43:15minus h of B
  882. 43:19is equal
  883. 43:21to minus UI of uh
  884. 43:25R minus UI
  885. 43:29of R Prime of rho of r
  886. 43:35minus UI of rho of R Prime
  887. 43:39okay
  888. 43:41if I manage to construct such a function
  889. 43:44which in a sense now I think the kind of
  890. 43:48functional of all these densities
  891. 43:50then as I've shown in the icing case I
  892. 43:54ensure that the choice at the individual
  893. 43:57level corresponds to detailed balance at
  894. 44:00the global level okay
  895. 44:03so I'm going to assume that there exists
  896. 44:06such a function so I'm going to assume
  897. 44:09that h of C is a sudden function
  898. 44:13of all the rows
  899. 44:22and I need to understand how does this
  900. 44:25function evolve when I go from C to C
  901. 44:27Prime so
  902. 44:29[Music]
  903. 44:31if I assume that
  904. 44:33L is sufficiently large so that one over
  905. 44:36L squared
  906. 44:37is very small compared to one
  907. 44:41I can make a kind of failure expansion
  908. 44:44if you want
  909. 44:45of how the change of density on R and on
  910. 44:49R Prime is going to change the function
  911. 44:52H that depends on all the density
  912. 44:55and so what you find is that
  913. 44:57h of e Prime
  914. 44:59minus h of C
  915. 45:03and all that the rows that have not
  916. 45:06changed don't contribute at all
  917. 45:09and only the change that I've uh
  918. 45:12imposed to the the density at R and that
  919. 45:15R Prime will contribute to this change
  920. 45:17so what I get is
  921. 45:20uh
  922. 45:25derivative of H with respect to rho of r
  923. 45:32times uh
  924. 45:34-1
  925. 45:38or let me set it that way dh0 prime time
  926. 45:431 over L squared
  927. 45:45minus
  928. 45:47DH
  929. 45:50e row of r
  930. 45:54times one over Rel Square
  931. 45:58I'm assuming that H is a function of all
  932. 46:00the densities is the density is changed
  933. 46:03by a little bit then I can tailor expand
  934. 46:06the variation so I have the derivative
  935. 46:09of each but with respect to rho of R
  936. 46:11Prime Times the change one over L
  937. 46:13squared plus the derivative of the H
  938. 46:16with respect to rho times the change
  939. 46:18minus one over real squared okay
  940. 46:22and as I said this must be equal to what
  941. 46:24it must be equal to minus
  942. 46:30U of rho of r
  943. 46:33Prime
  944. 46:35minus
  945. 46:37U of Rover
  946. 46:51okay
  947. 46:53so
  948. 46:54big thanks to this equation here I can
  949. 46:58you know
  950. 46:59guess what H should be
  951. 47:02if I take H to be
  952. 47:05uh the anti-derivative of U with respect
  953. 47:09to rho it's going to work so let's let
  954. 47:13me write it down and then we'll check
  955. 47:16so this is the function this is the
  956. 47:18equation
  957. 47:20which must be true for all row of R rho
  958. 47:22of R Prime
  959. 47:24that ensures that if I can find a
  960. 47:26function H that obeys this equation this
  961. 47:29differential equation in row if you want
  962. 47:32then I'm sure that I will have detailed
  963. 47:35balance okay I will have a detailed
  964. 47:38balance although
  965. 47:39people act individually and only follow
  966. 47:42their use
  967. 47:44uh the function H will ensure that
  968. 47:46globally the system away details balance
  969. 47:48even taking into account the interaction
  970. 47:52this is exactly the same story as for
  971. 47:54the icing model where you can find an
  972. 47:58age
  973. 47:58which is not the sum of the use but
  974. 48:02which ensures that skill balance is a
  975. 48:05base
  976. 48:05okay so let me give you the solution and
  977. 48:09then we'll see by eye that it works
  978. 48:12foreign
  979. 48:26[Music]
  980. 48:28so what I'm claiming is that if I choose
  981. 48:31h
  982. 48:32of all the rows
  983. 48:34of x
  984. 48:40equal
  985. 48:42L squared
  986. 48:45thumb over all r's
  987. 48:50or X's
  988. 48:53of
  989. 48:55the integral from 0 to rho of x
  990. 49:01is a minus sign that I shouldn't forget
  991. 49:04U
  992. 49:08of
  993. 49:09um row Prime
  994. 49:11hero Prime
  995. 49:15and then plus an arbitrary constant a
  996. 49:18times
  997. 49:19wrote
  998. 49:21okay
  999. 49:33so this is the general solution of the
  1000. 49:36detailed balance uh Criterion because
  1001. 49:39you see that if I take the derivative of
  1002. 49:42this function of all rows with respect
  1003. 49:45to a certain row of r
  1004. 49:47I'm going to pick in this sum
  1005. 49:50r equal to X and I will take the
  1006. 49:53derivative with respect to rho which is
  1007. 49:55easy because it's the
  1008. 49:57anti-derivative so the derivative
  1009. 49:59respect row of R will give me U of uh
  1010. 50:03row of R which is exactly what I need
  1011. 50:06okay
  1012. 50:08and this will give a constant and the
  1013. 50:10constant will disappear because if I'm
  1014. 50:13subtracting uh the two derivatives
  1015. 50:16computed at different points a just
  1016. 50:19cancels out okay
  1017. 50:21so this is the solution I'm looking for
  1018. 50:25and you see right away that what is
  1019. 50:28interesting is that this is not equal
  1020. 50:32to uh
  1021. 50:35integral
  1022. 50:37sum of Rex
  1023. 50:40of rho of x
  1024. 50:44U of of row of x
  1025. 50:50that should be maybe an elsewhere
  1026. 50:52normalizing but anyway it's it's a
  1027. 50:55different
  1028. 50:56uh functional of row this would be the
  1029. 51:00naive thing you know if each agent has a
  1030. 51:03utility u of rho then the number of
  1031. 51:06Agents having that utility is number of
  1032. 51:09people in neighborhood X rho of x times
  1033. 51:12U so this is the this would be the
  1034. 51:15independent
  1035. 51:19assumption
  1036. 51:22but you see clearly that what I have
  1037. 51:24here is not row U of rho is the the
  1038. 51:27anti-derivative
  1039. 51:29of you
  1040. 51:32okay
  1041. 51:35great so that's the solution I was
  1042. 51:38looking for
  1043. 51:40and now what can I say about the
  1044. 51:43long-time evolution of the system
  1045. 51:45so let me recall what uh we know we know
  1046. 51:49that if
  1047. 51:50we call
  1048. 51:53if
  1049. 51:54w c to C Prime
  1050. 51:58over WC Prime to C
  1051. 52:01obey detail balance
  1052. 52:07then at long time
  1053. 52:10I know that the equilibrium distribution
  1054. 52:13the probability to find the sun
  1055. 52:15configuration is one over Z exponential
  1056. 52:19of minus beta HSE
  1057. 52:24so now I'm going to use this result to
  1058. 52:27try to understand what this result tells
  1059. 52:31me in terms of the densities I'm going
  1060. 52:33to try to interpret what it means
  1061. 52:35but uh that's the whole power of having
  1062. 52:40a model that obeys detailed balance is
  1063. 52:42the fact that you know right away what
  1064. 52:44the stationary state is going to be
  1065. 52:47but at this stage I should put a big
  1066. 52:51warning sign
  1067. 52:55which is the possibility of slow dynamic
  1068. 53:01okay so it's always the case that you
  1069. 53:04know when you read papers on
  1070. 53:07uh
  1071. 53:09Monte Carlo Dynamics or Master equations
  1072. 53:12or Markov chain Evolutions then it's
  1073. 53:15great because you can get a stationary
  1074. 53:18State that's explicit which would not be
  1075. 53:21the case
  1076. 53:22for arbitrary choices of the W's but on
  1077. 53:26the other hand you know you don't know
  1078. 53:28at all
  1079. 53:29if you're going to reach the stage 3
  1080. 53:31State quickly or slowly
  1081. 53:34and this is the problem that sometimes
  1082. 53:37is not present that is on reasonable
  1083. 53:41time scales you reach the equilibrium
  1084. 53:43but in some cases
  1085. 53:46and in particular in this model when you
  1086. 53:48try to make the numerical simulation you
  1087. 53:50realize that although the stationary
  1088. 53:52state is uh that one then you can have a
  1089. 53:57very slow Dynamic setting in and uh and
  1090. 54:00so you know there's a whole discussion
  1091. 54:01that should be made and this often
  1092. 54:03eluded in uh
  1093. 54:06in in the literature in particular in
  1094. 54:09economics literature is how fast do you
  1095. 54:12reach Equity room and in this question
  1096. 54:14of the speed at which you reach
  1097. 54:16equilibrium is of course absolutely
  1098. 54:19crucial to know whether what you're
  1099. 54:21talking about is Meaningful or
  1100. 54:23meaningless and there's a lot of uh
  1101. 54:25models in economics where people assume
  1102. 54:27equilibrium without
  1103. 54:29really trying to answer the question of
  1104. 54:31is it reasonable to think that the
  1105. 54:33Dynamics is going to lead me to
  1106. 54:34equilibrium quickly or slowly and in
  1107. 54:37particular well in in the physics the
  1108. 54:40problem there's a lot of examples where
  1109. 54:43uh the system has a boltzmann
  1110. 54:46distribution in equilibrium but never
  1111. 54:50reaches it like glasses glassy systems
  1112. 54:53or the spin blasters that I'm going to
  1113. 54:55talk about there are special systems in
  1114. 54:58the sense that although you know their
  1115. 55:00equilibrium state in reality If You
  1116. 55:03observe the system even over you know
  1117. 55:07if
  1118. 55:09astronomical time or geological times
  1119. 55:11they are actually out of equilibrium so
  1120. 55:14you know beware of these General
  1121. 55:17statements that look great but actually
  1122. 55:20sweep a lot of issues under the rug
  1123. 55:25okay so having said that
  1124. 55:27let me apply
  1125. 55:32this General
  1126. 55:34result to the problem at hand
  1127. 56:01so what I want to know is what is the
  1128. 56:04stationary
  1129. 56:05distribution of the equilibrium
  1130. 56:07distribution
  1131. 56:09of some
  1132. 56:13set of row of x okay so again a
  1133. 56:17configuration is
  1134. 56:21described by
  1135. 56:24a set of densities you should know all
  1136. 56:26the densities in all the neighborhoods
  1137. 56:28row of row one row two Row three and so
  1138. 56:32on
  1139. 56:33and this gives me uh
  1140. 56:37a description of the coarse grain
  1141. 56:39description of the equilibrium because
  1142. 56:41at this stage I've lost
  1143. 56:43the information of who lives who
  1144. 56:46I just have a an information about the
  1145. 56:50densities in each neighborhood
  1146. 56:52and the probability to observe a certain
  1147. 56:55configuration Row one road to row three
  1148. 56:57well I know it is
  1149. 57:01going to be given by
  1150. 57:04the Wilson Way so there's a
  1151. 57:05normalization
  1152. 57:08there's a boltzmann weight
  1153. 57:10that I've
  1154. 57:12written here so
  1155. 57:15it's going to be given by
  1156. 57:18exponential of minus beta
  1157. 57:21L squared
  1158. 57:24sum over X
  1159. 57:28of V
  1160. 57:30of row of x
  1161. 57:35where I've introduced the notation
  1162. 57:40here I'm going to call the
  1163. 57:42antiderivative of U
  1164. 57:45V so well
  1165. 57:50let's write it here
  1166. 57:52so V is such that D Prime of rho is
  1167. 57:56equal to U
  1168. 58:04and importantly because there's a minus
  1169. 58:07sign in H
  1170. 58:09and the minus in front of the
  1171. 58:13Aviation the Bossman way there's a plus
  1172. 58:15in the end that comes here
  1173. 58:19um the sum of rects of rho of X this is
  1174. 58:22the the total number of people in the
  1175. 58:25city so this doesn't change so a is uh
  1176. 58:28is arbitrary constant and it actually
  1177. 58:31you can reabsorb it in the normalization
  1178. 58:34it doesn't play any role I'm dropping it
  1179. 58:38but there's something that you should uh
  1180. 58:42be familiar with which is the fact that
  1181. 58:46this is
  1182. 58:48the weight that comes from
  1183. 58:50uh the people the choice of the people
  1184. 58:53but there's on top of that in the
  1185. 58:56property distribution of all the row of
  1186. 58:57X the entropy term which comes from the
  1187. 59:00fact that as I've said I'm describing
  1188. 59:02the configuration in terms of densities
  1189. 59:05and knots in terms of who lives where
  1190. 59:07and therefore for a given choice of rho
  1191. 59:11there's a there's a community
  1192. 59:13combinatorial problem which is which
  1193. 59:16leads to an entropy term on top of that
  1194. 59:18which is given by I'm going to write it
  1195. 59:21exponential of s of rho
  1196. 59:25which is the number of possible choices
  1197. 59:28to put my all my individuals in the city
  1198. 59:32with the correct
  1199. 59:34uh choice of densities and S of row is
  1200. 59:38given by the familiar
  1201. 59:41entropy term which is the
  1202. 59:44the ideal gas entropy if you want so
  1203. 59:47it's sum of Rex
  1204. 59:49of row of x
  1205. 59:53log
  1206. 59:56of 4 of x
  1207. 59:58Plus
  1208. 1:00:001 minus rho of x
  1209. 1:00:03log
  1210. 1:00:04of 1 minus 4.
  1211. 1:00:08and there's an overall minus sign
  1212. 1:00:11so if you want to be you know very
  1213. 1:00:14precise about
  1214. 1:00:16going from individuals to densities you
  1215. 1:00:19should take into account this entropy
  1216. 1:00:22which you can see it is a kind of
  1217. 1:00:24Jacobian in the transformation
  1218. 1:00:26from people's uh
  1219. 1:00:29physician to the dentist eco
  1220. 1:00:32but the entropy is going to actually as
  1221. 1:00:36usual at low temperature the entropy is
  1222. 1:00:38not going to matter so I'm going to
  1223. 1:00:40focus
  1224. 1:00:43on
  1225. 1:00:45beta large
  1226. 1:00:49such that
  1227. 1:00:51s is negligible
  1228. 1:00:57one can actually do the theory
  1229. 1:00:58completely also with the entropy term
  1230. 1:01:01and I'll give you the results at the end
  1231. 1:01:03but what I'm going to focus on is just
  1232. 1:01:06this term here
  1233. 1:01:08uh and I'm going to disregard the
  1234. 1:01:11entropy contribution
  1235. 1:01:14so okay so now I have my the probability
  1236. 1:01:17of a given set of densities
  1237. 1:01:21which is given by the exponential of
  1238. 1:01:23beta the sum of Rex of some function V
  1239. 1:01:25of the density
  1240. 1:01:28right okay so what what should I do I
  1241. 1:01:32mean this is uh this is what the
  1242. 1:01:34probability of observing a certain set
  1243. 1:01:36of density is but if I want to make this
  1244. 1:01:39more concrete more visible I should you
  1245. 1:01:43know try to speak about the most
  1246. 1:01:45probable uh configuration
  1247. 1:01:48and in particular when beta goes to
  1248. 1:01:50Infinity
  1249. 1:01:51this is everything that's going to
  1250. 1:01:53matter is what are the most probable
  1251. 1:02:00the most probable
  1252. 1:02:02configuration
  1253. 1:02:04configuration
  1254. 1:02:20foreign
  1255. 1:02:32X and try to find the configuration of
  1256. 1:02:36row that maximize such an object with
  1257. 1:02:40the definition that D Prime is equal to
  1258. 1:02:41U and so if I want to give you the
  1259. 1:02:45explicit
  1260. 1:02:47function D of rho is equal to
  1261. 1:02:50you star rho squared
  1262. 1:02:54when rho is less than one half
  1263. 1:02:57and U star
  1264. 1:03:00two row minus row squared minus one half
  1265. 1:03:05when rho is greater or equal to the half
  1266. 1:03:10and what I need to do is
  1267. 1:03:12um
  1268. 1:03:13to try to find the configurations of the
  1269. 1:03:15rows that maximize
  1270. 1:03:18this V of row
  1271. 1:03:20with the constraint
  1272. 1:03:22that the average value of rho is equal
  1273. 1:03:24to one half
  1274. 1:03:30okay this is the case that I've chosen
  1275. 1:03:32because it's the most uh uh
  1276. 1:03:36spectacular case if you want
  1277. 1:03:39so V of rho has a certain shape here
  1278. 1:03:41that I could draw but it doesn't really
  1279. 1:03:43matter uh this is the explicit form and
  1280. 1:03:47here I'm left with a problem that we
  1281. 1:03:51used to in uh the statistical mechanics
  1282. 1:03:56which is you know in a sense the problem
  1283. 1:03:59of a liquid gas transition where
  1284. 1:04:03the there's an entropy contribution that
  1285. 1:04:05I'm discarding anyway and then there's
  1286. 1:04:07an energy contribution telling you uh
  1287. 1:04:10you know what is the typical energy of a
  1288. 1:04:14gas without with a sudden density
  1289. 1:04:19and so by analogy
  1290. 1:04:23and one can show that it indeed the case
  1291. 1:04:26but by analogy one can look for a
  1292. 1:04:29solution where
  1293. 1:04:31rho takes two values
  1294. 1:04:42so
  1295. 1:04:45look for a solution
  1296. 1:04:49such that
  1297. 1:04:52rho is equal to
  1298. 1:04:54row plus
  1299. 1:04:55greater than one half
  1300. 1:04:58with probability
  1301. 1:05:02p
  1302. 1:05:04and row minus less than one half
  1303. 1:05:07with probability
  1304. 1:05:09one minus t
  1305. 1:05:11okay
  1306. 1:05:13so
  1307. 1:05:15if I do this I see that the sum over X
  1308. 1:05:19of V of rho of x
  1309. 1:05:25is equal to the number of neighborhoods
  1310. 1:05:37times
  1311. 1:05:39p V of row Plus
  1312. 1:05:421 minus t
  1313. 1:05:46of rho minus
  1314. 1:05:49and I should optimize over
  1315. 1:05:52p rho plus and row minus with uh the
  1316. 1:05:57constraint
  1317. 1:05:59so
  1318. 1:06:01I'm looking for the maximum of this
  1319. 1:06:06with a constraint that P row plus plus
  1320. 1:06:09one might one minus P row minus must be
  1321. 1:06:13equal to one half
  1322. 1:06:15or more generally to robot
  1323. 1:06:20okay
  1324. 1:06:21so you know if I do this well maybe I I
  1325. 1:06:25will find that in the end row plus is
  1326. 1:06:27equal to row minus or that P is equal to
  1327. 1:06:29one so that would be a uniform solution
  1328. 1:06:33but I can also find solution where row
  1329. 1:06:36plus and row minus are different and P
  1330. 1:06:38is neither equal to uh zero node to a
  1331. 1:06:42half
  1332. 1:06:43and
  1333. 1:06:44again in the limits where beta goes to
  1334. 1:06:47Infinity in the low temperature limits
  1335. 1:06:49and for this particular choice of V of
  1336. 1:06:52rho I'm
  1337. 1:06:55I'm not going to you know give you the
  1338. 1:06:57calculation which is not very difficult
  1339. 1:06:59but a little heavy
  1340. 1:07:01um one has to you know distinguish
  1341. 1:07:03different cases but in the end what one
  1342. 1:07:06finds is that the configuration that
  1343. 1:07:08maximizes
  1344. 1:07:10so the optimal configuration
  1345. 1:07:13or the most probable configuration
  1346. 1:07:15because you see that if I maximize this
  1347. 1:07:18object
  1348. 1:07:21again I'm insisting on the fact that
  1349. 1:07:23most probable configurations this amount
  1350. 1:07:26to maximizing this object so if I
  1351. 1:07:29maximize the object I'm optimizing this
  1352. 1:07:31object I'm also maximizing the
  1353. 1:07:34probability of observing such a
  1354. 1:07:36configuration and the optimal Choice the
  1355. 1:07:38optimal uh uh configuration
  1356. 1:07:45are such that
  1357. 1:07:48rho minus equals zero
  1358. 1:07:51rho plus equals
  1359. 1:07:53uh
  1360. 1:07:54square root of two over two
  1361. 1:07:58and this is also equal to p
  1362. 1:08:03it turns out that you know don't give
  1363. 1:08:05too much meaning to this but it turns
  1364. 1:08:08out that row plus is square root of two
  1365. 1:08:09over two which is 0.7
  1366. 1:08:12and uh rho minus the zero so you see by
  1367. 1:08:16you know inspection that P times row
  1368. 1:08:18plus is one half
  1369. 1:08:21and because row minus is zero this
  1370. 1:08:23doesn't contribute so I'm satisfying the
  1371. 1:08:25constraint but you also see that the
  1372. 1:08:28optimal configurations the
  1373. 1:08:29configurations that you'll see most
  1374. 1:08:31often are such are the following
  1375. 1:08:34so if I draw my little city again with
  1376. 1:08:37neighborhoods
  1377. 1:08:39I will have with probability
  1378. 1:08:410.3 completely empty spaces
  1379. 1:08:45and with probability 0.7
  1380. 1:08:50neighborhoods that are over crowded with
  1381. 1:08:54a density row plus which is
  1382. 1:08:56square root of two over two
  1383. 1:08:59and this is the most likely
  1384. 1:09:01configuration
  1385. 1:09:03and so this is the you know very
  1386. 1:09:05surprising result that
  1387. 1:09:08um
  1388. 1:09:09shelling
  1389. 1:09:11was able to
  1390. 1:09:13show experimentally I mean it's quite
  1391. 1:09:16remarkable the way shedding did shedding
  1392. 1:09:18simulated uh this his model with coin
  1393. 1:09:23and he was making you know the the the
  1394. 1:09:25changes without any computer at the time
  1395. 1:09:29he was making these changes by hand and
  1396. 1:09:32he was seeing that systematically by
  1397. 1:09:34following rules similar to this he was
  1398. 1:09:37you know uh led to uh segregation of
  1399. 1:09:40these coins coins of different colors
  1400. 1:09:42and so it was a very also visual uh way
  1401. 1:09:46to to see it
  1402. 1:09:48but in any case uh the the transposition
  1403. 1:09:52of the shedding model to the physics
  1404. 1:09:54language is due to a paper by clover
  1405. 1:10:02Berta
  1406. 1:10:06at all
  1407. 1:10:08that you can find easily on on the net
  1408. 1:10:10that I can also give you I can give you
  1409. 1:10:13the reference but it's it's in tnaf
  1410. 1:10:15proceedings of National Academy of
  1411. 1:10:18Sciences and uh and so they they
  1412. 1:10:21essentially do what I've uh told you
  1413. 1:10:24today
  1414. 1:10:25so what is nice is that we have this
  1415. 1:10:28completely paradoxical resolve
  1416. 1:10:31if you want you know the story of uh
  1417. 1:10:33Adam Smith Adam Smith
  1418. 1:10:36thinks that if people act act selfishly
  1419. 1:10:39uh and optimize their own welfare then
  1420. 1:10:43the society as a whole is going to
  1421. 1:10:45benefit and here in this case you see an
  1422. 1:10:48example of the exact opposite that
  1423. 1:10:50people follow what they want to do and
  1424. 1:10:53everybody you know is doing something
  1425. 1:10:55that he or she feels is good for him or
  1426. 1:10:59her but in the end Collective leads a
  1427. 1:11:02disaster
  1428. 1:11:03and it's a disaster because there's this
  1429. 1:11:08the the fact that the rule of the game
  1430. 1:11:09doesn't take into account
  1431. 1:11:11uh the pain you leave behind Okay the
  1432. 1:11:14fact that when you change your your
  1433. 1:11:16position the people living in your ex
  1434. 1:11:19neighborhood are worse off and so they
  1435. 1:11:22won't they will try to leave too and so
  1436. 1:11:25on and this is the mechanism by which uh
  1437. 1:11:28the configuration where everybody lives
  1438. 1:11:30in the same neighborhood is actually
  1439. 1:11:31unstable Dynamics if you start by a
  1440. 1:11:34configuration where all the
  1441. 1:11:36neighborhoods are filled with the
  1442. 1:11:37density one half you can show that you
  1443. 1:11:40know accidentally someone who is going
  1444. 1:11:41to leave and then the whole situation
  1445. 1:11:44will evolve how this situation although
  1446. 1:11:47maybe on long time scale
  1447. 1:11:49so it's a very beautiful model I think
  1448. 1:11:51in that sense
  1449. 1:11:53and let me give you a few more
  1450. 1:11:57information about the model
  1451. 1:12:00uh one is what happens if
  1452. 1:12:04beta is non-infinite if beta is
  1453. 1:12:09is if we're not in the low temperature
  1454. 1:12:12limits well in the Lo if you increase
  1455. 1:12:16temperature
  1456. 1:12:19you decrease beta
  1457. 1:12:23and you see that in the limit where beta
  1458. 1:12:26goes to zero but a very high temperature
  1459. 1:12:30only the entropy matters
  1460. 1:12:32and clearly as you all know the entropy
  1461. 1:12:36is maximized for row equal one-half
  1462. 1:12:39and so obviously if people take choices
  1463. 1:12:42completely at random
  1464. 1:12:44then the density is going to be uniform
  1465. 1:12:47right because if you completely choose
  1466. 1:12:49randomly then all neighborhoods are
  1467. 1:12:51completely equivalent and in the end
  1468. 1:12:53you'll end up with a uniform
  1469. 1:12:55distribution and this is driven by
  1470. 1:12:58entropy exactly as in the liquid gas
  1471. 1:13:00transition as you increase temperature
  1472. 1:13:02at one point energy won't matter anymore
  1473. 1:13:05and you'll recover
  1474. 1:13:07a gas phase which is the uniform in
  1475. 1:13:11space but if you lower temperature you
  1476. 1:13:13know that in the liquid gas transition
  1477. 1:13:15there's a space stress separation the
  1478. 1:13:16liquid goes on one side and leaves the
  1479. 1:13:19void behind and so in a sense it's the
  1480. 1:13:22same thing that we see here
  1481. 1:13:25um and so you can show that in this
  1482. 1:13:27model that there exists a critical
  1483. 1:13:30temperature basic C
  1484. 1:13:32such that at higher temperature so for
  1485. 1:13:35data greater than beta C there's
  1486. 1:13:37segregation
  1487. 1:13:42and for beta less than beta C there's
  1488. 1:13:45the the solution is uniform
  1489. 1:13:51so that's an Insight that we know very
  1490. 1:13:54well from physics but uh which is maybe
  1491. 1:13:57more surprising if you don't know the
  1492. 1:13:59nominology of this transition and so on
  1493. 1:14:02so
  1494. 1:14:04we're in in known territories here we
  1495. 1:14:08know that uh Collective effects
  1496. 1:14:10can completely change what you uh within
  1497. 1:14:15what your intuition would tell you from
  1498. 1:14:18microscopic elements here we see that
  1499. 1:14:21microscopically people want to live in
  1500. 1:14:23half neighborhood a half cell
  1501. 1:14:25neighborhood but collectively because of
  1502. 1:14:28this systematic application systematic
  1503. 1:14:31iteration of the dynamical rule that is
  1504. 1:14:33the one that I've given you you end up
  1505. 1:14:35in uh
  1506. 1:14:37in Dire Straits
  1507. 1:14:40okay so is there a way to improve
  1508. 1:14:58the situation so
  1509. 1:15:00as the question also that is addressed
  1510. 1:15:03in the paper that I've
  1511. 1:15:06that I've referred to
  1512. 1:15:08is there
  1513. 1:15:10a solution
  1514. 1:15:15to this conundrum
  1515. 1:15:26so is there a way that maybe the state
  1516. 1:15:29or maybe
  1517. 1:15:32social
  1518. 1:15:34solution can help the system coordinate
  1519. 1:15:37and find a more acceptable uh maximum
  1520. 1:15:43configuration
  1521. 1:15:45optimal configuration
  1522. 1:15:47so the idea that um
  1523. 1:15:50they propose in the paper that the
  1524. 1:15:52office that I've uh mentioned proposed
  1525. 1:15:55in the paper is to say well let's
  1526. 1:15:59help people in doing the right thing by
  1527. 1:16:03imposing a kind of tax
  1528. 1:16:05which is that
  1529. 1:16:09um
  1530. 1:16:10as I've shown you there's h
  1531. 1:16:14but there's also
  1532. 1:16:16the total U
  1533. 1:16:19which is uh
  1534. 1:16:21the sum over X of rho of x
  1535. 1:16:26U of rho of x
  1536. 1:16:31so this is something that people don't
  1537. 1:16:34really know about individually the total
  1538. 1:16:37satisfaction of people but
  1539. 1:16:40a superstructure like the state could
  1540. 1:16:43measure This Global utility and
  1541. 1:16:47as people make their choice they should
  1542. 1:16:50be aware of the change in total utility
  1543. 1:16:53that they their choice
  1544. 1:16:55uh
  1545. 1:17:01induces so instead of only looking at
  1546. 1:17:04the change of individual utility you can
  1547. 1:17:07think that maybe if I in the in the
  1548. 1:17:11decision rule if I change Delta U
  1549. 1:17:14of rho R minus U of rho of R Prime into
  1550. 1:17:18Delta U plus Theta
  1551. 1:17:22times
  1552. 1:17:24Delta capital u minus Delta U
  1553. 1:17:32so sorry maybe my capital u is not
  1554. 1:17:36different enough from small you so what
  1555. 1:17:39I'm saying here is that there's a
  1556. 1:17:40parameter data which on top of the
  1557. 1:17:43change of your own utility
  1558. 1:17:45adds some contributions from the change
  1559. 1:17:48of the global utility that you'll move
  1560. 1:17:50uh provokes okay
  1561. 1:17:53so if data is equal to zero you recover
  1562. 1:17:56the previous model
  1563. 1:17:58if Theta is equal to one you don't take
  1564. 1:18:01into account your own utility you only
  1565. 1:18:03take into account the global utility
  1566. 1:18:07so
  1567. 1:18:08you can think of that as a kind of tax
  1568. 1:18:11right if you change it you think you
  1569. 1:18:13have others you must pay something and
  1570. 1:18:15therefore it's going to reduce the
  1571. 1:18:17probability of making your your move
  1572. 1:18:21so Theta here is a parameter that you
  1573. 1:18:23can interpret as a tax
  1574. 1:18:27and you can redo the whole calculation
  1575. 1:18:29that I've done
  1576. 1:18:31uh it's actually quite easy because in
  1577. 1:18:34the end what you find if you redo the
  1578. 1:18:37whole step is you find that V of row the
  1579. 1:18:40empty derivative of U that I found
  1580. 1:18:43before this one is just transformed into
  1581. 1:18:46one minus data V of rho
  1582. 1:18:51plus Theta
  1583. 1:18:53row U of row
  1584. 1:18:57and this is not surprising it's just uh
  1585. 1:19:00you know looking at what I've uh defined
  1586. 1:19:04here I see that there's the part that
  1587. 1:19:06comes from the V of row that I had
  1588. 1:19:10before but a part that also comes from
  1589. 1:19:13the total utility row UFO
  1590. 1:19:16so you turn the crank you do the same
  1591. 1:19:19calculation as the one I've sketched for
  1592. 1:19:22you you look for the maximum uh probably
  1593. 1:19:25the configurations with maximum
  1594. 1:19:27probability and what you find is that
  1595. 1:19:31as a function of
  1596. 1:19:33data
  1597. 1:19:37the total utility per agent
  1598. 1:19:41U divided by n
  1599. 1:19:45is going to have this the following
  1600. 1:19:47shape so this is one here
  1601. 1:19:56red you don't like so
  1602. 1:20:00choose blue for example
  1603. 1:20:02so what happens is that for data equals
  1604. 1:20:050
  1605. 1:20:07um with the values of row plus equals
  1606. 1:20:09square root of 2 over 2 that I've given
  1607. 1:20:11you you can compute
  1608. 1:20:13um
  1609. 1:20:14the maximum the the utility
  1610. 1:20:17per agent is given by
  1611. 1:20:21I don't know blue you shouldn't either
  1612. 1:20:25maybe yellow
  1613. 1:20:28or green
  1614. 1:20:32so you start from a value that's around
  1615. 1:20:350.3 U star
  1616. 1:20:37foreign
  1617. 1:20:41by the way the the completely uniform
  1618. 1:20:44solution
  1619. 1:20:53you can also compute
  1620. 1:20:55its utility it
  1621. 1:20:58it's U star over four
  1622. 1:21:04so Point 25 you star if you if you're
  1623. 1:21:07all mixed
  1624. 1:21:09but the segregated solution has a better
  1625. 1:21:11you start per person which is 0.3
  1626. 1:21:14instead of 0.25 so it's just re-saying
  1627. 1:21:17what I was saying that the system will
  1628. 1:21:20segregate but what's really interesting
  1629. 1:21:23is that
  1630. 1:21:26as you increase data
  1631. 1:21:31there's a value of data which is one
  1632. 1:21:33third where you reach
  1633. 1:21:37uh
  1634. 1:21:39U star over 2.
  1635. 1:21:45sorry U star
  1636. 1:21:52so
  1637. 1:21:54um what you see is that by introducing
  1638. 1:21:57this extra tags at first you improve the
  1639. 1:21:59situation but it still remains
  1640. 1:22:01sub-optimal
  1641. 1:22:02and then at one point you reach
  1642. 1:22:06um
  1643. 1:22:08uh you reach the optimal state
  1644. 1:22:11of everybody segregates everybody living
  1645. 1:22:14in in the same neighborhood
  1646. 1:22:22so that's an example where the the
  1647. 1:22:25um Adam Gibbs Adam Smith
  1648. 1:22:29invisible hand fails but you can help it
  1649. 1:22:32by having
  1650. 1:22:34um
  1651. 1:22:35these taxes that I talked about
  1652. 1:22:38okay
  1653. 1:22:41so
  1654. 1:22:43that was the the main message what I
  1655. 1:22:45wanted to finally end on this the
  1656. 1:22:48problem is that I've assumed uh in the
  1657. 1:22:52choice Theory I've assumed a very
  1658. 1:22:54particular shape of hopping rate
  1659. 1:22:57you remember that I've insisted on that
  1660. 1:23:00from the beginning
  1661. 1:23:02um I've assumed that the W's
  1662. 1:23:05are given by this the so-called logistic
  1663. 1:23:11rule
  1664. 1:23:23w c to C Prime
  1665. 1:23:27is given by gamma over one plus
  1666. 1:23:30exponential beta Delta U
  1667. 1:23:34so this has allowed me to find an H
  1668. 1:23:37function that
  1669. 1:23:39is such that the whole system of a
  1670. 1:23:42detailed balance and thanks to detail
  1671. 1:23:44balance I can find the stationary
  1672. 1:23:46distribution and show that the system is
  1673. 1:23:49going to segregate
  1674. 1:23:50but what happens if I take different
  1675. 1:23:54choices for this transition rate
  1676. 1:23:58as I've said in physics it's something
  1677. 1:24:01that is Justified from first principle
  1678. 1:24:04but
  1679. 1:24:05in social sciences you know why on Earth
  1680. 1:24:08would people follow exactly that rule
  1681. 1:24:11uh and here is a little bit of an open
  1682. 1:24:13question is whether
  1683. 1:24:15the results that I've shown you today
  1684. 1:24:17are uh robust against different choices
  1685. 1:24:20of this individual uh hopping rate or if
  1686. 1:24:26this whole phenomenology is going to
  1687. 1:24:29completely disappear if I change uh
  1688. 1:24:32sufficiently this rule so for example I
  1689. 1:24:35could choose I don't know if I if I go
  1690. 1:24:38from this particular shape to the sun
  1691. 1:24:41function of Delta U
  1692. 1:24:45which is General
  1693. 1:24:49will this change completely the the
  1694. 1:24:51final results or will the final results
  1695. 1:24:54be you know qualitatively similar
  1696. 1:24:59are the results
  1697. 1:25:05robust
  1698. 1:25:10and in a sense this is a very general
  1699. 1:25:12question because the
  1700. 1:25:14if you lose detailed balance
  1701. 1:25:17then we're in the realm of uh
  1702. 1:25:19non-equilibrium statistical physics in a
  1703. 1:25:21sense where many dynamical systems don't
  1704. 1:25:24obey detailed balance
  1705. 1:25:26and there's no general theory for that
  1706. 1:25:28so uh phase transitions in some cases in
  1707. 1:25:33some cases they resist the existence of
  1708. 1:25:36uh of non-detailed balance effects in
  1709. 1:25:40other cases the the phenomenology is
  1710. 1:25:43completely different as soon as you
  1711. 1:25:45introduce a little bit of
  1712. 1:25:48the violation of detail balance so
  1713. 1:25:51because of that intuition it I I draw
  1714. 1:25:54your attention to the fact that in
  1715. 1:25:56social sciences
  1716. 1:25:57there's a you know there's the this
  1717. 1:26:00question of knowing how robust are the
  1718. 1:26:03results is very uh rarely posed because
  1719. 1:26:07it's difficult because we lack tools and
  1720. 1:26:10I think it's a it's a very interesting
  1721. 1:26:12question in general to know whether
  1722. 1:26:15these segregation effects for example
  1723. 1:26:17all these phase transitions they exist
  1724. 1:26:21beyond the realm of detailed balance and
  1725. 1:26:23Bolston Gibbs or if they're very fragile
  1726. 1:26:27to any change of the retail balance
  1727. 1:26:30condition
  1728. 1:26:31okay so that's uh what I wanted to say
  1729. 1:26:35on the shedding model
  1730. 1:26:44and what I like to finish on is the
  1731. 1:26:48oh my
  1732. 1:26:51you don't see any more the outline of
  1733. 1:26:53the lecture but it doesn't matter
  1734. 1:26:56so I want to finish on a few words on
  1735. 1:26:59spin glasses
  1736. 1:27:06so the spin glass problem is uh
  1737. 1:27:10is the problem of spins
  1738. 1:27:13which is given by an energy which I call
  1739. 1:27:17H
  1740. 1:27:19of the configurations s i
  1741. 1:27:23which is simply the term
  1742. 1:27:28of interaction between bins
  1743. 1:27:31and for the for now I'm completely
  1744. 1:27:33neglecting all the uh individual terms
  1745. 1:27:37I'm putting to zero h i n capital h
  1746. 1:27:45so there's only interaction and the jijs
  1747. 1:27:49are random
  1748. 1:27:52for example gaussian
  1749. 1:27:57variables
  1750. 1:28:01of zero mean
  1751. 1:28:06okay
  1752. 1:28:08so what does it mean to have jij's
  1753. 1:28:11random of Euro mean it means that for
  1754. 1:28:14some pairs of spins
  1755. 1:28:17the J is positive and therefore spins
  1756. 1:28:21want to be aligned either up
  1757. 1:28:24or or down
  1758. 1:28:29but if jij is negative then spins want
  1759. 1:28:33to be anti-aligned
  1760. 1:28:38okay
  1761. 1:28:39and so there's a mixture of that
  1762. 1:28:42some spins want to be aligned with one
  1763. 1:28:44another some spins want to be
  1764. 1:28:46anti-aligned to one another
  1765. 1:28:48and this causes a headache in a sense so
  1766. 1:28:51it's called frustration
  1767. 1:28:53and so the typical little graph that you
  1768. 1:28:56can draw is a triangle where you have
  1769. 1:28:58for example J negative here J negative
  1770. 1:29:01here uh and
  1771. 1:29:04J positive here and J positive here
  1772. 1:29:07so if this spin is up
  1773. 1:29:10this pin wants to be up but this one
  1774. 1:29:13doesn't know what to do okay
  1775. 1:29:18so you have a problem with many
  1776. 1:29:20constraints and these constraints are
  1777. 1:29:23contradictory to one another so this is
  1778. 1:29:25the archetype example of an optimization
  1779. 1:29:28problem with constraints that are not
  1780. 1:29:31compatible with one another okay
  1781. 1:29:34and it leads to a very very interesting
  1782. 1:29:37set of uh a phenomenon that I'm going to
  1783. 1:29:40summarize in a few moments but uh you
  1784. 1:29:44know you you can think of this problem
  1785. 1:29:46in a in a social context
  1786. 1:29:49in the following way I mean it's of
  1787. 1:29:51course a toy example but I think it's a
  1788. 1:29:54very visual one
  1789. 1:29:55so imagine that you have a a class of 50
  1790. 1:29:59students and you want to organize a boat
  1791. 1:30:02trip
  1792. 1:30:03but you have only boats with 25 capacity
  1793. 1:30:06so you you want to split your
  1794. 1:30:09your your class in two groups
  1795. 1:30:15so groups that are going to a group that
  1796. 1:30:17is going to go to
  1797. 1:30:18both a and a group that's going to go to
  1798. 1:30:21both d
  1799. 1:30:23and you make a little survey beforehand
  1800. 1:30:26and you try to know who likes whom in
  1801. 1:30:28your class
  1802. 1:30:29okay and so you have 50 individuals and
  1803. 1:30:33you're going to map out all the 50 times
  1804. 1:30:3749 divided by two if you assume that
  1805. 1:30:41liking is a symmetric
  1806. 1:30:44uh condition which is unfortunately not
  1807. 1:30:46always the case but anyway so if uh if
  1808. 1:30:50gij is are symmetric then um
  1809. 1:30:53you're looking for 50 times 49 over 2 uh
  1810. 1:30:58information about your class
  1811. 1:31:00pieces of information and if jij is
  1812. 1:31:04positive it means that
  1813. 1:31:06the two people in question like each
  1814. 1:31:08other and would prefer being on the same
  1815. 1:31:10boat and if jij is negative
  1816. 1:31:15then they would like to be on separate
  1817. 1:31:17boats okay
  1818. 1:31:19uh well the question of
  1819. 1:31:23optimizing this uh function over the SI
  1820. 1:31:28so you you need to find which sis are
  1821. 1:31:32plus and which S5 are minus which will
  1822. 1:31:34correspond to which people you put on
  1823. 1:31:36the a boat and which people you put on
  1824. 1:31:38the E-boat in such a way that the global
  1825. 1:31:43satisfaction is maximized
  1826. 1:31:45so that what it would correspond in
  1827. 1:31:48terms of uh of this city example and the
  1828. 1:31:52problem is that that although the the
  1829. 1:31:55problem although the equation seems
  1830. 1:31:58incredibly simple
  1831. 1:32:00finding the ground state finding the
  1832. 1:32:02optimal configuration for a given choice
  1833. 1:32:05of gij is extremely difficult
  1834. 1:32:07algorithmically
  1835. 1:32:09the the algorithms allowing you to find
  1836. 1:32:14the true ground say the true optimal
  1837. 1:32:16configuration
  1838. 1:32:17uh are exponentially long in N so as you
  1839. 1:32:22grow the system size uh the time you
  1840. 1:32:25need to spend to find the real ground
  1841. 1:32:27state is going to grow exponentially
  1842. 1:32:29with the size of the system we don't
  1843. 1:32:30know
  1844. 1:32:31yet maybe
  1845. 1:32:33one day we will
  1846. 1:32:36show that there's very little hope of
  1847. 1:32:38that that this problem is polynomial in
  1848. 1:32:42the number of bins but everybody
  1849. 1:32:44believes that it's actually not and that
  1850. 1:32:47even the best algorithms won't be able
  1851. 1:32:49to
  1852. 1:32:50find a solution in a time that
  1853. 1:32:53polynomial in the in the system side so
  1854. 1:32:56it's an incredibly complicated problem
  1855. 1:32:58to solve
  1856. 1:32:59but at the same time there are many
  1857. 1:33:01configurations that are quasi-optimal so
  1858. 1:33:04if you're really insisting on finding
  1859. 1:33:06the optimal configuration is very
  1860. 1:33:08difficult but on the other hand there's
  1861. 1:33:11a lot of configurations that are locally
  1862. 1:33:13optimal so what does it mean that it's
  1863. 1:33:16locally optimal it means that
  1864. 1:33:20locally optimal
  1865. 1:33:24configuration
  1866. 1:33:27or one spin flip stable it means that
  1867. 1:33:31each spin s i
  1868. 1:33:33is in the direction of the local field
  1869. 1:33:37so you remember
  1870. 1:33:41the random clizing model where there was
  1871. 1:33:44on top of that
  1872. 1:33:45an idiosyncratic scale and external
  1873. 1:33:47field but
  1874. 1:33:49here I'm I'm having a simplified view on
  1875. 1:33:52that where there's only the interaction
  1876. 1:33:54term and if
  1877. 1:33:56everybody every spin is in such a
  1878. 1:34:00configuration it means that you know I
  1879. 1:34:02cannot improve that if I flip SI it's
  1880. 1:34:06going to be worth so nobody wants to
  1881. 1:34:08change individually of course there
  1882. 1:34:10might be the collective move improving
  1883. 1:34:14uh uh the energy or improving the
  1884. 1:34:17utility of everybody but individually
  1885. 1:34:20people cannot do that people are locally
  1886. 1:34:22happy if you want
  1887. 1:34:25so you can look at the number of
  1888. 1:34:27solutions of this problem
  1889. 1:34:29and what you find is that the number of
  1890. 1:34:31solutions the number of configurations
  1891. 1:34:33touched that this is true
  1892. 1:34:35is
  1893. 1:34:36is exponentially large in n
  1894. 1:34:39so the number of configurations in a
  1895. 1:34:41spin problem is of course 2 to the N
  1896. 1:34:44okay
  1897. 1:34:46and the number of configurations that
  1898. 1:34:48satisfy such a constraint when J's are
  1899. 1:34:52random gaussian variables of zero mean
  1900. 1:34:55is
  1901. 1:34:56exponential of 0.2 times n
  1902. 1:35:01so of course 2 to the N is much greater
  1903. 1:35:04than exponential of 0.2 times n
  1904. 1:35:08because log 2 is 0.7 and not uh 0.2 but
  1905. 1:35:14um but you see that you still have an
  1906. 1:35:16enormous amount of possible choices
  1907. 1:35:19such that this is uh satisfied so
  1908. 1:35:24there's a lot of metastable states in
  1909. 1:35:26the system a lot of configurations that
  1910. 1:35:28are locally stable and a lot means
  1911. 1:35:30really a lot because you have a
  1912. 1:35:33combinatorial type of explosion of the
  1913. 1:35:36number of solutions
  1914. 1:35:39so it's a it's an interesting problem
  1915. 1:35:43where
  1916. 1:35:45although the the true solution is is
  1917. 1:35:48hard to find there's a lot of
  1918. 1:35:51secondary Minima if you want or
  1919. 1:35:53secondary Maxima if you want to think of
  1920. 1:35:56it in terms of utility
  1921. 1:35:58secondary Minima in terms of energy
  1922. 1:36:01technology
  1923. 1:36:02Maxima in terms of utility
  1924. 1:36:07and so let's look a little bit at
  1925. 1:36:10graphically at what happens
  1926. 1:36:15so it's traditional to draw the graph
  1927. 1:36:18that I'm going to draw although it
  1928. 1:36:21doesn't make sense really because
  1929. 1:36:24the configurations P space that spins is
  1930. 1:36:28uh is not a one-dimensional space at all
  1931. 1:36:30you see that you know for example if I
  1932. 1:36:34want to look at the configuration of
  1933. 1:36:36n equal to spins it's a
  1934. 1:36:39it's a square
  1935. 1:36:41up up
  1936. 1:36:43down
  1937. 1:36:45and down down
  1938. 1:36:47up
  1939. 1:36:49so this is the configuration space
  1940. 1:36:53for n equal to
  1941. 1:36:55and for n equals three it's the it's a
  1942. 1:36:58cube and if you go to higher Dimension
  1943. 1:37:00it's the hypercube of Dimension n
  1944. 1:37:02uh so I'm going to you know plot
  1945. 1:37:06this
  1946. 1:37:08space which is you know logically
  1947. 1:37:11completely different from a line I'm
  1948. 1:37:13still going to draw it as a line because
  1949. 1:37:15we can't do anything
  1950. 1:37:17else on the board but you know be
  1951. 1:37:19careful that this is very misleading by
  1952. 1:37:21many accounts anyway so it's a
  1953. 1:37:23traditional way to make the point so if
  1954. 1:37:25I plot H as a function of configuration
  1955. 1:37:27what you find for the spin glass problem
  1956. 1:37:30is an extremely rough and complex
  1957. 1:37:32landscape
  1958. 1:37:35let me try to do it right
  1959. 1:37:39so there's a lot of it's very rough so
  1960. 1:37:41as soon as you change the configuration
  1961. 1:37:42a little bit you change the energy in a
  1962. 1:37:46kind of random way
  1963. 1:37:47but also if you look at so here I'm
  1964. 1:37:50speaking in terms of physics where I'm
  1965. 1:37:53looking at the low energy State and you
  1966. 1:37:55should flip this up down if you want to
  1967. 1:37:58think of it in terms of utility but you
  1968. 1:38:01see that on my graph I guess that this
  1969. 1:38:04is the absolute minimum
  1970. 1:38:07okay
  1971. 1:38:08so this is the ground state I should
  1972. 1:38:10choose if I'm a rational person
  1973. 1:38:14but
  1974. 1:38:15or if you want at zero temperature this
  1975. 1:38:17is where the system should be because
  1976. 1:38:19that zero temperature it should be in
  1977. 1:38:21the absolute ground state but what you
  1978. 1:38:22see is that very close to the ground
  1979. 1:38:24state but very far very close in energy
  1980. 1:38:28but very far in configuration space
  1981. 1:38:30there are other
  1982. 1:38:32uh candidate
  1983. 1:38:34that are nearly as good
  1984. 1:38:36but they are very different in terms of
  1985. 1:38:38the configuration of spin
  1986. 1:38:41and so this is the kind of landscape
  1987. 1:38:44that you need to think about to
  1988. 1:38:46understand in this in the context of
  1989. 1:38:48physics what's going to happen
  1990. 1:38:50dynamically what's going to happen
  1991. 1:38:52dynamically is that the system is never
  1992. 1:38:54going to reach equilibrium is going to
  1993. 1:38:56get stuck in in valleys that are not the
  1994. 1:39:00optimal values but that are you know
  1995. 1:39:03good enough and the time it needs to
  1996. 1:39:06reach the true Crown state is going to
  1997. 1:39:08grow uh like the exponential of the size
  1998. 1:39:11of the system for such a problem
  1999. 1:39:14so in physics it's called you know aging
  2000. 1:39:18and out of the equilibrium Dynamics but
  2001. 1:39:20in terms of uh what I warned you before
  2002. 1:39:23in terms of optimization in terms of
  2003. 1:39:25finding the optimal solution uh using
  2004. 1:39:28Monte Carlo for example it means that
  2005. 1:39:31the algorithm is going to never contact
  2006. 1:39:34uh actually
  2007. 1:39:36but on the other hand it might find
  2008. 1:39:38solutions that are good enough
  2009. 1:39:40okay it might find solutions that are
  2010. 1:39:43not the true best one but are close in
  2011. 1:39:47terms of energy or utility to the to the
  2012. 1:39:50best one so they are good enough
  2013. 1:39:52Solutions
  2014. 1:39:53uh satisfying Solutions
  2015. 1:40:01and the problem is that you don't really
  2016. 1:40:03know which one you're going to find
  2017. 1:40:04because depending on your algorithms
  2018. 1:40:07maybe you'll end up here maybe you'll
  2019. 1:40:08never there maybe you'll end up there
  2020. 1:40:10and so what is interesting from a
  2021. 1:40:13philosophical point of view uh you know
  2022. 1:40:16thinking that agents are rational and
  2023. 1:40:17try to optimize their utility function
  2024. 1:40:19is that if you're confronted with such a
  2025. 1:40:22complicated problem to solve then you
  2026. 1:40:25don't know what others are going to do
  2027. 1:40:28because some of them are going to choose
  2028. 1:40:30one solution which is good enough and
  2029. 1:40:33some others are going to choose another
  2030. 1:40:34solution so you cannot use rationality
  2031. 1:40:36as a way to infer what other people are
  2032. 1:40:39doing so I think that in a philosophical
  2033. 1:40:42sense it's a very important uh model
  2034. 1:40:45that shows that the reality can be
  2035. 1:40:48extremely compact something else related
  2036. 1:40:51to this
  2037. 1:40:52is that this is uh the the landscape for
  2038. 1:40:57a given set of gij
  2039. 1:41:00but maybe you know maybe I don't measure
  2040. 1:41:04the jic correctly maybe there's a little
  2041. 1:41:06bit of noise in the gijs or maybe gijs
  2042. 1:41:08are evolving with time
  2043. 1:41:10so maybe today jij is equal to this and
  2044. 1:41:15tomorrow a gij will be changed by some
  2045. 1:41:18small
  2046. 1:41:21uh
  2047. 1:41:22perturbation Delta jij
  2048. 1:41:25or maybe you know I've not measured the
  2049. 1:41:28jic correctly so there's a little bit of
  2050. 1:41:30error and what happens is that because
  2051. 1:41:33of this very small perturbation you can
  2052. 1:41:37have some of the
  2053. 1:41:38secondary Minima that become
  2054. 1:41:43the new Minima
  2055. 1:41:46okay so when you change Delta i j a
  2056. 1:41:48little bit you can have
  2057. 1:41:50a change of what you call the ground
  2058. 1:41:53state in a chaotic manner so
  2059. 1:41:57when the system size goes to Infinity
  2060. 1:41:59the Delta gij you need to change the
  2061. 1:42:03order of the different configuration is
  2062. 1:42:06going to zero so this this is called
  2063. 1:42:08chaos and uh and I've alluded to that
  2064. 1:42:11earlier in my lecture so it's a kind of
  2065. 1:42:14again of a fragile optimization
  2066. 1:42:21in the sense that
  2067. 1:42:24if you change a little bit the value of
  2068. 1:42:26the parameters
  2069. 1:42:27you can completely change the structure
  2070. 1:42:30of the solution so again this is a very
  2071. 1:42:32I think this is a very important uh
  2072. 1:42:34Paradigm to understand that optimization
  2073. 1:42:37alone often is misleading because it's
  2074. 1:42:40the it's it's it's useless in a way to
  2075. 1:42:44understand what people are going to do
  2076. 1:42:45because depending on what they actually
  2077. 1:42:48assume about the gij they might end up
  2078. 1:42:51even if they are able to solve the
  2079. 1:42:53problem in the the they might end up in
  2080. 1:42:56very different considerations
  2081. 1:42:58and finally not only you can have these
  2082. 1:43:01small changes but because of small
  2083. 1:43:04perturbations in the gigs some of the
  2084. 1:43:06Minima that existed before May
  2085. 1:43:09completely disappear so for example
  2086. 1:43:11because of a Delta IJ that's very small
  2087. 1:43:14this minimum here can suddenly
  2088. 1:43:18you know be bypassed completely and
  2089. 1:43:21disappear
  2090. 1:43:22and so you know you might be in a
  2091. 1:43:24situation which is locally stable
  2092. 1:43:26for some gigs and because you've changed
  2093. 1:43:29the Delta gig a little bit you're not
  2094. 1:43:31locally stable anymore
  2095. 1:43:33so uh this is again often called chaos
  2096. 1:43:40in a sense a little different from chaos
  2097. 1:43:43in dynamical systems it's chaos with
  2098. 1:43:45respect to the uh to the data you give
  2099. 1:43:48to the optimization problem
  2100. 1:43:56right so that's
  2101. 1:43:59of course the I mean spin glass
  2102. 1:44:01literature has exploded in the last 50
  2103. 1:44:04years in the in physics and there's
  2104. 1:44:07there's a lot of ramifications of this
  2105. 1:44:10the I think very beautiful example that
  2106. 1:44:13I've only touched upon very quickly in
  2107. 1:44:16the last 15 minutes but I I think it's
  2108. 1:44:19an important uh item to add in these
  2109. 1:44:23lectures for you to understand the well
  2110. 1:44:26where I think we're going in terms of uh
  2111. 1:44:30transposing problems from physics into
  2112. 1:44:33uh
  2113. 1:44:35economics and sociology
  2114. 1:44:37and so on that note I'm ending the set
  2115. 1:44:40of lectures of course there's a lot I
  2116. 1:44:42would have liked to talk about and uh
  2117. 1:44:44for some reason I haven't had time so I
  2118. 1:44:46don't know if it's because uh you're not
  2119. 1:44:49in the room so I'm I was a little slower
  2120. 1:44:52than usual I don't know but anyway
  2121. 1:44:55um this is what I roughly what I want to
  2122. 1:44:57speak about to you this year
  2123. 1:45:00uh I hope that the exam will be
  2124. 1:45:03interesting and that we can hold it in
  2125. 1:45:07normal conditions and I'm and I'm
  2126. 1:45:10reiterating my proposal to speak with
  2127. 1:45:13any of you next week Wednesday I'll send
  2128. 1:45:16a link I won't be in the room but I'll
  2129. 1:45:19send the link and if you have any
  2130. 1:45:21anything you want to chat about then
  2131. 1:45:24feel free to connect
  2132. 1:45:26that's it folks
  2133. 1:45:28any question now I don't know
  2134. 1:45:31is the
  2135. 1:45:35hey Valentina is here
  2136. 1:45:38I mean Valentina is on the
  2137. 1:45:41not physically in the room but she's
  2138. 1:45:43present
  2139. 1:45:46so in 15 minutes you'll have Valentina
  2140. 1:45:48but until then any comment question
  2141. 1:45:52so she's here
  2142. 1:45:59no
  2143. 1:46:07in the room questions
  2144. 1:46:13I'm surprised I mean that's one of the
  2145. 1:46:15big changes is that they are really
  2146. 1:46:17really very few questions I don't know
  2147. 1:46:20what you're
  2148. 1:46:21taking out anyway
  2149. 1:46:27okay
  2150. 1:46:32well I'll end the recording session and
  2151. 1:46:35wish you good luck for the exam
  2152. 1:46:38this conference will now be recorded
  2153. 1:46:42Okay so
  2154. 1:46:45welcome back to everybody to the last
  2155. 1:46:47day
  2156. 1:46:48So the plan for today is to discuss a
  2157. 1:46:52little bit uh the model which is given
  2158. 1:46:55in the paper that I I think was in the
  2159. 1:46:58uh yes folder I hope or in any case I
  2160. 1:47:01just sent it to you via email
  2161. 1:47:05so this is a paper of uh 2015 and it is
  2162. 1:47:10a little bit an excuse for us to discuss
  2163. 1:47:12about uh
  2164. 1:47:14say checking the stability of solutions
  2165. 1:47:18of focus blank equations
  2166. 1:47:20so let me first tell you what is the
  2167. 1:47:22idea of the paper that included first
  2168. 1:47:28and then I will tell you what we are
  2169. 1:47:31actually going to discuss
  2170. 1:47:32so the idea is to write down a simple
  2171. 1:47:36model of interactive firms so we will
  2172. 1:47:38just think at the model in terms of
  2173. 1:47:41firms indeed but if you look at the
  2174. 1:47:43paper towards the end and there is a
  2175. 1:47:45discussion on how to interpret the model
  2176. 1:47:47uh for example then epidemiological
  2177. 1:47:51models or or as a model of interacting
  2178. 1:47:54banks in a financial market and so on so
  2179. 1:47:58there are plenty of possible
  2180. 1:47:59interpretation
  2181. 1:48:00and the interesting thing is that there
  2182. 1:48:03are regimes in which this the behavior
  2183. 1:48:07of the system shows persistent
  2184. 1:48:09oscillations which are called We Will
  2185. 1:48:12Call some synchronization phenomena and
  2186. 1:48:16now this is interesting because uh
  2187. 1:48:18somehow it's telling you that you have a
  2188. 1:48:20model where you go from having a moment
  2189. 1:48:23or period of prosperity if you think of
  2190. 1:48:26this in terms of of an economy where
  2191. 1:48:29everything seems to to go well and then
  2192. 1:48:32suddenly you have
  2193. 1:48:34the negative oscillation you have abrupt
  2194. 1:48:37crisis in your economy and this goes on
  2195. 1:48:40in a cyclical way and this is
  2196. 1:48:43interesting because this crisis again
  2197. 1:48:45happen without any external shocks which
  2198. 1:48:48perturbs your economy but are really
  2199. 1:48:51built in in the choice of parameters of
  2200. 1:48:53your model
  2201. 1:48:55so what we're going to do today is not
  2202. 1:48:57really uh go into detail of this phase
  2203. 1:49:00uh where we where we have oscillations
  2204. 1:49:02but rather we are going to
  2205. 1:49:04estimate and compute what is the
  2206. 1:49:07boundary of stability of the phase
  2207. 1:49:09without uh oscillation so what we want
  2208. 1:49:11to do uh today so these are
  2209. 1:49:16introductory comments if you want
  2210. 1:49:19and this starts so if you have the paper
  2211. 1:49:23with you if you look at people two
  2212. 1:49:26just so I have an idea
  2213. 1:49:27what the paper is about so figure two
  2214. 1:49:30gives you the behavior in time of a
  2215. 1:49:33quantity that I will introduce in a
  2216. 1:49:35minute that is essentially
  2217. 1:49:37the fraction of firms in your model that
  2218. 1:49:41are uh
  2219. 1:49:43that go bankrupt so which have financial
  2220. 1:49:46problems if you want and you see from
  2221. 1:49:49that figure that there are two different
  2222. 1:49:50regimes of parameters so in one regime
  2223. 1:49:52of parameter you find that the behavior
  2224. 1:49:54of this dynamical quantity uh looks like
  2225. 1:49:57this so you have some initial
  2226. 1:50:00oscillation a transient but then you
  2227. 1:50:01converge to some positional value for
  2228. 1:50:04this fraction and this happens for the
  2229. 1:50:07parameter five that I will introduce in
  2230. 1:50:08a minute which is all
  2231. 1:50:11efficiently small whereas you have
  2232. 1:50:14another phase if you want where this
  2233. 1:50:16type of oscillations appears so if you
  2234. 1:50:18look at this plot at that plot so I
  2235. 1:50:20don't change colors because I know that
  2236. 1:50:23is very hard to see them on the screen
  2237. 1:50:26but somehow in the second phase you see
  2238. 1:50:29that you have this
  2239. 1:50:30Collective Global synchronized
  2240. 1:50:33oscillations in the number of firms that
  2241. 1:50:37are bankrupt and these items
  2242. 1:50:42is large
  2243. 1:50:44and so the idea is that we are not going
  2244. 1:50:46as I said to compute explicitly the
  2245. 1:50:49solution so the time behavior of this
  2246. 1:50:51fieste but we want uh somehow to
  2247. 1:50:54estimate
  2248. 1:50:55right
  2249. 1:50:59estimate
  2250. 1:51:01when
  2251. 1:51:04the
  2252. 1:51:05express stationary solution
  2253. 1:51:09which is not postulating
  2254. 1:51:13becomes unstable
  2255. 1:51:23and by when I mean uh of course for
  2256. 1:51:25which values of parameter uh this first
  2257. 1:51:28regime becomes dynamically unstable
  2258. 1:51:32so what does it mean technically well
  2259. 1:51:34technical it means that we are going to
  2260. 1:51:36try to solve for the stationary state of
  2261. 1:51:39a focal blank equation which describes
  2262. 1:51:42our model
  2263. 1:51:43and then so this would come into one
  2264. 1:51:47and then we are going to look at the
  2265. 1:51:50stability of this focal Planck equation
  2266. 1:51:53so let me add a comment on this
  2267. 1:51:58so what does it mean to look at the
  2268. 1:52:00stability well let's
  2269. 1:52:03um think about a very simple example
  2270. 1:52:06that we discussed also last time so
  2271. 1:52:08let's think about
  2272. 1:52:09the case in which for instance we are
  2273. 1:52:11looking at some Optima of some function
  2274. 1:52:16like the one that I'm drawing here
  2275. 1:52:19and you can have different points which
  2276. 1:52:22are stationary points one which is for
  2277. 1:52:23instance a local minimum and one which
  2278. 1:52:25is a local maximum and they are
  2279. 1:52:27distinguished by their properties of
  2280. 1:52:29stability so of course the local minimum
  2281. 1:52:32is stable and the local maximum is not
  2282. 1:52:33stable
  2283. 1:52:35and one way to check this that we are
  2284. 1:52:37going to generalize the function today
  2285. 1:52:39is just to uh to do the following so you
  2286. 1:52:43sit into your point which is a solution
  2287. 1:52:45of your equation in this case the
  2288. 1:52:47equation is the potential the equation
  2289. 1:52:50will just be
  2290. 1:52:51that we are asking the derivative of the
  2291. 1:52:55potential uh is equal to zero so you
  2292. 1:52:58have different solutions and to check
  2293. 1:52:59the stability what you can do is to do a
  2294. 1:53:02little bit
  2295. 1:53:03of distribution around your uh your
  2296. 1:53:05stable point and to check whether doing
  2297. 1:53:08the preservation and then letting the
  2298. 1:53:10system evolve the system goes back to
  2299. 1:53:12your original solution or it goes
  2300. 1:53:15somewhere else of course in this case
  2301. 1:53:18with with gradient descent like dynamics
  2302. 1:53:21that we discussed last time if we go
  2303. 1:53:23back so you preserve a little bit under
  2304. 1:53:25the system relaxes back to the local
  2305. 1:53:28minimum so this is
  2306. 1:53:30table
  2307. 1:53:32whereas if you see them here as you
  2308. 1:53:35easily realize as soon as you do
  2309. 1:53:36preservation your system flows somewhere
  2310. 1:53:39else and therefore this point will be
  2311. 1:53:44so the idea is to use the same type of
  2312. 1:53:47reasoning today but for full functions
  2313. 1:53:50which are the solutions to uh
  2314. 1:53:54to our Focus line equation as I said
  2315. 1:53:57and now perhaps let's make a third
  2316. 1:54:00comment and then we
  2317. 1:54:02start
  2318. 1:54:03and the third comment is about
  2319. 1:54:06[Music]
  2320. 1:54:08current and stationary States so
  2321. 1:54:16and and this introduces a little bit uh
  2322. 1:54:19the problem of today so the difference
  2323. 1:54:21with respect to the soccer Planet
  2324. 1:54:23equation that we are discussing today
  2325. 1:54:24and the one that we discussed in the
  2326. 1:54:27last day is that today we are going to
  2327. 1:54:30have a system with uh
  2328. 1:54:32what people call some sources or some
  2329. 1:54:36things
  2330. 1:54:38they
  2331. 1:54:42we are having a soccer blank equation
  2332. 1:54:49we've
  2333. 1:54:51accuracies
  2334. 1:54:53and things
  2335. 1:54:55because this will become clear and once
  2336. 1:54:58we write it down
  2337. 1:54:59but I just wanted to anticipate it
  2338. 1:55:01because I want to comment on a
  2339. 1:55:04difference with respect to what we have
  2340. 1:55:06seen last time
  2341. 1:55:07so last time
  2342. 1:55:11and in the previous study we were always
  2343. 1:55:14looking at soccer blank equations which
  2344. 1:55:16we could write in the in the form of a
  2345. 1:55:18continuity equation so we had expression
  2346. 1:55:21of the following form so let's think
  2347. 1:55:24about one dimension
  2348. 1:55:25we have the derivative of our
  2349. 1:55:27probability was
  2350. 1:55:29minus the derivative with respect to
  2351. 1:55:33the position let's say of a current
  2352. 1:55:39and the current was depending itself on
  2353. 1:55:42the probability and on its derivative
  2354. 1:55:43over time
  2355. 1:55:45so this is this is what is usually
  2356. 1:55:47called the continuity
  2357. 1:55:51equation
  2358. 1:55:55and then when we looked at the
  2359. 1:55:57stationary points uh the session and
  2360. 1:56:00state sorry what we were doing is well
  2361. 1:56:02if the stationary state
  2362. 1:56:04stationary it means that the derivative
  2363. 1:56:07over time has to be equal to zero and
  2364. 1:56:10the derivative over time being equal to
  2365. 1:56:12zero because of this relation was the
  2366. 1:56:16same as asking the current
  2367. 1:56:19is equal to constant
  2368. 1:56:24and we always assume that we could
  2369. 1:56:27choose this constant to be
  2370. 1:56:30to be equal to zero
  2371. 1:56:32and there are arguments so in some cases
  2372. 1:56:35there are arguments to to make this
  2373. 1:56:37choice for instance if you have a focal
  2374. 1:56:40plant equation which is defined uh in
  2375. 1:56:43the space which goes from minus infinity
  2376. 1:56:45to infinity and you have currents which
  2377. 1:56:48are usually functions of the probability
  2378. 1:56:51it says
  2379. 1:56:53and of the derivative
  2380. 1:56:55then you can say well in order for the
  2381. 1:56:57probability to be well normalized
  2382. 1:57:00if the probability itself and the
  2383. 1:57:02derivatives have to go to zero to
  2384. 1:57:04Infinity but if they are constant and
  2385. 1:57:06they are 0 to Infinity then they have to
  2386. 1:57:07be equal to 0 everywhere
  2387. 1:57:10which is true if you have an unbounded
  2388. 1:57:12interval if you have a boundary interval
  2389. 1:57:15like the one that we discussed in the
  2390. 1:57:18exercise about the model or the
  2391. 1:57:22Kirman and more than last time you can
  2392. 1:57:25still argue in a similar way so you just
  2393. 1:57:28say okay I expect that there is no
  2394. 1:57:30current in my stationary solution and
  2395. 1:57:33therefore I set this to zero and setting
  2396. 1:57:36these two zero gives me then an equation
  2397. 1:57:37that I can solve very easily with with
  2398. 1:57:41the separation of variables that we saw
  2399. 1:57:44now today this is going to be a little
  2400. 1:57:46bit different because precisely because
  2401. 1:57:48we will have this sources and change
  2402. 1:57:51so this means that our equation will be
  2403. 1:57:54defined in some intervals of X and we
  2404. 1:57:57will have special points
  2405. 1:57:59such that whenever
  2406. 1:58:02our variable reaches this point it
  2407. 1:58:05either dies in some way so it disappears
  2408. 1:58:09from the model and this will be the sink
  2409. 1:58:11or it is injected back at that
  2410. 1:58:14particular point in our model and this
  2411. 1:58:17will be assert so it is like having an
  2412. 1:58:20open system in which you have some
  2413. 1:58:22special points where you start
  2414. 1:58:24inserting a new probability for your
  2415. 1:58:27variable and points where you
  2416. 1:58:30say eject the probability from your
  2417. 1:58:33model and therefore you can easily
  2418. 1:58:35understand that if I start increasing
  2419. 1:58:38probability here and taking it back in
  2420. 1:58:41here there might be even in the
  2421. 1:58:43stationary State some constant parents
  2422. 1:58:45in my system which goes current of
  2423. 1:58:48probability which goes in this direction
  2424. 1:58:51and therefore we should not put this J
  2425. 1:58:54equal to zero but we will
  2426. 1:58:56expect it to be gone
  2427. 1:58:58and this is what is going to happen in
  2428. 1:59:00this in the example of today
  2429. 1:59:04okay so this was a little bit verbal but
  2430. 1:59:06maybe it becomes more clear
  2431. 1:59:09when doing the uh the exercise
  2432. 1:59:12so let me see
  2433. 1:59:17the direction
  2434. 1:59:25okay
  2435. 1:59:26it just it is
  2436. 1:59:36let's introduce the model and the
  2437. 1:59:39equation and then I think
  2438. 1:59:42all of this talking will be a little bit
  2439. 1:59:46more transparent
  2440. 1:59:58so the model looks like this you can
  2441. 2:00:01look at the paper if you want
  2442. 2:00:05a more detailed description but the idea
  2443. 2:00:07is as follows so you have n firms
  2444. 2:00:15it was um
  2445. 2:00:18from one to one
  2446. 2:00:21and you have a variable which describes
  2447. 2:00:23each of these firms which is the
  2448. 2:00:25so-called fragility
  2449. 2:00:32which you can think of as a measure of
  2450. 2:00:35how bad this sperm is doing so this is
  2451. 2:00:39the ratio between the dabs
  2452. 2:00:42that the sperm uh Escape
  2453. 2:00:49the bank or
  2454. 2:00:51whoever
  2455. 2:00:53gives blown to the firm I divided by the
  2456. 2:00:56total asset so this is the amount of
  2457. 2:00:59money if you want
  2458. 2:01:01of the Easter so of course the larger is
  2459. 2:01:05the dead so let's say if uh if you have
  2460. 2:01:08a lot of that then this variable
  2461. 2:01:10X will be negative and the more negative
  2462. 2:01:14is this variable the worse is
  2463. 2:01:17is the state of your firm
  2464. 2:01:21now this firm uh have a Dynamics so the
  2465. 2:01:24idea of the model is to assume that the
  2466. 2:01:26Dynamics is like around the wall so you
  2467. 2:01:28have
  2468. 2:01:29diffusion
  2469. 2:01:33this agility space of the firms with
  2470. 2:01:37some diffusion content B and then you
  2471. 2:01:40have also some brief terms the constant
  2472. 2:01:43velocity
  2473. 2:01:46which is given by B which are parameters
  2474. 2:01:51and then you have uh two special points
  2475. 2:01:55that based on what I said before can be
  2476. 2:01:58interpreted as a surf and as a sink so
  2477. 2:02:03the surf the sink will be
  2478. 2:02:08at
  2479. 2:02:09a value of x which we call let's say
  2480. 2:02:13minus Theta
  2481. 2:02:15and it is as follows so you have your X
  2482. 2:02:18variable
  2483. 2:02:20yes zero somewhere and then you put a
  2484. 2:02:23special at some particular point of your
  2485. 2:02:26choice is minus Theta
  2486. 2:02:29and you have all of these points which
  2487. 2:02:32are performing some diffusion in this
  2488. 2:02:34our x-axis and we say that whenever
  2489. 2:02:37the point
  2490. 2:02:39has adapt which becomes as large as
  2491. 2:02:43a negatives
  2492. 2:02:46these are now negatively smaller than uh
  2493. 2:02:49than my Theta so if you if you have a
  2494. 2:02:52firm which crosses this particular
  2495. 2:02:55threshold in here
  2496. 2:02:56then you say that the depth is too large
  2497. 2:02:59and therefore the firm goes bankrupt
  2498. 2:03:03threshold
  2499. 2:03:06for
  2500. 2:03:10bankrupt
  2501. 2:03:17so what this means is that healthy firms
  2502. 2:03:19we live in this part of your
  2503. 2:03:22configuration space
  2504. 2:03:25these are the firms which are active
  2505. 2:03:29and then as soon as you cross the
  2506. 2:03:32special your firm becomes uh say
  2507. 2:03:35inactive
  2508. 2:03:38so they hire for bankruptcy and
  2509. 2:03:41therefore they are in some sense no
  2510. 2:03:42longer uh they freeze they are no longer
  2511. 2:03:45into your model
  2512. 2:03:47so in terms of the soccer plan equation
  2513. 2:03:49this will be translated into the
  2514. 2:03:51presence of an absorbing boundary so
  2515. 2:03:54whenever you reach that point then the
  2516. 2:03:57corresponding probability has to go to
  2517. 2:03:58here we will see this so we have this
  2518. 2:04:01special value which is uh if you want
  2519. 2:04:03the sink
  2520. 2:04:04of our model and then we also have a
  2521. 2:04:07surf and the source
  2522. 2:04:11is
  2523. 2:04:13at x equal to zero
  2524. 2:04:16so what this means is that you have some
  2525. 2:04:18firms which to die or become inactive
  2526. 2:04:22but then you also decide that with a
  2527. 2:04:24given rate you can take one of these
  2528. 2:04:26terms and give some loan or give some
  2529. 2:04:29money to it and revive it so put it back
  2530. 2:04:32into the model and you do this by
  2531. 2:04:35putting it back at this particular value
  2532. 2:04:39of agility which is which is you know
  2533. 2:04:43so this means that with some frequencies
  2534. 2:04:45I can take one of the firms which are
  2535. 2:04:47that and I can arrange like them into my
  2536. 2:04:50uh
  2537. 2:04:51say Axis or regime of active firms
  2538. 2:04:54precisely F0
  2539. 2:04:57and so this will be the source
  2540. 2:04:59where some firms will appear with a
  2541. 2:05:02certain frequency
  2542. 2:05:04and then you have a next ingredient the
  2543. 2:05:07final one which is interactions
  2544. 2:05:14so these firms perform their run work
  2545. 2:05:17with a given list and with the diffusion
  2546. 2:05:20sometimes they die sometimes they are
  2547. 2:05:21they injected but they also have some
  2548. 2:05:24sort of interaction that takes the form
  2549. 2:05:26of feedback
  2550. 2:05:30which happens whenever one firm dies or
  2551. 2:05:34becomes inactive so the idea is that
  2552. 2:05:36when the firm becomes so bad that it
  2553. 2:05:40reaches the values minus Theta then what
  2554. 2:05:43happens is that the fact that this sperm
  2555. 2:05:45is failing influences negatively all of
  2556. 2:05:48the other sperms because you have a
  2557. 2:05:51depth that this firm had to pay and that
  2558. 2:05:53now it's unable to pay anymore because
  2559. 2:05:55it is sales that gets redistributed to
  2560. 2:05:58all of the other firms which are alive
  2561. 2:06:01so what this means
  2562. 2:06:03uh
  2563. 2:06:05maybe I should write it in words and
  2564. 2:06:07then we look at the formulas
  2565. 2:06:09so the for
  2566. 2:06:12uh
  2567. 2:06:15yeah
  2568. 2:06:18terms
  2569. 2:06:21the tail
  2570. 2:06:27that that's
  2571. 2:06:29which is of the order of theta is
  2572. 2:06:31redistributed
  2573. 2:06:40to
  2574. 2:06:42all of the others
  2575. 2:06:46uh
  2576. 2:06:48Optics first
  2577. 2:06:53and the way we model this is by
  2578. 2:06:55modifying the drift of those firms which
  2579. 2:06:58are active
  2580. 2:07:00towards let's say the negative axis
  2581. 2:07:02whenever one of those reaches this
  2582. 2:07:06actual value might be
  2583. 2:07:08so let's look at this with formulas
  2584. 2:07:10which I hope
  2585. 2:07:14it's perhaps the best thing to do
  2586. 2:07:17so all of these ingredients
  2587. 2:07:19that I mentioned enter into some
  2588. 2:07:22chocolate blank equation
  2589. 2:07:24that is written in the paper for this
  2590. 2:07:26model
  2591. 2:07:371.1
  2592. 2:07:41which is to justify the focal blank
  2593. 2:07:43equation that is given in the paper so
  2594. 2:07:45the focal blank equation looks like this
  2595. 2:07:46so now this is of course the probability
  2596. 2:07:49who have a firm which has a fragility X
  2597. 2:07:52at a given time t
  2598. 2:07:55which of course depends on time
  2599. 2:07:58so you have a drift term
  2600. 2:08:01that
  2601. 2:08:03depends on time itself that I call BLT
  2602. 2:08:10multiplied by the space derivative so if
  2603. 2:08:12you remember
  2604. 2:08:14uh well okay let me comment later
  2605. 2:08:18then you have the diffusion curve
  2606. 2:08:21recognized
  2607. 2:08:25and then you have to we have to model
  2608. 2:08:27this sort so the fact that we are
  2609. 2:08:30sometimes pre-injecting ferns at zero
  2610. 2:08:34and we model it in the following way so
  2611. 2:08:37first I forgot to tell you something so
  2612. 2:08:39from now on let me see
  2613. 2:08:43the x axis and then we find it
  2614. 2:08:492x minus beta so I shift it in such a
  2615. 2:08:52way
  2616. 2:08:54I shift everything forward in such a way
  2617. 2:08:57that now the threshold for bankruptcy
  2618. 2:08:59becomes zero and I have active firm in
  2619. 2:09:02the positive synapses
  2620. 2:09:05and so the injection which before was
  2621. 2:09:07Zero now that I shifted happens at the
  2622. 2:09:09point x which is equal to Beta
  2623. 2:09:13so curious if you are
  2624. 2:09:17at that particular point
  2625. 2:09:19of the Delta function s like
  2626. 2:09:22the poinsettia you reject your firms
  2627. 2:09:26with a given rate that is this parameter
  2628. 2:09:28five
  2629. 2:09:30and the rate is multiplied by
  2630. 2:09:33the fraction of firms
  2631. 2:09:36which are inactive
  2632. 2:09:39so which are in the negatives can I ask
  2633. 2:09:41this every given time T which I call 1
  2634. 2:09:43minus Phi of t
  2635. 2:09:45so what is Phi of t
  2636. 2:09:47I of T is the fraction of a live firm so
  2637. 2:09:51this would be the integral
  2638. 2:09:53in the position my Axis once I shifted
  2639. 2:09:55everything off
  2640. 2:09:58the elections
  2641. 2:10:01so this is a fractional
  2642. 2:10:06off
  2643. 2:10:09ER
  2644. 2:10:13which of course is not constant in the
  2645. 2:10:16model so they put a number of firms is
  2646. 2:10:18constant so if you if you want if you
  2647. 2:10:20expand this integration to the fully
  2648. 2:10:22interval and take into account also
  2649. 2:10:24those which are inactive
  2650. 2:10:26your probability is normalized one but
  2651. 2:10:28if you focus only on the sub interval
  2652. 2:10:31which corresponds
  2653. 2:10:33firms which are really participating to
  2654. 2:10:36the economy then you have a quantity
  2655. 2:10:37which increases
  2656. 2:10:41so this explains the
  2657. 2:10:44here which is another source
  2658. 2:10:50and then where is uh the interaction uh
  2659. 2:10:53hidden the interaction that I mentioned
  2660. 2:10:55well this is hidden in this drift
  2661. 2:10:58coefficient e of e which has a
  2662. 2:11:02particular form foreign
  2663. 2:11:07is equal to some constant drift that is
  2664. 2:11:10the B that I introduced before
  2665. 2:11:14and then you have an extra term which
  2666. 2:11:16accounts for this redistribution of the
  2667. 2:11:18debt uh whenever somebody dies
  2668. 2:11:22will become
  2669. 2:11:24bankrupt
  2670. 2:11:26which is of the following form so beta
  2671. 2:11:28here is uh you want another
  2672. 2:11:30phenomenological concept of the model it
  2673. 2:11:33is the strengths
  2674. 2:11:34of the interaction if you want
  2675. 2:11:37or of the feedback
  2676. 2:11:40of one firm
  2677. 2:11:44on all the others
  2678. 2:11:49which is telling you that of course in
  2679. 2:11:51an economy whenever one firm uh fails
  2680. 2:11:54this is not good for the others as well
  2681. 2:11:56maybe because they were depending on the
  2682. 2:11:58product of that firm and which they will
  2683. 2:12:01have available anymore or because they
  2684. 2:12:04they were exchanging with it and so on
  2685. 2:12:06and so forth so there is a negative
  2686. 2:12:07feedback between the different firms
  2687. 2:12:10with the strengths encoded in this
  2688. 2:12:12system
  2689. 2:12:14then you have Theta so this accounts for
  2690. 2:12:17how much depth is ready to be has to be
  2691. 2:12:20redistributed and between all of the
  2692. 2:12:22other firms
  2693. 2:12:23and then in here to uh to control this
  2694. 2:12:27feedback you have P times the derivative
  2695. 2:12:33space
  2696. 2:12:34your probability distribution
  2697. 2:12:36distribution evaluated
  2698. 2:12:38h0
  2699. 2:12:40so at the point where where the firms
  2700. 2:12:44are disappearing from from the economy
  2701. 2:12:48and why does this term has this form so
  2702. 2:12:52first of all what is this so the way you
  2703. 2:12:55can interpret this term in here is as a
  2704. 2:12:58flux so this is the flux
  2705. 2:13:02of
  2706. 2:13:05ability
  2707. 2:13:11or the flags of firms
  2708. 2:13:14okay
  2709. 2:13:18the speech
  2710. 2:13:26so uh what do I mean by your snaps while
  2711. 2:13:29a flax is telling you what is the
  2712. 2:13:31probability for unit time and for uh
  2713. 2:13:35unit of surface in this case uh if you
  2714. 2:13:39focus on a small interval
  2715. 2:13:41uh around
  2716. 2:13:43minus beta that now became zero because
  2717. 2:13:46we have
  2718. 2:13:47is with everything so this flux controls
  2719. 2:13:51uh if you want what is the current of
  2720. 2:13:54probability that crosses a little
  2721. 2:13:57interval of
  2722. 2:13:59size DX around the special Point here so
  2723. 2:14:02it is measuring
  2724. 2:14:04if you want how much firms are are
  2725. 2:14:07failing in a given unit of time
  2726. 2:14:11and well maybe if you
  2727. 2:14:15okay let me add the first comments
  2728. 2:14:19and then we explain this term a little
  2729. 2:14:21bit better
  2730. 2:14:22so for us the idea is I hope it's clear
  2731. 2:14:25so what happens is that if you have a
  2732. 2:14:28lot of firms which are uh which are
  2733. 2:14:32failing then you start getting a
  2734. 2:14:35velocity that is more and more negative
  2735. 2:14:38so all of the other firms start all
  2736. 2:14:41together to breathe themselves towards
  2737. 2:14:44the absorbing point because of this
  2738. 2:14:46feedback term
  2739. 2:14:48and what happens at the observing point
  2740. 2:14:50so this is the last thing that we need
  2741. 2:14:53for defining the model
  2742. 2:14:56well the observing Point as I just
  2743. 2:14:58mentioned is an absorbing point so which
  2744. 2:15:00means that the probability
  2745. 2:15:03any time at the point zero has to be set
  2746. 2:15:08to zero
  2747. 2:15:11and with all of these terms we have
  2748. 2:15:14somehow defined
  2749. 2:15:16models that we are going to okay
  2750. 2:15:20so this is often called an absorbing
  2751. 2:15:22boundary
  2752. 2:15:24in the focus which
  2753. 2:15:27so let me perhaps
  2754. 2:15:29make a little bit of a comment uh about
  2755. 2:15:33this flux
  2756. 2:15:34right
  2757. 2:15:45backwards
  2758. 2:16:01foreign
  2759. 2:16:07why can we interpret this as a slacks or
  2760. 2:16:10what is the idea
  2761. 2:16:12but the idea is a little bit as follows
  2762. 2:16:16so you have again your x-axis you have
  2763. 2:16:19this point
  2764. 2:16:20zero and here you have some
  2765. 2:16:24absorbing point so whatever goes beyond
  2766. 2:16:27this point uh
  2767. 2:16:30diminutive so it's no longer in your
  2768. 2:16:32border
  2769. 2:16:33you have this special Point uh Theta
  2770. 2:16:36where you start injecting firms so you
  2771. 2:16:38somehow expect that you will have an
  2772. 2:16:40access
  2773. 2:16:41of probability around this point because
  2774. 2:16:45that is where you put
  2775. 2:16:47your firms with a given rate
  2776. 2:16:51Phi so I'm now drawing what one can
  2777. 2:16:53expect for the shape of this probability
  2778. 2:16:56and then you will have something that
  2779. 2:16:58you impose
  2780. 2:16:59has to go to zero in here and then it
  2781. 2:17:03has to remain exactly equal to zero
  2782. 2:17:07for whatever value of x which is
  2783. 2:17:10negative because these are no longer in
  2784. 2:17:12your mother so you don't track them with
  2785. 2:17:15your Dynamics equation and then at
  2786. 2:17:17Infinity you should go down in such a
  2787. 2:17:19way that they are normalizable
  2788. 2:17:22but the way you go to zero here is with
  2789. 2:17:24the derivative which is uh which is
  2790. 2:17:26non-finite and and somehow this gives
  2791. 2:17:29you what is the probability flux to go
  2792. 2:17:32to zero so you will have a current of
  2793. 2:17:34probability that flows uh towards this
  2794. 2:17:37point
  2795. 2:17:38and the way you can make sense uh of of
  2796. 2:17:42this expression here I think it follows
  2797. 2:17:45so you look at the focal flank equation
  2798. 2:17:47you should describe your model
  2799. 2:17:49and then you try to integrate this in a
  2800. 2:17:52small interval uh DX which is around
  2801. 2:17:55your special point
  2802. 2:17:57let me take the left hand side
  2803. 2:18:01and then we integrate
  2804. 2:18:03this derivative in here with respect to
  2805. 2:18:06X which goes from
  2806. 2:18:08Epsilon
  2807. 2:18:11so you don't have to write this noun
  2808. 2:18:13it's just to
  2809. 2:18:14try to motivate
  2810. 2:18:16this term here
  2811. 2:18:19so if I do this I take the derivative
  2812. 2:18:20over time outside and what do I get well
  2813. 2:18:23I get the derivative
  2814. 2:18:26over time of the probability
  2815. 2:18:29uh
  2816. 2:18:32well
  2817. 2:18:33if I approximate this
  2818. 2:18:36as if I assume that P is somehow
  2819. 2:18:39constant in this middle interval or let
  2820. 2:18:41me let me write it like this
  2821. 2:18:44so this already tells you what I want to
  2822. 2:18:46say so this is how much it changes the
  2823. 2:18:49amount of probability that you have in a
  2824. 2:18:51small interval around zero
  2825. 2:18:53and using the right hand side you do the
  2826. 2:18:55same thing so you integrate
  2827. 2:18:57now this expression over X in this case
  2828. 2:19:00you don't have to worry about this Delta
  2829. 2:19:02function because this Delta function is
  2830. 2:19:04far away at this value of theta which is
  2831. 2:19:06not around
  2832. 2:19:07an Infinity
  2833. 2:19:10close to zero so I can forget about the
  2834. 2:19:12source term
  2835. 2:19:14and I can integrate whatever remains
  2836. 2:19:16which has the form of a total derivative
  2837. 2:19:19and if I integrate what do I get I get a
  2838. 2:19:22contribution which is
  2839. 2:19:24P of t
  2840. 2:19:26of sine over P minus P of minus
  2841. 2:19:32and then I get the contribution from the
  2842. 2:19:34diffusion which is Plus
  2843. 2:19:37these
  2844. 2:19:38the derivative
  2845. 2:19:40in x
  2846. 2:19:42Cylon
  2847. 2:19:43minus the derivative of minus 5.
  2848. 2:19:49I hope you see this okay
  2849. 2:19:53and then I take Epsilon to zero and if I
  2850. 2:19:56take Epsilon to zero well actually if
  2851. 2:19:59you are with the last of these intervals
  2852. 2:20:02as minus the challenge we are assuming
  2853. 2:20:04that everything is equal to zero so this
  2854. 2:20:05will be zero but
  2855. 2:20:07oh
  2856. 2:20:08and the derivative will also be zero
  2857. 2:20:12and if I take
  2858. 2:20:14flash Epsilon
  2859. 2:20:17which goes towards zero as well what I
  2860. 2:20:20realized is that because of the
  2861. 2:20:21absorbing boundary this is also a
  2862. 2:20:24converging to zero so in the limit of
  2863. 2:20:26Epsilon small which is what we're
  2864. 2:20:28interested in because
  2865. 2:20:30flux then this term will disappear and
  2866. 2:20:33what you are left with is precisely
  2867. 2:20:36this derivative of the probability with
  2868. 2:20:39respect to X which is what we are
  2869. 2:20:41putting it here
  2870. 2:20:44so this was just to motivate why the
  2871. 2:20:46term which appears
  2872. 2:20:48in the driest has has this particular
  2873. 2:20:52form
  2874. 2:20:54okay so so for the model uh we are more
  2875. 2:20:58or less there so you see the source is
  2876. 2:21:01here
  2877. 2:21:02the sink if you want is encoded in this
  2878. 2:21:05absorbing boundary and the interaction
  2879. 2:21:06is encoded in this time dependence drift
  2880. 2:21:11for our shorts
  2881. 2:21:13and now what we have to do is to try to
  2882. 2:21:15solve for the stationary state of this
  2883. 2:21:18program and then look
  2884. 2:21:20at the stability
  2885. 2:21:24which are points uh so this was point
  2886. 2:21:26one motivate the model and now let's do
  2887. 2:21:29point
  2888. 2:21:30uh two and three and I just realized
  2889. 2:21:33that
  2890. 2:21:35backwards
  2891. 2:21:43back here
  2892. 2:21:45okay
  2893. 2:21:49so before we start for the stationary
  2894. 2:21:51state
  2895. 2:21:52let's try to organize a little bit all
  2896. 2:21:55of the parameters that we have
  2897. 2:21:57which are many
  2898. 2:22:15foreign
  2899. 2:22:17ters
  2900. 2:22:21in the model when we have essentially
  2901. 2:22:23five parameters so we have the
  2902. 2:22:26drift B and diffusion
  2903. 2:22:28as in a user wrap work then we have the
  2904. 2:22:32strength of the interactions or the
  2905. 2:22:33feedback which will be stopping beta
  2906. 2:22:36then we have the threshold for failure
  2907. 2:22:40which is
  2908. 2:22:41parameters
  2909. 2:22:44and then what did I forget then we have
  2910. 2:22:47this High which is the rate at which you
  2911. 2:22:49range at the firms into the model
  2912. 2:22:54so these are many but what you can show
  2913. 2:22:58by solving the model is that
  2914. 2:23:01essentially everything will depend on a
  2915. 2:23:04combination of this
  2916. 2:23:05of this parameter so you can reduce
  2917. 2:23:08everything to the behavior of three
  2918. 2:23:10parameters
  2919. 2:23:14one is beta which remains is
  2920. 2:23:18then you can introduce a ratio which is
  2921. 2:23:21called the clear number that is
  2922. 2:23:23something which appears when you study
  2923. 2:23:26transport of his shoes
  2924. 2:23:30that will not appear in what we are
  2925. 2:23:33going to discuss but let me introduce
  2926. 2:23:35it anyway
  2927. 2:23:37the papers so this is the ratio between
  2928. 2:23:40beta theta over the diffusion constant
  2929. 2:23:44and it is if you want a measure of
  2930. 2:23:47the drift versus the diffusion
  2931. 2:23:50of your work where the interaction does
  2932. 2:23:53not enter
  2933. 2:23:56and then we have another parameter which
  2934. 2:23:57is instead important for us that I call
  2935. 2:24:00is that
  2936. 2:24:01here
  2937. 2:24:03which is a ratio of time
  2938. 2:24:06and in particular it is the ratio of the
  2939. 2:24:10injection time the rate at which one
  2940. 2:24:13over the rate at which you
  2941. 2:24:15research firms in your model so this is
  2942. 2:24:17one over five
  2943. 2:24:20divided by uh the time which is the time
  2944. 2:24:24space at which typically your firms are
  2945. 2:24:28suppressed from the model so this is
  2946. 2:24:30your firm dies and and this is computed
  2947. 2:24:34in the limits
  2948. 2:24:35when beta is particularly small
  2949. 2:24:39so when we can neglect this feedback
  2950. 2:24:43then what is the typical science case at
  2951. 2:24:46which a firm dies well this is basically
  2952. 2:24:49controlled uh just by the drift constant
  2953. 2:24:52B so I
  2954. 2:24:53at a given time P0 I range Act a firm at
  2955. 2:24:57C time then I ask what is the typical
  2956. 2:25:00time which is required for each for each
  2957. 2:25:03to reach zero and therefore disappears
  2958. 2:25:05from the model and I can estimate this
  2959. 2:25:08if I can neglect beta if I can neglect
  2960. 2:25:10the diffusion essentially as
  2961. 2:25:13uh as B divided by so I want these what
  2962. 2:25:19B is a velocity
  2963. 2:25:21will be the in order to go from here to
  2964. 2:25:23here I have to cover a distance that is
  2965. 2:25:26equal to Theta with a velocity B so what
  2966. 2:25:29is the time that I need to do this well
  2967. 2:25:32it is related to B by by this
  2968. 2:25:35relationship
  2969. 2:25:36but now that I'm interested in is just
  2970. 2:25:42okay and this is what I put in here
  2971. 2:25:45but
  2972. 2:25:46one over five use a time and then I
  2973. 2:25:48divide by another time which is
  2974. 2:25:51Theta over B
  2975. 2:25:53which is my parameter be time this is
  2976. 2:25:55that sorry and that is what will appear
  2977. 2:25:58in our calculation in a minute
  2978. 2:26:02so it could be introduce it
  2979. 2:26:04and it's good to take or to have in mind
  2980. 2:26:08a limit
  2981. 2:26:09that will be useful later on
  2982. 2:26:12which is the limit
  2983. 2:26:15when
  2984. 2:26:17that is going to zero and again
  2985. 2:26:20God is having mine for instance that
  2986. 2:26:22data is very very small
  2987. 2:26:24so when that is going to uh
  2988. 2:26:28zero
  2989. 2:26:31then what we are saying so so this is
  2990. 2:26:33the time at which we reinject
  2991. 2:26:36versus uh the time uh for for the first
  2992. 2:26:41guy and so the idea is that whenever we
  2993. 2:26:45take this limit we should
  2994. 2:26:47uh
  2995. 2:26:48we have essentially that every time
  2996. 2:26:51somebody dies it gets immediately
  2997. 2:26:53reinject it so you don't have to wait a
  2998. 2:26:55lot in order to see it rejected so in
  2999. 2:26:59this limit
  3000. 2:27:00any
  3001. 2:27:04Burns
  3002. 2:27:06but
  3003. 2:27:08nice I say nice but of course and it
  3004. 2:27:11means it goes
  3005. 2:27:13bankrupt
  3006. 2:27:17is immediately
  3007. 2:27:21Ranger
  3008. 2:27:27and we will use this fact in a minute to
  3009. 2:27:31fix some boundary condition
  3010. 2:27:33or to select some solutions
  3011. 2:27:36of office consistent equation so just
  3012. 2:27:39this is just a common keep in mind this
  3013. 2:27:41limit because it will be useful in the
  3014. 2:27:44following
  3015. 2:27:47okay so now that we have all of this we
  3016. 2:27:51can now try to solve
  3017. 2:27:53for the stationary state of this
  3018. 2:27:56particular equation
  3019. 2:27:59and I don't know what the best space
  3020. 2:28:03uh Solutions so
  3021. 2:28:10I will keep the equation to this point
  3022. 2:28:13three
  3023. 2:28:15and these I will erase
  3024. 2:28:18but we will use it all the time
  3025. 2:28:22keep in mind all of this definition
  3026. 2:28:31absolutely
  3027. 2:28:35okay
  3028. 2:28:38so now let's look for this stationary
  3029. 2:28:41solution
  3030. 2:28:44so what does stationary means
  3031. 2:28:46well
  3032. 2:28:48in general it means that you won't
  3033. 2:28:53seems not to depend
  3034. 2:28:55sometimes but to be constant
  3035. 2:28:57time
  3036. 2:28:59so the first thing that you can ask is
  3037. 2:29:01that your fraction
  3038. 2:29:03of
  3039. 2:29:05active terms which we Define that
  3040. 2:29:08Phi of t
  3041. 2:29:09in the stationary state is time
  3042. 2:29:12Independence and it is just equal to a
  3043. 2:29:15constant that I call five zero
  3044. 2:29:21and with a very similar reasoning
  3045. 2:29:26you can also ask that all of the other
  3046. 2:29:30time dependent quantities that you have
  3047. 2:29:33in your model reach a stationary state
  3048. 2:29:35where as a human depend on time so for
  3049. 2:29:38instance it will ask that b of t
  3050. 2:29:41will
  3051. 2:29:44reach a constant value which is d0
  3052. 2:29:49and what is b0 well
  3053. 2:29:51if you remember what was this fraction
  3054. 2:29:53for B of t
  3055. 2:29:55will be zero was B plus
  3056. 2:30:02and then you add B times the derivative
  3057. 2:30:06which following the notation of the
  3058. 2:30:08paper I will call so the flux at 0 and
  3059. 2:30:12we call it J of T so this is d times the
  3060. 2:30:15derivative of e
  3061. 2:30:19evaluated at x equal to zero
  3062. 2:30:25so this is a quantity which in general
  3063. 2:30:26depends on time which enters in my
  3064. 2:30:28definition of d of T but of course if I
  3065. 2:30:30ask that b does not depend on time
  3066. 2:30:32anymore then J should have submerged
  3067. 2:30:35or be equal to a constant we check for
  3068. 2:30:37j0
  3069. 2:30:40and of course
  3070. 2:30:48and of course
  3071. 2:30:50you have another quantity in here which
  3072. 2:30:52depends on time which is the itself so
  3073. 2:30:54the fourth thing that you have to ask is
  3074. 2:30:58that your field
  3075. 2:31:00X and E
  3076. 2:31:02is something which does not depend on
  3077. 2:31:04time which I will call be stationary
  3078. 2:31:06effects
  3079. 2:31:11okay now how can this be true that you
  3080. 2:31:14reach a Time independent value for this
  3081. 2:31:17fraction of a live terms
  3082. 2:31:20whenever you have certain I think
  3083. 2:31:24so whenever your system is open
  3084. 2:31:26at this particular point of zero and
  3085. 2:31:30Theta
  3086. 2:31:31well in order for the fraction of firms
  3087. 2:31:33not to change what you have to ask
  3088. 2:31:36is that uh somehow the the Flux Of firms
  3089. 2:31:41that you inject
  3090. 2:31:42at the point x equal to Theta so the
  3091. 2:31:45incoming flux of probability has to be
  3092. 2:31:48equal to the flux which goes out from
  3093. 2:31:51your system at the point here
  3094. 2:31:53which was exactly given by this jfp
  3095. 2:31:57so with this stationarity uh implies or
  3096. 2:32:00what we have to impose in addition to
  3097. 2:32:03this is that the fluxes
  3098. 2:32:12are equally
  3099. 2:32:14so the rate at which firms 9 is the same
  3100. 2:32:17rate which firms are introduced into our
  3101. 2:32:20model in such a way that the total
  3102. 2:32:21number of firms for the fraction remains
  3103. 2:32:25so what this means is that
  3104. 2:32:29J of T which is the slot of
  3105. 2:32:32outgoing firms
  3106. 2:32:35which we assume be equal to a constant
  3107. 2:32:38in the stationary state
  3108. 2:32:40has to be equal to the Flux Of incoming
  3109. 2:32:42terms which is given by this Search
  3110. 2:32:46terms here
  3111. 2:32:47so it has to be equal
  3112. 2:32:49y
  3113. 2:32:511 minus
  3114. 2:32:535 0.
  3115. 2:32:56so in principle you have Phi of T but in
  3116. 2:32:58the stationary State we assume that all
  3117. 2:33:00of them
  3118. 2:33:02so we have to impose this uh particular
  3119. 2:33:05relation in order for this
  3120. 2:33:08assumption here to make sense
  3121. 2:33:13okay
  3122. 2:33:14so now given this let's try to plug this
  3123. 2:33:19into the equation so let's try to
  3124. 2:33:23impose this and solve the four fourth DP
  3125. 2:33:28of x t already t
  3126. 2:33:30equal to zero as we did also last time
  3127. 2:33:35with this assumption
  3128. 2:33:41Here and Now
  3129. 2:33:42as I commented at the beginning
  3130. 2:33:46so DP DT equal to zero means that the
  3131. 2:33:49right hand side of our equation is zero
  3132. 2:33:51and before we could
  3133. 2:33:53translate this
  3134. 2:33:56or in simpler models we could translate
  3135. 2:33:59it or if you want in simpler model we
  3136. 2:34:01could write
  3137. 2:34:02the right hand side in the form of a
  3138. 2:34:05continuity equation so as the total
  3139. 2:34:07derivative something and then we add a
  3140. 2:34:09current and then we could set the
  3141. 2:34:10current to zero but now we have that
  3142. 2:34:12Delta function which
  3143. 2:34:18and how embed this term
  3144. 2:34:21between some continuity equation
  3145. 2:34:25so we have to do something else
  3146. 2:34:28let's see looks a little bit different
  3147. 2:34:29but actually you will see it more or
  3148. 2:34:32less the same thing
  3149. 2:34:34for
  3150. 2:34:36a specialized state
  3151. 2:34:41so instead of putting the current to
  3152. 2:34:43zero what we do is to integrate
  3153. 2:34:47our soccer plan equation with respect to
  3154. 2:34:49X
  3155. 2:34:51it is essentially the same way in which
  3156. 2:34:53you get a current so if you remember
  3157. 2:34:56in the usual continuity equation you
  3158. 2:34:58have something like this DP over DC
  3159. 2:35:00equal to something
  3160. 2:35:02you set it to zero and now getting the
  3161. 2:35:04current means that you're integrating
  3162. 2:35:06the right side with respect to X and if
  3163. 2:35:09you do this this is the anti-derivative
  3164. 2:35:11so you just get J which then you said
  3165. 2:35:14you know so here we are not setting it
  3166. 2:35:16to zero but
  3167. 2:35:17uh we are not setting J
  3168. 2:35:20directly to zero but we are exciting the
  3169. 2:35:24integral of the focused blank equation
  3170. 2:35:27so these were many words
  3171. 2:35:30pretty easy
  3172. 2:35:31actually so this means
  3173. 2:35:35again dbvt of XP
  3174. 2:35:38equals zero
  3175. 2:35:40and now what I do
  3176. 2:35:42this is also equal to the
  3177. 2:35:44right side and then I integrate both
  3178. 2:35:48sides
  3179. 2:35:49with respect to X
  3180. 2:35:55and because I have a data function I
  3181. 2:35:57have to split two different cases so if
  3182. 2:36:00I integrate
  3183. 2:36:02in an interval which does not contain
  3184. 2:36:05Theta where the function will not
  3185. 2:36:07contribute or as if I integrate in an
  3186. 2:36:09interval which contains Theta it will
  3187. 2:36:12actually continue let's split the two
  3188. 2:36:15cases so let me fix the value of x
  3189. 2:36:18which is smaller than Theta
  3190. 2:36:20and then let me integrate the right hand
  3191. 2:36:23side from x0 to this particular value of
  3192. 2:36:26x
  3193. 2:36:28and we will choose x0
  3194. 2:36:32so if I do it the left hand side is just
  3195. 2:36:35the integral of 0 which is 0 and then
  3196. 2:36:37what do I have I have
  3197. 2:36:39P of T times V integral of the
  3198. 2:36:43derivative I hope you can see
  3199. 2:36:46of course not
  3200. 2:36:48uh
  3201. 2:36:51the focal plant equation
  3202. 2:37:00sorry what is x0
  3203. 2:37:03yes x0 is the is the horizontal is
  3204. 2:37:06arbitrary but
  3205. 2:37:07I will later on
  3206. 2:37:09so you can well
  3207. 2:37:12we can choose it directly now let me
  3208. 2:37:14leave it we will choose it to be zero so
  3209. 2:37:16for the moment I just take my focus
  3210. 2:37:18equation and I integrate over an
  3211. 2:37:20interval which goes from some point x 0
  3212. 2:37:23largely zero to some arbitrary point x
  3213. 2:37:27smaller than Theta
  3214. 2:37:28okay
  3215. 2:37:31I can choose a 0 and it will be
  3216. 2:37:33convenient to choose it equal to zero
  3217. 2:37:35because there and we know that P has to
  3218. 2:37:37be equal to zero so this is what I'm
  3219. 2:37:39doing in a minute
  3220. 2:37:41so sorry I don't think you you see the
  3221. 2:37:43equation but I hope you have it in the
  3222. 2:37:45notes I'm just integrating the right
  3223. 2:37:47hand side and I get the following
  3224. 2:37:50so this term was multiplied by a space
  3225. 2:37:52derivative so if I integrate I just have
  3226. 2:37:54P of x p minus P of x 0 t
  3227. 2:37:59and then I have the diffusion term
  3228. 2:38:04which
  3229. 2:38:05I have two derivatives I integrate one
  3230. 2:38:08and I get
  3231. 2:38:10the other one
  3232. 2:38:12so so far this looks like the normal
  3233. 2:38:13copper plank equation because
  3234. 2:38:16X is smaller than T times so the Delta
  3235. 2:38:18is not
  3236. 2:38:19giving any
  3237. 2:38:23and then I choose as you pointed out x0
  3238. 2:38:26equal to zero so if I choose
  3239. 2:38:29x videos arbitrary so if I choose x 0
  3240. 2:38:31equals to zero
  3241. 2:38:33this term here is Vanishing because I
  3242. 2:38:35have my absorbing boundary condition f x
  3243. 2:38:380.
  3244. 2:38:40and what is this term in here well I
  3245. 2:38:44have remember that this is equal
  3246. 2:38:46to this uh quantity J
  3247. 2:38:50uh
  3248. 2:38:53that I defined before so J of P was
  3249. 2:38:57e times the derivative of P
  3250. 2:39:01of x e the X evaluated Steel
  3251. 2:39:06which is precisely disturbing here
  3252. 2:39:12and now of course I'm using uh the wrong
  3253. 2:39:15notation because if I put a zero on the
  3254. 2:39:18left hand side it means that I'm already
  3255. 2:39:19considering the stationary state so
  3256. 2:39:23this is actually be stationary
  3257. 2:39:26wax
  3258. 2:39:28there should be no time dependent
  3259. 2:39:30this is the stationary attack zero this
  3260. 2:39:33is the derivative
  3261. 2:39:34with respect to work stationary
  3262. 2:39:38variable Vision this was the derivative
  3263. 2:39:40of the stationary
  3264. 2:39:46compute and therefore this product in
  3265. 2:39:48here will just give me under my
  3266. 2:39:51stationary assumption the constant Json
  3267. 2:39:57okay so all together and this is under
  3268. 2:40:00my stationary assumption between
  3269. 2:40:04so the equation reads the zero the
  3270. 2:40:07stationary events
  3271. 2:40:10Mr banishing
  3272. 2:40:13plus b
  3273. 2:40:15derivative of the stationary of x
  3274. 2:40:20minus j0
  3275. 2:40:22equal to zero
  3276. 2:40:27and now I can use the usual trick
  3277. 2:40:32that I use whenever I want to find a
  3278. 2:40:34Stationary State and indeed
  3279. 2:40:36as long as Theta is X is smaller than
  3280. 2:40:39Theta because it's just the user for the
  3281. 2:40:40Planck equation so what I can do to
  3282. 2:40:42solve this equation is
  3283. 2:40:44the usual separation of variables that
  3284. 2:40:47we have discussed last time
  3285. 2:40:52so let me write it
  3286. 2:40:55in a faster way
  3287. 2:41:00actually
  3288. 2:41:02write it as
  3289. 2:41:08so this is just a little bit of algebra
  3290. 2:41:10that's going to change Zero mine
  3291. 2:41:14zero
  3292. 2:41:16stationary events
  3293. 2:41:21divided by D
  3294. 2:41:26okay
  3295. 2:41:31and then
  3296. 2:41:34do the separation of variables I have
  3297. 2:41:37remember I have bring everything which
  3298. 2:41:39depends on p on one side and everything
  3299. 2:41:41which depends on X on the other side so
  3300. 2:41:44this in differential form
  3301. 2:41:46can be read recent as
  3302. 2:41:49deep stationary divided by
  3303. 2:41:520 over D minus d0 over d
  3304. 2:41:57ictionary
  3305. 2:41:59equal to X
  3306. 2:42:03okay
  3307. 2:42:07then I integrate
  3308. 2:42:11with it last time again from some
  3309. 2:42:13arbitrary
  3310. 2:42:150 to X more than beta
  3311. 2:42:200.
  3312. 2:42:26okay
  3313. 2:42:29and as usual what you get on the left
  3314. 2:42:32hand side is a logarithm and what you
  3315. 2:42:34get on the right hand side is just
  3316. 2:42:37X
  3317. 2:42:49now we have to track the minus sign
  3318. 2:42:52foreign
  3319. 2:42:56side you would have
  3320. 2:42:58minus the logarithm
  3321. 2:43:01if I do the integrand
  3322. 2:43:03I do therefore
  3323. 2:43:06minus the logarithm of
  3324. 2:43:10j0 over D minus
  3325. 2:43:17the other side
  3326. 2:43:23so
  3327. 2:43:25this I will have to evaluate
  3328. 2:43:27from X to Zero and then I have another
  3329. 2:43:30constant which is
  3330. 2:43:34front which is minus B over B right
  3331. 2:43:40so if I take the so this is the
  3332. 2:43:42anti-derivative now if I take the
  3333. 2:43:43derivative of the log I get 1 over this
  3334. 2:43:46and then I have
  3335. 2:43:48a constant which is minus P0 over D
  3336. 2:43:50which I have to count to this Factor
  3337. 2:43:53and I have to evaluate it from X
  3338. 2:43:56zero or if you want P of x
  3339. 2:44:00V of zero
  3340. 2:44:02this should be CLI
  3341. 2:44:08speed of 0
  3342. 2:44:14so if I do this I will just get the log
  3343. 2:44:17of this evaluated at X the minus the log
  3344. 2:44:20of this evaluated that's zero which I
  3345. 2:44:22can write as the log of a ratio
  3346. 2:44:26and the P stationary S 0 we know that is
  3347. 2:44:30equal to because I think
  3348. 2:44:32once you get something like this for the
  3349. 2:44:35left side
  3350. 2:44:36if we check and the right hand side is
  3351. 2:44:38easy it is just a factor of x
  3352. 2:44:43okay
  3353. 2:44:47so now let me bring this constant on the
  3354. 2:44:50other side so that I have minus is 0
  3355. 2:44:53over d
  3356. 2:44:55x negative is
  3357. 2:44:58and now I can exponentiate so if I take
  3358. 2:45:01the exponential of this expression what
  3359. 2:45:03do I get
  3360. 2:45:05yeah
  3361. 2:45:060 over d
  3362. 2:45:09nine would be 0 over d p stationery
  3363. 2:45:13X
  3364. 2:45:15is equal to this constant that now I
  3365. 2:45:17bring this on the other side which is
  3366. 2:45:20already into the minus
  3367. 2:45:23zero over d i
  3368. 2:45:29which means that might be
  3369. 2:45:33stationary next
  3370. 2:45:37East
  3371. 2:45:40what
  3372. 2:45:42B you see that I can eliminate it here
  3373. 2:45:48I divide everything by this in it
  3374. 2:45:52and my uh this stationary will be
  3375. 2:45:55j0 over v0
  3376. 2:45:581 minus E to the minus is zero over Z
  3377. 2:46:10of course under the assumption that X is
  3378. 2:46:13smaller than Theta
  3379. 2:46:16foreign
  3380. 2:46:22of our solution
  3381. 2:46:25and now what do we have to do well now
  3382. 2:46:27we have to look at what is the V over
  3383. 2:46:29when X is larger than Theta and when X
  3384. 2:46:33larger than Theta then we have an extra
  3385. 2:46:35contribution to our integrated soccer
  3386. 2:46:39plant equation which comes from the
  3387. 2:46:40Delta so now I assume that X is larger
  3388. 2:46:43than did I play the same game that I did
  3389. 2:46:46before
  3390. 2:46:49so I say 0 equals to be integral from x
  3391. 2:46:530 equal to 0 up to this x of the right
  3392. 2:46:57side
  3393. 2:47:00and what I get is the following so let
  3394. 2:47:02me write
  3395. 2:47:08shorter than well I get to zero equal to
  3396. 2:47:12one contribution from
  3397. 2:47:15as before from b0 so b0 stationary
  3398. 2:47:20of x
  3399. 2:47:22then I have the contribution from the
  3400. 2:47:24diffusion
  3401. 2:47:26and this was
  3402. 2:47:32B
  3403. 2:47:35the derivative attacks
  3404. 2:47:38minus D times the derivative at 0 which
  3405. 2:47:41we say was equal to J zero
  3406. 2:47:45and then we have the final contribution
  3407. 2:47:48from Delta function which is just Phi
  3408. 2:47:51one line
  3409. 2:47:59in this remember these two fellowships
  3410. 2:48:06okay and now we should remember
  3411. 2:48:10something
  3412. 2:48:13so do you recognize any consolation
  3413. 2:48:17IRAs
  3414. 2:48:19all of the formula but remember
  3415. 2:48:21that when we impose a stationarity and
  3416. 2:48:25we equated the flux the equation
  3417. 2:48:28was precisely the following so the flags
  3418. 2:48:30of firms which were dying has to be
  3419. 2:48:33equal to the slacks of those which were
  3420. 2:48:36injected which was five one minus
  3421. 2:48:39the different five years
  3422. 2:48:42so this was because
  3423. 2:48:45missionaries so we can use this in here
  3424. 2:48:48and we see that these two terms
  3425. 2:48:50constant
  3426. 2:48:54so the equation is now particularly
  3427. 2:48:56simple it's just uh it's telling me that
  3428. 2:48:59my stationary
  3429. 2:49:03distribution for X larger than Theta has
  3430. 2:49:05an exponential form so it will be a
  3431. 2:49:07constant
  3432. 2:49:09times e to these
  3433. 2:49:12this minus zero
  3434. 2:49:15over D times h
  3435. 2:49:18or X largest
  3436. 2:49:24right
  3437. 2:49:27thank you
  3438. 2:49:30okay
  3439. 2:49:34so now there is a final little step to
  3440. 2:49:37do so this would one piece of the
  3441. 2:49:39solution the other one is up here
  3442. 2:49:45small in effect it is for large enough X
  3443. 2:49:51and you see that I have some
  3444. 2:49:52undetermined constant a in here
  3445. 2:49:58so what is a clever way to match uh
  3446. 2:50:03so it is a clever way to uh determine
  3447. 2:50:07the value of the constant well uh what
  3448. 2:50:09you can do is you you ask that
  3449. 2:50:12the division is
  3450. 2:50:15so it's derivative will not be
  3451. 2:50:17continuous because you have the data
  3452. 2:50:18fund but the distribution itself
  3453. 2:50:20is continuous so you have to equate the
  3454. 2:50:23expression that you have for smaller
  3455. 2:50:25values of x to the expression that you
  3456. 2:50:28have for larger values of X when
  3457. 2:50:30computed exactly at Theta
  3458. 2:50:37so this
  3459. 2:50:38is that
  3460. 2:50:44which is perfect
  3461. 2:50:47for almost the last step
  3462. 2:50:59which is to fix my constant a
  3463. 2:51:03using continuity
  3464. 2:51:08of B
  3465. 2:51:17B
  3466. 2:51:19okay so for X smaller than Theta we add
  3467. 2:51:23the expression that U perhaps to get
  3468. 2:51:26more
  3469. 2:51:27but let me write it so if x is smaller
  3470. 2:51:30or equal
  3471. 2:51:33s Theta
  3472. 2:51:35we have an expression and then I compute
  3473. 2:51:37this expression exactly as at sometimes
  3474. 2:51:40it gives me j0 over b0
  3475. 2:51:451 minus E to the minus b0 over D times
  3476. 2:51:49Theta
  3477. 2:51:52and then I equate it to the expression
  3478. 2:51:55that I get for X largely Theta that is
  3479. 2:51:58just the exponential
  3480. 2:52:01a e to the minus
  3481. 2:52:04P0 over it B times Theta
  3482. 2:52:09and this allows me to fix
  3483. 2:52:12the value of a so a will just be equal
  3484. 2:52:16j0 over P0 e to be
  3485. 2:52:200 over d
  3486. 2:52:22Theta minus one
  3487. 2:52:24by multiplying each side of the equation
  3488. 2:52:26by e to the BC over B
  3489. 2:52:31okay and once I have this here the full
  3490. 2:52:34solution for
  3491. 2:52:35almost the full solution for my
  3492. 2:52:39for my stationary space
  3493. 2:52:43should I rewrited
  3494. 2:52:48foreign
  3495. 2:52:56X
  3496. 2:53:00or X
  3497. 2:53:02foreign
  3498. 2:53:04and it was
  3499. 2:53:0680.
  3500. 2:53:09X for x
  3501. 2:53:11larger equals 3 then it discontinues to
  3502. 2:53:13Theta and a is given here
  3503. 2:53:19okay so this is
  3504. 2:53:21almost the solution
  3505. 2:53:26why do I say almost because now we have
  3506. 2:53:29to remember that we did some assumptions
  3507. 2:53:31when we
  3508. 2:53:32point
  3509. 2:53:34and we have to check that these
  3510. 2:53:36assumptions are actually self-consistent
  3511. 2:53:38with the solution that we found
  3512. 2:53:42and this is a step which substitutes a
  3513. 2:53:44little bit of C in the user solution for
  3514. 2:53:47this additional state which is the
  3515. 2:53:48normalization
  3516. 2:53:54so in here we don't we don't want to
  3517. 2:53:57check the normalization in fully
  3518. 2:54:00interval but remember that we
  3519. 2:54:02had this parameters 5
  3520. 2:54:07by 0
  3521. 2:54:09which was which we assumed to be fixed
  3522. 2:54:13and this was the fraction of terms which
  3523. 2:54:17are active
  3524. 2:54:19that was defined as the integral from
  3525. 2:54:22zero to Infinity index
  3526. 2:54:24of
  3527. 2:54:27this case stationary solution
  3528. 2:54:30to stationary of x
  3529. 2:54:37and now what I have to do is I plug my
  3530. 2:54:40solution for the stationary I compute
  3531. 2:54:42this Instagram I'm not going to do this
  3532. 2:54:45this is just integrated explanation you
  3533. 2:54:48just have to split into the different
  3534. 2:54:50regime from zero to P time from C to
  3535. 2:54:52Infinity
  3536. 2:54:53and you get out
  3537. 2:54:55simple constants
  3538. 2:54:58that is j0
  3539. 2:55:01Theta
  3540. 2:55:03divided by
  3541. 2:55:05b0
  3542. 2:55:09so this was the last point to see
  3543. 2:55:13and this
  3544. 2:55:14is nothing but a self-conception
  3545. 2:55:23question
  3546. 2:55:28for
  3547. 2:55:30five zero
  3548. 2:55:34why is it just consistent well because
  3549. 2:55:37you have in here this constant v0
  3550. 2:55:41but then you have to remember what would
  3551. 2:55:43be zero so this zero
  3552. 2:55:45uh here
  3553. 2:55:48and you have to remember what is j0
  3554. 2:55:52so remember that J
  3555. 2:55:54zero was the Flux Of or was equal in the
  3556. 2:55:58stationary states to the flags of uh I
  3557. 2:56:01mean Burns for this we both could be
  3558. 2:56:04equal to one minus by zero
  3559. 2:56:08so inside this j0 there is a Phi zero
  3560. 2:56:12which appears and also inside of b0 so
  3561. 2:56:16if you remember this was B
  3562. 2:56:18Plus
  3563. 2:56:20beta Sita
  3564. 2:56:22itself
  3565. 2:56:24and therefore this is
  3566. 2:56:26B plus beta Theta Phi
  3567. 2:56:301 minus five zero
  3568. 2:56:34so if you plug
  3569. 2:56:36these two expressions
  3570. 2:56:38inside this equation you get
  3571. 2:56:41an equation for your five zero which you
  3572. 2:56:43need to solve in order to complete this
  3573. 2:56:46uh the solution of your mother
  3574. 2:56:50because spicero is not a parameters
  3575. 2:56:54it's part of the solution of the model
  3576. 2:56:55so let me rewrite the equation and then
  3577. 2:56:58you see that it is simple
  3578. 2:57:02so Phi 0 is beta times j0 so it is a
  3579. 2:57:06Theta times pi 1 minus Pi zero and I
  3580. 2:57:10will divide both numerator and
  3581. 2:57:12denominator by Theta times Phi so what
  3582. 2:57:15I'm left with is 1 minus by zero in the
  3583. 2:57:18numerator
  3584. 2:57:19and then I have in the denominator
  3585. 2:57:22B divided by
  3586. 2:57:24C plus five
  3587. 2:57:27Plus
  3588. 2:57:30beta
  3589. 2:57:33and then I have Theta Phi 1 minus Pi
  3590. 2:57:36zero but I divided by so theorem left
  3591. 2:57:38with one minus zero
  3592. 2:57:45and the reason why I wrote it in this
  3593. 2:57:47form is just that you recognize you hear
  3594. 2:57:50something that we defined at the
  3595. 2:57:53beginning so this was the ratio between
  3596. 2:57:54time scales that we called said
  3597. 2:58:00so we can rewrite this as a quadratic
  3598. 2:58:03equation for sine zeros to this by zero
  3599. 2:58:06Z Plus beta
  3600. 2:58:091 minus by zero is equal to 1 minus 5 0.
  3601. 2:58:15and then we can solve this
  3602. 2:58:22uh where
  3603. 2:58:25after
  3604. 2:58:41so we just saw this second order
  3605. 2:58:44equation and we have a now decide how to
  3606. 2:58:47choose the sign in front of the square
  3607. 2:58:49root
  3608. 2:58:54in general we get two solutions plus or
  3609. 2:58:57minus which will be of the following
  3610. 2:58:59form I have one or two beta
  3611. 2:59:05Z Plus beta plus one
  3612. 2:59:09lash line square roots
  3613. 2:59:13that plus beta plus one where
  3614. 2:59:18minus 4
  3615. 2:59:21.
  3616. 2:59:22okay
  3617. 2:59:26and here comes
  3618. 2:59:31here comes the comment that we made at
  3619. 2:59:34the beginning so when we introduced uh
  3620. 2:59:36we said so now we have to choose
  3621. 2:59:39what is the meaningful solution between
  3622. 2:59:41plus and minus and we can use this
  3623. 2:59:43equation that we have when introducing
  3624. 2:59:45that so this idea that
  3625. 2:59:47when Z goes to zero
  3626. 2:59:50and always
  3627. 2:59:52besides the should be small
  3628. 2:59:54then you should expect that whenever
  3629. 2:59:57somebody dies it gets immediately
  3630. 2:59:59reinjected with a time space which is
  3631. 3:00:01much much faster than the one of that
  3632. 3:00:04and therefore if you are in this
  3633. 3:00:06situation what do we expect
  3634. 3:00:09in this limit for the value of 5
  3635. 3:00:12well if whoever dies gets immediately
  3636. 3:00:15rejected then we expect that all of the
  3637. 3:00:18firms in our model will be in the
  3638. 3:00:20interval of active first because as soon
  3639. 3:00:23as they go out I put them back
  3640. 3:00:25immediately or very fast into the model
  3641. 3:00:28at x equals Theta and therefore we
  3642. 3:00:31should expect that in this limit
  3643. 3:00:33i0 goes to one
  3644. 3:00:37so this is just to say that using this
  3645. 3:00:39we can select what is the good solution
  3646. 3:00:43so we just have to look at the limit
  3647. 3:00:45instead going to zero for this equation
  3648. 3:00:47and see if we get 1 with a with either
  3649. 3:00:51with Plus or with minus
  3650. 3:00:54and what you find is that the good
  3651. 3:00:56solution if you do this is actually the
  3652. 3:00:58one with the mind
  3653. 3:01:00so the good price zero tools
  3654. 3:01:02as a minus sign
  3655. 3:01:04in front
  3656. 3:01:13well why because when Z is equal to zero
  3657. 3:01:15here you just have to there is let's
  3658. 3:01:17tell you this thing let me point it out
  3659. 3:01:19so when Z is equal to zero you can yes B
  3660. 3:01:22plus one square minus four B you can
  3661. 3:01:24rewrite it as
  3662. 3:01:25Theta minus one square
  3663. 3:01:29and then you you have to remember that
  3664. 3:01:33parameters data that we introduced was
  3665. 3:01:36the ratio of time scales when we can
  3666. 3:01:39neglect
  3667. 3:01:40uh data so we we always have this
  3668. 3:01:42assumption that beta is small
  3669. 3:01:44and if beta is small then this value is
  3670. 3:01:47negative so when you take the square
  3671. 3:01:49root of the square you have an absolute
  3672. 3:01:50value which Clips one sign and this is
  3673. 3:01:53why if you do the math you find that
  3674. 3:01:56minus is a good solution just just keep
  3675. 3:01:58in mind that this uh
  3676. 3:02:00what you have inside the square is
  3677. 3:02:02typically negative if the issue that we
  3678. 3:02:04have
  3679. 3:02:06that we are where you should expect if
  3680. 3:02:07you're going to want
  3681. 3:02:11okay so with this
  3682. 3:02:13uh we uh
  3683. 3:02:15conclude the first part
  3684. 3:02:19with super late well
  3685. 3:02:22okay
  3686. 3:02:23so let me give you an idea so what this
  3687. 3:02:25shows is that you can find a solution
  3688. 3:02:29for your stationary State and actually
  3689. 3:02:31you can argue that you always have a
  3690. 3:02:34solution to this self-consistent
  3691. 3:02:36equation uh which always lives in a good
  3692. 3:02:39regime so in some sense
  3693. 3:02:41[Music]
  3694. 3:02:43so you may wonder when does when do I
  3695. 3:02:45have to throw away this solution well
  3696. 3:02:46one thing that you could expect which
  3697. 3:02:48would be a trivial thing is that at a
  3698. 3:02:51certain point you find values of Phi
  3699. 3:02:53zero such that you get that one of these
  3700. 3:02:57parameters flows and these two signals
  3701. 3:02:59that what you're doing is not good any
  3702. 3:03:02longer and you have to look for another
  3703. 3:03:04suit now this is not what happens in
  3704. 3:03:06this smallness so in this model you
  3705. 3:03:08always find that Phi 0 is a solution
  3706. 3:03:12that is admissible
  3707. 3:03:16but what you have to check is and
  3708. 3:03:19therefore
  3709. 3:03:20stationary that we found
  3710. 3:03:23is an admissible solution but what you
  3711. 3:03:26have to check is really as I said before
  3712. 3:03:27the stability so what changes
  3713. 3:03:35is its stability
  3714. 3:03:40so let me go very fast forward or
  3715. 3:03:42through the second exercise where you
  3716. 3:03:45and give you the idea of how you check
  3717. 3:03:48actually the stability and determine
  3718. 3:03:51when it breaks down
  3719. 3:03:59an idea used to use precisely this
  3720. 3:04:02picture of preserving a little bit and
  3721. 3:04:05seeing to get back to your original
  3722. 3:04:08solution
  3723. 3:04:09except that now what we have to preserve
  3724. 3:04:11well we have to preserve a full function
  3725. 3:04:13which is our solution for uh for the
  3726. 3:04:16plant equation
  3727. 3:04:18so how do we preserve a function where
  3728. 3:04:20we introduce
  3729. 3:04:22foreign
  3730. 3:04:32plus some small perturbation in
  3731. 3:04:34functional space which I call B1
  3732. 3:04:39that now being a preservation we can
  3733. 3:04:41assume is no longer stationary but it
  3734. 3:04:43will depend
  3735. 3:04:44on time and this is small because I'm
  3736. 3:04:47putting
  3737. 3:04:48a factor of a child in front
  3738. 3:04:52so we make this answers for our equation
  3739. 3:04:55then of course if we perturb our
  3740. 3:04:57distribution we are also perturbing all
  3741. 3:05:00of the parameters which implicitly
  3742. 3:05:01depend
  3743. 3:05:02on the distribution so we have to assume
  3744. 3:05:05that beta
  3745. 3:05:07goes to some
  3746. 3:05:09sorry B goes to be zero plus F times P1
  3747. 3:05:11J goes to j0 Plus
  3748. 3:05:16a one and what else Phi
  3749. 3:05:25foreign
  3750. 3:05:31all of these
  3751. 3:05:36into our soccer plank equation
  3752. 3:05:41and we will get the term
  3753. 3:05:43which does not depend on Epsilon which
  3754. 3:05:46counts as because
  3755. 3:05:48precisely so if we select b00 I zero
  3756. 3:05:52empty stationary yet before
  3757. 3:05:54the soccer blank equation is satisfied
  3758. 3:05:56and it is stationary so that term
  3759. 3:05:57resunction
  3760. 3:05:59and then we will get a correction which
  3761. 3:06:01is uh of the order of Epsilon
  3762. 3:06:05so I will just
  3763. 3:06:07we've gone for like five minutes don't
  3764. 3:06:09worry I will just
  3765. 3:06:12write
  3766. 3:06:15what is the equation that you get
  3767. 3:06:19and how do you study it
  3768. 3:06:21so if you plug into the blank
  3769. 3:06:23equation you do the math you isolate the
  3770. 3:06:25term which is a word that Epsilon you
  3771. 3:06:27get an equation for this
  3772. 3:06:29correction P1 of accent if
  3773. 3:06:32that they write in this form so you have
  3774. 3:06:34a b over DT now I collect all the terms
  3775. 3:06:38which depend on P1 on the left side
  3776. 3:06:42you have a diffusion term
  3777. 3:06:45and then you also have a Drifter
  3778. 3:06:52all of this applied P1 respective
  3779. 3:06:57and on the right hand side you will get
  3780. 3:07:00terms which depend on the correction
  3781. 3:07:03on our family Bank quantities
  3782. 3:07:06and if you do this properly you should
  3783. 3:07:08find this V1 of t
  3784. 3:07:10times our stationary
  3785. 3:07:15so this is over the zero and afternoon
  3786. 3:07:16that this was over there absolute so
  3787. 3:07:18that's why you get a distribution and
  3788. 3:07:20then you also get a contribution from
  3789. 3:07:22the source which depends on this
  3790. 3:07:24correction file
  3791. 3:07:29okay
  3792. 3:07:36and now you can so now you have to solve
  3793. 3:07:39this equation to get T1
  3794. 3:07:43is a function of your time dependent
  3795. 3:07:46quantities
  3796. 3:07:48and this is not something that we are
  3797. 3:07:50going to do so you can look at the paper
  3798. 3:07:52but what is the idea so the idea is that
  3799. 3:07:54what you have in here
  3800. 3:07:55is an operator
  3801. 3:08:01that I call
  3802. 3:08:03G to the minus one
  3803. 3:08:06and so you have what you have to do to
  3804. 3:08:08get P1 is just to invert this operator
  3805. 3:08:11and this operator so you see it's an
  3806. 3:08:13operator which depends
  3807. 3:08:16derivative but you know how to write the
  3808. 3:08:19inverse so G is
  3809. 3:08:22doing function for those
  3810. 3:08:24who have this terminology mind but
  3811. 3:08:26anyway you can show that this equation
  3812. 3:08:28can be inverted
  3813. 3:08:30well formally
  3814. 3:08:33I call this function
  3815. 3:08:36f of x and t
  3816. 3:08:39my P1 will just be my operator G applied
  3817. 3:08:43to the function f
  3818. 3:08:46and this will itself give a function
  3819. 3:08:48which will dependency
  3820. 3:08:51and you can show so this is
  3821. 3:08:54similar to what you do when you want to
  3822. 3:08:55sort of keep the equation which is
  3823. 3:08:58basically the equation that we are
  3824. 3:09:00looking at we can show that the inverse
  3825. 3:09:02so G which is the inverse of this
  3826. 3:09:05operator
  3827. 3:09:06we know how to solve for for this we
  3828. 3:09:08know uh that this is an integral
  3829. 3:09:11operation with a kernel which is
  3830. 3:09:14that we can compute so there will be
  3831. 3:09:18uh kernel that is given in the paper
  3832. 3:09:21explicitly and I can write this right
  3833. 3:09:25side as
  3834. 3:09:27the kernel evaluated myself
  3835. 3:09:32times my function that's why now
  3836. 3:09:34integrated in d y
  3837. 3:09:39and this kernel is
  3838. 3:09:42is essentially a gaussian
  3839. 3:09:47is the usual kernel that you get when
  3840. 3:09:50you look at problems of diffusion
  3841. 3:09:52so if you want details you can look at
  3842. 3:09:54the paper
  3843. 3:10:02but somehow The crucial point is that we
  3844. 3:10:04can solve for P1 and we have P1 as a
  3845. 3:10:08function of C like this D1 and C1 and
  3846. 3:10:11Phi 1.
  3847. 3:10:12but now B1 and Phi 1 are also
  3848. 3:10:16somehow unknown they are the perforation
  3849. 3:10:19that we used in our functional space
  3850. 3:10:22so once we have P1 we then have to
  3851. 3:10:24impose
  3852. 3:10:25some self-consistency
  3853. 3:10:30okay
  3854. 3:10:33so you have to impose
  3855. 3:10:37as consistency
  3856. 3:10:44so yes P1 as a function of Pi one but
  3857. 3:10:47then remember what was Phi 1 well Pi one
  3858. 3:10:49is
  3859. 3:10:51to order Epsilon is the integral of C1
  3860. 3:10:55it says the first that consistent
  3861. 3:10:57equation that you have is that Phi 1 has
  3862. 3:11:00to be equal to the integral
  3863. 3:11:02text of your P1 electricity
  3864. 3:11:09and then you have a self-consistent
  3865. 3:11:11equation for B1
  3866. 3:11:15which is related to the derivative of uh
  3867. 3:11:18of one
  3868. 3:11:22so B1
  3869. 3:11:25should be equal to the following three
  3870. 3:11:33okay so these are the two circumstances
  3871. 3:11:36equations that we are supposed once you
  3872. 3:11:37have uh this solution for B1
  3873. 3:11:42and now our last
  3874. 3:11:44comments
  3875. 3:11:46how do you
  3876. 3:11:48check and try to find a solution to this
  3877. 3:11:50equation
  3878. 3:11:57well one thing that you can do is to
  3879. 3:11:59make an Anzac for the form of this Phi 1
  3880. 3:12:02and T1 and this is what they do in the
  3881. 3:12:04paper
  3882. 3:12:10and you make an answer which
  3883. 3:12:13Heat
  3884. 3:12:16to the presence of
  3885. 3:12:18population but
  3886. 3:12:21if you understand from the full solution
  3887. 3:12:23of the model but anyway you make the
  3888. 3:12:25following answer
  3889. 3:12:29assume that you can write Phi 1 as some
  3890. 3:12:32constant High Times
  3891. 3:12:34some exponential will where Alpha is
  3892. 3:12:38General complex
  3893. 3:12:43and B1
  3894. 3:12:45you can write it as some other constant
  3895. 3:12:47times the same
  3896. 3:12:49extension
  3897. 3:12:51you plug this into the self-consistent
  3898. 3:12:53equation you do all of the algebra and
  3899. 3:12:56what you get out of this are
  3900. 3:12:58the equation then the paper
  3901. 3:13:06so now we have three parameters to fix
  3902. 3:13:09five b and Alpha and you see that the
  3903. 3:13:12equation 10 in the paper that maybe you
  3904. 3:13:14also looked at
  3905. 3:13:16can be homework have the following form
  3906. 3:13:19so you can
  3907. 3:13:20rewrite the process consistent equation
  3908. 3:13:22in in the form of a matrix which depends
  3909. 3:13:26explicitly on Alpha
  3910. 3:13:29acting on the vector
  3911. 3:13:31constants
  3912. 3:13:33being equal to zero
  3913. 3:13:40now you ask how can I find a solution to
  3914. 3:13:43this equation which is non-trivial of
  3915. 3:13:45course a previous Solution that's sine
  3916. 3:13:46Theta zero but we have no previous
  3917. 3:13:48solution you need this Matrix
  3918. 3:13:50it's not The Interpreter which is
  3919. 3:13:52objective so that you have no zero
  3920. 3:13:54vectors
  3921. 3:13:55which belong to the kernel of the Matrix
  3922. 3:13:59M so such that if I apply M to them I
  3923. 3:14:02guess zero and so what you have to ask
  3924. 3:14:04is that the determinant
  3925. 3:14:07Alpha
  3926. 3:14:08is equal to zero because this tells you
  3927. 3:14:11that the kernel of Matrix
  3928. 3:14:14so the set of vectors where they
  3929. 3:14:16actually be zero is not just given by
  3930. 3:14:18the zero sir
  3931. 3:14:21and in this way you get
  3932. 3:14:24an equation
  3933. 3:14:28that you try to solve
  3934. 3:14:30you have different regimes so here you
  3935. 3:14:32have played solve this numerically play
  3936. 3:14:35a little bit remember that Alpha the
  3937. 3:14:39answers that we are making complex so we
  3938. 3:14:42will get the equation for the real
  3939. 3:14:43participation imaginary part
  3940. 3:14:46and you will find when this is the
  3941. 3:14:48final point
  3942. 3:14:50you will find three type of solution so
  3943. 3:14:53three regimes
  3944. 3:14:56depending on the parameter you can find
  3945. 3:14:58three type of solutions
  3946. 3:15:00for your Alpha
  3947. 3:15:05so in the first case you find that
  3948. 3:15:09your real part of alpha
  3949. 3:15:11is smaller than zero and imaginary parts
  3950. 3:15:13of alpha is zero
  3951. 3:15:19and this is precisely
  3952. 3:15:22the regime
  3953. 3:15:25where you can claim
  3954. 3:15:29that your solution is stable because if
  3955. 3:15:31we go back
  3956. 3:15:33in here
  3957. 3:15:35so remember if I want it was the
  3958. 3:15:36preservation of Phi so we are assuming
  3959. 3:15:38that Phi is equal to 5 0 plus some
  3960. 3:15:41perturbation that we are imposing we are
  3961. 3:15:44assuming that it has this form but then
  3962. 3:15:46you see that this exponential will be e
  3963. 3:15:49to the real part of alpha times p and
  3964. 3:15:51then you have two sine of imaginary
  3965. 3:15:54parts of alpha times T Plus either sine
  3966. 3:15:57simply
  3967. 3:15:59so if the imaginary part is zero
  3968. 3:16:02of alpha this constant this is equal to
  3969. 3:16:04one and if the real part is negative you
  3970. 3:16:07you see that you have an exponential
  3971. 3:16:08which indicates very fast to zero and
  3972. 3:16:11therefore in your preserved Dynamic you
  3973. 3:16:13go back to a value of Phi of T which is
  3974. 3:16:16precisely the size zero that you have to
  3975. 3:16:18determined before
  3976. 3:16:19and so this corresponds to stability of
  3977. 3:16:21your equation
  3978. 3:16:23and then you find another regime where
  3979. 3:16:26your imaginary part is different from
  3980. 3:16:29zero but the real part of alpha is still
  3981. 3:16:31uh more than zero so this is still
  3982. 3:16:34stable
  3983. 3:16:37but you see that if you have an anterior
  3984. 3:16:39imaginary part this somehow suggests
  3985. 3:16:42ventilation so that you converge back
  3986. 3:16:45let me do a little drawing
  3987. 3:16:47you preserve your fine you will have
  3988. 3:16:50some populations and then eventually you
  3989. 3:16:52converge to the stationary valued by
  3990. 3:16:54zero
  3991. 3:16:56and finally as you expect you have a
  3992. 3:16:59regime of parameter where actually you
  3993. 3:17:01find that the real part
  3994. 3:17:03of alpha is larger than zero and the
  3995. 3:17:06imaginary parts do whatever
  3996. 3:17:09and this is really so the first value of
  3997. 3:17:12parameters
  3998. 3:17:13at which this happens is really what is
  3999. 3:17:16telling you that you are developing an
  4000. 3:17:18ability
  4001. 3:17:24and therefore that you should throw away
  4002. 3:17:26the solution that we have we alluded in
  4003. 3:17:28the first exercise because as soon as
  4004. 3:17:31you preserve a little bit from that you
  4005. 3:17:33flow somewhere else and to determine how
  4006. 3:17:36you flow in this regime you then have to
  4007. 3:17:38solve for the full time dependent soccer
  4008. 3:17:42plan problem in this generally you don't
  4009. 3:17:44know how to do so there are in the paper
  4010. 3:17:46used to marriage uh
  4011. 3:17:49for simulation of the Dynamics but let's
  4012. 3:17:52say General this
  4013. 3:17:54going into this unstable phase and
  4014. 3:17:56finding the solution is very hard
  4015. 3:17:58problem
  4016. 3:18:00that there is no discussed analytically
  4017. 3:18:03in the paper
  4018. 3:18:05okay so that's it sorry it is very late
  4019. 3:18:09and so for uh for the last exercise on
  4020. 3:18:14the formograph
  4021. 3:18:15so you have it
  4022. 3:18:17and the solutions of the today and of
  4023. 3:18:19course if you want we can discuss it on
  4024. 3:18:23Wednesday or if the in the question and
  4025. 3:18:25the answer file and if you want to write
  4026. 3:18:28questions before Wednesday in there uh
  4027. 3:18:31feel free to do it and we will address
  4028. 3:18:32them
  4029. 3:18:34either there or any discussion
  4030. 3:18:38questions
  4031. 3:18:39no questions yeah
  4032. 3:18:51yes so just to make it clear there is a
  4033. 3:18:54I will write an email because I think it
  4034. 3:18:56was not clear so there was a question on
  4035. 3:18:58the exam the exam will be uh written I
  4036. 3:19:02think
  4037. 3:19:03unless she was maternity today today or
  4038. 3:19:06tomorrow but I think it will be written
  4039. 3:19:07and it's gonna be a paper to read and to
  4040. 3:19:11discuss so there are some technical
  4041. 3:19:13questions and then many other questions
  4042. 3:19:15about the interpretation uh of the paper
  4043. 3:19:18so it is uh there is not the choice
  4044. 3:19:21between let's say a standard exam and a
  4045. 3:19:23paper exam but it is only the paper and
  4046. 3:19:25you can look at it the exams from last
  4047. 3:19:29years which are in the folders who have
  4048. 3:19:32an idea
  4049. 3:19:33okay
  4050. 3:19:35okay so if there are no questions
  4051. 3:19:40have a nice study week

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