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Complex Systems - Jean-Philippe Bouchaud - Lecture 8: Hawkes; Kirman & Moran models (Valentina Ros) — Transcript

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  1. 0:01this conference will now be recorded
  2. 0:04great
  3. 0:06okay so good morning everybody
  4. 0:12so today we are gonna have a
  5. 0:15longer session
  6. 0:17and what I'd like to do is to
  7. 0:19uh discuss maybe uh first the end of the
  8. 0:24today five or six that we started last
  9. 0:26time
  10. 0:27so this was about uh melee hoax
  11. 0:30processes but as we will see we will
  12. 0:32also connect to some of the things that
  13. 0:34were discussed in the last lecture about
  14. 0:36meta stability and we are going to do
  15. 0:38this looking at a very simple model of
  16. 0:41financial transactions and exchanges and
  17. 0:45that's part one then I think we will
  18. 0:47make a break and then we will go to uh
  19. 0:50what was supposed to be the S7
  20. 0:52and that is about
  21. 0:54some simple model of opinion Dynamics if
  22. 0:58you want so this is a close again to
  23. 1:01what has been discussed in the last
  24. 1:03lecture and this is called in the
  25. 1:05literature either the kiermann model or
  26. 1:07the Moran model so this is also
  27. 1:09connected to uh to the homework
  28. 1:12number seven
  29. 1:15and uh so we will try to do this in
  30. 1:19detail and then if there is time I will
  31. 1:21give you just the idea of the third part
  32. 1:24of the seven slash eight which is uh
  33. 1:28going back a little bit to statistics
  34. 1:30and discussing using idea of brown and
  35. 1:33motion to discuss tests about or what
  36. 1:36are called goodness of fit test so how
  37. 1:39do you check that assumptions that you
  38. 1:42make on on a given set of data and on
  39. 1:45their underlying distribution are
  40. 1:46actually good or or whether you have to
  41. 1:49discard them so this is in case
  42. 1:51we managed to arrive them there but
  43. 1:54let's say the first two parts are the
  44. 1:57most important ones uh today so let's
  45. 2:00start with uh with the first one
  46. 2:03that is in the first uh today uh after
  47. 2:09the exercise that we discussed last time
  48. 2:12and I just wanted to start by recalling
  49. 2:14something that you saw in the lecture so
  50. 2:17this was
  51. 2:21from the last lecture
  52. 2:24and the idea is to recall a little bit
  53. 2:26this concept of meta stability
  54. 2:35and activated Dynamics because this is
  55. 2:38what we are going to discuss in more
  56. 2:40detail later on
  57. 2:42so in in the last lecture you were
  58. 2:44discussing things related to these
  59. 2:47models of choice where you have many
  60. 2:50agents that need to choose between
  61. 2:53different options and at a certain point
  62. 2:56you introduced
  63. 2:59some Dynamics so s was one of the
  64. 3:03possible binary choices of the agent
  65. 3:05label by I and you were writing
  66. 3:08something like this
  67. 3:10so the choice of the agent I at time T
  68. 3:13was related to the one of
  69. 3:15all of the other agents by uh by the
  70. 3:19following Expressions so this was the
  71. 3:20sign of some external field which I
  72. 3:23think was called Capital H then there
  73. 3:26was some uh let's see
  74. 3:28term which which was specific and
  75. 3:31typically randomly distributed and
  76. 3:33specific for agent I and then you add an
  77. 3:37interaction term
  78. 3:38that I write already in the meme field
  79. 3:41Expressions that was jij that I here
  80. 3:45write as j0 Over N so the normalization
  81. 3:48comes from the fact that you have all to
  82. 3:51all interactions between the agents so
  83. 3:53you have to divide by a factor of n in
  84. 3:55order for this to be of the same order
  85. 3:57of magnitude of your external field and
  86. 4:00then you have
  87. 4:01the choice of the agent J at the
  88. 4:04previous time T minus 1.
  89. 4:08and in order to discuss this model at a
  90. 4:11certain point uh we we or you made the
  91. 4:14assumption that this uh different random
  92. 4:17Fields were set equal to zero and then
  93. 4:19the model can be uh discussed in terms
  94. 4:23of a global meanful like variable which
  95. 4:27you can think of as the magnetization if
  96. 4:30you want in in the language of spins
  97. 4:32which was just the sum overall of your
  98. 4:35agents
  99. 4:36of the corresponding variable at time t
  100. 4:40and this quantity satisfies a dynamical
  101. 4:43equation that is essentially launch
  102. 4:44events so there was
  103. 4:47DM so this is a total derivative
  104. 4:50over DT was of the following form so the
  105. 4:54first term
  106. 4:56it was convenient to write it
  107. 4:59as a derivative of some potential which
  108. 5:02depend on the particular value of
  109. 5:04magnetization that you have at time T
  110. 5:06and then there was a noise term which
  111. 5:09contains some coefficients so the
  112. 5:11coefficient was set to one in the
  113. 5:13lecture I think but let me call it
  114. 5:15capital sigma
  115. 5:17divided by n and then there is the usual
  116. 5:21White Noise term
  117. 5:23and so as you see your Dynamics is given
  118. 5:26by as usual you have
  119. 5:29some noisy fluctuations
  120. 5:31and then the first term is what people
  121. 5:34usually call some gradient descent
  122. 5:38theorem
  123. 5:45so what you are saying is that you have
  124. 5:47a Dynamics in a given potential the
  125. 5:49Dynamics wants to push you downhill uh
  126. 5:53at the points which are or towards the
  127. 5:56points that are essentially Minima for
  128. 5:59for this potential or in general
  129. 6:00stationary points where the gradient of
  130. 6:02the potential is equal to zero and if
  131. 6:05you had no noise once you reach a
  132. 6:07stationary Point as you see the Dynamics
  133. 6:09this is equal to zero so your Dynamics
  134. 6:11would become stationary and you just
  135. 6:13staying there forever but if you have a
  136. 6:16little bit of noise then you can have a
  137. 6:18more richer Dynamics so you can use the
  138. 6:21noise to escape from these stationary
  139. 6:24points and this is what we are going to
  140. 6:26see today
  141. 6:27so in particular the shape
  142. 6:29of the potential in the lecture
  143. 6:33was or maybe I can draw it here
  144. 6:42so if you remember
  145. 6:50your potential was looking like the
  146. 6:54usual potential in using like problems
  147. 6:56so this was V beta
  148. 6:58of M when your field h capital H in here
  149. 7:03is different from zero
  150. 7:05it had a shape
  151. 7:08that was more or less like this with two
  152. 7:12Minima one of which is the global
  153. 7:14minimum in here and the other one is
  154. 7:16instead a local minimum which is
  155. 7:19sub-optimal with respect to uh to the
  156. 7:21global one
  157. 7:23and now what we're going to discuss
  158. 7:25today is how to interpret this local
  159. 7:28minimum so in particular
  160. 7:30in our language this will be
  161. 7:33a metastable state
  162. 7:38so what metastable state means is
  163. 7:41roughly the following so if you think
  164. 7:43about these Dynamics and you imagine
  165. 7:44that you start
  166. 7:46somewhere within the Basin of Attraction
  167. 7:49of this minimum so let's say that my
  168. 7:52Dynamics starts now maybe blue is not a
  169. 7:54good color
  170. 7:56starts somewhere in here than what you
  171. 7:58expect
  172. 7:59your system to do under these Dynamics
  173. 8:01if the noise is small
  174. 8:04then the dominant term will be this
  175. 8:06gradient term so this gradient term
  176. 8:08pushes you towards this point in here
  177. 8:11where indeed the right hand side is
  178. 8:14equal to zero so you would expect that
  179. 8:15you have some noisy dynamics that
  180. 8:17somehow goes down into this landscape
  181. 8:20and then it relaxes into this metastable
  182. 8:23state and maybe it performs a little bit
  183. 8:25of fluctuations within the Basin of this
  184. 8:28local minimum because you have the noise
  185. 8:32and if you're looking at your system in
  186. 8:35the limit in which n is exactly equal to
  187. 8:38Infinity so in general we think it n as
  188. 8:41being a large parameter but in the limit
  189. 8:44in which n is strictly Infinity which is
  190. 8:46the mean limit then that's it so you
  191. 8:49would converge to into this minimum and
  192. 8:52you will stay there essentially forever
  193. 8:54but if n is finite if you remember the
  194. 8:57comments that were made in the last
  195. 8:59lecture something more trivial and more
  196. 9:01or less trivial actually can happen
  197. 9:04namely you will have a certain instance
  198. 9:07of times which are very rare where your
  199. 9:11system
  200. 9:12which is confined in this region uses
  201. 9:15the noise to escape from this local
  202. 9:17minimum and to eventually converge
  203. 9:20to the global minimum of your potential
  204. 9:22in here
  205. 9:23but doing this is very hard with this
  206. 9:26Dynamics if your noise is small because
  207. 9:29as you see so if your noise is small
  208. 9:31then typically this is the term that
  209. 9:33wins and this term as I said pushes you
  210. 9:37down so in order to overcome this
  211. 9:39barrier so this is what was called B in
  212. 9:43the lecture is the difference in
  213. 9:45potential between let's say one of the
  214. 9:47Minima and the local maximum so to
  215. 9:50overcome this barrier you need very
  216. 9:52large fluctuations of your noise that
  217. 9:56are typically very rare So Rare means
  218. 9:59that you have to wait a lot of time to
  219. 10:01see this process occur and you can
  220. 10:04estimate what is the time so this was
  221. 10:05given uh in the lecture as well
  222. 10:09so let me call Tau the typical time
  223. 10:12scales for this type of jumps
  224. 10:16then
  225. 10:18what explicit calculations tell you
  226. 10:24is that this Tau will depend
  227. 10:27on the parameter that you have
  228. 10:30in the following way so it will be
  229. 10:32exponentially large in the barrier so
  230. 10:36what I call B here or actually to be
  231. 10:40more
  232. 10:41intuitive let me call it DV so this is
  233. 10:44the difference in potential between the
  234. 10:47local minimum and the local maximum and
  235. 10:50then in front you have this factor of n
  236. 10:52which is nothing but so it would be a
  237. 10:56factor of 1 over a sigma Square where
  238. 10:58Sigma is the variance of your noise
  239. 11:01and our unusual applications whenever
  240. 11:03you look at launch event what people do
  241. 11:06is to choose the variance of the noise
  242. 11:08to be proportional to temperature so
  243. 11:11noise is a measure of thermal
  244. 11:13fluctuations so this square root is in
  245. 11:17typical in the usual launch events
  246. 11:19formalism is of the order of square root
  247. 11:22of temperature so you see that this
  248. 11:24expression here you can write it as e to
  249. 11:27the beta
  250. 11:29times DV
  251. 11:31and this is uh what people call in the
  252. 11:35literature the the so-called Arena's
  253. 11:41Arrhenius Behavior so it tells you that
  254. 11:44the time that you need to wait in order
  255. 11:46to jump this barrier grows exponentially
  256. 11:49in the barrier itself but also in the
  257. 11:52temperature or in the inverse
  258. 11:54temperature or if you want in the
  259. 11:56inverse
  260. 11:57of the variance of your noise and in
  261. 12:00here because you're looking at models
  262. 12:02that are main field or fully connected
  263. 12:05you have this factor of n which makes so
  264. 12:07when n is large this makes your jump
  265. 12:09processes very very rare meaning that in
  266. 12:13the limit when n goes to Infinity these
  267. 12:15jumps will never occur because Tau goes
  268. 12:17to Infinity but if you have a finite
  269. 12:19size system even if fully connected you
  270. 12:23do have some finite time scales over
  271. 12:25which you will see this jump occurring
  272. 12:27and these are called activated processes
  273. 12:32or activated jumps
  274. 12:36I hope that you can see
  275. 12:44that are something that is studied even
  276. 12:48currently in situation a little bit more
  277. 12:50complicated than these for example in
  278. 12:52systems that are Glacier which have very
  279. 12:55many metastable states
  280. 12:57so what we are going to see today with
  281. 12:59the exercise number one is something
  282. 13:01quite similar so we will also estimate
  283. 13:04times for jumps over barriers of a
  284. 13:08potential but in this time so this time
  285. 13:11this let's say JUMP time will be also
  286. 13:14large in the model that we are going to
  287. 13:16see but it will be large in a parameter
  288. 13:18that is not the number of agent capital
  289. 13:21N but which is another parameter that we
  290. 13:25will call Epsilon or one over Epsilon
  291. 13:28which is related to non-linearities in
  292. 13:31your model so the setting is a little
  293. 13:33bit different but this was just to
  294. 13:35somehow remind you that in essence the
  295. 13:39type of processes that we want to
  296. 13:40describe are exactly of the form of what
  297. 13:43you saw in the previous lecture
  298. 13:45and let's keep in mind this expression
  299. 13:48because
  300. 13:50at the end of the exercise we will
  301. 13:51compare with uh with uh with the case of
  302. 13:56easing-like potentials
  303. 13:59okay so having say this let's go to the
  304. 14:02exercise and let me take the text
  305. 14:07and check where can I write
  306. 14:11[Music]
  307. 14:12um
  308. 14:14here is fine no here it's probably fine
  309. 14:17okay
  310. 14:18so this is the exercise number two I
  311. 14:21think uh of the today
  312. 14:23and it is a very simple model of uh
  313. 14:27Financial exchange or if you want
  314. 14:30transactions
  315. 14:32and you may look at the reference so
  316. 14:35this exercise is taken from this paper
  317. 14:44that you find in the archive
  318. 14:501 9 12.
  319. 14:54zero zero three five nine so there are
  320. 14:57more details in here that you can you
  321. 15:00can easily look at
  322. 15:02so let's introduce the model dance
  323. 15:07okay so as I say this
  324. 15:10is a model for
  325. 15:15Financial transactions
  326. 15:23so what does it mean well what it means
  327. 15:25is that as usual you have many agents
  328. 15:29or some agents
  329. 15:33and these agents want to exchange a
  330. 15:35given Financial products so they want to
  331. 15:38buy
  332. 15:40or to sell
  333. 15:42some financial asset
  334. 15:49it doesn't matter what this is so for us
  335. 15:51it will be something that they want to
  336. 15:53either buy or uh or or sell so this can
  337. 15:57be stocks
  338. 15:58bonds
  339. 16:02whatever you can think of
  340. 16:07and how do they do this well they do not
  341. 16:10exchange directly by the way they trade
  342. 16:13is by placing uh what people call an
  343. 16:16order so they
  344. 16:20place
  345. 16:22orders
  346. 16:26and an order is basically an an
  347. 16:29intention to buy or to sell something so
  348. 16:31an order is made of three things in
  349. 16:34general
  350. 16:35so one is what I will call the
  351. 16:38directions so you have to say
  352. 16:41whether you want to buy or whether you
  353. 16:43want to sell the given Financial
  354. 16:45products
  355. 16:49okay then you have to specify what is
  356. 16:52the size of your order so what is the
  357. 16:56amount of product that you want to bound
  358. 16:58to buy or sell
  359. 17:02and then you want to specify the price
  360. 17:05so
  361. 17:07in general
  362. 17:10what you say is I want to buy I don't
  363. 17:12know six units of my given financial
  364. 17:16asset at a given fixed price so you you
  365. 17:19place this order into the market and all
  366. 17:22of these orders are collected into what
  367. 17:24people call an order book
  368. 17:29okay
  369. 17:31which is just a collection of the
  370. 17:33intentions of uh of all of the agents uh
  371. 17:37as we specified in here so let me give
  372. 17:40just a sketch so this is you don't need
  373. 17:42to write this down it's just to uh to
  374. 17:45give an example of how we may think
  375. 17:46about this uh order book
  376. 17:54so let me denote the agents
  377. 17:58with I don't know symbols so there will
  378. 18:00be an agent that is a square an agent
  379. 18:03which is a circle an agent which is a
  380. 18:06triangle and so on
  381. 18:08and then let me take an axis which is
  382. 18:11the price
  383. 18:15and I divide this axis into slots
  384. 18:20okay
  385. 18:22and for each of these slots I put a
  386. 18:25symbol whenever the agent wants to buy
  387. 18:28or to sell the amount of quantity that
  388. 18:31we are thinking about at the given price
  389. 18:34which corresponds to the slot so suppose
  390. 18:36that the agent denoted with the square
  391. 18:39wants to buy something wants to buy
  392. 18:42three amounts
  393. 18:44of this asset at this price in here so I
  394. 18:48will
  395. 18:50put it here with the three squares then
  396. 18:53there is another agent that wants to buy
  397. 18:59two amounts of this thing at a lower
  398. 19:01price and then so so as you can imagine
  399. 19:05when the price is lower these are the
  400. 19:07people that want to buy
  401. 19:10they typically want to buy it at a lower
  402. 19:12price and then you will have
  403. 19:14at a higher price the people that want
  404. 19:17to sell so let's say that the guy which
  405. 19:20is the triangle wants to sell
  406. 19:24three units
  407. 19:25at this price and then there will be
  408. 19:27another one I don't know stars that
  409. 19:30wants to sell in this at this price and
  410. 19:32so on and so forth
  411. 19:34and as you see there might be a gap
  412. 19:36between
  413. 19:37best price that we
  414. 19:40've got that we saw the higher price at
  415. 19:42which people are available to buy and
  416. 19:44the best sell price so let me denote to
  417. 19:47this
  418. 19:47uh price here at a given instant of time
  419. 19:51with BT and then with the know this with
  420. 19:5480. so there might be a gap between
  421. 19:58these two quantity and this Gap is what
  422. 20:00is called uh the spread
  423. 20:02so the spread
  424. 20:06is
  425. 20:07s of T at any instant of time and it is
  426. 20:10just the difference a T minus v t
  427. 20:18okay
  428. 20:20so just one last thing about the
  429. 20:24terminology just to understand the model
  430. 20:25so this is uh discussed again in here
  431. 20:29but uh so what I'm what I've been
  432. 20:32talking about so far uh are actually
  433. 20:34called limit orders so I should add
  434. 20:39a limiting here so a limit order is when
  435. 20:42you state indeed what is your intention
  436. 20:45so you say as I said in here that you
  437. 20:47want to bound to buy a given amount at a
  438. 20:50fixed price
  439. 20:51but now there might be people that just
  440. 20:53want to bow to buy or to sell a given
  441. 20:56amount at whatever price the market
  442. 20:58chooses uh for them so there will be
  443. 21:01people that that say I really want to
  444. 21:04sell as fast as possible three units of
  445. 21:08this uh of this financial asset at the
  446. 21:13best price uh which I can at which I
  447. 21:16find people to buy and these type of
  448. 21:20orders which are executed immediately
  449. 21:22are called
  450. 21:24uh in in this financial language Market
  451. 21:30orders
  452. 21:37so this means when you place a market
  453. 21:39order what you're saying is that you
  454. 21:40want to buy or sell
  455. 21:42a given amount
  456. 21:46X
  457. 21:48immediately
  458. 21:55at any price
  459. 21:58foreign
  460. 22:02to give you the terminology of the more
  461. 22:05General models of dynamics of order
  462. 22:08books
  463. 22:09and now what we are going to do to do
  464. 22:11the exercise we are going to simplify uh
  465. 22:14the model uh quite a lot so we want to
  466. 22:18simplify it in such a way that the only
  467. 22:20thing that we care about to describe the
  468. 22:24Dynamics of the system is the spread so
  469. 22:27it is just the gap between the best sell
  470. 22:30price and the best price at which people
  471. 22:32want to buy
  472. 22:33this this particular asset so how do we
  473. 22:37simplify it so can I use that part of
  474. 22:40the Blackboard yes
  475. 22:44so we will make the following
  476. 22:46assumptions
  477. 22:52which Define our model
  478. 22:55so the first one is that
  479. 22:58the size of each order we fix it to be
  480. 23:01equal to one so in this drawing this
  481. 23:04means that each of these different agent
  482. 23:07can only buy or sell a fixed amount of
  483. 23:10of this quantity so we will have
  484. 23:13to adjust the drawing in such a way that
  485. 23:16you have only one
  486. 23:17symbol for each agent
  487. 23:19okay so please stop me if if this is not
  488. 23:23clear
  489. 23:26in the meantime I will write it so size
  490. 23:29is fixed to one
  491. 23:34then we make a second assumption that is
  492. 23:37that once one is locked in this price
  493. 23:42axis is filled and you are a new agent
  494. 23:44that wants to place another order on top
  495. 23:47of what it is already contained in the
  496. 23:49book
  497. 23:50you can only place it in front so at a
  498. 23:54higher price if you want to buy or at a
  499. 23:57lower price if you want to sell so in
  500. 23:59front of those price slots which are
  501. 24:02already occupied
  502. 24:05so
  503. 24:11once the slot is filled
  504. 24:16Place orders
  505. 24:19at only
  506. 24:24in the let's say in the
  507. 24:27let me run it in higher
  508. 24:32or lower slot
  509. 24:37okay so what this means is that the
  510. 24:40people that come first will occupy so
  511. 24:42now I ran out of symbols but let me
  512. 24:45repeat a little bit the symbols but the
  513. 24:47idea is that the people who come first
  514. 24:49will occupy already all of the slots
  515. 24:52which are
  516. 24:54lower or higher so this will be all
  517. 24:57occupied
  518. 24:59and therefore you get a model in which
  519. 25:01you essentially have no holes so you can
  520. 25:03think of this in physics language like
  521. 25:06uh like fermions so you can put only one
  522. 25:09agent at each slot they cannot pile up
  523. 25:13at the same slot and if you want to add
  524. 25:15something you have to add something
  525. 25:17either in here or in here
  526. 25:20okay
  527. 25:22and then the third assumption has to do
  528. 25:24with this Market orders that I just
  529. 25:27introduced
  530. 25:28so a market order so whenever somebody
  531. 25:32places a market order this gets executed
  532. 25:35immediately so he says or she says I
  533. 25:38want to buy at this price at this price
  534. 25:40at this price slot there is a guy that
  535. 25:43wants to sell so whenever this happens
  536. 25:45this guy sells the amount and therefore
  537. 25:47this order disappears
  538. 25:51so this means
  539. 25:52that
  540. 25:54orders
  541. 25:57are executed
  542. 26:00so you actually buy or sell
  543. 26:03only at the boundary
  544. 26:13so if you have a situation like this
  545. 26:16the idea is that you cannot buy at this
  546. 26:18price whenever you really buy and
  547. 26:21execute the order you do it at the best
  548. 26:23possible sell price
  549. 26:25so why are we introducing this uh these
  550. 26:28assumptions well because once you have
  551. 26:30this as you can easily realize the only
  552. 26:33thing that can happen so you have such a
  553. 26:35situation at a given time t
  554. 26:38you assume that now there is somebody
  555. 26:40who wants to place an order and the only
  556. 26:42thing that he or she can do is either to
  557. 26:45place an order inside the so-called
  558. 26:48spread or to cancel one of the orders
  559. 26:52which are at the boundary of the spread
  560. 26:54which means that all of the Dynamics of
  561. 26:58this type of order book is encoded into
  562. 27:00the evolution of the spread of this
  563. 27:02difference
  564. 27:04okay so I hope this was more or less
  565. 27:07clear and now we are going to write
  566. 27:09formulas so maybe it will become even
  567. 27:13more clear but if you have questions
  568. 27:14don't hesitate to stop me
  569. 27:18foreign
  570. 27:20so I think this gives a little bit of
  571. 27:22context but in essence the only thing
  572. 27:24that we have to keep in mind is that we
  573. 27:26have a model of order books where there
  574. 27:28are no holes in this price axis and
  575. 27:31everything is encoded in the Dynamics of
  576. 27:34this quantity in here
  577. 27:36okay so now that we have this assumption
  578. 27:38let's write down the model
  579. 27:41so writing on the model means that now
  580. 27:44we have to specify what is the frequency
  581. 27:47at which
  582. 27:48uh we or the agents
  583. 27:52actually Place their orders in the order
  584. 27:56books
  585. 27:59and this is where
  586. 28:01we introduce these hoax processes that
  587. 28:03we have discussed
  588. 28:07in the previous exercise
  589. 28:24okay first of all a general question on
  590. 28:26the model so we say that everything
  591. 28:28depends or is encoded in the Dynamics of
  592. 28:31the spread
  593. 28:33so now I basically saved it already in
  594. 28:35words but what are the events that
  595. 28:38decrease the spread and what are the
  596. 28:40events that increase the spread
  597. 28:43uh in the smaller
  598. 28:46and this is question one
  599. 28:49so anybody has a guess
  600. 28:58okay so we basically have just two type
  601. 29:01of events so if you execute
  602. 29:07or cancel you can even cancel
  603. 29:10an order
  604. 29:14then does the spread increase or does it
  605. 29:17decrease
  606. 29:24any guess
  607. 29:29okay so if you go back to this picture
  608. 29:31executing an order means
  609. 29:33that now I come into the order book and
  610. 29:35I say that I want to buy to buy one unit
  611. 29:37at whatever is the available price so I
  612. 29:40will buy
  613. 29:41one unit of my product that's this
  614. 29:43particular price which means that this
  615. 29:45order will be executed and if this order
  616. 29:47is executed you are enlarging as you see
  617. 29:50your spread
  618. 29:56okay
  619. 29:59whereas if you place
  620. 30:02what I call the both a limit order
  621. 30:10then as I said you have to place it in
  622. 30:13front
  623. 30:13of those which are already in there so
  624. 30:16if I say that I want to buy I will have
  625. 30:18to place myself in this
  626. 30:20slot in here and therefore I will
  627. 30:22decrease
  628. 30:24the spread
  629. 30:34okay
  630. 30:37so we have only these two type of
  631. 30:39possible events and now what we have to
  632. 30:42say is what is the frequency at which
  633. 30:45this type of events or these type of
  634. 30:48events occur
  635. 30:50and this as I said is modeled via these
  636. 30:53hoax processes so
  637. 30:55there will be a rate for the events
  638. 30:58which increase uh the spread and I will
  639. 31:00call it
  640. 31:02Lambda Plus
  641. 31:06and this will be given by
  642. 31:08a hoax process so the hoax process as as
  643. 31:13you remember
  644. 31:14gives you the intensity in terms of a
  645. 31:17self-excited kernel so there is first a
  646. 31:19term which is the so-called background
  647. 31:21intensity so this we call this mu before
  648. 31:25but now let me stick to the notation of
  649. 31:26the paper so this is a constant Lambda 0
  650. 31:29Plus
  651. 31:30and then you have the term which
  652. 31:32contains a
  653. 31:34kernel
  654. 31:36that I will write in general like this
  655. 31:39so this is a quantity which depends on
  656. 31:42time so we have Alpha
  657. 31:45so now here we go again back to this
  658. 31:47issue of notations so
  659. 31:51in the lecture Alpha was called beta and
  660. 31:53we are going to call beta what was
  661. 31:54called Alpha so forgive me for that but
  662. 31:58I think this is good because if you go
  663. 32:00back to the paper at least you have the
  664. 32:02same notation
  665. 32:03so we have this term in here where X of
  666. 32:07T well I will specify it later so this
  667. 32:10would be the linear hoax process that we
  668. 32:13have discussed already and then what we
  669. 32:14do
  670. 32:15is to add some small non-linearity which
  671. 32:19is important in here so we add a term
  672. 32:21which is proportional to Epsilon and
  673. 32:24which goes like
  674. 32:25X of t to the power of 2
  675. 32:28where what is X of T well X of T is the
  676. 32:32usual self-excited exciting kernel so
  677. 32:36this will be the integral
  678. 32:37from 0 to T
  679. 32:40in the Tau
  680. 32:42of a function Phi
  681. 32:45of T minus Tau so in the previous
  682. 32:48exercise and also later on we are going
  683. 32:50to choose this to be an exponential
  684. 32:54and then you have so let me call the S
  685. 32:58the differential Associated to this
  686. 33:01process
  687. 33:03so what d s of Tau tells you is
  688. 33:06what is the number of events that occur
  689. 33:10in a given small interval D Tau
  690. 33:13of time
  691. 33:15and I put a plus in here and what I mean
  692. 33:18is that this
  693. 33:21yes plus
  694. 33:23of tau is
  695. 33:26the maximum between the s
  696. 33:30of Tau and zero
  697. 33:32so what do I mean by this well what I
  698. 33:35mean is that the self-exciting part of
  699. 33:38the kernel is only or gets on the
  700. 33:41contribution from those events that
  701. 33:44occurs at previous times that increased
  702. 33:47the spread so if you have somebody that
  703. 33:50wants to execute an order and therefore
  704. 33:52increase this difference in here
  705. 33:56whenever this effect occur this will
  706. 33:59influence the total rate of your plus
  707. 34:04spread increasing events but if you have
  708. 34:06an event that decreases the spread so if
  709. 34:08somebody places a limit order then this
  710. 34:10has no effect into this kernel
  711. 34:14okay so this is for Lambda plus and then
  712. 34:17what about uh the others well the others
  713. 34:20in the model
  714. 34:21so the rate for uh limit orders is just
  715. 34:25taken to be a constant
  716. 34:28so it's like a it's a poisson process if
  717. 34:30you
  718. 34:31uh
  719. 34:35remember from the lecture
  720. 34:38and from
  721. 34:40homework 5.
  722. 34:44okay so this is the model in full
  723. 34:48detail
  724. 34:50the model of the paper
  725. 34:57now what are we interested in well we
  726. 35:00want to understand
  727. 35:01whether this models can gives give rise
  728. 35:05to crisis
  729. 35:07and how can we understand how this
  730. 35:10Crisis occur
  731. 35:12so that's point
  732. 35:14so this was point two of the exercise
  733. 35:19and point threes
  734. 35:26is how do we describe
  735. 35:30a crisis
  736. 35:34in this model
  737. 35:38well a crisis in this setting means that
  738. 35:42you are in a situation in which
  739. 35:44dynamically you see that your spread
  740. 35:46starts increasing and it it increases
  741. 35:49without bounds and if the spread
  742. 35:52increases
  743. 35:53this means that this difference becomes
  744. 35:55larger and larger which means that
  745. 35:56essentially you have no longer exchanges
  746. 35:59in your economy in the sense that the
  747. 36:01people that want to buy want to buy at a
  748. 36:04price which is much lower than those uh
  749. 36:06that want to sell and they people keep
  750. 36:09canceling their order or executing their
  751. 36:12order and therefore there are no longer
  752. 36:14exchanges and and this is how you uh
  753. 36:17interpret that Uprising is occurring so
  754. 36:20more formally what this means is that X
  755. 36:22of t
  756. 36:24becomes
  757. 36:29infinite
  758. 36:31infinite time
  759. 36:42which means basically that you start
  760. 36:44having an explosion of the events that
  761. 36:46are increasing the spread
  762. 36:49okay now in the usual linear case so let
  763. 36:54me just add this comment when Epsilon is
  764. 36:57equal to zero we know one way
  765. 36:59to generate a crisis
  766. 37:01so let's forget about Lambda minus so if
  767. 37:04we have just a hoax process we know what
  768. 37:07is the limit in which the number of
  769. 37:08events is exploding
  770. 37:11and this is
  771. 37:13the case in which if you remember
  772. 37:16this parameter Alpha was going to one
  773. 37:25so the problem is well defined whenever
  774. 37:27Alpha is smaller than one if Phi is
  775. 37:30normalized to one
  776. 37:31and as you increase Alpha and you get
  777. 37:34closer and closer to one the process
  778. 37:35becomes unbounded and this is encoded in
  779. 37:38the fact that X of T explodes so this is
  780. 37:42something that of course already in the
  781. 37:44linear case and now in here we are going
  782. 37:46to see another way in which a crisis can
  783. 37:48occur which is instead due to the
  784. 37:50presence of this non-linearity and which
  785. 37:53is related to this idea of metastability
  786. 37:58okay so let's do this so this was a
  787. 38:02little bit an introduction to the model
  788. 38:04and how to actually uh do the proper
  789. 38:08calculation
  790. 38:09let's simplify it further
  791. 38:13so what we do from now on is forget
  792. 38:15about the events that decrease the
  793. 38:19spread so I will put this Lambda 0 minus
  794. 38:23exactly equal to zero so after all we
  795. 38:26are interested into this scenario of
  796. 38:27Crisis so we only want to care about the
  797. 38:30events which increase the spread so I
  798. 38:33just simplify the Dynamics I set this to
  799. 38:35zero and then I will denote the Lambda
  800. 38:38plus simply by Lambda so I forget about
  801. 38:42so the Lambda t plus
  802. 38:45let me simply call it Lambda t
  803. 38:47so in the end we are going to focus on
  804. 38:50this non-linear hoax process and
  805. 38:54see what's going on
  806. 38:58yes
  807. 39:12yes
  808. 39:16so the question is that in here I should
  809. 39:19add so the idea is that you can
  810. 39:22only place orders if you have a spread
  811. 39:27which is non-zero
  812. 39:29so if in this drawing
  813. 39:32you are in a situation in which these
  814. 39:34two somehow collapse then there is no
  815. 39:36space to place any further order in
  816. 39:38there
  817. 39:44yes so you're asking why I don't put one
  818. 39:47if we yes okay so that depends on
  819. 39:50whether
  820. 39:52so what since they cannot overlap so I
  821. 39:55execute
  822. 39:56the order if I have a guy in here that
  823. 39:58wants to buy and the guy in here wants
  824. 39:59to sell them this they match I consider
  825. 40:02it in this way so the question for those
  826. 40:04who uh didn't listen
  827. 40:07is the following so in the text indeed I
  828. 40:09forgot that here you should put an
  829. 40:10indicator function
  830. 40:12that asks you that at the given time
  831. 40:15the spread is larger or equal to two
  832. 40:18because if the spread is equal to 1 so
  833. 40:21this means in our drawing
  834. 40:25that these are the people that want to
  835. 40:27buy and I have a guy in here these are
  836. 40:29the people that want to sell
  837. 40:31and I have a guy in here so yes okay
  838. 40:37so in here in principle
  839. 40:40yeah this is a little bit of a choice so
  840. 40:42in principle you could place an order in
  841. 40:44here
  842. 40:45and then execute this and this will give
  843. 40:48you immediately
  844. 40:49an event which is opening so we want to
  845. 40:52forget about this so we just ask
  846. 40:55that you have at least two slots so that
  847. 40:58if the guy puts an event in here you're
  848. 41:01really decreasing the spread and you're
  849. 41:03not executing directly
  850. 41:05so there is this a little caveat in here
  851. 41:09thanks for
  852. 41:19yes exactly so so the question is
  853. 41:22why do we include
  854. 41:25this self-exciting Dynamics in here well
  855. 41:28I think that one way to think about this
  856. 41:30is that
  857. 41:32uh if you have some stocks or bonds and
  858. 41:36you start so there is some sort of uh
  859. 41:39they say Dynamics which depends on what
  860. 41:41the other people are doing which is
  861. 41:43encoded in here so the idea would be
  862. 41:45that if you see that many people uh are
  863. 41:48selling the stocks that they have
  864. 41:51because there is no longer Trust on
  865. 41:54on the company or on whatever is
  866. 41:56associated with the stocks then you are
  867. 41:58also pushed to sell and this is why uh
  868. 42:00or to execute very fast your orders and
  869. 42:03this is why you self-excite these type
  870. 42:06of processes
  871. 42:08okay
  872. 42:10people online please also stop me
  873. 42:13if something is not clear
  874. 42:16okay
  875. 42:19okay so this was all basically
  876. 42:20introduction to the model and now let's
  877. 42:22go to the actual mass
  878. 42:25well it's not enough
  879. 42:28and this is exercise three I think
  880. 42:56foreign
  881. 43:08so now we have let me rewrite the
  882. 43:11process without the Plus
  883. 43:13we have this nonlinear box process
  884. 43:17D plus Epsilon XF Square
  885. 43:22X of t
  886. 43:27is my kernel
  887. 43:30the answer file so that's the
  888. 43:33differential of the process and as usual
  889. 43:36we are going to make the
  890. 43:38Simple Choice for our kernel which is
  891. 43:40the exponential so we choose V of T to
  892. 43:43be
  893. 43:44beta e to the minus
  894. 43:47beta t as we did in the linear case
  895. 43:50in the exercise of last time
  896. 43:53okay so the first point
  897. 44:00of these exercises to write down
  898. 44:02an equation for our
  899. 44:05dynamical variable X of t
  900. 44:08and the starting point is as follows so
  901. 44:11we are going to assume so this is
  902. 44:14something that you can do rigorously but
  903. 44:16I'm not going to do it uh in here but
  904. 44:19what we are going to assume is that beta
  905. 44:21which controls the decay of your kernel
  906. 44:24is small
  907. 44:28so whenever you say small you have to
  908. 44:30specify with respect to what so in our
  909. 44:32case it would be for instance small with
  910. 44:35respect to
  911. 44:37lambda zero
  912. 44:39okay which in words means that your
  913. 44:43kernel is slowly varying in time so if
  914. 44:47if beta is small at least for for the
  915. 44:50smaller times or for a window of time
  916. 44:52which becomes larger this will be equal
  917. 44:55to a constant or roughly equal to a
  918. 44:57constant beta and whenever you are in
  919. 44:59this situation what you can show is that
  920. 45:01you can simplify the Dynamics of your
  921. 45:05process so let me write it you can
  922. 45:08assume that the Dynamics of your process
  923. 45:10is given by adrift that is simply given
  924. 45:14by lambdarti and a variance or a noise
  925. 45:17which has a strength which is of the
  926. 45:19order of square root of Lambda T so I
  927. 45:21will write it and then I will comment
  928. 45:24so the assumption is that
  929. 45:27you can use that
  930. 45:29your Dynamics
  931. 45:32vs of t
  932. 45:35looks like this so you have a Lambda t
  933. 45:38DT
  934. 45:40and then you have a nice term
  935. 45:43foreign
  936. 45:50T I always put it as a subscript in here
  937. 45:53but
  938. 45:54it's just a notation so ETA of T DT
  939. 45:56where ETA is the usual white noise
  940. 46:00so what this means so if you if you
  941. 46:02imagine that Lambda is constant then you
  942. 46:04will have a poisson process and for the
  943. 46:06poisson process you know that this would
  944. 46:09be true so this is telling you that the
  945. 46:11average of your process is Lambda and
  946. 46:14the variance of your process is Lambda
  947. 46:16again these are precisely properties of
  948. 46:19your poisson process so this is like a
  949. 46:22poisson
  950. 46:24it has the same structure
  951. 46:29of a poisson process
  952. 46:31but now you have still this dependence
  953. 46:34on time in your uh in your rate Lambda
  954. 46:37of t
  955. 46:38and this is something that as I said you
  956. 46:41can argue more rigorously using the fact
  957. 46:44that beta is sufficiently small so that
  958. 46:46your kernel varies does not very very uh
  959. 46:50very fast
  960. 46:52okay so once we have this then we can
  961. 46:54try to compute an equation for
  962. 46:58the changes in time of our variable X of
  963. 47:01T so remember that to characterize
  964. 47:03crisis we want to check whether X can go
  965. 47:05to Infinity so let's look at what is the
  966. 47:08Dynamics of X of t
  967. 47:11so let me write the differential of X of
  968. 47:14T So to compute the differential I have
  969. 47:15to take the derivative of this object
  970. 47:18with respect to time
  971. 47:20so time appears twice it appears as an
  972. 47:24extreme
  973. 47:25of the integration and it appears inside
  974. 47:27of the kernel so if I first take the
  975. 47:30derivative with respect to the extremum
  976. 47:33this means that I have to compute
  977. 47:35whatever is inside precisely at the
  978. 47:39value Tau equal to T
  979. 47:41and if I do this my kernel simplifies
  980. 47:44because the exponential of Tau minus tau
  981. 47:47is is equal to one so this first term
  982. 47:50will give me a contribution which is
  983. 47:52beta
  984. 47:53times
  985. 47:54BS of t
  986. 47:59and then I have a second contribution
  987. 48:00which comes from deriving inside the the
  988. 48:04Integra so I have to take the derivative
  989. 48:06of the kernel and this will bring me
  990. 48:07down a factor of minus beta
  991. 48:10so I will have
  992. 48:13from here minus beta times
  993. 48:16again the integral
  994. 48:19from 0 to T
  995. 48:21of
  996. 48:22uh now I write it
  997. 48:26so okay
  998. 48:28e to the minus beta
  999. 48:31T minus Tau d s of Tau
  1000. 48:33okay
  1001. 48:39and if I
  1002. 48:41look at my definition of X of T then
  1003. 48:43what I recognize is that this is
  1004. 48:45precisely
  1005. 48:46wait I forgot a DT because now I'm
  1006. 48:49looking
  1007. 48:50at the differential
  1008. 48:53so I have a DT in here
  1009. 48:56and this closes the parenthesis
  1010. 48:59so again this is the derivative with
  1011. 49:00respect to the extremum and this is the
  1012. 49:02derivative inside the integration and
  1013. 49:04what is this quantity in here well this
  1014. 49:07is just
  1015. 49:08my original X of tip
  1016. 49:12foreign
  1017. 49:15because of how we defined it
  1018. 49:19okay
  1019. 49:20and in here I have this the S but yes I
  1020. 49:24just told you
  1021. 49:27what is the form of the differential for
  1022. 49:29the S so what I can do is to plug this
  1023. 49:32expression inside here and use the
  1024. 49:35explicit expression for Lambda which
  1025. 49:37appears here and here
  1026. 49:39so
  1027. 49:43let's do it in here
  1028. 49:45and I hope that you can see
  1029. 49:48yes
  1030. 49:49where does the two less Expressions come
  1031. 49:51from
  1032. 49:52this one
  1033. 49:55yes and the one above
  1034. 49:57okay so this one is something that we
  1035. 50:00are not proving
  1036. 50:02it is let's say an assumption and if you
  1037. 50:05really want to prove this it takes a
  1038. 50:07little bit of work but what you have to
  1039. 50:08use is that you're you're assuming that
  1040. 50:11the parameter beta which controls how
  1041. 50:14fast your kernel is decaying you're
  1042. 50:16assuming that this is small so that the
  1043. 50:19kernel decays uh slower and under this
  1044. 50:23assumption you can argue that the
  1045. 50:26equation for your process so this is
  1046. 50:29what gives you the number of events that
  1047. 50:31you expect to occur in a given interval
  1048. 50:33DP
  1049. 50:34this can be written in the following way
  1050. 50:37so it has a drift term which is
  1051. 50:39proportional to your excitation rate
  1052. 50:42which is Lambda plus and then it has
  1053. 50:45some noise which is proportional to uh
  1054. 50:47to the square root of this excitation
  1055. 50:49rate and the way you can motivate this
  1056. 50:51is having in mind a person process so
  1057. 50:54the person process would be the case in
  1058. 50:56which Alpha is equal to zero and Epsilon
  1059. 50:58is equal to zero
  1060. 50:59and in that case you know that the
  1061. 51:01number of events in a small interval of
  1062. 51:03time DT is poisson distributed so being
  1063. 51:07poisson distributed means that your
  1064. 51:09average is equal to Lambda 0 and your
  1065. 51:13variance so the sigma square is again
  1066. 51:16equal to Lambda and this is what is
  1067. 51:19encoded in here so in our case we do not
  1068. 51:21have really a person process but we are
  1069. 51:23somehow assuming that this Lambda of T
  1070. 51:27changes very slowly so we can kind of
  1071. 51:29think at it as a constant and this is
  1072. 51:31why eventually you get out this
  1073. 51:34expression in here but this way we we
  1074. 51:36are not proving this let's say this is
  1075. 51:38uh what we are assuming and once we
  1076. 51:42assume this then we can write down an
  1077. 51:45equation for the X
  1078. 51:47so where does this come from now so you
  1079. 51:50I want to write a differential for this
  1080. 51:52quantity X of T is given in here so what
  1081. 51:55I have to do so I could I could write
  1082. 51:58directly the derivative
  1083. 52:01over time and now I'm writing it in the
  1084. 52:03differential form but you see that if I
  1085. 52:05take the derivative over time of this
  1086. 52:06expression
  1087. 52:08I have that the time appears both in
  1088. 52:11here and appears inside the kernel so
  1089. 52:13when I derive I have two contributions
  1090. 52:16so the first contribution comes from
  1091. 52:17evaluated the integrand the into the the
  1092. 52:20quantity which is inside the integral at
  1093. 52:22the time t
  1094. 52:24and this is this quantity in here right
  1095. 52:26because if you evaluate the kernel at
  1096. 52:29the time Tau equal to T then this is
  1097. 52:33like evaluating Phi at 0 so you get a
  1098. 52:36factor of beta and then this DS of time
  1099. 52:39of Tau becomes the S of T okay
  1100. 52:43and then the second contribution to the
  1101. 52:45derivative I keep the integral as it is
  1102. 52:47and I take the derivative of the kernel
  1103. 52:50itself with respect to T
  1104. 52:53and this is the expression that you see
  1105. 52:55in here
  1106. 52:58so if I derive this with respect to P I
  1107. 53:01get a factor of minus beta that I am
  1108. 53:03collecting outside with a minus sign and
  1109. 53:06then the rest I recognize that it is
  1110. 53:08just X of T is it here
  1111. 53:11yes
  1112. 53:13okay great
  1113. 53:16okay so now
  1114. 53:18let's try to write this in a way which
  1115. 53:21is cleaner so I have this beta
  1116. 53:26then I plug the expression for the uh
  1117. 53:28the S of T and I plug the expression for
  1118. 53:31Lambda itself so let me try to collect
  1119. 53:34everything so I have a Lambda 0
  1120. 53:38DT
  1121. 53:41let's do this I have a Lambda 0 plus
  1122. 53:43alpha x t
  1123. 53:46DT
  1124. 53:50which comes from here then I have the
  1125. 53:52noise so the the ah sorry I forgot the
  1126. 53:54Epsilon
  1127. 53:57plus Epsilon
  1128. 53:59XP Square Times VT the noise I will
  1129. 54:03write it as a last contribution let me
  1130. 54:06write this so then I have minus beta
  1131. 54:10sorry the beta minus X of t
  1132. 54:13times DT
  1133. 54:15and then I have the noise which is
  1134. 54:18encoded in here which was square root of
  1135. 54:20Lambda so I will write it as plus square
  1136. 54:24root of Lambda t
  1137. 54:26e times T DT
  1138. 54:31okay
  1139. 54:35and now that I have this so now you see
  1140. 54:37that this is uh
  1141. 54:39now a closed equation for x
  1142. 54:42so let me try to rewrite it in the way
  1143. 54:45we wrote the language of an equation
  1144. 54:48before
  1145. 54:50so
  1146. 54:56let me try to write it
  1147. 54:58now I divide by the T if you want so I I
  1148. 55:01run I want DX
  1149. 55:04T over DT
  1150. 55:09so let's
  1151. 55:11collect everything so I have a Lambda 0
  1152. 55:14beta
  1153. 55:17foreign
  1154. 55:22term
  1155. 55:24so there is a factor of beta always in
  1156. 55:27front and the linear term is Alpha minus
  1157. 55:30one so this is minus
  1158. 55:331 minus Alpha times beta X of t
  1159. 55:37then I have the non-linearity beta
  1160. 55:39Epsilon X of T Square
  1161. 55:43and then I add the noise
  1162. 55:46plus beta square root of Lambda t e
  1163. 55:50times t
  1164. 55:51okay
  1165. 55:54and now what I want to do
  1166. 55:56as before
  1167. 55:58is to write this quantity in here
  1168. 56:02as the derivative of sample tension so
  1169. 56:05as minus
  1170. 56:07the derivative of some potential that I
  1171. 56:09call V
  1172. 56:11which depends on x
  1173. 56:13derivative with respect to X evaluated
  1174. 56:17to x equal to my dynamical variable X of
  1175. 56:21t
  1176. 56:22so this will be the gradient descent
  1177. 56:25term and then we will have a nice term
  1178. 56:26as it was done in the case of the
  1179. 56:29magnetization in the lecture
  1180. 56:32so what is the potential well what I
  1181. 56:34have to do to recover
  1182. 56:36the potential is so this is minus its
  1183. 56:39derivative so I have to integrate this
  1184. 56:42expression with respect to X to X
  1185. 56:45all right so I will have
  1186. 56:47well a minus sign in front
  1187. 56:52integrated with respect to X will give
  1188. 56:54me Lambda 0 beta X
  1189. 56:58then I have something that is linear so
  1190. 57:02the integral
  1191. 57:03will be x square over 2.
  1192. 57:07and then I have the quadratic term which
  1193. 57:10will give me
  1194. 57:13x cubed over 3.
  1195. 57:17so if I now take minus the derivative of
  1196. 57:20this object I recover what I have in the
  1197. 57:22right hand side
  1198. 57:39uh you mean that ah yes because I killed
  1199. 57:43all the events which
  1200. 57:46decrease the spread by setting Lambda 0
  1201. 57:49minus to zero so the question is uh why
  1202. 57:53don't I put in here the constraint or it
  1203. 57:56was actually inside the x that BS is
  1204. 57:59actually the S Plus so it counts only
  1205. 58:01the
  1206. 58:02spread increasing events and the reason
  1207. 58:05is that to simplify the model I kill the
  1208. 58:07rate at which the spread decreasing
  1209. 58:09event support so I set Lambda 0 minus to
  1210. 58:13zero
  1211. 58:14so all of the events which occur are
  1212. 58:17those that increase the spread
  1213. 58:19so my DS coincides with
  1214. 58:22with Ds Plus
  1215. 58:24for uh
  1216. 58:26pointing out
  1217. 58:28okay so now this is our potential which
  1218. 58:32depends on our non-linearity Epsilon
  1219. 58:36and now to try to understand the
  1220. 58:39Dynamics what you have to do is to study
  1221. 58:40what we have to do is to study this
  1222. 58:42potential so let me rewrite it
  1223. 58:46a little bit so let me write this as
  1224. 58:50beta
  1225. 58:521 minus Alpha over two
  1226. 58:55and then I want to
  1227. 58:57compose these two terms in such a way it
  1228. 58:59was Global Square so I will write it as
  1229. 59:03x minus
  1230. 59:05Lambda 0 over
  1231. 59:07one minus Alpha Square
  1232. 59:11so if I take x square I recover this
  1233. 59:14if I take the double product I recover
  1234. 59:17the linear term
  1235. 59:19and then I have a console a global
  1236. 59:22constant which I have added that I will
  1237. 59:24need to subtract so false
  1238. 59:29oops
  1239. 59:30the cubic term and then let me subtract
  1240. 59:34the remaining term which I just added so
  1241. 59:36this will be Lambda 0 square beta
  1242. 59:39uh divided by two one minus Alpha but
  1243. 59:43this we don't really care about it
  1244. 59:44because it's just a global shift the
  1245. 59:46concept
  1246. 59:48that will not
  1247. 59:50matter when we look at the shape of the
  1248. 59:52potential
  1249. 59:57very good
  1250. 1:00:00okay
  1251. 1:00:04okay so let's study this
  1252. 1:00:09and let's start from
  1253. 1:00:11Epsilon equal to zero where we go back
  1254. 1:00:14to our linear hoax
  1255. 1:00:29so I will forget about the
  1256. 1:00:32oops the constant term
  1257. 1:00:37that doesn't really matter so in the
  1258. 1:00:38case of sine equal to zero then the
  1259. 1:00:40shape of our potential is simple
  1260. 1:00:42because I'm killing the cubic term and I
  1261. 1:00:46just have essentially a parabola so if I
  1262. 1:00:49plot
  1263. 1:00:51the Epsilon equal to zero
  1264. 1:00:54of x
  1265. 1:00:57plus the constant
  1266. 1:00:59Lambda 0 square beta over 2 1 minus
  1267. 1:01:02Alpha
  1268. 1:01:04then I have a parabola and the center of
  1269. 1:01:07the parabolize a quantity that you might
  1270. 1:01:09recognize
  1271. 1:01:12it is Lambda 0 divided by y minus Alpha
  1272. 1:01:16so my potential will look like this
  1273. 1:01:19okay
  1274. 1:01:21and so
  1275. 1:01:24is there anybody who recognizes what was
  1276. 1:01:26this expression
  1277. 1:01:28for the linear hoax process so I'm
  1278. 1:01:31changing the notation so maybe that's a
  1279. 1:01:33bit
  1280. 1:01:34so that was in the exercise of last time
  1281. 1:01:37that was mu
  1282. 1:01:39over one minus beta
  1283. 1:01:42but anyway if if you go back to that
  1284. 1:01:45notation you will recognize that this is
  1285. 1:01:47the average intensity of uh the uh of
  1286. 1:01:52the linear hoax process so this was uh
  1287. 1:01:56if you want the average
  1288. 1:02:00sorry
  1289. 1:02:04in this notation
  1290. 1:02:07it was the average of the S of T
  1291. 1:02:09actually
  1292. 1:02:19okay
  1293. 1:02:22which was also the stationary values so
  1294. 1:02:24there were if you recall if you remember
  1295. 1:02:27there was a discussion about the process
  1296. 1:02:29being stationary for Alpha smaller than
  1297. 1:02:31one so the value at which this rate
  1298. 1:02:34eventually converges was given precisely
  1299. 1:02:39or was related to this expression in
  1300. 1:02:42here and this is this is good because
  1301. 1:02:45what we recover with this potential
  1302. 1:02:48description is precisely this so in here
  1303. 1:02:50if you think at the process in terms of
  1304. 1:02:53this language Dynamics then what do we
  1305. 1:02:55expect to happen well you have just one
  1306. 1:02:57minimum
  1307. 1:02:57so your Dynamics will have some noise
  1308. 1:02:59will descend because of the gradient
  1309. 1:03:03term and eventually it will relax into
  1310. 1:03:06this unique uh this unique minimum that
  1311. 1:03:10is what will govern your your stationary
  1312. 1:03:14state so if you ask what will be the
  1313. 1:03:16stationary value of my X of t
  1314. 1:03:20then this because of uh
  1315. 1:03:24ergodicity if you want this will be
  1316. 1:03:27given by
  1317. 1:03:29so I'm just
  1318. 1:03:33this is just a definition then remember
  1319. 1:03:35that you have here this vs of Tau so at
  1320. 1:03:39very large time you expect that this
  1321. 1:03:41converges to to the average of this
  1322. 1:03:44quantity and if you take the average
  1323. 1:03:47what you have to average is this DS
  1324. 1:03:54and if this average of the S converges
  1325. 1:03:57to this quantity in here using then you
  1326. 1:04:01the this is independent of time you
  1327. 1:04:03bring it out of the integral the kernel
  1328. 1:04:05is normalized so what you get is
  1329. 1:04:07precisely that the long time limit of
  1330. 1:04:09your value of x coincides with with this
  1331. 1:04:12expression in here that we had already
  1332. 1:04:13computed so this is consistent with our
  1333. 1:04:17previous analysis of the linear hoax
  1334. 1:04:20case
  1335. 1:04:21but now if you add uh Epsilon which is
  1336. 1:04:24positive of course this picture will
  1337. 1:04:26change
  1338. 1:04:28and it will change because if you add
  1339. 1:04:30some non-linearity there are
  1340. 1:04:33more stationary points of your potential
  1341. 1:04:36which appear so let's compute them
  1342. 1:04:39so now let's
  1343. 1:04:42look at Epsilon larger than zero
  1344. 1:04:47so how does one compute the stationary
  1345. 1:04:49points of the potential well what you
  1346. 1:04:51have to do so stationary points are the
  1347. 1:04:53Minima or or the maximum
  1348. 1:04:55so to compute them what you have to do
  1349. 1:04:57is to take the derivative and set it to
  1350. 1:05:00zero so the derivative we have it in
  1351. 1:05:02here
  1352. 1:05:04up to the minus sign so we have to
  1353. 1:05:07compute those values of X where this
  1354. 1:05:09expression is equal to zero so this is a
  1355. 1:05:12quadratic equation for x
  1356. 1:05:14that we can solve so let me just give
  1357. 1:05:17you
  1358. 1:05:18being it quadratic it will have two
  1359. 1:05:20solutions
  1360. 1:05:22so let me give I have a two solution
  1361. 1:05:26directly so this will be 1 minus Alpha
  1362. 1:05:30plus minus
  1363. 1:05:32square root of 1 minus Alpha Square so
  1364. 1:05:35the beta simplifies
  1365. 1:05:38and you get something like this
  1366. 1:05:44okay
  1367. 1:05:48so these points will be stationary
  1368. 1:05:51meaning that they are either Maxima or
  1369. 1:05:54or Minima
  1370. 1:05:56and now what should you do to understand
  1371. 1:05:59which one is the maximum and which is
  1372. 1:06:01the minimum
  1373. 1:06:02and yes
  1374. 1:06:11so in general the way in which you
  1375. 1:06:14distinguish whether you are in a minimum
  1376. 1:06:16or in a maximum is to look at the second
  1377. 1:06:18derivative right so if the second
  1378. 1:06:20derivative is positive you are in a
  1379. 1:06:21minimum if the second derivative is
  1380. 1:06:23negative you are in a maximum
  1381. 1:06:26now here you can compute the second
  1382. 1:06:27derivative and check the sign when you
  1383. 1:06:30evaluate it at this point but let's do a
  1384. 1:06:33shortcut so what is the shortcut well is
  1385. 1:06:37to understand
  1386. 1:06:41is to use what we already know
  1387. 1:06:44from Epsilon equal to zero
  1388. 1:06:49and to guess what is then the shape of
  1389. 1:06:51the potential for Epsilon different from
  1390. 1:06:53zero
  1391. 1:06:55so this will be now v e of X Epsilon
  1392. 1:06:59plus the constant
  1393. 1:07:01so before this was a minimum now we
  1394. 1:07:04switch on Epsilon so first of all
  1395. 1:07:08as you see if you take X which is very
  1396. 1:07:11very large
  1397. 1:07:13the term which dominates in this
  1398. 1:07:15expression will be the cubic term that
  1399. 1:07:17has quite importantly the minus sign in
  1400. 1:07:21front so this is telling you is that 4X
  1401. 1:07:24very very large this potential will
  1402. 1:07:27Decay like minus X cubed
  1403. 1:07:31in here
  1404. 1:07:33and then you know that you have two
  1405. 1:07:35stationary points so it is quite easy to
  1406. 1:07:38expect if you study the behavior at x
  1407. 1:07:40equal to zero you will find something
  1408. 1:07:42like this so it is easy to expect that
  1409. 1:07:44your potential will have some shape like
  1410. 1:07:46this
  1411. 1:07:48with a minimum and then a maximum that
  1412. 1:07:51allows you then to Decay to minus
  1413. 1:07:53infinity
  1414. 1:07:55so we have to understand which one is x
  1415. 1:07:57minus and which one is X Plus
  1416. 1:07:59and a fast way to do this is to
  1417. 1:08:04try to look at the behavior of this
  1418. 1:08:08quantity when Epsilon is small because
  1419. 1:08:09we know that when Epsilon is zero the
  1420. 1:08:12minimum will collapse to lambda zero
  1421. 1:08:15divided by 1 minus Alpha so let's expand
  1422. 1:08:19this two terms
  1423. 1:08:21these two points for small Epsilon
  1424. 1:08:26so if I look
  1425. 1:08:28at the term with a plus
  1426. 1:08:31when Epsilon is zero I can kill this
  1427. 1:08:34term inside the square root I just have
  1428. 1:08:361 minus Alpha to the power of 2 it's
  1429. 1:08:40square root so this quantity is positive
  1430. 1:08:42so it's just 1 minus Alpha I have a plus
  1431. 1:08:45so I have twice 1 minus Alpha divided by
  1432. 1:08:48Epsilon so this will go
  1433. 1:08:50when Epsilon is very small
  1434. 1:08:53like one minus Alpha
  1435. 1:08:56over Epsilon
  1436. 1:08:59and this is X Plus
  1437. 1:09:02whereas if I look at x minus and I do
  1438. 1:09:05the expansion
  1439. 1:09:08I have to be a little bit more careful
  1440. 1:09:10because
  1441. 1:09:11then the order one terms will cancel
  1442. 1:09:14because I have a minus so I have to keep
  1443. 1:09:17also the expansion toward the Epsilon
  1444. 1:09:19that comes from expanding the square
  1445. 1:09:21root
  1446. 1:09:22okay and if I do this so this is
  1447. 1:09:27you you can do it for money so this will
  1448. 1:09:30be one minus Alpha I just look at the
  1449. 1:09:32numerator now
  1450. 1:09:33plus minus
  1451. 1:09:361 minus Alpha so I bring 1 minus Alpha
  1452. 1:09:39outside the square root and then I have
  1453. 1:09:411 minus 4 Epsilon Lambda 0 divided by
  1454. 1:09:451 minus Alpha Square
  1455. 1:09:48and then if Epsilon is small I can
  1456. 1:09:50expand this square root so this is 1
  1457. 1:09:53minus x to the power one alpha and the
  1458. 1:09:55expansion for X being small is so this
  1459. 1:09:59will be the expansion of this is 1 minus
  1460. 1:10:01one alpha times x
  1461. 1:10:04as you can check so if you do this
  1462. 1:10:07in the limit
  1463. 1:10:09Epsilon being small you find that this
  1464. 1:10:12is precisely
  1465. 1:10:13Lambda 0 over 1 minus Alpha plus terms
  1466. 1:10:17which are of order of Epsilon whereas in
  1467. 1:10:20here you have plus terms which are
  1468. 1:10:22ordered one
  1469. 1:10:25so this is to say that by continuity in
  1470. 1:10:28epsilon we expect that the point which
  1471. 1:10:30is the minimum is x minus so this here
  1472. 1:10:34will be x minus
  1473. 1:10:37that when we switch Epsilon to zero
  1474. 1:10:40we'll collapse to this point in here
  1475. 1:10:43whereas the new stationary point that we
  1476. 1:10:46have
  1477. 1:10:47is X Plus
  1478. 1:10:49which as you see is is very far away if
  1479. 1:10:52Epsilon is small because it is of the
  1480. 1:10:54order of 1 minus
  1481. 1:10:56Alpha divided by Epsilon
  1482. 1:11:00okay
  1483. 1:11:03so this tells you that in the limit
  1484. 1:11:06Epsilon going to zero this goes to
  1485. 1:11:09infinity and you recover this picture
  1486. 1:11:11with a unique uh with a unique minimum
  1487. 1:11:16okay so the last thing that we need uh
  1488. 1:11:19to to understand the Dynamics is then to
  1489. 1:11:21compute the barrier
  1490. 1:11:23and the battery is a measure so you what
  1491. 1:11:26we can do is to compute then the value
  1492. 1:11:28of the potential at this
  1493. 1:11:31local maximum that tells you uh so if
  1494. 1:11:34you shift the potential this is actually
  1495. 1:11:36zero so it tells you what is the barrier
  1496. 1:11:38B what is uh the difference in potential
  1497. 1:11:40that you have to overcome with this type
  1498. 1:11:42of jumps or activated processes
  1499. 1:11:46so this means that we want to compute V
  1500. 1:11:51evaluated at X Plus
  1501. 1:11:54so this is algebra it's a you you can do
  1502. 1:11:57it so let me go a little bit fast I will
  1503. 1:11:59expand it so this is
  1504. 1:12:02no I don't expand it this is exact
  1505. 1:12:07ly if you do the math you will find that
  1506. 1:12:09this barrier goes like
  1507. 1:12:11one over Epsilon Square
  1508. 1:12:17so when Epsilon is small this point is
  1509. 1:12:19very very uh
  1510. 1:12:21up this is very very large and very very
  1511. 1:12:24far away
  1512. 1:12:25so this barrier here
  1513. 1:12:28Delta V is of the order of one over
  1514. 1:12:30Epsilon Square
  1515. 1:12:33and so again what happens you take
  1516. 1:12:35Epsilon going to zero this X Plus goes
  1517. 1:12:38to Infinity the barrier shoots up and
  1518. 1:12:41you recover as you see the the nice
  1519. 1:12:43Parabola that we had before
  1520. 1:12:47okay so this is the potential and now
  1521. 1:12:49that we have uh the potential we can ask
  1522. 1:12:53this question about Activation so in a
  1523. 1:12:56similar way as for the double well of of
  1524. 1:12:59the magnetization of the easing we can
  1525. 1:13:02imagine that the Dynamics if you start
  1526. 1:13:04from somewhere within the Basin of
  1527. 1:13:05Attraction of x minus will relax
  1528. 1:13:08in this metastable state but then there
  1529. 1:13:10will be very rare activated
  1530. 1:13:15processes that kick you up across this
  1531. 1:13:20barrier and once you go across this
  1532. 1:13:23barrier then you start rolling down
  1533. 1:13:26because from where on the potential goes
  1534. 1:13:28to minus infinity and therefore if you
  1535. 1:13:30manage to kick this barrier then you go
  1536. 1:13:35into this scenario in which you have a
  1537. 1:13:37crisis of your economy or of of your
  1538. 1:13:40financial exchanges that if you remember
  1539. 1:13:42was defined by X exploding and uh and
  1540. 1:13:48going to Infinity
  1541. 1:13:51so how often does this happen
  1542. 1:13:55well
  1543. 1:13:57we can use
  1544. 1:13:59results
  1545. 1:14:01in the literature to compute what is the
  1546. 1:14:03average time that is required to see
  1547. 1:14:06this type of jump events
  1548. 1:14:12and there are explicit expressions for
  1549. 1:14:14this
  1550. 1:14:18and
  1551. 1:14:19for this particular example
  1552. 1:14:23the expression for the time is given
  1553. 1:14:28in full detail
  1554. 1:14:30in the text of the today
  1555. 1:14:37so this is now 0.3
  1556. 1:14:43okay so if you if you look at there
  1557. 1:14:47what you see is that you can write down
  1558. 1:14:49what is the average time for this
  1559. 1:14:51activity jumps
  1560. 1:14:53which will be given by a pre-factor that
  1561. 1:14:55I just call a I'm not going to rewrite
  1562. 1:14:57it so that is the square root that you
  1563. 1:14:59see in the text
  1564. 1:15:01and then you have the exponential
  1565. 1:15:04that is what we want to compute
  1566. 1:15:08of what of an integral so the integral
  1567. 1:15:10goes from so in the text I wrote X
  1568. 1:15:14equilibrium and X star so what I mean by
  1569. 1:15:16this
  1570. 1:15:18X equilibrium is x minus is our
  1571. 1:15:20metastable minimum and F star is is the
  1572. 1:15:23point where you at the barrier so
  1573. 1:15:26let me call it x minus
  1574. 1:15:29NX Plus in DX
  1575. 1:15:33and then you have a ratio so you have
  1576. 1:15:35the ratio between the derivative
  1577. 1:15:37of your potential V Prime of x
  1578. 1:15:40and another quantity that is called d of
  1579. 1:15:43x
  1580. 1:15:45that if you look at it you will
  1581. 1:15:47recognize that it is basically
  1582. 1:15:51the variance of the noise of our lunch
  1583. 1:15:53event process so D of X is
  1584. 1:15:57B squared over 2
  1585. 1:16:01Lambda 0 plus alpha x square
  1586. 1:16:04sorry X
  1587. 1:16:06Plus
  1588. 1:16:08Epsilon s x square
  1589. 1:16:12so this was basically Lambda T and if
  1590. 1:16:15you look at your language
  1591. 1:16:18in here
  1592. 1:16:21it is basically the square of this
  1593. 1:16:24expression so it is the variance of the
  1594. 1:16:25noise
  1595. 1:16:27foreign
  1596. 1:16:30this time what we have to do is to
  1597. 1:16:32compute the this integral which is at
  1598. 1:16:36the exponent so
  1599. 1:16:38this is a little bit lengthy so I will
  1600. 1:16:40not do it in detail but you find it in
  1601. 1:16:43the solution maybe I will just give you
  1602. 1:16:45uh
  1603. 1:16:48an idea so and the idea so it's lengthy
  1604. 1:16:51because
  1605. 1:16:52well
  1606. 1:16:53you have to integrate on a finite
  1607. 1:16:55interval the ratio of two quantity which
  1608. 1:16:57are quadratic so what's the fastest way
  1609. 1:17:00to do this
  1610. 1:17:01well in I think that the fastest way is
  1611. 1:17:04first of all to look at the denominator
  1612. 1:17:06and try to write it as a sum of two
  1613. 1:17:10terms which are only linear in in x
  1614. 1:17:13so to do this what you can do is you
  1615. 1:17:15compute The Roots
  1616. 1:17:17now I will sketch just how to do the
  1617. 1:17:20computation so you compute the roots of
  1618. 1:17:22this expression let me call it
  1619. 1:17:25X1 and X2 so you you set this equal to
  1620. 1:17:28zero and you will get two values for x
  1621. 1:17:31and then you can show that you can write
  1622. 1:17:331 over DX
  1623. 1:17:35as
  1624. 1:17:37so if you compute the root then you know
  1625. 1:17:39that the X
  1626. 1:17:41is essentially equal to a constant so DX
  1627. 1:17:45will be
  1628. 1:17:46some constant
  1629. 1:17:48x minus X1 x minus X2
  1630. 1:17:51right and the constant is chosen to
  1631. 1:17:54adjust the coefficient of the term x
  1632. 1:17:57square
  1633. 1:17:59so you plug this into the denominator
  1634. 1:18:02and then you try to split these two
  1635. 1:18:04terms into a sum of two terms which are
  1636. 1:18:06only linear in the denominator and you
  1637. 1:18:08can do this you will find that
  1638. 1:18:11you will have an expression like this
  1639. 1:18:15you have a pre-factor and then you have
  1640. 1:18:161 minus 1 over x minus X1 minus
  1641. 1:18:211 over x minus X2
  1642. 1:18:24okay
  1643. 1:18:25and this helps
  1644. 1:18:28because now let me call
  1645. 1:18:32this integral
  1646. 1:18:34at the exponent
  1647. 1:18:36curly I
  1648. 1:18:38so this expression is the coefficient
  1649. 1:18:39times the exponential of the integral
  1650. 1:18:44so then you can write your integral as
  1651. 1:18:47what as the prefactor
  1652. 1:18:56times the difference of two integrands
  1653. 1:19:02one which contains
  1654. 1:19:04V Prime of x
  1655. 1:19:07minus X1
  1656. 1:19:09minus the one which contains
  1657. 1:19:15V Prime of x
  1658. 1:19:18x minus X2
  1659. 1:19:22then what you have to check is that X1
  1660. 1:19:24and X2 are always smaller than x minus
  1661. 1:19:27so you see you have in principle a
  1662. 1:19:29singularity but this is outside the
  1663. 1:19:31domain of integration and then you can
  1664. 1:19:33this integral is something that you can
  1665. 1:19:35do quite easily so now you have a
  1666. 1:19:37quadratic form
  1667. 1:19:39in the numerator
  1668. 1:19:41and you can rewrite
  1669. 1:19:44so that's just the hint
  1670. 1:19:47for the math
  1671. 1:19:49but you can rewrite
  1672. 1:19:52V Prime of x
  1673. 1:19:54as
  1674. 1:19:57x minus X1 so suppose that we want to do
  1675. 1:20:00this integral what I have to do is to
  1676. 1:20:02play a little bit with my V Prime of X
  1677. 1:20:05and I can rewrite it as a constant
  1678. 1:20:07times x minus X1 Square
  1679. 1:20:11Plus
  1680. 1:20:13another constant times x
  1681. 1:20:16plus another constant so this is an
  1682. 1:20:18exercise and once you rewrite it in this
  1683. 1:20:21way you plug it in here and you see that
  1684. 1:20:24you have either terms which are linear
  1685. 1:20:26in X or the only
  1686. 1:20:28most non-trivial term that you get is of
  1687. 1:20:31the form gamma over x minus X1 that will
  1688. 1:20:34give you a logarithm so if you do these
  1689. 1:20:36tricks you can compute these Expressions
  1690. 1:20:39quite easily
  1691. 1:20:40but I'll uh leave it to you
  1692. 1:20:43and you can of course check the
  1693. 1:20:44solutions
  1694. 1:20:46and now let's comment uh what comes out
  1695. 1:20:48of this
  1696. 1:20:51so doing all of the math
  1697. 1:20:58and then doing an expansion
  1698. 1:21:00for small Epsilon which is
  1699. 1:21:03what we are interested in
  1700. 1:21:19the expression that you get is as
  1701. 1:21:21follows so you get that this e of Tau
  1702. 1:21:27or actually
  1703. 1:21:29the integral that you have at the
  1704. 1:21:31exponential
  1705. 1:21:33will go like
  1706. 1:21:35Alpha Square minus one
  1707. 1:21:38minus two alpha log Alpha
  1708. 1:21:42divided by
  1709. 1:21:43Alpha Beta Epsilon
  1710. 1:21:46plus you have a logarithmic Corrections
  1711. 1:21:50in epsilon
  1712. 1:21:53plus terms which are regular
  1713. 1:21:55when you send epsilons to zero
  1714. 1:22:01okay
  1715. 1:22:02and of course I am assuming here that
  1716. 1:22:05Alpha is different from 0 if Alpha is
  1717. 1:22:07equal to zero
  1718. 1:22:08you will have to redo the calculation
  1719. 1:22:11uh with a little bit of hair but you get
  1720. 1:22:13a very similar result
  1721. 1:22:16and so the important point and with this
  1722. 1:22:18we can conclude is that you find then
  1723. 1:22:21that your average time for your Escape
  1724. 1:22:24or activated processes
  1725. 1:22:26goes like e to the some constant
  1726. 1:22:30times 1 over Epsilon and so again
  1727. 1:22:34when you take Epsilon to zero you see
  1728. 1:22:37that you recover the situation in which
  1729. 1:22:40this time explodes and you cannot have
  1730. 1:22:43any of these activated processes but as
  1731. 1:22:46long as Epsilon is finite and you have
  1732. 1:22:48some non-linearity in your process
  1733. 1:22:51you go back to this meta stable
  1734. 1:22:53situation so you you have to wait a very
  1735. 1:22:56large time but eventually you have
  1736. 1:22:58situations in which the noise kicks you
  1737. 1:23:00up this very large barrier and if this
  1738. 1:23:03happens then after that you are bound to
  1739. 1:23:06roll down uh to minus infinity and
  1740. 1:23:09therefore you have a crisis for your for
  1741. 1:23:12your economy and this is a scenario that
  1742. 1:23:14is different with respect to
  1743. 1:23:18so let me add two comments
  1744. 1:23:24one on the content which is the last
  1745. 1:23:26point of the exercise
  1746. 1:23:28so this is a scenario for the crisis
  1747. 1:23:37that is different
  1748. 1:23:41with respect to what we have already
  1749. 1:23:43discussed
  1750. 1:23:44that was the case in which
  1751. 1:23:47Alpha is very close to one
  1752. 1:23:50that is what was called in the
  1753. 1:23:52literature as self-organized
  1754. 1:23:55criticality
  1755. 1:24:05so it is different because in this
  1756. 1:24:07scenario here you have an economy or
  1757. 1:24:09whatever you are describing that is
  1758. 1:24:11always at the verge of being critical so
  1759. 1:24:13any small fluctuations will pull you
  1760. 1:24:17into the unstable phase where Alpha
  1761. 1:24:21reaches one and then you have an
  1762. 1:24:22explosion in the number of events
  1763. 1:24:25whereas in here you have something very
  1764. 1:24:27different because you have a state a
  1765. 1:24:29local minimum that actually looks quite
  1766. 1:24:32stable and it looks stable for very
  1767. 1:24:33large times so you are in this economy
  1768. 1:24:35and you think that everything is going
  1769. 1:24:38well because you are in your meta stable
  1770. 1:24:40local minimum and you have no clue so
  1771. 1:24:43your parameter Alpha is very far away
  1772. 1:24:44from one so you have no clue that
  1773. 1:24:46something could go wrong but just
  1774. 1:24:49because you have this little non-linear
  1775. 1:24:52term
  1776. 1:24:53eventually if you wait long enough then
  1777. 1:24:56your noise will actually bring you up uh
  1778. 1:25:00uphill in here and will lead you to a
  1779. 1:25:02crisis which has uh which is very hard
  1780. 1:25:05to predict a priority if you don't have
  1781. 1:25:08this picture in here in mind so the
  1782. 1:25:10scenario for the behavior of the system
  1783. 1:25:13is really very very different this is a
  1784. 1:25:15crisis which is due to activated
  1785. 1:25:17processes whereas if you choose Alpha
  1786. 1:25:20cross one you go back to this idea of
  1787. 1:25:23self-organized criticality
  1788. 1:25:25and the second comment that I wanted to
  1789. 1:25:27just point out and then the details you
  1790. 1:25:30can figure them out is that this matches
  1791. 1:25:34the calculation that we just did so in
  1792. 1:25:36particular
  1793. 1:25:37this time going like one over Epsilon
  1794. 1:25:40matches with
  1795. 1:25:41the scaling that I wrote at the
  1796. 1:25:45beginning for the easing like case which
  1797. 1:25:48was that this time was going like uh the
  1798. 1:25:51the barrier in your potential divided by
  1799. 1:25:54the variance of the noise
  1800. 1:25:56why is it so well because in here so it
  1801. 1:25:59it might be a bit surprising that you
  1802. 1:26:01have one over Epsilon because if you
  1803. 1:26:03remember the height of the barrier
  1804. 1:26:06was of the order of one over Epsilon
  1805. 1:26:09Square
  1806. 1:26:11so you would expect a priori one over X
  1807. 1:26:13Epsilon squaring here but the point is
  1808. 1:26:16that you have to be careful about the
  1809. 1:26:18noise
  1810. 1:26:18and the noise depends on on the
  1811. 1:26:21particular point x where you are because
  1812. 1:26:24the noise in our lunge of an equation
  1813. 1:26:26was the square root of Lambda t
  1814. 1:26:30or was going let's say the variance
  1815. 1:26:33what I call Sigma Square there
  1816. 1:26:39you know our problem goes like Lambda T
  1817. 1:26:41and Lambda T goes like Lambda 0 plus
  1818. 1:26:45Alpha X Plus Epsilon x squared
  1819. 1:26:49and what you can check is that if you
  1820. 1:26:51compute this expression at the barrier
  1821. 1:26:54which was X Plus
  1822. 1:26:57you see that this goes like one over
  1823. 1:27:00Epsilon
  1824. 1:27:04I am not mistaken
  1825. 1:27:10but this we can check so this should go
  1826. 1:27:12when computed at the battery it goes
  1827. 1:27:15like uh one over Epsilon so if you plug
  1828. 1:27:17it into this expression you will have DV
  1829. 1:27:20which is one over Epsilon Square
  1830. 1:27:22and then you have a factor of so you
  1831. 1:27:26have a sigma Square
  1832. 1:27:28which is or Sigma Square over n and now
  1833. 1:27:30becomes
  1834. 1:27:311 over Epsilon and combining these two
  1835. 1:27:35scalings you get out precisely this
  1836. 1:27:38factor of one over Epsilon for the
  1837. 1:27:40relaxation time now this is not quite
  1838. 1:27:43the right argument because uh the noise
  1839. 1:27:47changes all along the potential so to
  1840. 1:27:50recover the scaling I computed it only
  1841. 1:27:53at the barrier but what you have to do
  1842. 1:27:55properly is precisely what I sketched in
  1843. 1:27:58here
  1844. 1:28:00so you you really have to compute this
  1845. 1:28:03integral all over your path so
  1846. 1:28:06what I'm saying is that if your noise is
  1847. 1:28:09constant you could bring this out of the
  1848. 1:28:11integral and then you just have the
  1849. 1:28:13integral of uh of a derivative which
  1850. 1:28:16gives you the difference of the
  1851. 1:28:18potential at the two points so that will
  1852. 1:28:19be the barrier divided by B if D was
  1853. 1:28:22constant now here it is known constants
  1854. 1:28:24so you have to go through all of the
  1855. 1:28:25integration which depends on X but you
  1856. 1:28:28somehow recover the scaling if you just
  1857. 1:28:30compute the uh precisely at the point
  1858. 1:28:33which corresponds to your barrier and so
  1859. 1:28:35you see that you have an expression
  1860. 1:28:38which matches with what we know from the
  1861. 1:28:41lecture
  1862. 1:28:42okay so I think now
  1863. 1:28:45we can maybe
  1864. 1:28:47[Music]
  1865. 1:28:48so this was it for this exercise on meta
  1866. 1:28:51stability are there questions
  1867. 1:29:01okay if there are no questions I think
  1868. 1:29:03we can
  1869. 1:29:04maybe make a break now and then go to
  1870. 1:29:06the second part
  1871. 1:29:08if you agree
  1872. 1:29:11so now is 10 40 so we kind of 15 minutes
  1873. 1:29:19of break and then we go to uh to part
  1874. 1:29:23two
  1875. 1:29:25okay
  1876. 1:29:46this conference will now be recorded
  1877. 1:29:49okay good
  1878. 1:29:52good so let's start again with part two
  1879. 1:29:56and the text is in the the seven slash
  1880. 1:29:59eight
  1881. 1:30:02and what we are gonna discuss in here is
  1882. 1:30:05uh something which goes under the name
  1883. 1:30:07of uh imitation models or models for
  1884. 1:30:10herding
  1885. 1:30:11uh
  1886. 1:30:13uh or even
  1887. 1:30:15well let's say imitation models
  1888. 1:30:17and in particular we are looking at a
  1889. 1:30:19particular model that was introduced by
  1890. 1:30:21Kirman in this paper of 1993 and the
  1891. 1:30:26motivation of human so this is called
  1892. 1:30:27the ants model so once like the animals
  1893. 1:30:30and his motivation was to understand
  1894. 1:30:32indeed behavior of animals so the idea
  1895. 1:30:36is that if you have this collection of
  1896. 1:30:39uh of animals and then you put two
  1897. 1:30:42sources of food what he was realizing is
  1898. 1:30:45that these animals always somehow choose
  1899. 1:30:49to go to it either in the source a or in
  1900. 1:30:52the source B but somehow sometimes there
  1901. 1:30:55are some very abrupt changes where all
  1902. 1:30:58of the animals suddenly want to go to
  1903. 1:31:00the source a or all of the animals want
  1904. 1:31:02to go to the source speed and so the
  1905. 1:31:04idea was to write down a simple model to
  1906. 1:31:06uh to try to understand this type of if
  1907. 1:31:10you want Collective behavior of or
  1908. 1:31:12behavior of a large number of agents and
  1909. 1:31:16we can generalize it a little bit so we
  1910. 1:31:18can think of this as being a description
  1911. 1:31:20also of human behavior so whenever you
  1912. 1:31:23have a choice between two binary choice
  1913. 1:31:25between two uh options
  1914. 1:31:29and there is a huge amount of people
  1915. 1:31:32that have to make choices sometimes you
  1916. 1:31:34see that you have this abrupt switches
  1917. 1:31:37between one choice or the other and we
  1918. 1:31:40would like to understand why this
  1919. 1:31:42happens and what is a good description
  1920. 1:31:44for this so this could also be
  1921. 1:31:46in economic Trends where some you have
  1922. 1:31:50some reversal of of the behavior of
  1923. 1:31:53people you can also so the
  1924. 1:31:55it was mentioned in the lecture this
  1925. 1:31:57example of using cell phones
  1926. 1:31:59so people have to choose whether buying
  1927. 1:32:02or not a cell phone and this can change
  1928. 1:32:04massively over time so these are all
  1929. 1:32:07things that we can think of in terms of
  1930. 1:32:10this very simple models so the kiermann
  1931. 1:32:13model that we are discussing today you
  1932. 1:32:15also find something about that in the
  1933. 1:32:19lecture notes so I uploaded yesterday
  1934. 1:32:21night a new chapter which is a chapter
  1935. 1:32:24which is about random field using model
  1936. 1:32:26and which contains something about what
  1937. 1:32:30we are going to discuss today
  1938. 1:32:31and the Amazon which is similar is the
  1939. 1:32:35Moran model that if you have time you
  1940. 1:32:38can look at in the homework number seven
  1941. 1:32:41and again I will upload the solutions uh
  1942. 1:32:45after the day today
  1943. 1:32:47so let's describe the models so what are
  1944. 1:32:49the rules of the game so the idea is
  1945. 1:32:51that you have again many uh agents
  1946. 1:32:54that
  1947. 1:32:56interact with each other and which are
  1948. 1:32:58of two types so
  1949. 1:33:05rules of the game so you have two
  1950. 1:33:07species if you want
  1951. 1:33:12A and B
  1952. 1:33:14so this can denote uh I don't know the
  1953. 1:33:17people uh who want to buy a cell phone
  1954. 1:33:20and the people who don't or the people
  1955. 1:33:21who want to vote for something and the
  1956. 1:33:23people who want to vote for something
  1957. 1:33:25else and and whatever you want to think
  1958. 1:33:28of the ants which want to go to the
  1959. 1:33:30source of food on the right versus those
  1960. 1:33:33which want to go to the source of food
  1961. 1:33:34on the left
  1962. 1:33:36and uh all of these individuals interact
  1963. 1:33:40in the following way so there is they
  1964. 1:33:43meet so let's choose a typical time
  1965. 1:33:46scale so an interval of time
  1966. 1:33:53DT
  1967. 1:33:56and what happens is that we assume that
  1968. 1:33:59uh well these people
  1969. 1:34:02or these agents can meet uh with each
  1970. 1:34:06other in within this interval of time in
  1971. 1:34:08pairs
  1972. 1:34:09and they meet with a rate so the rate
  1973. 1:34:14of let's say
  1974. 1:34:18meetings
  1975. 1:34:23we denote it with gamma
  1976. 1:34:26and whenever they meet if they are of a
  1977. 1:34:29different type some discussion takes
  1978. 1:34:32place there is some influence of uh one
  1979. 1:34:35uh with uh on the other and there can be
  1980. 1:34:38some conversion so you can have
  1981. 1:34:41let's say some conversion
  1982. 1:34:45so the conversion means that you have
  1983. 1:34:48two individuals one of type A and one of
  1984. 1:34:51type B that meet together with the rate
  1985. 1:34:54gamma and as a result
  1986. 1:34:57either the individual of type A is able
  1987. 1:35:01to recruit the individual of type B in
  1988. 1:35:04its team or the vice versa kind of core
  1989. 1:35:07so you have a process in which you start
  1990. 1:35:09from this configuration and you end up
  1991. 1:35:10in either one of these two
  1992. 1:35:12configurations and in in this model now
  1993. 1:35:14we assume that this happens
  1994. 1:35:17with equal probability
  1995. 1:35:20whereas if you look at the model
  1996. 1:35:23uh well you have some Fitness so if you
  1997. 1:35:25look at the homework the situation is a
  1998. 1:35:27little bit different but let's stick to
  1999. 1:35:29this example for the moment
  2000. 1:35:32so you have some conversion which can
  2001. 1:35:35occur with rate gamma and you also have
  2002. 1:35:38something else so you can have that some
  2003. 1:35:40individual decides to change uh its team
  2004. 1:35:44spontaneously and this also happens with
  2005. 1:35:46a fixed rate which I call in here
  2006. 1:35:49Epsilon so this will be uh
  2007. 1:35:55so let me put a slash in here you have a
  2008. 1:35:58rate
  2009. 1:35:59of
  2010. 1:36:01let's say self
  2011. 1:36:03okay
  2012. 1:36:06I'll write it properly
  2013. 1:36:13so you have conversion and you have
  2014. 1:36:16what I can call self-switching
  2015. 1:36:23self-switching means that without
  2016. 1:36:26meeting anybody else an individual of
  2017. 1:36:28type A can decide to become of type B
  2018. 1:36:31and vice versa
  2019. 1:36:33and this happens with a rate that I call
  2020. 1:36:37Epsilon and I call it Epsilon for a
  2021. 1:36:39reason that we will discover
  2022. 1:36:41afterwards
  2023. 1:36:44okay so these are the rules and now uh
  2024. 1:36:47well before going to the exercise let me
  2025. 1:36:49stress something so we are going to
  2026. 1:36:51solve this modus and from the technical
  2027. 1:36:54point of view
  2028. 1:36:55what will be important in here is what I
  2029. 1:36:58will discuss in point two of the
  2030. 1:37:00exercise and the idea will be to go from
  2031. 1:37:03a discrete setting which is the one that
  2032. 1:37:06I'm sketching in here to some sort of
  2033. 1:37:09continuous limit which in essence means
  2034. 1:37:11that we are going to start from some
  2035. 1:37:13master equation with transition rates
  2036. 1:37:15and then we will try to derive from that
  2037. 1:37:17a kind of focal Planck equation for uh
  2038. 1:37:21for the process taking a continuous
  2039. 1:37:22limit
  2040. 1:37:23and and this I will do a little bit in
  2041. 1:37:25detail and I think it is uh important uh
  2042. 1:37:28for you to uh to have a look at how you
  2043. 1:37:31can do this properly but this is point
  2044. 1:37:34two now let me start from point
  2045. 1:37:36one
  2046. 1:37:41so point one which allows to understand
  2047. 1:37:44a little bit better what I wrote in here
  2048. 1:37:46so the idea is
  2049. 1:37:48now to describe this process in terms of
  2050. 1:37:51transition rates so let me fix one type
  2051. 1:37:55so let's choose type A and let me
  2052. 1:37:59introduce a variable case Okay will be
  2053. 1:38:01just the number
  2054. 1:38:03of individuals
  2055. 1:38:11of type A
  2056. 1:38:14out of n so let's say that we have
  2057. 1:38:18a total of n individuals so as you see
  2058. 1:38:21with this type of Dynamics and remains
  2059. 1:38:24constant because every time
  2060. 1:38:26two individuals meet
  2061. 1:38:28they can change their opinion but you
  2062. 1:38:31end up with two individuals at the end
  2063. 1:38:33so n remains constant and K is a number
  2064. 1:38:36is the variable which changes uh with
  2065. 1:38:38time which denotes uh if you want the
  2066. 1:38:41number of individuals of a given type
  2067. 1:38:43and then we write down transition rates
  2068. 1:38:46which tell you what is the probability
  2069. 1:38:48that you increase or decrease this value
  2070. 1:38:51of K so
  2071. 1:38:54I will call them W as it was done in the
  2072. 1:38:57lecture so w will be the transition rate
  2073. 1:39:00to go from K for example to K plus 1
  2074. 1:39:06okay
  2075. 1:39:07and what the rate means is that this is
  2076. 1:39:09a probability divided by time so if I
  2077. 1:39:12write it as W Times
  2078. 1:39:16my small interval DT then this will be a
  2079. 1:39:19full probability so this will be the
  2080. 1:39:21probability that over a small interval
  2081. 1:39:24of time DT I go from having K
  2082. 1:39:27individuals of type A to K plus 1
  2083. 1:39:29individuals of of type A
  2084. 1:39:32and if you uh if you look at the model
  2085. 1:39:35what we are always assuming is that the
  2086. 1:39:38interval is chosen in such a way that
  2087. 1:39:40you have at most one encounter between
  2088. 1:39:43two individuals at each interval DT
  2089. 1:39:47so what is this rate now this is given
  2090. 1:39:49already in the text so let me write it
  2091. 1:39:54in a slightly different way and let me
  2092. 1:39:56comment
  2093. 1:39:57so this is one half times gamma
  2094. 1:40:01and then you have Phi so Phi is defined
  2095. 1:40:04as a fraction so I would write it as K
  2096. 1:40:07Over capital n
  2097. 1:40:101 minus K Over capital n
  2098. 1:40:14Plus
  2099. 1:40:16Epsilon 1 over K Over capital n
  2100. 1:40:21so indeed what this is describing is uh
  2101. 1:40:25is what we just saved when describing
  2102. 1:40:28the model so the idea is that in this
  2103. 1:40:30small interval of time
  2104. 1:40:32two individuals can meet and they will
  2105. 1:40:34meet with the rate so let me
  2106. 1:40:38erase the DT here
  2107. 1:40:40so two individuals we will meet with the
  2108. 1:40:42rate gamma and if they meet a conversion
  2109. 1:40:47can occur only if they are of different
  2110. 1:40:49species so you need that one of those uh
  2111. 1:40:52is of the species a and this will happen
  2112. 1:40:55with a probability that is equal to the
  2113. 1:40:57fraction of individuals of the species a
  2114. 1:40:59so it's K Over capital N the other one
  2115. 1:41:01has to be of species B so this is the
  2116. 1:41:04corresponding probability
  2117. 1:41:06and then when they meet a conversion
  2118. 1:41:08will occur and the conversion can be so
  2119. 1:41:11you have an equal probability that the
  2120. 1:41:13conversion is good for the individual of
  2121. 1:41:15type A so that the type B converts and
  2122. 1:41:19becomes type A and therefore you
  2123. 1:41:22increase your population or the
  2124. 1:41:24conversion can go uh on the other side
  2125. 1:41:26but the probability for the good
  2126. 1:41:29conversion to occur is encoded in this
  2127. 1:41:31Factor one alpha in here
  2128. 1:41:34so the first term is uh describing when
  2129. 1:41:37you increase your population because of
  2130. 1:41:39this recruitment or interaction effect
  2131. 1:41:42and then as I say do you have this extra
  2132. 1:41:44contribution of the self-switching and
  2133. 1:41:47uh and this of course has to be
  2134. 1:41:49proportional so this will occur with the
  2135. 1:41:51rate Epsilon and it has to be
  2136. 1:41:54proportional to the population of type B
  2137. 1:41:57because only those of type B will
  2138. 1:41:59convert to type a and increase your
  2139. 1:42:02population
  2140. 1:42:04so this is essentially encoding just the
  2141. 1:42:07rules of the game that we wrote uh
  2142. 1:42:09upstairs in words and of course you have
  2143. 1:42:12uh the other way
  2144. 1:42:16so you have the rate of decrease of your
  2145. 1:42:19population
  2146. 1:42:20and now as you can easily guess the
  2147. 1:42:22first term uh will be exactly the same
  2148. 1:42:24so
  2149. 1:42:26you have the same probability that two
  2150. 1:42:29individuals so core and now you have
  2151. 1:42:33the conversion of both to type B which
  2152. 1:42:36decreases your population whereas in
  2153. 1:42:39here
  2154. 1:42:40to decrease your population you need
  2155. 1:42:42that an individual of type A converts to
  2156. 1:42:45type B and this happens with a rate
  2157. 1:42:47which is Epsilon and with a probability
  2158. 1:42:49that is equal to the fraction of
  2159. 1:42:52individual of type A
  2160. 1:42:54foreign
  2161. 1:43:00of your model in a small interval DP
  2162. 1:43:05and now from here
  2163. 1:43:09what we want to do
  2164. 1:43:11is uh to so if you have these rates you
  2165. 1:43:14can write down some generic Master
  2166. 1:43:17equations for the behavior of your
  2167. 1:43:22probabilities so let me call it
  2168. 1:43:26P of K at time T so this is the
  2169. 1:43:30probability of course to have
  2170. 1:43:39of having K individuals of type A
  2171. 1:43:46at time t
  2172. 1:43:48and the master equation will contain the
  2173. 1:43:51transition rate so if you want we can
  2174. 1:43:53write
  2175. 1:43:54with this type of notation we can
  2176. 1:43:57interpret
  2177. 1:44:00our transition rates times the small
  2178. 1:44:04interval DT as
  2179. 1:44:06the conditional probability that you are
  2180. 1:44:08at K plus 1
  2181. 1:44:10time t plus VT given that you were at K
  2182. 1:44:14at time t
  2183. 1:44:19okay now
  2184. 1:44:21I will not write down well yes I will do
  2185. 1:44:24it uh in a minute or actually let me do
  2186. 1:44:28it so let me write down
  2187. 1:44:30a discrete Master equation for this
  2188. 1:44:33process
  2189. 1:44:34foreign
  2190. 1:44:39I think so
  2191. 1:44:43so I ask what is the probability that
  2192. 1:44:46the time P plus delta T I have K
  2193. 1:44:50individuals
  2194. 1:44:56so this will be equal to the following
  2195. 1:44:59so
  2196. 1:45:01I have a certain probability that at the
  2197. 1:45:03previous time I already have K
  2198. 1:45:05individuals and then I am I'm asking
  2199. 1:45:08that nothing happens in the interval DT
  2200. 1:45:10so that the situation remains unchanged
  2201. 1:45:14and the probability that nothing happens
  2202. 1:45:16is 1 minus the probability that
  2203. 1:45:18something happens
  2204. 1:45:20so this is 1 minus the probability that
  2205. 1:45:24two individuals meet and and sweet and
  2206. 1:45:28one of those switches and this is
  2207. 1:45:32gamma K Over N times 1 minus K Over N
  2208. 1:45:42and then I also have to subtract the
  2209. 1:45:45probability that one of those switches
  2210. 1:45:47by itself
  2211. 1:45:49thank you
  2212. 1:45:51so I remember I add the DT because gamma
  2213. 1:45:54is always a rate so it has a dimension
  2214. 1:45:56of one over time and the probability
  2215. 1:45:58that one of those switches is just
  2216. 1:46:00Epsilon DT
  2217. 1:46:08okay so this is the contribution when
  2218. 1:46:11nothing happens and then of course you
  2219. 1:46:13have contributions to this probability
  2220. 1:46:16coming from a conversion which occurs in
  2221. 1:46:20the small interval DT
  2222. 1:46:22so you will have here A plus the
  2223. 1:46:25probability that you were at K minus 1
  2224. 1:46:28at time t
  2225. 1:46:31times the probability that somebody
  2226. 1:46:33converts
  2227. 1:46:35to the type A during the small interval
  2228. 1:46:38DT and this is precisely given by the
  2229. 1:46:41rates that we wrote before so I will
  2230. 1:46:43write them compactly so this is w
  2231. 1:46:47to go from K minus 1 to K
  2232. 1:46:51times DT
  2233. 1:46:55okay
  2234. 1:46:57and then you have
  2235. 1:46:59the term coming from above if you want
  2236. 1:47:01so you have to add
  2237. 1:47:04the probability that you were at K plus
  2238. 1:47:061
  2239. 1:47:07at time T and then somebody goes
  2240. 1:47:12to type B
  2241. 1:47:15which is the other rate
  2242. 1:47:20okay so all of this is in the
  2243. 1:47:23description setting
  2244. 1:47:25and now to do exercise two
  2245. 1:47:28so I'm modifying it a little bit with
  2246. 1:47:30respect to the text
  2247. 1:47:31but the idea is that I just want to show
  2248. 1:47:34you a little bit
  2249. 1:47:36how one goes from the discrete setting
  2250. 1:47:39to The Continuous plank like
  2251. 1:47:41equation
  2252. 1:47:44so we will do it in two steps
  2253. 1:47:48so I will first sketch how you do this
  2254. 1:47:50properly and then I will sketch a
  2255. 1:47:53shortcut
  2256. 1:47:56that uses some of the things that we
  2257. 1:47:58discussed in pedia 3 and also very
  2258. 1:48:01briefly
  2259. 1:48:02at the end of the last today
  2260. 1:48:08okay so the point too is go to the
  2261. 1:48:11continue
  2262. 1:48:17which means
  2263. 1:48:19that we want to take the number of uh
  2264. 1:48:22animals or or people or agents going to
  2265. 1:48:26Infinity
  2266. 1:48:27and write down an equation which holds
  2267. 1:48:30uh in this limit
  2268. 1:48:32and to do this we have to introduce some
  2269. 1:48:35continuous quantity which are kind of
  2270. 1:48:38what you introduce whenever you look at
  2271. 1:48:41this and going to Infinity limit so you
  2272. 1:48:43introduce densities and you try to
  2273. 1:48:45develop a description in terms of
  2274. 1:48:47density like the magnetization as we did
  2275. 1:48:49for the spins
  2276. 1:48:51so let me introduce this quantity five
  2277. 1:48:54so if I will
  2278. 1:48:56just be the fraction K Over N
  2279. 1:49:01and let me also introduce something that
  2280. 1:49:03hopefully uh
  2281. 1:49:06will become clear in a minute
  2282. 1:49:08so I will also think at the fact that if
  2283. 1:49:11I want to develop a continuous
  2284. 1:49:13description I not only I have to rescale
  2285. 1:49:16k
  2286. 1:49:17to be able to send n to Infinity but as
  2287. 1:49:21we will see I will also have to rescale
  2288. 1:49:23time to have a properly defined equation
  2289. 1:49:27so I will write it down here and then we
  2290. 1:49:30will
  2291. 1:49:31see this in action concretely but the
  2292. 1:49:34idea is that I will need to rescale my
  2293. 1:49:37time variable with a given power of n
  2294. 1:49:39which for the moment uh that I will have
  2295. 1:49:43to choose to get a well-defined limit
  2296. 1:49:45when n goes to Infinity so for the
  2297. 1:49:47moment let me write down a generic power
  2298. 1:49:49and to the alpha
  2299. 1:49:52and then what I want to do is that I
  2300. 1:49:54want to show
  2301. 1:49:58uh that
  2302. 1:50:03I get
  2303. 1:50:05a well-defined
  2304. 1:50:08equation
  2305. 1:50:10which will be of the type soccer
  2306. 1:50:12plank type
  2307. 1:50:14or a new probability which I it's now a
  2308. 1:50:19function of this continuous variable now
  2309. 1:50:22Phi end of my rescale time
  2310. 1:50:26and which I can think
  2311. 1:50:28as the limit
  2312. 1:50:31when n goes to Infinity
  2313. 1:50:33of the probability of my discrete
  2314. 1:50:36process
  2315. 1:50:37evaluated at K which is nothing but
  2316. 1:50:42n times Phi so this is a bit formal but
  2317. 1:50:44then we will see what I mean
  2318. 1:50:48and at the previous time T which is
  2319. 1:50:52very scaled with respect to
  2320. 1:50:55to the one of the continuous process
  2321. 1:50:59so I will start from my master equation
  2322. 1:51:02for this capital P and then I will try
  2323. 1:51:05to write it down in terms as an equation
  2324. 1:51:07of for a function which is always a
  2325. 1:51:09function of only a function of Phi and
  2326. 1:51:11of summary scale time
  2327. 1:51:14and I will see if uh doing that I can
  2328. 1:51:17reach uh I can take then the limit and
  2329. 1:51:20go into infinity and find a closed
  2330. 1:51:22equation for this quantity in here
  2331. 1:51:24so this is all in words but I think it's
  2332. 1:51:26much clearer if one does the calculation
  2333. 1:51:30directly
  2334. 1:51:36so to do the calculation let me start
  2335. 1:51:38from
  2336. 1:51:40the master equation observed
  2337. 1:51:43and maybe I go
  2338. 1:51:46I go down here
  2339. 1:51:52okay so you see that you have P of k t
  2340. 1:51:55plus DT and then on the right hand side
  2341. 1:51:56you have P of k t
  2342. 1:51:59plus something which depends on DT so
  2343. 1:52:01the idea is that I want to get on the
  2344. 1:52:03left hand side some derivative so I
  2345. 1:52:06rewrite
  2346. 1:52:07that as P of k p plus DT minus
  2347. 1:52:13P of KT divided by DT
  2348. 1:52:18and then I start manipulating what
  2349. 1:52:21remains on the right hand side
  2350. 1:52:26and I started doing that so since
  2351. 1:52:28eventually I want to introduce this
  2352. 1:52:30variable file let me try to introduce uh
  2353. 1:52:32to rewrite what I have on the right in
  2354. 1:52:35terms of five
  2355. 1:52:37so let me try not to do mistakes
  2356. 1:52:41so the first term which I get is a minus
  2357. 1:52:45gamma
  2358. 1:52:47then I have an instruction which is
  2359. 1:52:49precisely 5.
  2360. 1:52:51then I have 1 minus 5.
  2361. 1:52:57and then I have I can also put
  2362. 1:53:01plus Epsilon in here
  2363. 1:53:05and everything is multiplied by my
  2364. 1:53:08probability of k and t
  2365. 1:53:11and using now for this type of relation
  2366. 1:53:15for for finite and what I can say is
  2367. 1:53:18that
  2368. 1:53:20in in the limit okay so let me
  2369. 1:53:23I will write it down and then so the
  2370. 1:53:25idea is that you have in mind that you
  2371. 1:53:27will take the limit and go into Infinity
  2372. 1:53:28of what you have on the right hand side
  2373. 1:53:30but if you take the limit I'm going to
  2374. 1:53:32Infinity this P you expect it to
  2375. 1:53:35converge uh to a function which is a
  2376. 1:53:38function of Phi and Tau for
  2377. 1:53:42and so
  2378. 1:53:44I will write it here so this will be my
  2379. 1:53:47P of Phi and Tau in terms of T since I
  2380. 1:53:52have t still t on the left hand side let
  2381. 1:53:54me keep T so this will be
  2382. 1:53:57e n to the minus Alpha
  2383. 1:54:05so if you see p of KT is precisely this
  2384. 1:54:07then I am assuming that this has a limit
  2385. 1:54:10when n goes to Infinity so I replace
  2386. 1:54:13uh I take the limit on the right hand
  2387. 1:54:15side and I replace with my limiting
  2388. 1:54:18function curly p
  2389. 1:54:20but then if I look at what I have below
  2390. 1:54:23things are a little bit more complicated
  2391. 1:54:26so now
  2392. 1:54:28we have to remember which were
  2393. 1:54:31the rates in there
  2394. 1:54:34but are a little bit more complicated
  2395. 1:54:36because so what is what was w
  2396. 1:54:41so this was W going from K minus 1 to K
  2397. 1:54:44so you have to look at this expression
  2398. 1:54:47in here and you have to replace K with K
  2399. 1:54:50minus 1.
  2400. 1:54:52so I will write just the first terms so
  2401. 1:54:55I will have in here Plus
  2402. 1:54:58what is the rate from K minus 1 to K so
  2403. 1:55:00it's the constant terms so is one half
  2404. 1:55:04gamma
  2405. 1:55:06and then since I'm starting from K minus
  2406. 1:55:081 instead of K Over N I will have K
  2407. 1:55:11minus 1
  2408. 1:55:12Over N so K minus 1 over n is Phi
  2409. 1:55:17minus
  2410. 1:55:18uh yes
  2411. 1:55:20is 5 minus 1 over n
  2412. 1:55:24do you agree because K Over N is is just
  2413. 1:55:26Phi and then i s
  2414. 1:55:29a 1 over n
  2415. 1:55:34then I have 1 minus K minus 1 over n and
  2416. 1:55:37this I can write as 1 minus 5 plus
  2417. 1:55:411 over n
  2418. 1:55:46and then the same thing for the term
  2419. 1:55:48with Epsilon so this will be plus
  2420. 1:55:51Epsilon
  2421. 1:55:54yeah sorry for the spacing but
  2422. 1:55:57you have the same thing you have 1 minus
  2423. 1:55:59five plus one over n
  2424. 1:56:02When I close the parenthesis I don't
  2425. 1:56:05know if you see this but all of this
  2426. 1:56:07thing in parenthesis then is multiplied
  2427. 1:56:11by
  2428. 1:56:13by what well in principle I have capital
  2429. 1:56:16p
  2430. 1:56:17of K minus 1 t
  2431. 1:56:20so let me rewrite it so let me take
  2432. 1:56:24assume that n is large and this I can
  2433. 1:56:26rewrite
  2434. 1:56:28basically as my curly p
  2435. 1:56:36evaluated at what is case Okay is
  2436. 1:56:41uh
  2437. 1:56:43so it's my so this is
  2438. 1:56:46if you want n over Phi
  2439. 1:56:49minus 1
  2440. 1:56:51so I can rewrite it as n times P minus 1
  2441. 1:56:55over n
  2442. 1:56:57and then I know that my probability p
  2443. 1:57:00as a function of n times something will
  2444. 1:57:03map into my function curly P evaluated
  2445. 1:57:07at the something so let me write it down
  2446. 1:57:10so this will be Phi minus 1 over n
  2447. 1:57:16and then I have to rescale time as above
  2448. 1:57:20foreign
  2449. 1:57:37and now I have done the other terms so
  2450. 1:57:39the other term is is quite similar
  2451. 1:57:41except that this rate in here is
  2452. 1:57:45changing but if you do this
  2453. 1:57:47along the same line of reasoning you
  2454. 1:57:50have
  2455. 1:57:51foreign
  2456. 1:57:53the first part of the rate is unchanged
  2457. 1:58:03and the second part was just multiplying
  2458. 1:58:09so now you go
  2459. 1:58:12no it was not unchanged because I have a
  2460. 1:58:15plus somewhere
  2461. 1:58:25okay so to compute the second term you
  2462. 1:58:28have to evaluate the rate now which goes
  2463. 1:58:30from K plus 1 to K
  2464. 1:58:33so if I use the expression that I wrote
  2465. 1:58:35before and I do the same expansion you
  2466. 1:58:37realize that I have a plus in front of
  2467. 1:58:39the correction because it's K plus 1 and
  2468. 1:58:42not K minus 1 so you should find
  2469. 1:58:44something like this please stop me if
  2470. 1:58:47if this is not immediate
  2471. 1:58:50then I will do it explicitly and then
  2472. 1:58:52the term in here is proportional to K
  2473. 1:58:55plus 1 over n which I will write
  2474. 1:58:58I will rewrite as V plus 1 over n
  2475. 1:59:07times
  2476. 1:59:09my curly p
  2477. 1:59:11which now is evaluated at K plus 1 which
  2478. 1:59:15in my new variable is V plus 1 over n
  2479. 1:59:19and then the rescale the time
  2480. 1:59:26okay
  2481. 1:59:42yes
  2482. 1:59:45this this is minus yes because I have a
  2483. 1:59:48minus in front thanks
  2484. 1:59:51exactly
  2485. 1:59:56okay so now I'm doing things a little
  2486. 1:59:59bit it's loppy so as you see I'm
  2487. 2:00:00translating from one notation to another
  2488. 2:00:02and taking first one limit uh before the
  2489. 2:00:06other but let's
  2490. 2:00:08so you can do things more properly but
  2491. 2:00:11what I just want to emphasize is the
  2492. 2:00:13step
  2493. 2:00:14that comes now
  2494. 2:00:17and the step that comes now is that you
  2495. 2:00:20now have
  2496. 2:00:22so you rewrite things in such a way that
  2497. 2:00:24on the right hand side it appears the
  2498. 2:00:27function uh of which you want to compute
  2499. 2:00:29or for which you want to compute an
  2500. 2:00:31equation
  2501. 2:00:32the left hand side we have to work on
  2502. 2:00:34that but we will do it last but the
  2503. 2:00:37point now is that this function is now
  2504. 2:00:40computed at Phi which is good but then
  2505. 2:00:42you have this correction of 1 over n
  2506. 2:00:45and so what we can think of is
  2507. 2:00:48now to do an expansion of uh of what
  2508. 2:00:52appears in the right hand side in powers
  2509. 2:00:54of 1 over n which is uh which is our
  2510. 2:00:58small parameter when n goes to Infinity
  2511. 2:01:05so I'll just give the idea
  2512. 2:01:19and then we will not do all of the
  2513. 2:01:21calculations because it's a bit tedious
  2514. 2:01:24but
  2515. 2:01:26foreign
  2516. 2:01:29give the idea so now you assume that you
  2517. 2:01:33can expand your functions so whenever
  2518. 2:01:35you have P of
  2519. 2:01:36Phi minus 1 over n
  2520. 2:01:40and
  2521. 2:01:42my T to the N minus Alpha will be what I
  2522. 2:01:46will later on call Tau
  2523. 2:01:49this you will write as P of Phi Tau
  2524. 2:01:53and you're happy with that
  2525. 2:01:55then you have the first derivative
  2526. 2:02:02over Phi times minus 1 over n so let me
  2527. 2:02:06put
  2528. 2:02:08and this is evaluated at 3 and Tau times
  2529. 2:02:111 over n
  2530. 2:02:14and then it turns out for reason that
  2531. 2:02:16you realize when you do the calculation
  2532. 2:02:17that you have to go
  2533. 2:02:19to second order here
  2534. 2:02:23so you will have a second derivative
  2535. 2:02:28to keep into account
  2536. 2:02:34within one knife in front
  2537. 2:02:39one over n Square
  2538. 2:02:43and of course you do the same whenever
  2539. 2:02:45you have a p evaluated at five plus one
  2540. 2:02:48over n
  2541. 2:02:51and now what you have to do is to plug
  2542. 2:02:54these expansions on the right hand side
  2543. 2:02:59combine all of the terms so you see that
  2544. 2:03:01also the rates will have a term which is
  2545. 2:03:04of order one which just depend on Phi
  2546. 2:03:06and then we'll have terms of order one
  2547. 2:03:08over n in terms of order 1 over n Square
  2548. 2:03:12and you have to collect everything to
  2549. 2:03:14expand your right hand side in in powers
  2550. 2:03:18of 1 over n
  2551. 2:03:20now if you do this this is a little bit
  2552. 2:03:22lengthy but what you realize is that
  2553. 2:03:24many terms will cancel so in particular
  2554. 2:03:27the term of order one of order 0 and the
  2555. 2:03:29term of order one over n will exactly
  2556. 2:03:31cancel from this expression
  2557. 2:03:34and so in the end
  2558. 2:03:36you end up with the following things so
  2559. 2:03:38let me keep the left hand side
  2560. 2:03:54which was this
  2561. 2:03:57and then on the right hand side so if
  2562. 2:03:59you trust me
  2563. 2:04:02you will see that you reduce everything
  2564. 2:04:04to the following so you have a one over
  2565. 2:04:06n Square
  2566. 2:04:09times the second derivative
  2567. 2:04:15of your
  2568. 2:04:18original rates times now your function
  2569. 2:04:22evaluated at 3 Tau
  2570. 2:04:29minus
  2571. 2:04:33minus
  2572. 2:04:37nope
  2573. 2:04:39a term which looks like this so there is
  2574. 2:04:41a term 1 over n
  2575. 2:04:46Cylon
  2576. 2:04:50D over d c
  2577. 2:04:54one minus 2 Phi
  2578. 2:04:57times your p
  2579. 2:05:03okay
  2580. 2:05:08okay so you have something that on the
  2581. 2:05:10right hand side
  2582. 2:05:12has some scaling within which remains
  2583. 2:05:14non-zero but the scaling has some
  2584. 2:05:17mismatch so you see that you have a 1
  2585. 2:05:19over n Square Times what you would like
  2586. 2:05:21to have quantities of order one in the
  2587. 2:05:24limit I'm going to Infinity minus 1 over
  2588. 2:05:26n instead times quantities of order one
  2589. 2:05:30so in order to get a meaningful right
  2590. 2:05:32hand side uh limit of this equation
  2591. 2:05:36I have to do an extra step which
  2592. 2:05:37explains why I choose this notation
  2593. 2:05:40Epsilon
  2594. 2:05:41so I have to assume that Epsilon also
  2595. 2:05:44scales whenever I look at the
  2596. 2:05:48discontinuous limit
  2597. 2:05:50I have to assume that if Cylon also
  2598. 2:05:52scales like 1 over n so I
  2599. 2:05:55say that Epsilon is equal to some
  2600. 2:05:57constant is zero
  2601. 2:06:01divided by n and in this way e0 is a
  2602. 2:06:05border one and I match the scaling
  2603. 2:06:07between these two quantities
  2604. 2:06:09so why do you do do I do this well if
  2605. 2:06:12you think about the usual
  2606. 2:06:14mean field or fully connected things
  2607. 2:06:17you realize that this is actually the
  2608. 2:06:20meaningful thing to do
  2609. 2:06:22and the reason is that uh so usually
  2610. 2:06:25whenever you have this uh interaction
  2611. 2:06:28terms
  2612. 2:06:29and and you have a scaling within you uh
  2613. 2:06:32you have to rescale with the interaction
  2614. 2:06:34to have something which remains uh of
  2615. 2:06:36order one uh in the limit angle is going
  2616. 2:06:39to Infinity but anyway in here you see
  2617. 2:06:41it directly from from the calculation
  2618. 2:06:43that in order for this to term uh to
  2619. 2:06:45match
  2620. 2:06:46you uh you assume that Epsilon
  2621. 2:06:49when n goes to Infinity scales as one
  2622. 2:06:53over capital n
  2623. 2:06:55and if I do this then I can replace
  2624. 2:06:59here so let me erase this
  2625. 2:07:03I put an upside on and I put an end
  2626. 2:07:05Square
  2627. 2:07:08and I have a global factor of 1 over n
  2628. 2:07:12Square on the right hand side that I
  2629. 2:07:15simply bring on the left hand side
  2630. 2:07:17so I will have a BT divided by n Square
  2631. 2:07:22in here
  2632. 2:07:24so of course this can be done properly
  2633. 2:07:27and rigorously but let me just
  2634. 2:07:29uh give you roughly the idea
  2635. 2:07:32and so you see that now my right hand
  2636. 2:07:35side looks like
  2637. 2:07:37uh a properly well defined Hawker blank
  2638. 2:07:41equation with a drift term which is a
  2639. 2:07:43order one and with a diffusion term and
  2640. 2:07:45my Tau
  2641. 2:07:48I Define it as some rescaled time with
  2642. 2:07:52an unknown power
  2643. 2:07:54and to the minus Alpha
  2644. 2:07:57and in order to make sense of this
  2645. 2:08:00equation what I want from the left hand
  2646. 2:08:02side is that I can rewrite this
  2647. 2:08:05as the derivative of my P
  2648. 2:08:12with respect to some to the same Tau
  2649. 2:08:15variable
  2650. 2:08:19so the dependence on K is fine you have
  2651. 2:08:22K on both of these terms so this once
  2652. 2:08:26every scale will become just a function
  2653. 2:08:29of Phi I don't have factors of plus
  2654. 2:08:31minus 1 over n the two care about
  2655. 2:08:34you see that what I have to do in order
  2656. 2:08:36to uh
  2657. 2:08:38for this mapping to make sense is to
  2658. 2:08:42choose my power
  2659. 2:08:44Alpha in here
  2660. 2:08:48in such a way that I can rewrite the
  2661. 2:08:51derivative over T if you want
  2662. 2:08:55which is related to the derivative of
  2663. 2:08:57our Tau by 1 over n to the uh to the
  2664. 2:09:02alpha I have to choose that I find such
  2665. 2:09:04a way that I cancel this factor and
  2666. 2:09:07square
  2667. 2:09:08in the left hand side of my equation so
  2668. 2:09:10this is to say if I rescale time
  2669. 2:09:13or if I introduce a variable of time Tau
  2670. 2:09:17which is rescaled
  2671. 2:09:19as t to the N minus 2.
  2672. 2:09:25which means that my Alpha
  2673. 2:09:27is equal to 2
  2674. 2:09:30then all of my scalings work correctly
  2675. 2:09:34because I add the right hand side which
  2676. 2:09:35had this factor of n to the two
  2677. 2:09:39globally so I bring it on the left hand
  2678. 2:09:42side and I have this new factor of P
  2679. 2:09:45Over N Square which I just defined it as
  2680. 2:09:48Tau and then I reproduce on the left
  2681. 2:09:50hand side the derivative with respect to
  2682. 2:09:53Tau
  2683. 2:09:54foreign
  2684. 2:10:02just to give an idea of how uh one
  2685. 2:10:05should do the things uh properly so I
  2686. 2:10:07think that what one has to remember
  2687. 2:10:11is that you want to
  2688. 2:10:14assume that you can rescale the
  2689. 2:10:17arguments of your function and then take
  2690. 2:10:19the limit and go into infinity and in
  2691. 2:10:21such a limit you recover a closed
  2692. 2:10:24equation for for a function which is
  2693. 2:10:26just a function of your rescaled
  2694. 2:10:27variables
  2695. 2:10:28now there is scaling for the density is
  2696. 2:10:30is very natural so the factor one over n
  2697. 2:10:33is what we always expect because of
  2698. 2:10:36extensivity of K and in here there is
  2699. 2:10:38the you also have to rescale time
  2700. 2:10:41in a way that you get a well-defined
  2701. 2:10:43equation and this is something that if
  2702. 2:10:45you think about it
  2703. 2:10:47uh it is quite natural because we are
  2704. 2:10:51assuming that
  2705. 2:10:52over a time scale DT
  2706. 2:10:55you have only one event which switch
  2707. 2:10:58your K by plus or minus one
  2708. 2:11:02but the equation that you're writing
  2709. 2:11:04down is actually an equation for
  2710. 2:11:06variations in Phi
  2711. 2:11:09that you can think of as K divided by by
  2712. 2:11:13a factor of n so to have a very small
  2713. 2:11:15variation of order 1 over n you have to
  2714. 2:11:18look at times which are which are much
  2715. 2:11:20much smaller than the ones of your
  2716. 2:11:22original discrete process so at least
  2717. 2:11:25you understand why your tau is is uh has
  2718. 2:11:29to be rescaled by a power which is
  2719. 2:11:31negative in in capital n and the fact
  2720. 2:11:33that this is equal to 2 well in this
  2721. 2:11:35case you
  2722. 2:11:36it just comes out from the explicit
  2723. 2:11:40expansion
  2724. 2:11:41and your calculation
  2725. 2:11:43okay so anyway this is just to give an
  2726. 2:11:46idea of how one takes a continuous limit
  2727. 2:11:49by doing expansions in terms of uh
  2728. 2:11:53powers of 1 over n
  2729. 2:11:55and as you see you get out
  2730. 2:11:58a Planck equation
  2731. 2:12:00uh that now we are gonna
  2732. 2:12:03interpret and solve for the stationary
  2733. 2:12:06state
  2734. 2:12:07and uh and this is a focal Planck
  2735. 2:12:10equation that is that you could guess
  2736. 2:12:14a priori
  2737. 2:12:17remembering how one derives Factor
  2738. 2:12:21Planck equation from uh from the
  2739. 2:12:23language one equation so now let's keep
  2740. 2:12:25this I will rewrite this expression
  2741. 2:12:28for the equation and then we
  2742. 2:12:33actually try to see how you could guess
  2743. 2:12:35it
  2744. 2:12:37without going through all of this
  2745. 2:12:39lengthy expansion
  2746. 2:12:43and this is actually point two of the
  2747. 2:12:45exercise
  2748. 2:12:48so this is very active in time so the
  2749. 2:12:51drift term
  2750. 2:12:52you have this uh D over D Phi of
  2751. 2:12:58Epsilon 0 1 minus two Phi
  2752. 2:13:04your Phi Tau and then you have the
  2753. 2:13:06diffusion term
  2754. 2:13:20foreign
  2755. 2:13:24which looks like this
  2756. 2:13:27okay
  2757. 2:13:48now let's forget about this calculation
  2758. 2:13:51that I just did and let's assume that I
  2759. 2:13:54give you
  2760. 2:13:56this blank equation and I ask you
  2761. 2:13:58to justify it
  2762. 2:14:00to justify why it looks like this given
  2763. 2:14:03what you know about the process in
  2764. 2:14:05discrete space and in discrete time
  2765. 2:14:10so this is 0.2
  2766. 2:14:13and the way you can justify it is
  2767. 2:14:18by recalling
  2768. 2:14:20something very that I that I
  2769. 2:14:24sketched very fast at the LA the end of
  2770. 2:14:26the last day but which you find so
  2771. 2:14:28recall
  2772. 2:14:32the solution of State A3
  2773. 2:14:35where you have a derivation of focal
  2774. 2:14:37Planck equation from the lunge of an
  2775. 2:14:39equation
  2776. 2:14:40and The crucial point in the derivation
  2777. 2:14:42is just to remember that you essentially
  2778. 2:14:45need to compute two quantities which are
  2779. 2:14:48an average and a variance that are what
  2780. 2:14:51entering here of your incremental step
  2781. 2:14:55in an interval DT so these are the
  2782. 2:14:58quantities that I defined
  2783. 2:14:59last time as E1 and E2
  2784. 2:15:04this is if you have a if you have in
  2785. 2:15:06mind an underlying large of an equation
  2786. 2:15:08they looked like this
  2787. 2:15:10so you add an average of your
  2788. 2:15:12incremental step
  2789. 2:15:18in the interval DT
  2790. 2:15:22and that is what I call D1 and then you
  2791. 2:15:24have the the same thing but with the
  2792. 2:15:26square
  2793. 2:15:28which was E2
  2794. 2:15:35and now this is the transition
  2795. 2:15:37probability coming from your underlying
  2796. 2:15:39lunge event
  2797. 2:15:40equation
  2798. 2:15:47and if you have these two moments
  2799. 2:15:49then
  2800. 2:15:51your focal Planck equation takes the
  2801. 2:15:55general form so your DP in this case it
  2802. 2:15:58would be of x and t
  2803. 2:16:01in our case X is equal to Phi but okay
  2804. 2:16:07equals what so it was minus D over DX of
  2805. 2:16:11your first moment E1 of x
  2806. 2:16:17P of x t and then you add the second
  2807. 2:16:19derivative
  2808. 2:16:37and this is something you you find uh if
  2809. 2:16:40you do the derivation properly
  2810. 2:16:44and I also mentioned last time that so
  2811. 2:16:47this form is generic whatever is uh is
  2812. 2:16:50the prescription for the noise that you
  2813. 2:16:52take
  2814. 2:16:53what changes and that will eventually
  2815. 2:16:55give you different forms of your
  2816. 2:16:57language of your focal Planck equation
  2817. 2:17:00is
  2818. 2:17:01uh is the computation of this i1 so this
  2819. 2:17:05quantity will be different whether you
  2820. 2:17:07choose ether versus strathana which but
  2821. 2:17:10this is not important in here but this
  2822. 2:17:11is just to connect with uh with what we
  2823. 2:17:14saw last time
  2824. 2:17:16so given this intuition that we know
  2825. 2:17:19what we want to do is essentially to
  2826. 2:17:22recognize that what you have in here is
  2827. 2:17:25an average increment and that what you
  2828. 2:17:26have in here is the average of the
  2829. 2:17:29square increment and therefore with this
  2830. 2:17:31argument we can justify uh the form of
  2831. 2:17:34our soccer plank
  2832. 2:17:36so how can we do this well we start from
  2833. 2:17:39our discrete process in terms of K
  2834. 2:17:45and we use the fact that in the discrete
  2835. 2:17:48setting
  2836. 2:17:49the probability
  2837. 2:17:52that you end up in so you can have only
  2838. 2:17:55increments by one unit
  2839. 2:17:58with a probability that
  2840. 2:18:01was just given by our rates
  2841. 2:18:12okay
  2842. 2:18:14and so now the analog of these averages
  2843. 2:18:17will be averages over this now
  2844. 2:18:21conditional transition probability
  2845. 2:18:25and the possible values that your
  2846. 2:18:27increments can take in the discrete
  2847. 2:18:29setting are always plus or minus one
  2848. 2:18:33so this means that so let me first
  2849. 2:18:35compute what is the average
  2850. 2:18:39increment Delta k
  2851. 2:18:43so this is equal to Delta k equals to
  2852. 2:18:46plus 1 times the probability the Delta K
  2853. 2:18:49is equal to plus one
  2854. 2:18:51minus Delta k equals to minus 1 times
  2855. 2:18:54the probability the Delta K is equal to
  2856. 2:18:57-1
  2857. 2:18:59and therefore if you just plug this
  2858. 2:19:02expression you see that this is just
  2859. 2:19:05BT times
  2860. 2:19:09the rate
  2861. 2:19:11of plus 1 plus the rate
  2862. 2:19:18minus one
  2863. 2:19:22now we plug in
  2864. 2:19:23our expression for the rate
  2865. 2:19:28and if you do a the algebra this you
  2866. 2:19:31recover that this is
  2867. 2:19:33sorry this is yes precisely
  2868. 2:19:38given by this
  2869. 2:19:46and I forgot the minus
  2870. 2:19:52so this comes with a minus because uh
  2871. 2:19:56should be Delta k equals to -1
  2872. 2:19:59times the corresponding probability
  2873. 2:20:04so the term which contains gamma cancels
  2874. 2:20:07and you just have to sum the terms which
  2875. 2:20:09contains Epsilon and you get this
  2876. 2:20:11and if you do the variance in terms of K
  2877. 2:20:16in this K case this will be just the sum
  2878. 2:20:19of the two transition rates so instead
  2879. 2:20:22of a minus you would have a plus
  2880. 2:20:24and you find that this is equal to DT
  2881. 2:20:28gamma Phi
  2882. 2:20:301 minus 5 plus Epsilon
  2883. 2:20:37so we are almost there
  2884. 2:20:40this looks almost like what we want
  2885. 2:20:43uh for our focal plank
  2886. 2:20:46except one thing
  2887. 2:20:49meaning that we are now reasoning
  2888. 2:20:52with respect to K but the increment that
  2889. 2:20:55we care about are actually with respect
  2890. 2:20:57to Phi
  2891. 2:20:59so we have to rescale everything by a
  2892. 2:21:02factor of n
  2893. 2:21:05so let me go it
  2894. 2:21:07do it up here
  2895. 2:21:17so what would be i1
  2896. 2:21:22foreign
  2897. 2:21:27in my notation of before is what is
  2898. 2:21:32the incrementing K divided by n
  2899. 2:21:35so this is simply
  2900. 2:21:38Epsilon 1 minus 2 Phi
  2901. 2:21:42DT divided by n
  2902. 2:21:45whereas I2
  2903. 2:21:53is just this
  2904. 2:21:56and so I have DT
  2905. 2:22:00Over N Square
  2906. 2:22:04gamma Phi
  2907. 2:22:071 minus 5 plus Epsilon
  2908. 2:22:11and now again you see that you have
  2909. 2:22:12these factors of n which appear and in
  2910. 2:22:15order
  2911. 2:22:16to have a well-defined process where you
  2912. 2:22:18have both drift and diffusion
  2913. 2:22:21you have to kill these extra factors of
  2914. 2:22:24n by rescaling both Epsilon in here and
  2915. 2:22:27rescaling the time
  2916. 2:22:29so this means that
  2917. 2:22:31the time in which your focal Planck
  2918. 2:22:33Dynamics will occur will be such that
  2919. 2:22:35this is a order one
  2920. 2:22:38and therefore you will define t Over N
  2921. 2:22:40Square
  2922. 2:22:41to be a rescaled time variable
  2923. 2:22:45and if you do this
  2924. 2:22:47this will be of order and
  2925. 2:22:53and therefore you have to redefine
  2926. 2:22:56Epsilon to be some constant Epsilon 0
  2927. 2:23:00divided by n so you recover
  2928. 2:23:02your your scaling of time
  2929. 2:23:05from this shortcut and once you do this
  2930. 2:23:07then this Epsilon will disappear because
  2931. 2:23:10it is over the one over n so your drift
  2932. 2:23:12will only contain this term which is
  2933. 2:23:14what you see in the focal Planck
  2934. 2:23:16equation up there and sorry your
  2935. 2:23:18diffusion and your drift will contain
  2936. 2:23:20Epsilon zero times one minus two Phi
  2937. 2:23:23which is what you see up there
  2938. 2:23:26so this is a way that is a little bit
  2939. 2:23:28shorter to avoid doing the lengthy
  2940. 2:23:32expansion or at least to justify
  2941. 2:23:35why your focal Planck equation takes uh
  2942. 2:23:38takes that form
  2943. 2:23:41okay so are there questions here
  2944. 2:23:45that was the most
  2945. 2:23:47uh let's say technical part
  2946. 2:23:51and if not then what remains to do is to
  2947. 2:23:55to to characterize the model is to try
  2948. 2:23:57to
  2949. 2:23:58in principle solve the full focal Planck
  2950. 2:24:01equation so we are not able to do this
  2951. 2:24:03but we can look at the stationary State
  2952. 2:24:05yes
  2953. 2:24:06foreign
  2954. 2:24:13yes
  2955. 2:24:23yes I think that whenever you write
  2956. 2:24:28um
  2957. 2:24:29when you start from the master equation
  2958. 2:24:31you are doing some so we're not starting
  2959. 2:24:34from a launch event
  2960. 2:24:36so the the problem is not uh let's say
  2961. 2:24:39defined from the start because we do not
  2962. 2:24:42have to specify prescriptions for the
  2963. 2:24:43noise but we always assume Independence
  2964. 2:24:46uh in in the label time interval and so
  2965. 2:24:49this will lead you to anito like
  2966. 2:24:51equation and indeed the focal Planck
  2967. 2:24:54equation that you get up there so the
  2968. 2:24:55question sorry for those who are nine is
  2969. 2:24:57uh we get a focal Planck equation that
  2970. 2:25:01is in the Ito formal is if you if you
  2971. 2:25:03remember
  2972. 2:25:04so why is it so uh from where is it
  2973. 2:25:08encoded from our derivation and and this
  2974. 2:25:11is embedded in the fact that we are
  2975. 2:25:12assuming uh somehow that the processes
  2976. 2:25:15that occur in the event uh DT are
  2977. 2:25:18independent and so this corresponds to
  2978. 2:25:19data
  2979. 2:25:21but this is a good observation so if you
  2980. 2:25:23what would be the form uh for uh
  2981. 2:25:27stratonovich
  2982. 2:25:28focal Planck equation
  2983. 2:25:32so if you remember
  2984. 2:25:34you would just have
  2985. 2:25:37foreign
  2986. 2:25:39which you have one derivative than one
  2987. 2:25:42factors of of G which is now the square
  2988. 2:25:46root of this and then you have the
  2989. 2:25:48derivative and then the square root of
  2990. 2:25:50the times p
  2991. 2:25:51and this is nice because now we are
  2992. 2:25:53going to solve for the stationary State
  2993. 2:25:55and we will find a solution that
  2994. 2:25:57corresponds indeed to The Ether solution
  2995. 2:26:00and if you have a different form if you
  2996. 2:26:02use the satanovic the the form of the
  2997. 2:26:04stationary state will change so you can
  2998. 2:26:06try to do this as an exercise
  2999. 2:26:12okay so let's now try to compute this
  3000. 2:26:14stationary State and then we conclude
  3001. 2:26:18uh there was maybe a comment before yes
  3002. 2:26:28so before or while I raise
  3003. 2:26:31just one comment on the form of the
  3004. 2:26:33equation so you see
  3005. 2:26:36you have the drift term and the noise
  3006. 2:26:38term and they somehow they
  3007. 2:26:41push you in different directions
  3008. 2:26:45so the drift term
  3009. 2:26:47vanishes when Phi is equal to one half
  3010. 2:26:51so one alpha means that you have
  3011. 2:26:53polish population of type A and half
  3012. 2:26:56relation of time type B
  3013. 2:27:00so the brief term is somehow push is
  3014. 2:27:02pushing you towards one out if you are
  3015. 2:27:05away from one else you have some kind of
  3016. 2:27:07force that pushes you to reach one half
  3017. 2:27:11whereas the noise term
  3018. 2:27:13is pushing you away from one alph
  3019. 2:27:15because the variance of the noise is
  3020. 2:27:17maximal at one half so the noise wants
  3021. 2:27:19you if you are sitting at one half it
  3022. 2:27:22tends to uh with with this random
  3023. 2:27:24fluctuations to put you push you away
  3024. 2:27:28uh from the middle towards the extrema
  3025. 2:27:32where the noise is zero which are
  3026. 2:27:34Phi equal to one or two zero which means
  3027. 2:27:36that all of the population is either in
  3028. 2:27:38state a
  3029. 2:27:39or in state B so there is a competition
  3030. 2:27:42between these two terms and so we expect
  3031. 2:27:45to see this competition also in the
  3032. 2:27:48stationary State and indeed we will have
  3033. 2:27:50a parameter Alpha
  3034. 2:27:54on which the stationary State depends
  3035. 2:27:57which is just the ratio of the two
  3036. 2:27:59with a factor of two so let me Define it
  3037. 2:28:01properly
  3038. 2:28:03um
  3039. 2:28:05yes
  3040. 2:28:08so depending on whether Alpha is larger
  3041. 2:28:10or smaller than one you will have
  3042. 2:28:12different forms for your stationary
  3043. 2:28:14solution
  3044. 2:28:16but let's compute them and then we are
  3045. 2:28:18done so this was 0.3
  3046. 2:28:22foreign
  3047. 2:28:23so what it means to compute the
  3048. 2:28:26stationary distribution so the
  3049. 2:28:28stationary distribution does not depend
  3050. 2:28:30on time it satisfies
  3051. 2:28:32the DP
  3052. 2:28:35stationary
  3053. 2:28:38you have to set to zero uh the left hand
  3054. 2:28:41side
  3055. 2:28:43so actually whenever this is true you
  3056. 2:28:45have a
  3057. 2:28:46stationary distribution which depends on
  3058. 2:28:49your own fight
  3059. 2:28:51and now if I set to zero the left hand
  3060. 2:28:54side let me look at the right hand side
  3061. 2:28:57so the right hand side contains uh many
  3062. 2:29:00derivatives and what I can do is
  3063. 2:29:03so the right hand side
  3064. 2:29:06I can write it as a global derivative
  3065. 2:29:11maybe with a minus
  3066. 2:29:13of something that I can call a current
  3067. 2:29:16so what is my current so here
  3068. 2:29:20is 1 minus 2 pi times p
  3069. 2:29:26minus one half
  3070. 2:29:28B over DC
  3071. 2:29:32of gamma Phi
  3072. 2:29:351 minus 5 times p
  3073. 2:29:44so if I set the if I set the left hand
  3074. 2:29:47side to zero then I'm saying that this
  3075. 2:29:49quantity has to be equal to zero which
  3076. 2:29:52means that whatever is in parenthesis
  3077. 2:29:55which just depends on Phi
  3078. 2:29:59it's derivative with respect to Phi has
  3079. 2:30:01to be equal to zero so this quantity
  3080. 2:30:04has to be equal to a constant
  3081. 2:30:07okay
  3082. 2:30:09when I evaluate it at the stationary
  3083. 2:30:12distribution
  3084. 2:30:17because in that case this derivative is
  3085. 2:30:19zero
  3086. 2:30:21now what is this constant well
  3087. 2:30:25since this constant dip is uh so you
  3088. 2:30:27have the pin here
  3089. 2:30:29and you don't want a dependence on Phi
  3090. 2:30:32so what you can argue is that you should
  3091. 2:30:34actually choose this constant J to be
  3092. 2:30:37itself equal to zero
  3093. 2:30:41and the reason is that if this was not
  3094. 2:30:43the case then you will uh so you would
  3095. 2:30:47get a distribution that is uh that is
  3096. 2:30:49not normalizable so what you want
  3097. 2:30:52is that P when Phi goes to
  3098. 2:30:55uh well here we have a bounded intervals
  3099. 2:30:58but in general if you think about
  3100. 2:31:00unbounded distributions you want to that
  3101. 2:31:03pdks such that you are normalized
  3102. 2:31:06and in order for p to Decay such that
  3103. 2:31:08you're normalized it must go to zero
  3104. 2:31:10when the argument goes to Infinity but
  3105. 2:31:13if it has to be constant that this means
  3106. 2:31:15that P itself uh or whatever or the
  3107. 2:31:18combination of p and its derivative has
  3108. 2:31:20to be equal to uh to zero so you can
  3109. 2:31:23argue in general that because of
  3110. 2:31:26normalization you can set your current
  3111. 2:31:29equal to zero or if you want you just
  3112. 2:31:32assume that this is zero and you find
  3113. 2:31:34the stationary solution
  3114. 2:31:36that satisfies your equation in which by
  3115. 2:31:39definition uh
  3116. 2:31:42will be stationary
  3117. 2:31:44so let's assume that our current is zero
  3118. 2:31:47so this now gives
  3119. 2:31:49a linear differential equation for our p
  3120. 2:31:53did I rewrite and that we can solve in
  3121. 2:31:56three steps
  3122. 2:31:59so we have
  3123. 2:32:010 1 minus two High
  3124. 2:32:05stationary
  3125. 2:32:07Pi minus one alpha
  3126. 2:32:10uh
  3127. 2:32:12Define
  3128. 2:32:15gamma Phi 1 minus 5 is stationary of
  3129. 2:32:20five
  3130. 2:32:24this is b equal to zero
  3131. 2:32:29and now we solve this equation in three
  3132. 2:32:32steps
  3133. 2:32:34so the first step or at least I find it
  3134. 2:32:36easier to solve it in three steps so the
  3135. 2:32:38first step is to do some rescaling
  3136. 2:32:42so you see I have a linear equation but
  3137. 2:32:44here I have Phi which appears everywhere
  3138. 2:32:47so let me Define this
  3139. 2:32:49foreign
  3140. 2:32:54so that I have the derivative of P tilde
  3141. 2:32:56which is easier to handle
  3142. 2:33:00so I introduce
  3143. 2:33:02such that
  3144. 2:33:04this is gamma Phi
  3145. 2:33:061 minus 5 is stationary
  3146. 2:33:12and then I write the equation for
  3147. 2:33:13pitilda so I will have 0 1 minus two Phi
  3148. 2:33:19the MP stationary is
  3149. 2:33:23the killer Phi divided by gamma
  3150. 2:33:27PSI 1 minus Phi
  3151. 2:33:30and on the right hand side I just have a
  3152. 2:33:32factor of one half so I bring the two up
  3153. 2:33:35here
  3154. 2:33:37and I just have B
  3155. 2:33:40over the side of my PT love Phi
  3156. 2:33:45okay
  3157. 2:33:48and now once I did this rescaling I can
  3158. 2:33:52do
  3159. 2:33:53something very easy which always
  3160. 2:33:56comes out from the structure of this
  3161. 2:33:59equation which is that I can integrate
  3162. 2:34:01this equation with separation of
  3163. 2:34:03variables
  3164. 2:34:17so in a natural separation of variables
  3165. 2:34:19the seen examples in the lecture already
  3166. 2:34:21means that I
  3167. 2:34:23bring on the right hand side all the
  3168. 2:34:25terms which depend on pitilda and I live
  3169. 2:34:28on the left hand side all the terms
  3170. 2:34:30which depend on Phi or if you want that
  3171. 2:34:33I rewrite this equation in differential
  3172. 2:34:35form
  3173. 2:34:40so if you are sloppy it means that you
  3174. 2:34:42take this Diffie and you bring it on the
  3175. 2:34:44other side
  3176. 2:34:45but in the financial form you see that
  3177. 2:34:48this is equal to
  3178. 2:34:502 Epsilon 0 over gamma
  3179. 2:34:54one minus two five five one minus five
  3180. 2:34:59times DC
  3181. 2:35:03so everything you have on the right
  3182. 2:35:05depends on fee everything you have on
  3183. 2:35:07the left depends on P tilde
  3184. 2:35:11and so now what you can do is to
  3185. 2:35:13integrate
  3186. 2:35:14both terms
  3187. 2:35:17so you integrate the right hand side
  3188. 2:35:19from sum Pi zero to some Phi
  3189. 2:35:22well let me call it five tilde
  3190. 2:35:26so that I integrate up to five
  3191. 2:35:29and the left hand side you integrate
  3192. 2:35:31from the corresponding value of the
  3193. 2:35:33distribution at Phi 0 and the one
  3194. 2:35:37fine
  3195. 2:35:39okay
  3196. 2:35:42and now these are integrals that you
  3197. 2:35:44know how to do so on the left hand side
  3198. 2:35:46you have a logarithm because you have
  3199. 2:35:48one over p
  3200. 2:35:50so you will get log of
  3201. 2:35:54field of Phi divided by
  3202. 2:35:5715.50
  3203. 2:36:01and on the right hand side we use
  3204. 2:36:04exactly the same trick
  3205. 2:36:06that I mentioned in the first exercise
  3206. 2:36:10so you have a quadratic expression
  3207. 2:36:13inside tilde in the denominator I want
  3208. 2:36:15to split it as we did
  3209. 2:36:17with the X1 X2 and here it's easy so
  3210. 2:36:21these you can write it I think as
  3211. 2:36:26simply this
  3212. 2:36:32you see that this matches exactly
  3213. 2:36:35and then you can integrate so these are
  3214. 2:36:37just logarithms
  3215. 2:36:39so if you integrate you have two apps
  3216. 2:36:42sign on zero gamma
  3217. 2:36:45and then you have the log of
  3218. 2:36:49I over Phi 0
  3219. 2:36:53minus but then the minus is already
  3220. 2:36:57is inside the derivative so this is the
  3221. 2:37:00derivative
  3222. 2:37:01of the log of 1 minus 5
  3223. 2:37:04so here I have a plus
  3224. 2:37:06log of 1 minus 5 divided by 1 minus 5 0.
  3225. 2:37:20and then while Phi 0 is arbitrary
  3226. 2:37:23so let me rewrite this as 2 Epsilon 0
  3227. 2:37:26gamma so this was the alpha that I
  3228. 2:37:28introduced before
  3229. 2:37:31then you have log of
  3230. 2:37:33Phi 1 minus 5 divided by Phi 0
  3231. 2:37:391 minus 5 0.
  3232. 2:37:41and then I can exponentiate right so if
  3233. 2:37:44I expunish it I get
  3234. 2:37:47my petilla
  3235. 2:38:05so PT La Phi will be some constant which
  3236. 2:38:08depends on this arbitrary Phi zero
  3237. 2:38:11which I just called C So eventually all
  3238. 2:38:13of the constants I will fix them by
  3239. 2:38:15normalization so I don't need to
  3240. 2:38:17keep track of what is the constant at
  3241. 2:38:20this stage and then I have Phi 1 minus
  3242. 2:38:22Phi
  3243. 2:38:26to the power of 2 Epsilon 0.
  3244. 2:38:30over gamma
  3245. 2:38:34but now I have to remember that this is
  3246. 2:38:36very scaled so this was tilde
  3247. 2:38:40so from here what is
  3248. 2:38:42I rescale back if you want my stationary
  3249. 2:38:46F5
  3250. 2:38:48is a is what is 1 over gamma which
  3251. 2:38:53is into my constant so I have a new
  3252. 2:38:55constant C Prime
  3253. 2:38:57and then I have a factor of 1 over 5 1
  3254. 2:39:00minus 5 in the denominator so this would
  3255. 2:39:02be
  3256. 2:39:05I will write it like this 5 1 minus 5
  3257. 2:39:09to the 1 minus
  3258. 2:39:11to Epsilon zero
  3259. 2:39:14over gamma
  3260. 2:39:18so all of the constants
  3261. 2:39:20which will not did not depend on Phi I
  3262. 2:39:23encoded them in C Prime
  3263. 2:39:26and the reason why I don't need to care
  3264. 2:39:28about those is that I can fix the global
  3265. 2:39:30constant Now by simply normalizing my
  3266. 2:39:34distribution so this is Step C
  3267. 2:39:41which is normalization
  3268. 2:39:46and this is a chance for me just to to
  3269. 2:39:48introduce
  3270. 2:39:49one identity that maybe is useful to
  3271. 2:39:52remember which is a gamma function but
  3272. 2:39:55anyway what I need
  3273. 2:39:56is that the integral
  3274. 2:39:59from 0 to 1 of my Phi
  3275. 2:40:03of my distribution
  3276. 2:40:05is equal to one and this is C Prime
  3277. 2:40:07integral from zero to one
  3278. 2:40:12of one over so actually now I will write
  3279. 2:40:16it 5.
  3280. 2:40:181 minus 5 to the
  3281. 2:40:21two Epsilon over gamma minus one in defy
  3282. 2:40:30okay so c will be the inverse of this
  3283. 2:40:32inter integral
  3284. 2:40:35and the reason why I'm writing it
  3285. 2:40:37explicitly is just to give you
  3286. 2:40:40something that you know so
  3287. 2:40:43this is an integral that is well known
  3288. 2:40:46in the literature it is related to the
  3289. 2:40:48so-called beta function
  3290. 2:40:50which in turns is related to the gamma
  3291. 2:40:53function so the gamma function
  3292. 2:40:55is a function which is defined in terms
  3293. 2:40:58of the following integral representation
  3294. 2:41:02T of x minus 1 e to the minus t
  3295. 2:41:07and the beta function so anytime you see
  3296. 2:41:09Phi x 1 minus X integrated between 0 and
  3297. 2:41:131.
  3298. 2:41:14it is almost always related to to this
  3299. 2:41:19beta function in here
  3300. 2:41:22which is precisely this t to the x minus
  3301. 2:41:251 1 minus t to the
  3302. 2:41:28y minus 1 in DT
  3303. 2:41:31and this is related to the gamma
  3304. 2:41:33function so you can show these are
  3305. 2:41:34identities
  3306. 2:41:36this is gamma of X gamma of Y divided by
  3307. 2:41:39gamma
  3308. 2:41:41of X Plus y
  3309. 2:41:45so using this you can compute
  3310. 2:41:48the normalization so you can find that c
  3311. 2:41:50Prime
  3312. 2:41:54is nothing but gamma of four
  3313. 2:41:57Epsilon zero
  3314. 2:42:00over a small gamma divided by gamma of
  3315. 2:42:04two Epsilon zero over gamma
  3316. 2:42:07so typically we don't care about the
  3317. 2:42:09normalization here I want to write it
  3318. 2:42:11down because I want to take now a limit
  3319. 2:42:13and discuss what happens when Epsilon 0
  3320. 2:42:16goes to zero
  3321. 2:42:19okay
  3322. 2:42:22so these are General identities
  3323. 2:42:25and what we also need is that
  3324. 2:42:30when X goes to zero your gamma function
  3325. 2:42:34is is Divergent so you you have
  3326. 2:42:39um a Divergence that you can compute
  3327. 2:42:41explicitly so you have an asymptotic
  3328. 2:42:44expansion when X
  3329. 2:42:45goes to zero which tells you that you
  3330. 2:42:47have a pole which goes like 1 over X
  3331. 2:42:50and then you have something of order one
  3332. 2:42:56okay now we use this just to comment a
  3333. 2:42:59little bit on the structure of the
  3334. 2:43:01solution
  3335. 2:43:05that we obtain and with this we finish
  3336. 2:43:08I think
  3337. 2:43:09foreign
  3338. 2:43:24so it's maybe two comments that are
  3339. 2:43:27related to point to the final point
  3340. 2:43:37so the first one is
  3341. 2:43:40that as we mentioned you have this
  3342. 2:43:42competition between Epsilon zero and
  3343. 2:43:45gamma
  3344. 2:43:45and you see that this emerges
  3345. 2:43:48in this combination in this ratio in the
  3346. 2:43:51distribution that you have so you have
  3347. 2:43:53Alpha
  3348. 2:43:55website on zero over gamma
  3349. 2:43:59and you have two situations for your
  3350. 2:44:01stationary distribution so
  3351. 2:44:08this goes from zero to one
  3352. 2:44:13so if Alpha is larger than one
  3353. 2:44:18then your distribution
  3354. 2:44:20is proportional to Phi 1 minus five so
  3355. 2:44:25let me rewrite it so be stationary
  3356. 2:44:29equals like Phi 1 minus five to the
  3357. 2:44:341 minus uh
  3358. 2:44:36Alpha minus one
  3359. 2:44:40so you see if Alpha is larger than one
  3360. 2:44:42the exponent is positive so you will
  3361. 2:44:44have something which vanishes at zero
  3362. 2:44:46and one and which is symmetric
  3363. 2:44:49with respect to one half and as a
  3364. 2:44:51maximum at one half so you expect
  3365. 2:44:53something like this
  3366. 2:44:59which means that if you think about your
  3367. 2:45:01animals half of those will likely go to
  3368. 2:45:05the source a half of those will likely
  3369. 2:45:07go to the source B and they will be more
  3370. 2:45:10or less evenly distributed but if Alpha
  3371. 2:45:13becomes smaller than one then your
  3372. 2:45:15distribution changes because now this
  3373. 2:45:17product goes into the denominator and so
  3374. 2:45:20you have a Divergence
  3375. 2:45:22at zero
  3376. 2:45:24and at one so your CC metric
  3377. 2:45:27but what I should use colors Maybe
  3378. 2:45:33you have something which
  3379. 2:45:35looks more like this for Alpha smaller
  3380. 2:45:37than one
  3381. 2:45:41and so this is the regime where you tend
  3382. 2:45:44to have uh
  3383. 2:45:46a very opinionated population if you
  3384. 2:45:48want so your population is either
  3385. 2:45:50strongly in favor of of the choice B
  3386. 2:45:53which corresponds to Phi equal to zero
  3387. 2:45:56or even strongly in favor of the choice
  3388. 2:45:58a which correspond to Phi equal to equal
  3389. 2:46:02to one and this is because the term
  3390. 2:46:05which corresponds to the noise which
  3391. 2:46:08pushes you toward this extrema is
  3392. 2:46:10winning with respect to the term which
  3393. 2:46:13corresponds to the drift that was given
  3394. 2:46:16by this spontaneous
  3395. 2:46:19change of opinions of of your population
  3396. 2:46:23and with all of the Expressions that we
  3397. 2:46:26derived you can even ask what happens in
  3398. 2:46:28the limit so this is the second comment
  3399. 2:46:35you can now take
  3400. 2:46:37the limit Epsilon going to zero
  3401. 2:46:42and in this limit so Alpha is going to
  3402. 2:46:46uh to zero and you get
  3403. 2:46:49so as you approach this limit
  3404. 2:46:54so should I do this
  3405. 2:46:58yes so with the expansion that I told
  3406. 2:47:00you up there
  3407. 2:47:03what you find from the normalization
  3408. 2:47:05constant is that
  3409. 2:47:08when Epsilon 0 is much smaller than one
  3410. 2:47:11this is going like one over Epsilon zero
  3411. 2:47:14I think
  3412. 2:47:18sorry this is going like
  3413. 2:47:21Epsilon 0
  3414. 2:47:26. so you see from this expression you
  3415. 2:47:28have a coefficient in front which goes
  3416. 2:47:30to zero when you send Epsilon 0 to 0 and
  3417. 2:47:33you have an exponent which is going to
  3418. 2:47:35zero so you have a term which is one
  3419. 2:47:37over five one minus pi times something
  3420. 2:47:39which is going to zero so this means
  3421. 2:47:41that as long as Phi is different from 0
  3422. 2:47:441
  3423. 2:47:45you are regular with this term and so
  3424. 2:47:48your distribution is going exactly to
  3425. 2:47:49zero in this limit except at the points
  3426. 2:47:52where Phi is equal to zero and Phi is
  3427. 2:47:54equal to one where you have a pole and
  3428. 2:47:56so your distribution is exploding so in
  3429. 2:47:58the limit if you picture this if you
  3430. 2:48:01make Epsilon 0 smaller and smaller you
  3431. 2:48:04start having distributions which become
  3432. 2:48:06more and more flat towards zero but then
  3433. 2:48:09which explode uh at zero one so this
  3434. 2:48:12means that your Phi stationary
  3435. 2:48:15in the limit
  3436. 2:48:16Epsilon going to zero converges to a
  3437. 2:48:19Delta
  3438. 2:48:20where all of your population
  3439. 2:48:24is either
  3440. 2:48:25in zero or it is either in one
  3441. 2:48:28with half an hour's probability so if
  3442. 2:48:31you average over time you will find or
  3443. 2:48:34over realizations you will find
  3444. 2:48:36that in half of your realization all of
  3445. 2:48:38your population chooses a in half of
  3446. 2:48:40your realizations all of your population
  3447. 2:48:42chooses B but they are somehow all
  3448. 2:48:45agreeing and there is not a well-defined
  3449. 2:48:49stationary distribution as you would get
  3450. 2:48:51uh
  3451. 2:48:53for
  3452. 2:48:54um in in the regime of parameters where
  3453. 2:48:57Alpha is non-zero
  3454. 2:48:59okay so this concludes and maybe
  3455. 2:49:02just the final comment
  3456. 2:49:05to comment on the first exercise
  3457. 2:49:09so for this type of model you can even
  3458. 2:49:11compute when Epsilon is different from
  3459. 2:49:14zero so this
  3460. 2:49:17says size three
  3461. 2:49:20when Epsilon is different from zero but
  3462. 2:49:21find it you still have let's say that
  3463. 2:49:24Alpha is smaller than one you still have
  3464. 2:49:25this distribution which is very
  3465. 2:49:27polarized
  3466. 2:49:30concentrating on zero and one
  3467. 2:49:34but in that case in in the Dynamics you
  3468. 2:49:36can still have
  3469. 2:49:38let's say uh
  3470. 2:49:40it is in this case if you start from
  3471. 2:49:42zero from one you speak to Zero part one
  3472. 2:49:45these are absorbing states of your
  3473. 2:49:49Dynamics in the case Epsilon 0 is is
  3474. 2:49:52positive you can still go from having
  3475. 2:49:55all of the population concentrated in
  3476. 2:49:56zero to having all of that concentrating
  3477. 2:49:59in one and you can compute what is the
  3478. 2:50:02switching time between these two uh
  3479. 2:50:06choices and you find that this is of the
  3480. 2:50:08order of one over two
  3481. 2:50:10uh Epsilon zero
  3482. 2:50:12so this we are not going to compute
  3483. 2:50:15but this is in a way
  3484. 2:50:18a little bit similar to this jump
  3485. 2:50:20calculation of the jump times that we
  3486. 2:50:23did in the first exercise and the
  3487. 2:50:25interesting thing is that this depends
  3488. 2:50:27only on Epsilon zero
  3489. 2:50:29and it does not depend on gamma
  3490. 2:50:32so on on the recruitment on the
  3491. 2:50:34discussion between your agents so in in
  3492. 2:50:36that situation which Epsilon 0 is small
  3493. 2:50:39you really have that one of your ants or
  3494. 2:50:43animals or or people changes its mind
  3495. 2:50:45and then you trigger a full Avalanche
  3496. 2:50:48where everybody else follows and you
  3497. 2:50:50jump from this situation to uh to this
  3498. 2:50:53situation so the Dynamics is is really
  3499. 2:50:55abrupt and this is related or similar to
  3500. 2:50:59avalanches
  3501. 2:51:03foreign in many other systems that are
  3502. 2:51:07complex
  3503. 2:51:09and with many agents
  3504. 2:51:13okay so I think that's enough
  3505. 2:51:17and the remaining exercise is as I said
  3506. 2:51:20it's a little bit different it goes back
  3507. 2:51:21to statistics but it's a nice way to see
  3508. 2:51:26an application of brown and motion so if
  3509. 2:51:28you have time have a look at that and
  3510. 2:51:30there is the arm work related to that
  3511. 2:51:32which is homework 8.
  3512. 2:51:36um and that's it so next time we will do
  3513. 2:51:39the final today I think
  3514. 2:51:44so is there any question otherwise
  3515. 2:51:51I will stop

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