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Complex Systems - Jean-Philippe Bouchaud - Lecture 6: Hawkes processes. Networks. — Transcript

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  1. 0:00this conference will now be recorded
  2. 0:06press the record button button
  3. 0:09and like last time sorry for that
  4. 0:13okay good so
  5. 0:15last time I told you about branching
  6. 0:17processes and Galton Watson model
  7. 0:20today I want to talk to you about horse
  8. 0:22processors
  9. 0:24I'll give you an introduction to network
  10. 0:26Theory speaking about yeah there's many
  11. 0:29networks which in a sense are very close
  12. 0:32to the Galton Watson process that I
  13. 0:35talked about and I'll expand on that and
  14. 0:38also the very famous by now but people
  15. 0:41call scale free Networks
  16. 0:44and then I'll talk about the giant
  17. 0:47components in these Networks and their
  18. 0:50resilience and this has a lot to do with
  19. 0:52uh
  20. 0:53uh efficiency of vaccination campaigns
  21. 0:56and all these uh
  22. 0:58interesting topics
  23. 1:00Okay so
  24. 1:02let me talk about hoax processes and
  25. 1:05I'll start by reminding you what
  26. 1:08question processes are
  27. 1:14so a question process is a sequence of
  28. 1:17events okay and this is the time axis
  29. 1:20and personal process are events that
  30. 1:23occur at random times so what does it
  31. 1:26really mean it means that
  32. 1:30um if you introduce
  33. 1:33accounts of the number of events that
  34. 1:36happen
  35. 1:37up to time T then each time something
  36. 1:41happens this n of P
  37. 1:43increased by one okay
  38. 1:46so you just count the number of events
  39. 1:48that occurred and you have something
  40. 1:50like this where each jump occurs as
  41. 1:54where one of these events takes place
  42. 1:57and so the randomness is defined by the
  43. 2:00fact that
  44. 2:01the probability that DN is equal to one
  45. 2:06is equal to at time T is equal to Lambda
  46. 2:11DT
  47. 2:12where Lambda is called the rate
  48. 2:16of the person process
  49. 2:19okay
  50. 2:21so this is very simple I mean things
  51. 2:23happen at random and on every little
  52. 2:26time interval DT there's a probability
  53. 2:28Lambda DT for something to happen and of
  54. 2:31course the probability that nothing
  55. 2:32happens
  56. 2:33is
  57. 2:361 minus Lambda DT
  58. 2:40okay
  59. 2:42so it's a very well known object and I'm
  60. 2:45sure many of you have seen it uh on many
  61. 2:48occasions so let me remind you a few
  62. 2:51basic properties of this question
  63. 2:54process
  64. 2:55so for example you can ask well I'm
  65. 2:58giving myself a time interval
  66. 3:01capital T
  67. 3:03okay
  68. 3:04and the question I'm asking is what is
  69. 3:07the probability P of n knowing T that I
  70. 3:12observed exactly n events in this
  71. 3:15interval of length capital T okay so in
  72. 3:19this particular case I observe six
  73. 3:21events
  74. 3:22but more generally I can ask the
  75. 3:24question and it's a little exercise for
  76. 3:27you if you want to derive it but it's
  77. 3:30very easy to show that this is given by
  78. 3:33what's called a poisson distribution
  79. 3:36so it's Lambda and Lambda t to the n
  80. 3:41exponential of minus Lambda T capital T
  81. 3:44divided by
  82. 3:46factorial n okay
  83. 3:49so this is just a consequence of the
  84. 3:52definition of the question process
  85. 3:54there's no correlation whatsoever
  86. 3:57between events and therefore you get you
  87. 4:00get this so for example
  88. 4:03and I've said that already several times
  89. 4:06before the average value of n is Lambda
  90. 4:10capital T this is pretty intuitive if
  91. 4:13Lambda is the rate of events per unit
  92. 4:15time so if you want this is the units is
  93. 4:18second minus one
  94. 4:20then in an interval of time of of length
  95. 4:24capital p uh they are on average Lambda
  96. 4:27T events
  97. 4:29and another property of personal
  98. 4:31processes is that the variance is equal
  99. 4:34to the mean
  100. 4:36so average value of N squared minus the
  101. 4:39average value of n
  102. 4:41squared is also Lambda T not squared
  103. 4:44Lambda t
  104. 4:47and so this leads to introduced to the
  105. 4:51introduction of a quantity that's that's
  106. 4:54quite interesting to consider in
  107. 4:57particular for practical application
  108. 4:59which is what I'm going to call the
  109. 5:01clustering ratio
  110. 5:10row and I'm going to define the
  111. 5:13clustering ratio by the the ratio of the
  112. 5:16variance
  113. 5:19over the mean
  114. 5:24and of course I'm going to go
  115. 5:27too far so let me move my camera already
  116. 5:31foreign
  117. 5:40process this is equal to one
  118. 5:45okay
  119. 5:47another interesting quantity that one
  120. 5:50can compute uh for personal processes
  121. 5:54is
  122. 5:55the insert time distribution so if I
  123. 5:58call S
  124. 5:59the difference between two consecutive
  125. 6:01events
  126. 6:03then it's easy again to show that P of s
  127. 6:07the probability to observe a certain
  128. 6:09interval between two consecutive events
  129. 6:12is
  130. 6:13a LaPlace distribution Lambda
  131. 6:16exponential minus Lambda s
  132. 6:21okay so these are my basic observations
  133. 6:25about
  134. 6:26personal processes
  135. 6:29shouldn't go too high
  136. 6:35and I'm going to tell you about various
  137. 6:39objects that are not personal processes
  138. 6:42and that need something different to be
  139. 6:46uh modeled with
  140. 6:57sorry I'm trying to find them right
  141. 7:00height
  142. 7:02okay
  143. 7:06a little bit
  144. 7:16so
  145. 7:18let me give an example of something that
  146. 7:22Ashley has a clustering ratio less than
  147. 7:26one
  148. 7:27and
  149. 7:28um and examples of things that have a
  150. 7:31clustering ratio larger than one
  151. 7:33so intuitively
  152. 7:35clustering ratio
  153. 7:40less than one
  154. 7:42means that the fluctuations
  155. 7:46are smaller than you would expect for a
  156. 7:48personal process okay so the way these
  157. 7:52events occur tend to be more regular
  158. 7:54than for a question process imagine for
  159. 7:58example that you have a perfectly
  160. 8:00regular set of events so these events
  161. 8:03occur not randomly but you know like
  162. 8:05every second exactly then
  163. 8:09for a very large T very large capital T
  164. 8:11there would be no fluctuations at all in
  165. 8:13the number of events and so the
  166. 8:16clustering ratio would be less than one
  167. 8:20so clustering less than one means that
  168. 8:23there's some kind of repulsion
  169. 8:27between events
  170. 8:29foreign
  171. 8:37so if something happens now
  172. 8:42it's less likely that something is going
  173. 8:44to happen just after that
  174. 8:47and a very well-known example of a set
  175. 8:50of points that follows
  176. 8:52um a repulsion type of process
  177. 8:57is the the set of eigenvalues of a
  178. 9:01random Matrix so if you take a large
  179. 9:03random Matrix and you diagonalize this
  180. 9:05random Matrix you can plot
  181. 9:08the eigenvalue
  182. 9:10like in quantum mechanics and if I plot
  183. 9:14the eigenvalues of a random Matrix
  184. 9:18I will find something that's much more
  185. 9:20regular than the personal process
  186. 9:22and this is called uh
  187. 9:26level repulsion
  188. 9:33and there's a long story about this in
  189. 9:36the
  190. 9:37Nuclear Physics literature fast this was
  191. 9:41introduced by wigner
  192. 9:43and and of course all
  193. 9:46the massive developments of random
  194. 9:48Matrix theory in the last 50 years a lot
  195. 9:51of that is about the precise description
  196. 9:54of the set of points so I won't go much
  197. 9:58into details but that's an example of
  198. 10:00clustering ratio lesson one
  199. 10:03and of course
  200. 10:05you know
  201. 10:07taking the the opposite of what I just
  202. 10:10said if you have a clustering ratio
  203. 10:12greater than one
  204. 10:14it means that uh fluctuations are larger
  205. 10:18than for a question process and this
  206. 10:21means that you have what's called
  207. 10:22clustering
  208. 10:29so on the contrary there are correlation
  209. 10:31between events if something happens it's
  210. 10:34more likely than for a personal process
  211. 10:37that something else happens very soon
  212. 10:38after and because of that you will have
  213. 10:42bursts of activity
  214. 10:44and then activity that's lower
  215. 10:48in such a way that the fluctuations of
  216. 10:50this of the number of events in the time
  217. 10:52interval is greater than one okay
  218. 10:57and so if you do this very simple test
  219. 11:00for several time series you realize that
  220. 11:03a lot of Time series that we are
  221. 11:06interested in in this uh in these
  222. 11:08lectures
  223. 11:09actually
  224. 11:10show some clustering properties so for
  225. 11:14example I told you about earthquakes
  226. 11:22and if you look at the time series
  227. 11:24of earthquakes then there's clear
  228. 11:27clustering I mean it's what people call
  229. 11:29aftershocks for example so we know that
  230. 11:32once an earthquake has happened somehow
  231. 11:35the crust the the crust of the earth
  232. 11:39it's rationalized and this leads to a
  233. 11:42higher probability to observe more
  234. 11:44earthquakes and in in what I'm going to
  235. 11:48talk to you about today hoax processors
  236. 11:50actually they were introduced by Mr
  237. 11:53Hawks in 72
  238. 11:56and uh it was in the context of
  239. 12:00uh earthquakes Dynamics
  240. 12:06so
  241. 12:07it is uh
  242. 12:10fair to associate as an example of
  243. 12:13clustering time series earthquakes as
  244. 12:15the primary ones but I told you about
  245. 12:18financial markets financial markets is
  246. 12:21also a prime example
  247. 12:24of clustering
  248. 12:27of activity so for example the activity
  249. 12:30in the financial markets is every time
  250. 12:32the price of a stock changes for example
  251. 12:35you can put a mark when the price
  252. 12:40changes
  253. 12:41and of course this um the the the means
  254. 12:45value of the activity rate the Lambda
  255. 12:48has increased over the years because as
  256. 12:51you know now uh people trade at the
  257. 12:54higher frequency so Lambda itself has
  258. 12:57increased but apart from this increase
  259. 13:00of activity when see something that has
  260. 13:02always been the case
  261. 13:04before uh high frequency trading before
  262. 13:08the electronization of markets and since
  263. 13:11then that hasn't changed is the fact
  264. 13:13that when the price when the price
  265. 13:15changes it's actually more probable that
  266. 13:18the price is going to change again very
  267. 13:20soon after
  268. 13:21and so you have this very very strong
  269. 13:23clustering I'm going to go back to that
  270. 13:26later
  271. 13:28in social sciences there's a very
  272. 13:31interesting story as well and hoax
  273. 13:33processors are used to model earthquake
  274. 13:37financial markets and some social
  275. 13:39sciences phenomena
  276. 13:43so for example a a case that's been
  277. 13:47studied empirically is is the case of
  278. 13:49riots
  279. 13:54so when you see
  280. 13:56um the way the Dynamics of Rise takes
  281. 13:58place it is clear that there is also uh
  282. 14:02in as in earthquakes in a sense the fact
  283. 14:04that when a riot has occurred then in
  284. 14:08the nearby City another ride tends to
  285. 14:10happen uh very close after and this was
  286. 14:13actually studied in detail in the case
  287. 14:16of what happened in France in 2005 there
  288. 14:19was a wave of riots uh some of you may
  289. 14:23remember in the suburbs of Paris and
  290. 14:26there is a very strong signal of
  291. 14:29clustering of these events
  292. 14:33okay so a lot of example of clustering
  293. 14:37starting from earthquakes and this has
  294. 14:40led Hawks to
  295. 14:43um
  296. 14:44provide a model
  297. 14:46a simple model for these clustering
  298. 14:48events
  299. 14:53that are named own
  300. 14:56these models as a box processors
  301. 15:15foreign
  302. 15:30processes are also called subordinated
  303. 15:35in a way that I'm going to define or
  304. 15:38donated
  305. 15:41question processes
  306. 15:44so what does that mean well it simply
  307. 15:46means that
  308. 15:48the personal process that I've
  309. 15:50considered up tuna had a fixed rate of
  310. 15:54events Lambda
  311. 15:56now I'm going to
  312. 15:57imagine that this person process has uh
  313. 16:01time varying
  314. 16:03rate of of events so
  315. 16:06the probability that DNT is equal to one
  316. 16:08is equal to Lambda T DT okay
  317. 16:14where Lambda T is now time dependent and
  318. 16:17the way it's time dependent is going to
  319. 16:20depend on what happened in the past
  320. 16:22so what hoax postulates
  321. 16:26is that Lambda t
  322. 16:28is equal to some
  323. 16:30base rate value mu
  324. 16:34which is going to be constant
  325. 16:36Plus
  326. 16:38the sum over all past events
  327. 16:42so I'm going to write TJ is the time at
  328. 16:45which the JS Event happened and so it's
  329. 16:49the sum Over All J's such that TJ is
  330. 16:52less than T of a sudden kernel k
  331. 16:56of T minus t j
  332. 17:01and K
  333. 17:03is the Hulk's kernel as a function of
  334. 17:06the lag Tau between
  335. 17:08the event that happened in the past and
  336. 17:10now
  337. 17:11this kernel K of tar
  338. 17:14is a certain decaying function
  339. 17:18for example
  340. 17:21exponential
  341. 17:25so for example I'm going to take a
  342. 17:28just after that
  343. 17:31a specific example where K of tar is
  344. 17:34exponential of minus
  345. 17:36Alpha Tau
  346. 17:38but it could be something else
  347. 17:40so what it means is that
  348. 17:43you're very affected by events that just
  349. 17:46happened
  350. 17:47which increase the probability of having
  351. 17:50something happening again
  352. 17:52but far away events so when T minus DJ
  353. 17:55becomes
  354. 17:57in this case much larger than one over
  355. 17:59Alpha then you tend to forget
  356. 18:02these past events okay
  357. 18:06so this is if you want
  358. 18:08what people it's called an influence
  359. 18:11kernel as well
  360. 18:15which means to insist on the fact that
  361. 18:18it's the influence of past events on the
  362. 18:21current level of activity
  363. 18:23and mu is a Baseline
  364. 18:27level
  365. 18:30okay
  366. 18:33so there's another way to rewrite this
  367. 18:36equation which in some cases is the
  368. 18:39useful so let me rewrite this as an
  369. 18:42identity as Mu the same Plus instead of
  370. 18:46having a discrete sum I'm going to write
  371. 18:49this as an integral it's minus integral
  372. 18:52from minus infinity to T
  373. 18:54of GNT Prime
  374. 18:58k
  375. 18:59of T minus t Prime
  376. 19:04okay and you see it's the same because
  377. 19:07BNT Prime this is equal to uh one if
  378. 19:12something happened
  379. 19:16if if there's an event at C Prime and
  380. 19:19zero if not okay
  381. 19:25so let me give you a few uh properties
  382. 19:28of this
  383. 19:29um
  384. 19:31of this model
  385. 19:33the first property is what happens for
  386. 19:36the average rate of events in this model
  387. 19:39so you see that Lambda now is time
  388. 19:42dependent
  389. 19:44so
  390. 19:46if I if I
  391. 19:47make a little drawing
  392. 19:50of Lambda t as a function of t
  393. 19:54then Lambda T is going to look look like
  394. 19:57this a little bit
  395. 20:01okay
  396. 20:02and so you already see uh clustering by
  397. 20:06the eye because there are moments where
  398. 20:08Lambda is going to be larger so many
  399. 20:11things will happen around these times
  400. 20:13but I can Define the average value of
  401. 20:16Lambda
  402. 20:18across time
  403. 20:21so that would be what I call Lambda bar
  404. 20:23okay this is the average level of
  405. 20:26activity
  406. 20:27when I average across time
  407. 20:30so one can show that in certain
  408. 20:33condition this hoax process is ergotic
  409. 20:36which means that I can think of Lambda
  410. 20:39bar either as a Time average or as a as
  411. 20:43an ensemble average in the sense that
  412. 20:45you see that things are all random here
  413. 20:48things happen at random so Lambda T is a
  414. 20:52random quantity
  415. 20:58it's random because it depends on random
  416. 21:00events and these random events are the
  417. 21:04underlying question process so you see
  418. 21:06why we one why this is called the
  419. 21:09subordinated platform process is because
  420. 21:11conditional to Lambda T is a personal
  421. 21:14process but it is subordinated on
  422. 21:18another process which in this case self
  423. 21:21consistently depends on the process
  424. 21:22itself okay
  425. 21:26so
  426. 21:27uh
  427. 21:29what happens if I try to compute uh lamb
  428. 21:32that the average value of Lambda well
  429. 21:35let me take the average of this equation
  430. 21:37here
  431. 21:40and what I get
  432. 21:42on the left hand side is Lambda bar by
  433. 21:44definition
  434. 21:46and on the right hand side I have mu
  435. 21:48plus and here I'm going to use this
  436. 21:52um expression
  437. 21:54and in this expression I'm going to note
  438. 21:56that the average value of BT DNC Prime
  439. 22:00this is equal
  440. 22:02to Lambda bar DG Prime
  441. 22:06well TT
  442. 22:10okay
  443. 22:11so
  444. 22:13what I get by take make taking the
  445. 22:15average of both sides of this equation
  446. 22:17is
  447. 22:20an equation where I get Lambda bar in
  448. 22:22both sides of the equation
  449. 22:30this is what I get
  450. 22:32okay
  451. 22:34and so I'm going to give a name
  452. 22:37to this integral over T Prime
  453. 22:41so you see first that I I can always
  454. 22:43change variables I can always call T
  455. 22:45minus t Prime Tau
  456. 22:48like I did in my drawing
  457. 22:50and this integral
  458. 22:52over T Prime from minus infinity T to T
  459. 22:55of K of T minus P Prime this is also
  460. 22:58equal to Lambda bar
  461. 23:01integral from 0 to Infinity D Tau KF
  462. 23:06Style
  463. 23:08okay
  464. 23:11so let me rewrite this equation
  465. 23:18here
  466. 23:38so what I get is Lambda bar
  467. 23:41equals mu
  468. 23:43plus Lambda Bar times what I'm going to
  469. 23:47call r0
  470. 23:48and of course I'm not using this
  471. 23:51notation uh randomly with r0
  472. 23:56which is defined as the integral from 0
  473. 23:58to Infinity
  474. 23:59beta of K of Tau
  475. 24:04and therefore you see that Lambda bar
  476. 24:07is equal to Mu over 1 minus r0
  477. 24:14okay well if you see this expression you
  478. 24:17see that it can only make sense if r0 is
  479. 24:20less than one
  480. 24:27because otherwise you find the Lambda
  481. 24:29bar which is negative which doesn't make
  482. 24:31sense and in this case when r0 is
  483. 24:34greater than one it means that the
  484. 24:36feedback is so strong that actually the
  485. 24:39process diverges
  486. 24:41there's no stationary State here I've
  487. 24:44assumed I got this t as I've mentioned
  488. 24:46before and this assumes that the process
  489. 24:49enters some kind of stationary state but
  490. 24:52if r0 is larger than one then each event
  491. 24:56affects so strongly the future rate of
  492. 24:59events that the process kind of gets
  493. 25:03self-excited so much that it runs the
  494. 25:06way to Infinity
  495. 25:08and actually I've used the term that's
  496. 25:10often used in this context which is
  497. 25:13self-excited process
  498. 25:17okay
  499. 25:23so K of tau is the self-excitation
  500. 25:26feedback which makes the the system uh
  501. 25:31interesting but potentially unstable
  502. 25:34so if r0 is greater than one
  503. 25:39the ox process is unstable
  504. 25:55so there's a lot of things that one can
  505. 25:57do with these uh polks processes they're
  506. 26:00they're actually very very nice from a
  507. 26:02mathematical point of view you can
  508. 26:03compute all sorts of things exactly
  509. 26:06for example you can compute correlation
  510. 26:09functions here I've computed the average
  511. 26:11but I can also compute correlation
  512. 26:13functions and correlation functions are
  513. 26:16going to be needed if you want to
  514. 26:18measure the variance because a variance
  515. 26:21is directly related to the second the
  516. 26:24two point correlation function of the
  517. 26:25process
  518. 26:27so one can do that one can actually very
  519. 26:30easily calibrate this process on data
  520. 26:32and that's why it's very successful in
  521. 26:35the literature there's a long list now
  522. 26:37of Time series on which people have
  523. 26:40tried to fit
  524. 26:42uh hoax processes
  525. 26:45and in particular what's really
  526. 26:46interesting about
  527. 26:49um
  528. 26:50the the two point function is the
  529. 26:53clustering ratio
  530. 26:55which is a summary of the two point
  531. 26:57function if you want and in this case
  532. 27:01it's actually uh well not completely
  533. 27:05trivial but one can show and I I'm not
  534. 27:08showing here
  535. 27:09so let me insist that it's not proven
  536. 27:11here
  537. 27:14and those who are interested uh I can
  538. 27:17give you some literature but it's not
  539. 27:19completely trivial actually
  540. 27:21is that for hoax processes row is given
  541. 27:24by one over one minus r0
  542. 27:28squared
  543. 27:34so what's nice about this result
  544. 27:38is that as you see rho this clustering
  545. 27:41ratio is independent
  546. 27:46of mu
  547. 27:48and
  548. 27:50of KF Tau
  549. 27:53except from the norm of K of Tau so what
  550. 27:57I'm saying is that
  551. 27:58you don't care about the detailed shape
  552. 28:01of K of Tau the only thing you care
  553. 28:03about
  554. 28:04except
  555. 28:06r0 of course
  556. 28:08so once you know the the norm of K
  557. 28:12then you don't need to know anything
  558. 28:15else you don't need to know mu either
  559. 28:17so you don't need to know the the
  560. 28:19underlying
  561. 28:21um uh based level Baseline level of
  562. 28:25activity you can derive the value of r0
  563. 28:29from the measurement of row only okay
  564. 28:32because for example imagine that you say
  565. 28:35but here I maybe that's a way to measure
  566. 28:38r0 well it's not because that priority
  567. 28:41you don't know what mu is okay
  568. 28:43so what's nice about the
  569. 28:46clustering ratio is that all reference
  570. 28:49to the details of the hoax process that
  571. 28:52is Mu or the detail shape of K is
  572. 28:56actually disappeared so you can have an
  573. 28:59idea of the value of r0 just but by
  574. 29:02looking at the clustering ratio
  575. 29:05so let me give you two limits
  576. 29:08one is the limit where r0 goes to zero
  577. 29:13so what happens if kl0 goes to zero well
  578. 29:15you see that if r0 goes to zero it means
  579. 29:18that somehow
  580. 29:20there's no feedback and what we recover
  581. 29:23is the poisson result row tensor on
  582. 29:28but what's more interesting is the case
  583. 29:31when r0 a goes to one
  584. 29:35by the way you know I haven't insisted
  585. 29:38on that but clearly this formula shows
  586. 29:41that it's always greater or equal to one
  587. 29:44right
  588. 29:45so there's always clustering in the Box
  589. 29:47processes
  590. 29:49which is what we wanted we wanted to
  591. 29:52describe
  592. 29:53um uh a clustering a model with
  593. 29:58clustering and let me come back to
  594. 30:00something I haven't said I should have
  595. 30:02said before in a second which is I'm
  596. 30:05assuming that K is is strictly positive
  597. 30:07here
  598. 30:08and if K is negative then the model is
  599. 30:12not very well defined so here I should
  600. 30:15have said that
  601. 30:17k
  602. 30:19is
  603. 30:20is positive
  604. 30:22so it's really something that describes
  605. 30:25self-excitation and not self-inhibition
  606. 30:30um
  607. 30:31so when all zero goes to 1 then you see
  608. 30:33from the formula that rows goes to
  609. 30:35Infinity
  610. 30:39and so what's surprising
  611. 30:42is that if you calibrate the hoax
  612. 30:44process to financial markets you find
  613. 30:50that
  614. 30:52r0 is indeed very close to one
  615. 31:02and this is interesting because it means
  616. 31:04that somehow financial markets are
  617. 31:07extremely fragile you see that our zero
  618. 31:10equal one again is the uh is the
  619. 31:13boundary between the stable process and
  620. 31:16an unstable process if the process would
  621. 31:19be slightly more
  622. 31:21self-exciting then it would be unstable
  623. 31:23and for some reason which are not which
  624. 31:27is not completely clear even at this
  625. 31:29stage
  626. 31:30financial markets if you calibrate them
  627. 31:33with a question with a hoax process
  628. 31:36systematically gives gives you values of
  629. 31:39r0 which are close to one suggesting
  630. 31:43um you know
  631. 31:45close to instability that
  632. 31:48financial markets are
  633. 31:50toys at the verge of instability
  634. 31:58so of course you could say well maybe
  635. 32:00it's because the Hawks process is not a
  636. 32:01good model for financial markets and
  637. 32:03that by calibrating your hoax model
  638. 32:05which is not the right model you get of
  639. 32:08zero close to one and that may well be
  640. 32:10but I'm just pointing that out to you
  641. 32:14which is a very interesting I think
  642. 32:16observation is that when calibrated to
  643. 32:21financial markets
  644. 32:23one finds a a kind of incipient
  645. 32:27instability
  646. 32:28from the model
  647. 32:31which goes actually hand in hand with
  648. 32:34many things I told you about financial
  649. 32:35markets already it seems that you know
  650. 32:38there are parallel distributions
  651. 32:40crashes happen all the time so maybe all
  652. 32:43this is related to some kind of
  653. 32:45intrinsic instability
  654. 32:48um
  655. 32:51of financial markets at least this is a
  656. 32:54this is something that researchers are
  657. 32:56investigating
  658. 32:58now is trying to understand whether or
  659. 33:02not there are good reasons for financial
  660. 33:04markets to be close to a critical point
  661. 33:10okay so let me finish this chapter on
  662. 33:14Hawke's processes by
  663. 33:16uh giving you
  664. 33:19the example of
  665. 33:21KF Tau
  666. 33:25exponential so if I write K of pi equal
  667. 33:28r0
  668. 33:29uh Alpha exponential of minus Alpha Tau
  669. 33:35then I've normalized it correctly in
  670. 33:38such a way that
  671. 33:40um it starts at r0 Alpha here
  672. 33:44and the area is is given by r0
  673. 33:50then let me give again
  674. 33:52the the equation Lambda T is Mu plus
  675. 33:56integral up to T
  676. 33:58of um
  677. 34:00DT DNT Prime
  678. 34:04K of T minus D Prime
  679. 34:11and the exponential uh distribution the
  680. 34:14exponential shape of K of tau is an
  681. 34:16interesting property which is always you
  682. 34:19know the things that work well with
  683. 34:21exponential is that if I take the
  684. 34:24derivative of this equation with respect
  685. 34:27to time
  686. 34:28then
  687. 34:31e Lambda T DT
  688. 34:34then I'm not going to you know detail
  689. 34:37the calculation it's it's uh easy enough
  690. 34:39to do what you get is
  691. 34:43minus Alpha
  692. 34:46Lambda T minus mu
  693. 34:50this comes from the the the derivative
  694. 34:54of K with respect to T and using the
  695. 34:58fact that K is an exponential which
  696. 35:00actually reproduces Lambda T minus mu
  697. 35:04and then Plus
  698. 35:07r0
  699. 35:12Alpha
  700. 35:15GNT DT
  701. 35:21and so what we know is that DNT
  702. 35:25is a is is a conditional question
  703. 35:28process
  704. 35:29so GNT
  705. 35:33can be written as a deterministic part
  706. 35:37which is related to the average value of
  707. 35:40VNT which by definition is Lambda T DT
  708. 35:44plus the fluctuating part
  709. 35:47and the fluctuating part so if you if
  710. 35:51you think of this process in a kind of
  711. 35:52coarse grain manner you see that the
  712. 35:55average value of the NT conditions to
  713. 35:57Lambda T is Lambda T DT but there are
  714. 36:00fluctuations
  715. 36:01and the fluctuations of a personal
  716. 36:03process is proportional out proportional
  717. 36:06to the rate of event so the the
  718. 36:09fluctuations can be written as
  719. 36:12PSI some noise
  720. 36:14square root of Lambda T DT
  721. 36:18so here I'm cheating a little bit
  722. 36:19because
  723. 36:20um
  724. 36:21this this is not very rigorous but I'm
  725. 36:23writing I mean DNT is either zero or one
  726. 36:26so in order to go from here to there I'm
  727. 36:30kind of course grading the system and
  728. 36:32applying a kind of central limit theorem
  729. 36:34to DNT so you see what I'm going and
  730. 36:37what I'm trying to give you here is not
  731. 36:38a mathematical proof although everything
  732. 36:41that I'm going to say can be shown to be
  733. 36:44rigorous in some limits but it's just a
  734. 36:48an intuition about what's going on in
  735. 36:50this model so what I'm saying is that
  736. 36:52this dntdp is going to be is going to
  737. 36:55have an average value Lambda T and
  738. 36:58fluctuation
  739. 37:00and so if I follow this thing at least
  740. 37:03naively
  741. 37:04what you get is that there's a piece
  742. 37:08here of this guy which is going to add
  743. 37:12to this one
  744. 37:14and a piece that's going to remain as a
  745. 37:17noise
  746. 37:18so again
  747. 37:20I'm not dictating the calculation that
  748. 37:22what you get by regrouping terms
  749. 37:26is minus alpha 1 minus r0
  750. 37:30Lambda T minus Lambda bar
  751. 37:35where Lambda bar is the Lambda bar that
  752. 37:37I defined before it's it's it's mu
  753. 37:40divided by 1 minus r0
  754. 37:45so actually here Lambda Bar times 1
  755. 37:48minus r0 is just the MU guy that you had
  756. 37:51here
  757. 37:52and the Lambda t one minus r0 comes from
  758. 37:56this sum plus the one coming from there
  759. 38:01Plus
  760. 38:03are zero
  761. 38:05Alpha
  762. 38:07square root of Lambda t
  763. 38:10times the noise PSI
  764. 38:15a large band noise let me call it ETA
  765. 38:18this is a larger noise
  766. 38:24you remember larger noise are
  767. 38:25ill-defined there of all the one over
  768. 38:27square root of DT and this is what you
  769. 38:30would get from here dividing by DT gives
  770. 38:33you a noise that's one over square root
  771. 38:35of DT so it's a large amount of noise
  772. 38:39okay so that's where I wanted to uh
  773. 38:43to arrive at because what you see is
  774. 38:47that you have a differential equation
  775. 38:49which is such that
  776. 38:52there's an average
  777. 38:54so what does this stochastic
  778. 38:56differential equation mean it means that
  779. 38:58Lambda T is fluctuating around Lambda
  780. 39:02bar you see this is a mean reversion
  781. 39:04term this is a kind of harmonic
  782. 39:05calculate oscillator term which
  783. 39:08a pool's Lambda T back to its average
  784. 39:11value so we already know that we already
  785. 39:13know that Lambda T fluctuates around an
  786. 39:17average value Lambda T but the strength
  787. 39:20of the reversion
  788. 39:22is decreased as r0 approaches one
  789. 39:28so if you want to see it simply you see
  790. 39:32that alpha 1 minus r0 is the time scale
  791. 39:35of the of the mean reversion
  792. 39:37you see dimensionally one alpha one
  793. 39:40minus r0 is the frequency
  794. 39:42and so this is the relaxation time
  795. 39:46or the inverse relaxation time
  796. 39:52and the in-house relaxation time is 1
  797. 39:54over Alpha One minus r0
  798. 40:00so this is you know if if I write here
  799. 40:03in a corner something that
  800. 40:07if I write a harmonic oscillator D
  801. 40:10Lambda T equals minus Omega
  802. 40:12Lambda T minus Lambda bar
  803. 40:15plus noise
  804. 40:18this is also called the Ornstein
  805. 40:21ullenbeck process then one knows that
  806. 40:24one over Omega is the characteristic
  807. 40:26time scale of the relaxation of such a
  808. 40:29process you can show it very easily so
  809. 40:32what plays the role of Omega here is
  810. 40:35Alpha One minus r0 so I get the
  811. 40:37relaxation time that is 1 over alpha 1
  812. 40:40minus r0
  813. 40:41so what it means is that when r0 goes to
  814. 40:43one
  815. 40:48you have two things happening at the
  816. 40:50same time you have that Lambda bar
  817. 40:53diverges
  818. 40:57so the process becomes more and more
  819. 40:58intense
  820. 40:59but at the same time
  821. 41:01the relaxation time of the process
  822. 41:04diverges as well
  823. 41:07so relaxation time
  824. 41:11also
  825. 41:15so this is this is a process this is a
  826. 41:17phenomenon that's very usual in
  827. 41:20statistical mechanics model where the
  828. 41:23approach to a critical point because r0
  829. 41:25equal one is a critical point it's a
  830. 41:27point Beyond which the model is unstable
  831. 41:31then at the same time there's something
  832. 41:34that diverges which here is the average
  833. 41:38rate of events so in a physical system
  834. 41:41it's often for example the
  835. 41:42susceptibility of the system that
  836. 41:44diverges and at the same time the
  837. 41:47relaxation time the speed of at which
  838. 41:50the system relaxes to equilibrium also
  839. 41:53diverges and that's what you see uh
  840. 41:56simply coming out
  841. 41:58of this equation and that was not clear
  842. 42:01from the
  843. 42:03quantities I've told you about earlier
  844. 42:06here one has on top of these results on
  845. 42:11Lambda bar and rho one has a result on
  846. 42:13the relaxation time
  847. 42:15so how this folks processes
  848. 42:19evolve with time really and we see that
  849. 42:22close to criticality they actually
  850. 42:23becomes very slow
  851. 42:27so the other thing I wanted to tell you
  852. 42:31is that there's a very close analogy
  853. 42:33between hoax processes
  854. 42:35and uh
  855. 42:37the
  856. 42:38Gelson Watson branching process that
  857. 42:40I've told you about one way to think
  858. 42:44about it is just looking at this
  859. 42:46equation here and this equation in a
  860. 42:50very precise mathematical way can be
  861. 42:53shown to mean that there are ancestors
  862. 42:57arriving in the system at right mu
  863. 42:59and then these ancestors they give rise
  864. 43:02to children
  865. 43:03and they give rise to Children exactly
  866. 43:06like in the Calvin Watson process and so
  867. 43:10what you get what you gain compared to
  868. 43:12the Galton Watson process here is that
  869. 43:15you have some time Dimension that allows
  870. 43:18you to to know exactly when these
  871. 43:21children get born if you want but in
  872. 43:24terms of the structure of the families
  873. 43:27um it's everything that happens
  874. 43:29underlying this model is the same as
  875. 43:31what happens in the gelton Watson
  876. 43:33process
  877. 43:35and one way to realize that this is the
  878. 43:37case
  879. 43:38is looking at this equation again
  880. 43:42and if you remember I told you that the
  881. 43:45Galton Watson process in the continuing
  882. 43:47continuous time limit had a term a
  883. 43:50growth term proportional to
  884. 43:52r0 minus one Lambda which is what I
  885. 43:56wrote last time I wrote something like
  886. 43:57oh 0 minus one
  887. 43:59n so that was the vndt
  888. 44:04and then a fluctuation term which is
  889. 44:07proportional to square root of n
  890. 44:11so I told you last time this is the
  891. 44:13continuous time limit of the Gauss and
  892. 44:14Watson process and you see that it's uh
  893. 44:17very very similar here
  894. 44:19so it's just a hint that these two
  895. 44:22models are very closely related
  896. 44:25I realized that there's something I
  897. 44:26didn't tell you uh to justify my
  898. 44:30my Mumble here about taking a a cause
  899. 44:35graining I mean in making this bold
  900. 44:39interpretation of the NDT as a noise
  901. 44:43actually it becomes more and more
  902. 44:45Justified to do this as the process
  903. 44:47becomes slower and slower so when r0
  904. 44:50goes to 1 as I just said the relaxation
  905. 44:53time goes to Infinity the system becomes
  906. 44:55slower and slower and so I I it it is
  907. 44:59possible to make a change of scale
  908. 45:02to read to cosgrain the system if you
  909. 45:04want and to actually think of this ENT
  910. 45:07as a gaussian process in the limit
  911. 45:09because the process is very slowly
  912. 45:12evolving so on the time scale of the
  913. 45:15evolution of the process I can aggregate
  914. 45:17many of these DNT which are only zero or
  915. 45:21one and by aggregating them I get what I
  916. 45:25wrote here which is a The Continuous
  917. 45:28time gaussian process
  918. 45:30so for those of you who are worried by
  919. 45:32my Cavalier way of handling this term
  920. 45:35it's actually everything is is well
  921. 45:37defined and justified in the limit when
  922. 45:39r0 goes to one and in that limit the
  923. 45:42process is equivalent to a critical
  924. 45:45branching process
  925. 45:51okay so let me leave hooks processes and
  926. 45:55go to networks now
  927. 45:57um the the only thing I wanted to tell
  928. 46:00you before leaving them is that hooks
  929. 46:03processes can be generalized in many
  930. 46:05ways so for example you can have a
  931. 46:09multi-dimensional hoax process you can
  932. 46:11have you can add indices you can have
  933. 46:15n
  934. 46:17processes happening simultaneously so
  935. 46:19for example imagine the activity of n
  936. 46:22different stocks in the stock market
  937. 46:24and then you can add
  938. 46:28vectorial
  939. 46:35and a matrix for generalization of these
  940. 46:38talks processes saying that what happens
  941. 46:40on I is affected by what happened on J
  942. 46:43mediated by an influence kernel that now
  943. 46:46is becomes a matrix
  944. 46:48in the stock space
  945. 46:50and has some time dependence so the
  946. 46:54whole artillery can be generalized to
  947. 46:57many cases and this is one of the case
  948. 47:01that's been considered in the literature
  949. 47:04okay
  950. 47:26so hoax processes are important because
  951. 47:28they can be calibrated to data and
  952. 47:30they're important because they are very
  953. 47:32closely related to
  954. 47:34branching processes
  955. 47:39so now let me
  956. 47:43leave or apparently leave what I told
  957. 47:47you about branching processes but you'll
  958. 47:49see that will soon recover them in
  959. 47:52another uh
  960. 47:54Incarnation and go to
  961. 47:58Network Theory
  962. 48:09so
  963. 48:10the reason people are very interested in
  964. 48:14networks is that their networks
  965. 48:17everywhere around us and they're
  966. 48:19extremely relevant in many uh
  967. 48:22situations for example electric grids or
  968. 48:26networks of cables and nodes which are
  969. 48:30the the places where electricity is is
  970. 48:33produced
  971. 48:34there's a physical example that you all
  972. 48:36know well which which is polymer gels
  973. 48:40for example uh the white of an egg is a
  974. 48:44liquid when the polymers are independent
  975. 48:47but then when you heat uh white the
  976. 48:51white of an egg then these polymers
  977. 48:54um
  978. 48:55attached to each other
  979. 48:57they create a kind of network
  980. 49:00and once the network is completed the
  981. 49:03object is is solid it's it's not not a
  982. 49:07liquid anymore and this is related to
  983. 49:09the phenomenon of calculation which I'm
  984. 49:12going to talk about so in the in the
  985. 49:14case of uh the why the the the white of
  986. 49:17an egg it's really interesting because
  987. 49:18one sees a transition that will comment
  988. 49:22later between a case where the network
  989. 49:25is made of disconnected clusters
  990. 49:28and it's in the case of Jag it's a
  991. 49:30liquid and the case when there is a
  992. 49:33giant component
  993. 49:35where the the network includes a very
  994. 49:39large number of different molecules and
  995. 49:43in the physical sense it's a it's a
  996. 49:45solid
  997. 49:47so social networks of course no need to
  998. 49:50speak about them social networks whether
  999. 49:53they are virtual like Facebook or other
  1000. 49:56type of social network or actual
  1001. 49:59physical Networks
  1002. 50:00networks created by contacts between
  1003. 50:03people and you know your social network
  1004. 50:06in the sense of who you meet every day
  1005. 50:09is of course extremely important in in
  1006. 50:12in view of uh of pandemic transmission
  1007. 50:15and so on
  1008. 50:17but there are also economic networks
  1009. 50:20like banking networks pool lens to whom
  1010. 50:23some networks who produces what so
  1011. 50:27that's called the input output Network
  1012. 50:29some firms produce Goods that are useful
  1013. 50:32for other firms who themselves produce
  1014. 50:35uh things so there's a network of
  1015. 50:39interaction between firms there are
  1016. 50:42ecological Networks
  1017. 50:44so some species eat other species so
  1018. 50:48there's a predator for prey relation
  1019. 50:49between species and all these networks
  1020. 50:53are crucial to understand emerging
  1021. 50:56phenomena
  1022. 50:57because depending on the on on the
  1023. 51:00property of the underlying networks you
  1024. 51:01can have in the case of kovitz for
  1025. 51:04example you can have either propagation
  1026. 51:07across the whole population or only
  1027. 51:10limited clusters of infection and in the
  1028. 51:13case of the wife of an egg as I said you
  1029. 51:16can either be in a liquid phase or in a
  1030. 51:20in a solid state there are many many
  1031. 51:22other examples like
  1032. 51:24and if you put conductors at random in
  1033. 51:29space you only have little islands of
  1034. 51:31conductors that overall do not conduct
  1035. 51:33electricity or is there a giant
  1036. 51:36component which allows the whole thing
  1037. 51:38to become carrying electricity from one
  1038. 51:42side to the other
  1039. 51:43of the samples
  1040. 51:45so there's a huge
  1041. 51:47um
  1042. 51:49incentive to understand the properties
  1043. 51:52of networks in general
  1044. 51:55so a network is made of nodes
  1045. 52:01okay so I have nodes
  1046. 52:04and I have links or edges
  1047. 52:07okay
  1048. 52:10so for example this is a network that
  1049. 52:14contains two clusters
  1050. 52:20so I'm going to use the terms edges or
  1051. 52:23links
  1052. 52:24to mean the same thing
  1053. 52:28and so you see here that
  1054. 52:30an ensemble of nodes that are
  1055. 52:33such that I can go from anyone to any
  1056. 52:37other one following edges is called the
  1057. 52:40cluster
  1058. 52:45and the question is do I have in my
  1059. 52:48network a lot of small independent
  1060. 52:51clusters or do I have on top of small
  1061. 52:54clusters do I have a giant cluster which
  1062. 52:57in this case would be something like
  1063. 53:00this which involves
  1064. 53:02maybe not all the nodes but at least the
  1065. 53:05finite fraction of all the nodes
  1066. 53:08so I will speak more about giant
  1067. 53:10components later but you have an
  1068. 53:12intuitive feeding already at this level
  1069. 53:14is to know whether there is a cluster
  1070. 53:18that covers a finite fraction of the
  1071. 53:21number of nodes in the limit Square this
  1072. 53:23number goes to infinity or if I only
  1073. 53:25have you know either isolated guys and
  1074. 53:29of course I can have a mixture of both
  1075. 53:30things for example in this case I would
  1076. 53:33have a big cluster and an isolated
  1077. 53:35cluster but of course this is hand
  1078. 53:37waving and one has to make more precise
  1079. 53:40statement later on okay
  1080. 53:44so I'm going to give you two ways to
  1081. 53:46construct these networks one
  1082. 53:50is the simplest and the oldest random
  1083. 53:54construction of network which is called
  1084. 53:57the the random range the Erdos Raini
  1085. 54:00Networks
  1086. 54:07and then
  1087. 54:08I'll give you another type of
  1088. 54:10construction which leads to in a sense
  1089. 54:12more interesting graphs which are scale
  1090. 54:15free Networks
  1091. 54:18okay so another training Network how's
  1092. 54:20how does that work
  1093. 54:22well so imagine that you have
  1094. 54:27end node
  1095. 54:35I pick at random a pair of nodes for
  1096. 54:38example this one and this one i j
  1097. 54:42and for each of these possible pair I
  1098. 54:45decide that there is a link
  1099. 54:47with probability p over n
  1100. 54:50and there is no link with probability 1
  1101. 54:53minus t over n
  1102. 54:55okay
  1103. 54:58so this is my Construction
  1104. 55:01it's only independent every link is
  1105. 55:03independent
  1106. 55:04I mean every potential link is
  1107. 55:06independent
  1108. 55:07and it becomes filled with probability p
  1109. 55:10over n
  1110. 55:12and it's left empty with probability 1
  1111. 55:14minus p over n
  1112. 55:16so you might ask why do I put a p over n
  1113. 55:19here
  1114. 55:21well it's because I want the model to
  1115. 55:23remain well defined in the limit when n
  1116. 55:25goes to Infinity
  1117. 55:27and if you think for two seconds you
  1118. 55:29realize that for each node there are n
  1119. 55:33minus one possible Neighbors
  1120. 55:36and since each
  1121. 55:38Edge is present with product DP over n
  1122. 55:42the average degree
  1123. 55:45so the average number of Neighbors
  1124. 55:56is given by P over n times n minus 1
  1125. 56:00. so for large n
  1126. 56:03this is equal to p
  1127. 56:07so in this model p is the average
  1128. 56:09connectivity of the graph or the average
  1129. 56:12number of Neighbors
  1130. 56:15okay
  1131. 56:16yes
  1132. 56:21no no p is the p is of all the one I'm
  1133. 56:23going to speak about this so the
  1134. 56:25question was if p is smaller than one so
  1135. 56:27here p
  1136. 56:30is the older one it's no other one
  1137. 56:33number but as we're going to see it can
  1138. 56:35be either smaller or larger than one and
  1139. 56:38as you've anticipated is going to be
  1140. 56:41important
  1141. 56:52so in the rest of these lectures I'm
  1142. 56:55going to call K
  1143. 56:58the degree
  1144. 57:00of a node
  1145. 57:04okay
  1146. 57:05which is the number of Neighbors
  1147. 57:08and so what I just shown is that the
  1148. 57:11average value of K is equal to p
  1149. 57:17but you can be a little more greedy and
  1150. 57:21ask what is the full distribution of of
  1151. 57:24K
  1152. 57:25which I'm going to call P of K
  1153. 57:28this is a distribution degree
  1154. 57:31distribution
  1155. 57:38foreign
  1156. 57:41well
  1157. 57:43if you want to know how many neighbors a
  1158. 57:46certain node has
  1159. 57:49it's going to be
  1160. 57:51the number of ways to choose K among n
  1161. 57:54minus one
  1162. 57:56times t t divided by n to the K 1 minus
  1163. 58:00P divided by n to the N minus 1 minus K
  1164. 58:04so it's a binomial distribution
  1165. 58:07but I'm not redoing the calculation it's
  1166. 58:09always the same calculation and the
  1167. 58:11limit when n goes to Infinity this
  1168. 58:12binomial distribution becomes a personal
  1169. 58:15distribution
  1170. 58:16and so what I get is that in this case
  1171. 58:19in the other shrenic case this is the
  1172. 58:22question distribution that we've seen
  1173. 58:24already today
  1174. 58:26which is p to the K exponential of minus
  1175. 58:29p
  1176. 58:30divided by factorial k okay
  1177. 58:34so this is a very simple graph
  1178. 58:36and it has a very simple distribution
  1179. 58:39which is a personal distribution
  1180. 58:42and note that this distribution decays
  1181. 58:45extremely quickly when K increases
  1182. 58:49so you know if you want a numerical
  1183. 58:52example
  1184. 58:53if I take P equal 1
  1185. 58:57so the average degree is one
  1186. 58:59then the probability to find
  1187. 59:03a node with 10 Neighbors which is not
  1188. 59:05that big it's just 10 times the average
  1189. 59:08this is already like 10 to the minus 7.
  1190. 59:14so the personal distribution is a little
  1191. 59:17bit like the gaussian distribution that
  1192. 59:19I talked about is it's extremely thin
  1193. 59:21distribution thin tail distribution that
  1194. 59:23decays incredibly quickly as K increases
  1195. 59:27and therefore it's a graph where
  1196. 59:30there's no hub
  1197. 59:32there's no site that has a very large
  1198. 59:36degree that has a very large number of
  1199. 59:39of of of
  1200. 59:41of neighbors or friends if you think
  1201. 59:44about
  1202. 59:45a a social network
  1203. 59:48and we know from empirical data that
  1204. 59:51many graphs are actually uh scale free
  1205. 59:54in the sense that they have a parallel
  1206. 59:56distribution of degrees some nodes have
  1207. 1:00:00an incredibly large number of of
  1208. 1:00:02neighbors While others have a small
  1209. 1:00:04number of Neighbors
  1210. 1:00:06so I'll go back to that in in the next
  1211. 1:00:10paragraph on scale free networks but let
  1212. 1:00:13me tell you a little more about
  1213. 1:00:17um what happens in the other ready
  1214. 1:00:20Network
  1215. 1:00:21well
  1216. 1:00:23although everything looks simple
  1217. 1:00:26there's still something non-trivial that
  1218. 1:00:28happens
  1219. 1:00:29in the regime where pay p is of all the
  1220. 1:00:32one
  1221. 1:00:33and what happens was is related to the
  1222. 1:00:36question that someone asked in the room
  1223. 1:00:37we have two
  1224. 1:00:39students today in the room
  1225. 1:00:42and pleases some of you want to come and
  1226. 1:00:45we can organize the
  1227. 1:00:48um that others take that turn so what
  1228. 1:00:51happens is that there's a phase
  1229. 1:00:53transition in Elder training networks
  1230. 1:00:55which is that when p is less than one
  1231. 1:00:58there are only
  1232. 1:01:03finite5 clusters
  1233. 1:01:11so all this is of course in the limits
  1234. 1:01:13where n goes to Infinity
  1235. 1:01:17so in when p is less than one I only
  1236. 1:01:20have you know things like this
  1237. 1:01:22isolated nodes or nodes that are
  1238. 1:01:25connected to a near
  1239. 1:01:26a few other nodes in the in the same
  1240. 1:01:30cluster but if p is greater than one
  1241. 1:01:34there exists a giant component
  1242. 1:01:38so GC
  1243. 1:01:39is going to be giant component
  1244. 1:01:45which means that
  1245. 1:01:48if I pick a node at random
  1246. 1:01:51there is a probability P Infinity
  1247. 1:01:54which is greater than zero that this
  1248. 1:01:57node belongs to an infinite cluster okay
  1249. 1:02:03so it doesn't mean that
  1250. 1:02:06this property is equal to one I may
  1251. 1:02:08still find nodes that are in isolated
  1252. 1:02:11clusters in in finite5 clusters even
  1253. 1:02:14nodes that are completely alone okay by
  1254. 1:02:18the way the probability
  1255. 1:02:19for K to be zero
  1256. 1:02:22is is always non-zero it's the it's
  1257. 1:02:25exponential of minus p
  1258. 1:02:27so there are always isolated class
  1259. 1:02:30isolated nodes we have zero is
  1260. 1:02:33exponential of minus B so
  1261. 1:02:36clearly even when T is greater than one
  1262. 1:02:38there are isolated nodes but there is
  1263. 1:02:41also an infinite size cluster
  1264. 1:02:45which is called a giant component or
  1265. 1:02:48it's also called in physics a
  1266. 1:02:50percolation cluster
  1267. 1:02:58so you'll see these two names depending
  1268. 1:03:00on the literature giant component or
  1269. 1:03:02percolation cluster but it means the
  1270. 1:03:04same and in my egg white analogy it's
  1271. 1:03:09when p is greater than one then when you
  1272. 1:03:12pull on a node you know imagine that
  1273. 1:03:14you're actually taking a an optical
  1274. 1:03:17tweezer and grabbing a polymer and try
  1275. 1:03:20to pull on it well if you're in the P
  1276. 1:03:23less than one phase you're going to only
  1277. 1:03:25pour finite clusters
  1278. 1:03:27so it's going to be easy and the thing
  1279. 1:03:29is a liquid so it is the reason why it's
  1280. 1:03:32it's easy
  1281. 1:03:33but if you're in the
  1282. 1:03:36um calculating phase then by taking a
  1283. 1:03:39node at random you might have to pull
  1284. 1:03:41the entire system
  1285. 1:03:43which means that it's a solid okay so
  1286. 1:03:47this is not a trivial
  1287. 1:03:52um effect that that happens in these
  1288. 1:03:55others ready Networks
  1289. 1:03:57and
  1290. 1:03:59I'm going to speak more about
  1291. 1:04:02the existence of giant components why is
  1292. 1:04:04it P equal 1 that makes the difference
  1293. 1:04:07here and the stability of these giant
  1294. 1:04:10components a little later
  1295. 1:04:21so this was my first construction of a
  1296. 1:04:24random Network
  1297. 1:04:26the other shreni which is simple enough
  1298. 1:04:28but as I said it's disappointing quote
  1299. 1:04:31unquote because there are a lot of
  1300. 1:04:34networks for which this personal
  1301. 1:04:36distribution of degree falls short of
  1302. 1:04:39explaining what's going on I mean as I
  1303. 1:04:41said as I said the probability of having
  1304. 1:04:43a node that's highly connected is so
  1305. 1:04:46small that you're never going to be able
  1306. 1:04:48to describe social networks for example
  1307. 1:04:52foreign
  1308. 1:04:54so let's look at another Construction
  1309. 1:05:19skill free
  1310. 1:05:22Networks
  1311. 1:05:27so these construction these
  1312. 1:05:30constructions are meant to uh generate
  1313. 1:05:33much broader distribution of degrees and
  1314. 1:05:37the most famous of them
  1315. 1:05:39is due to
  1316. 1:05:42um
  1317. 1:05:43who physicists
  1318. 1:05:48and all but
  1319. 1:05:54and that's a model from 2000
  1320. 1:05:59and it's an incredibly popular model
  1321. 1:06:02with this this paper of biology Albert
  1322. 1:06:05has a amazing number of citations I I
  1323. 1:06:08don't know it always already has like
  1324. 1:06:10several tens of thousands citations it's
  1325. 1:06:13cited in physics in computer science in
  1326. 1:06:16biology and in many different fields
  1327. 1:06:19uh by the way I told you at the
  1328. 1:06:21beginning of these lectures that if you
  1329. 1:06:22look at the distribution of
  1330. 1:06:24uh the citations a paper have it's a
  1331. 1:06:28very broad parallel distribution and
  1332. 1:06:30this clearly is one of the paper
  1333. 1:06:32contributing to the tale of uh the
  1334. 1:06:36distribution of citations
  1335. 1:06:39and by the way citations can be thought
  1336. 1:06:41of as
  1337. 1:06:43the network you know if you put a link
  1338. 1:06:45between a paper and another paper when
  1339. 1:06:49the the second paper is citing the first
  1340. 1:06:51then you construct a network and that's
  1341. 1:06:54a little bit the type of models that
  1342. 1:06:56we're going to construct here
  1343. 1:06:59so
  1344. 1:07:01what I'm going to
  1345. 1:07:02tell you about is a model that
  1346. 1:07:05is grown dynamically so there's some
  1347. 1:07:09kind of Dynamics
  1348. 1:07:13it's a dynamical model
  1349. 1:07:18and it works as follows
  1350. 1:07:21so I'm going to start at T equals 0
  1351. 1:07:25with a single node
  1352. 1:07:28then at t equal 1
  1353. 1:07:31I'm adding a node
  1354. 1:07:33and with this node
  1355. 1:07:35I'm adding a link so each new node adds
  1356. 1:07:39one Link in the system
  1357. 1:07:42and of course at this stage there's no
  1358. 1:07:44choice the link has to go to the
  1359. 1:07:47previously present node
  1360. 1:07:50then at t equal to
  1361. 1:07:53I already have these two guys
  1362. 1:07:56and I'm adding one more node and this
  1363. 1:07:59node has to connect to one of them
  1364. 1:08:02and in this case they have the same
  1365. 1:08:04degree each node already present node
  1366. 1:08:08has degree one
  1367. 1:08:09and so in this case it's going to be
  1368. 1:08:12with probability one half one half I'm
  1369. 1:08:15connecting to one of these two nodes so
  1370. 1:08:18at this level nothing much happens but
  1371. 1:08:20then at T equals three
  1372. 1:08:25when I'm adding
  1373. 1:08:26the fourth node
  1374. 1:08:30then the rule will be that I'm attaching
  1375. 1:08:33the new Edge preferentially to nodes
  1376. 1:08:36with high degrees
  1377. 1:08:38and the rule will be that I'm attaching
  1378. 1:08:41with a rule with a property that's
  1379. 1:08:43proportional to the already existing
  1380. 1:08:46number of of uh neighbors so to the
  1381. 1:08:49already existing degree
  1382. 1:08:52so here you see that I have three
  1383. 1:08:55choices but the probability to connect
  1384. 1:08:57to this thing will be twice the
  1385. 1:08:59probability to connect to these uh other
  1386. 1:09:03two guys so I have a probably two-thirds
  1387. 1:09:05to be connected to this one and one
  1388. 1:09:08third to be connected to one of these
  1389. 1:09:11two
  1390. 1:09:12and so you see what what's going to
  1391. 1:09:14happen so sometimes I'm going to connect
  1392. 1:09:16to this one but sometimes I'm going to
  1393. 1:09:18connect to that one
  1394. 1:09:19and because I'm connecting to that one
  1395. 1:09:21with higher probability is again going
  1396. 1:09:25to increase its degree and the next time
  1397. 1:09:28step is going to attract even more uh
  1398. 1:09:31links so it's a kind of Rich get richer
  1399. 1:09:34effect
  1400. 1:09:46and if you are following these lectures
  1401. 1:09:48since the beginning
  1402. 1:09:50uh you have already
  1403. 1:09:53um
  1404. 1:09:55recognized
  1405. 1:09:57proportional growth models because in a
  1406. 1:10:01sense the more you have grown
  1407. 1:10:04the more likely it's going it is going
  1408. 1:10:06to be that you grow again
  1409. 1:10:08and we know already that these types of
  1410. 1:10:10models tend to generate power laws
  1411. 1:10:15Okay so
  1412. 1:10:17at time t
  1413. 1:10:22I have a bunch of nodes
  1414. 1:10:24and the first node has
  1415. 1:10:28um
  1416. 1:10:29K1 Neighbors
  1417. 1:10:31the second node is K2 Neighbors
  1418. 1:10:34and so on
  1419. 1:10:36so
  1420. 1:10:39I have these uh
  1421. 1:10:43these degrees
  1422. 1:10:45and what I know is that each time and I
  1423. 1:10:48add a node a node
  1424. 1:10:51I also add a link and this link connects
  1425. 1:10:54to two nodes
  1426. 1:10:55and therefore the total
  1427. 1:10:58degree of the network
  1428. 1:11:00is twice the number of links I've added
  1429. 1:11:04you see here for example I have K1 equal
  1430. 1:11:081 K2 equal 1. so the sum over I of k i
  1431. 1:11:14is equal in general to 2 times t equal
  1432. 1:11:18to 2 here it's 4 here and so on okay
  1433. 1:11:24and the rule of the game will be that I
  1434. 1:11:27attach
  1435. 1:11:28to the ice side
  1436. 1:11:31probability to attach
  1437. 1:11:36to I
  1438. 1:11:38is equal to KI
  1439. 1:11:40divided by the sum of the kis which is
  1440. 1:11:432T
  1441. 1:11:46and so this is what's called
  1442. 1:11:48preferential attachment
  1443. 1:11:57and precisely it's preferential in a
  1444. 1:12:00linear way the more degree you have the
  1445. 1:12:03more likely it is to um
  1446. 1:12:07become the target of the new incoming
  1447. 1:12:10node
  1448. 1:12:12so
  1449. 1:12:13you can ask why do I choose the strict
  1450. 1:12:16linear uh relation here
  1451. 1:12:20well I'm going to give you a
  1452. 1:12:23generalizations of this result later on
  1453. 1:12:26at least discuss them quickly but it
  1454. 1:12:29seems reasonable that in many cases
  1455. 1:12:32your popularity is is going to be linear
  1456. 1:12:36for example if you think about papers
  1457. 1:12:39the more a paper is cited the more
  1458. 1:12:42likely it is that you're going to see it
  1459. 1:12:44cited in a paper you read and the more
  1460. 1:12:47likely it is that you're actually going
  1461. 1:12:49to cite your paper the same paper as
  1462. 1:12:51well in your own paper
  1463. 1:12:54so of course this has to be decided on
  1464. 1:12:56an empirical basis but it turns out that
  1465. 1:12:59in many cases this is not a bad
  1466. 1:13:01approximation
  1467. 1:13:06Okay so
  1468. 1:13:08now how does it work
  1469. 1:13:12thank you
  1470. 1:13:16[Music]
  1471. 1:13:25so the first thing I want to emphasize
  1472. 1:13:28is that this dynamical process is
  1473. 1:13:31stochastic it's not a deterministic
  1474. 1:13:33process
  1475. 1:13:35you see each time step there's a Droid
  1476. 1:13:38I said here I've chosen to connect to
  1477. 1:13:41the most likely side to side but of
  1478. 1:13:44course with probability uh I'm sorry
  1479. 1:13:46I've said something wrong here you
  1480. 1:13:48should have stopped me
  1481. 1:13:50this doesn't sound too
  1482. 1:13:52one
  1483. 1:13:55that's the problem when
  1484. 1:14:00so this is once half one fourth
  1485. 1:14:04one fourth
  1486. 1:14:08surprised nobody shouted but anyway
  1487. 1:14:11so what I'm saying is that there's a
  1488. 1:14:14higher probability to connect to that
  1489. 1:14:15one but it could have been that in the
  1490. 1:14:17in another history in another world I
  1491. 1:14:20would have connected to this one
  1492. 1:14:22okay and then this one and this one
  1493. 1:14:25would have had the same degree at the
  1494. 1:14:28name next time step so I'm generating an
  1495. 1:14:32ensemble of graph that are not all the
  1496. 1:14:34same
  1497. 1:14:36and so I can speak about averaging over
  1498. 1:14:40histories in this model okay
  1499. 1:14:44and that's what I'm going to introduce
  1500. 1:14:46now I'm going to call n of k and t
  1501. 1:14:51this is the average number
  1502. 1:14:56a side of nodes
  1503. 1:15:01with degree k
  1504. 1:15:05at time t
  1505. 1:15:10and it's the average over what
  1506. 1:15:13it's the average over all possible
  1507. 1:15:15histories of the construction
  1508. 1:15:17okay
  1509. 1:15:20and so having understood that it's an
  1510. 1:15:23average of a construction it's very easy
  1511. 1:15:25to
  1512. 1:15:27come up with a recursion relation for
  1513. 1:15:30nfk and T so let me write it
  1514. 1:15:33and then
  1515. 1:15:35I will comment
  1516. 1:15:38and justify
  1517. 1:15:40what I'm claiming is that n of k and t
  1518. 1:15:44plus one is n of k and t
  1519. 1:15:47plus K minus 1
  1520. 1:15:50divided by 2T
  1521. 1:15:52n of K minus 1
  1522. 1:15:55and T
  1523. 1:15:58minus K Over 2T
  1524. 1:16:01n of k and t
  1525. 1:16:05plus Delta of K and 1.
  1526. 1:16:11so this is the fundamental equation the
  1527. 1:16:14master equation if you want
  1528. 1:16:18that
  1529. 1:16:20um I want you to understand so what does
  1530. 1:16:23it mean it means that
  1531. 1:16:25in order to have K degree k at time t
  1532. 1:16:29plus one
  1533. 1:16:30then either you uh then you had the
  1534. 1:16:34number of sites is
  1535. 1:16:36at time T is n of k and t but you can
  1536. 1:16:39add to this number of sides that have
  1537. 1:16:41degree K by connecting the new incoming
  1538. 1:16:45node to a side that had degree K minus
  1539. 1:16:49one
  1540. 1:16:49and this happens with probability K
  1541. 1:16:52minus 1 divided by 2T remember this is
  1542. 1:16:56this is this
  1543. 1:16:57so on average is going to be the
  1544. 1:16:59probability to connect to a site to a
  1545. 1:17:02node of the green K minus 1 times the
  1546. 1:17:04number the average number of such sites
  1547. 1:17:08but if you connect to a site
  1548. 1:17:11to node with degree k then you're taking
  1549. 1:17:14away some of these nodes from the count
  1550. 1:17:19so there are less at time C plus one
  1551. 1:17:22there are less nodes with degree K and
  1552. 1:17:24this occurs before DK over to T so
  1553. 1:17:27there's a minus sign here and then every
  1554. 1:17:29time you add a node you add a degree
  1555. 1:17:34which is equal to one because the
  1556. 1:17:36incoming node always has a degree called
  1557. 1:17:38one see this guy here it has a only one
  1558. 1:17:41Edge going out
  1559. 1:17:43and um so this explains the Delta of K
  1560. 1:17:47and one here
  1561. 1:17:52so what can we say about this equation
  1562. 1:17:54well
  1563. 1:17:56it's very natural to think that
  1564. 1:17:59the number of nodes
  1565. 1:18:01of degree k
  1566. 1:18:04at large times
  1567. 1:18:09well first let me write it this way it's
  1568. 1:18:11it's natural to write it like that
  1569. 1:18:14T times P of k and t
  1570. 1:18:19where because the num the total number
  1571. 1:18:21of uh of sites is
  1572. 1:18:27sorry I'm using sites and nodes to mean
  1573. 1:18:31the same thing so the number of nodes is
  1574. 1:18:33t plus one
  1575. 1:18:35so maybe I should write t plus one here
  1576. 1:18:39and doing this I'm defining not the
  1577. 1:18:42number but the the probability this
  1578. 1:18:44thing is the probability
  1579. 1:18:46that
  1580. 1:18:48a node
  1581. 1:18:50has degree k
  1582. 1:18:57so that's a definition if you want but
  1583. 1:18:59then my assumption will be that when T
  1584. 1:19:02goes to Infinity
  1585. 1:19:05assumption which is very natural in a
  1586. 1:19:08way
  1587. 1:19:09is that when t
  1588. 1:19:12goes to Infinity
  1589. 1:19:15P of k and t
  1590. 1:19:17converges
  1591. 1:19:19through a stationary distribution which
  1592. 1:19:21I'm calling Peak star of K
  1593. 1:19:24okay
  1594. 1:19:25so I'm repeating this process over and
  1595. 1:19:27over again
  1596. 1:19:28so the number of sides the number of
  1597. 1:19:31nodes is increasing
  1598. 1:19:33so I take care of that by introducing
  1599. 1:19:36this Factor t or t plus 1 here
  1600. 1:19:39and then at very long times I'm
  1601. 1:19:42expecting this distribution to reach a
  1602. 1:19:44stationary state
  1603. 1:19:46so with these two items
  1604. 1:19:50this one and this assumption I can plug
  1605. 1:19:53into
  1606. 1:19:55um
  1607. 1:19:56the the master equation above and find
  1608. 1:19:59an equation for the stationary State
  1609. 1:20:01itself
  1610. 1:20:02and so what you find
  1611. 1:20:04again I'm not dictating the calculations
  1612. 1:20:07but it it's really easy to do that just
  1613. 1:20:10take this plug it in here
  1614. 1:20:13and then assume this to be true and then
  1615. 1:20:16what you find is that P star of K obeys
  1616. 1:20:18the following discrete equation one half
  1617. 1:20:23of K minus 1
  1618. 1:20:26P star of K minus 1.
  1619. 1:20:31minus k
  1620. 1:20:33T star of K
  1621. 1:20:36plus Delta of K 1.
  1622. 1:20:41so the one half here comes from the one
  1623. 1:20:43half that's here
  1624. 1:20:45K minus 1 P star of K minus one this is
  1625. 1:20:48this guy
  1626. 1:20:49KP star k this is this guy and Delta of
  1627. 1:20:51k n one remains unchanged okay
  1628. 1:20:55so this is the equation you should solve
  1629. 1:20:58to get the stationary state of this
  1630. 1:21:00Albert barabati model
  1631. 1:21:03and it's fortunate but it's it's it
  1632. 1:21:06happens that this equation can be
  1633. 1:21:08exactly solved
  1634. 1:21:11and what you find
  1635. 1:21:28foreign
  1636. 1:21:43if you want to check it yourself but
  1637. 1:21:46what you find is that P star of K
  1638. 1:21:51equals
  1639. 1:21:52k 4 over k
  1640. 1:21:55K plus 1
  1641. 1:21:57K plus 2
  1642. 1:22:00is an exact solution
  1643. 1:22:12okay so you know just have to put it in
  1644. 1:22:15there and check that it works and this
  1645. 1:22:17thing happens to be normalized to one so
  1646. 1:22:20it's the correct probability
  1647. 1:22:21distribution
  1648. 1:22:23and what you can notice is that when K
  1649. 1:22:27becomes large
  1650. 1:22:30this decays it's 4 over K to the 1 plus
  1651. 1:22:34mu
  1652. 1:22:36with mu equal to
  1653. 1:22:43so this mechanism this Rich get richer
  1654. 1:22:45mechanism
  1655. 1:22:46this proportional growth model leads to
  1656. 1:22:51um
  1657. 1:22:52an exponent with a parallel pair with an
  1658. 1:22:54exponent which is two
  1659. 1:22:56so the average degree exists but the
  1660. 1:23:00variance of the degree distribution
  1661. 1:23:02is infinite
  1662. 1:23:05okay
  1663. 1:23:08so that's one possible model there are
  1664. 1:23:12many variations around this model
  1665. 1:23:15that you can consider for example you
  1666. 1:23:18could consider an attachment rule
  1667. 1:23:22or some variations
  1668. 1:23:27so you could have an attachment rule
  1669. 1:23:29that's proportional to K
  1670. 1:23:33which becomes
  1671. 1:23:35proportional to K plus
  1672. 1:23:37some intercept
  1673. 1:23:40okay
  1674. 1:23:45personal
  1675. 1:23:47so it's still linear at large K but
  1676. 1:23:49there's a
  1677. 1:23:51there's an intercept m
  1678. 1:23:53and in this case you can also show that
  1679. 1:23:56the the solution
  1680. 1:23:58is a parallel
  1681. 1:24:04with an exponent
  1682. 1:24:06view that depends on M
  1683. 1:24:12okay so that's that's the natural uh
  1684. 1:24:15change but maybe you want to make us a
  1685. 1:24:18more drastic change what happens if
  1686. 1:24:21your attachment rule is proportional to
  1687. 1:24:24K to the beta
  1688. 1:24:26so
  1689. 1:24:28beta equal one
  1690. 1:24:30this is linear
  1691. 1:24:32attachments which leads to parallels
  1692. 1:24:39when beta is less than 1
  1693. 1:24:43but greater than zero
  1694. 1:24:45then I'm not doing the calculation but
  1695. 1:24:48what you get is that TFK
  1696. 1:24:51is not a parallel anymore but it decays
  1697. 1:24:54as exponential of minus
  1698. 1:24:57k
  1699. 1:24:58to the 1 minus beta
  1700. 1:25:03so this is called the stretch
  1701. 1:25:04exponential
  1702. 1:25:10you see it's when beta is positive it's
  1703. 1:25:14slower than any exponential
  1704. 1:25:16but it's faster than any power
  1705. 1:25:19so it's an intermediate regime
  1706. 1:25:23and what happens if beta is greater than
  1707. 1:25:25one
  1708. 1:25:28well when beta is greater than one
  1709. 1:25:30you're in a situation that in a sense
  1710. 1:25:33is similar to the situation of the hoax
  1711. 1:25:35processes when r0 is greater than one in
  1712. 1:25:38the sense that this assumption here
  1713. 1:25:42is no longer true there's no stationary
  1714. 1:25:45State because you see that the
  1715. 1:25:48attachment rule
  1716. 1:25:49grows so quickly with k that's that's
  1717. 1:25:54condensation
  1718. 1:26:01in the sense that
  1719. 1:26:03a finite number of nodes becomes become
  1720. 1:26:06attract everything
  1721. 1:26:09and have a degree that grows uh with
  1722. 1:26:13with tea
  1723. 1:26:14in an unbounded fashion
  1724. 1:26:17okay so here you have a completely
  1725. 1:26:20different regime where there's no
  1726. 1:26:22uh proper
  1727. 1:26:24stationary distribution for pfk
  1728. 1:26:27so in a sense if you want to have power
  1729. 1:26:31laws
  1730. 1:26:32this is the only case which naturally
  1731. 1:26:34gives rise to
  1732. 1:26:36power laws so if you have a parallel
  1733. 1:26:38degree distribution in your empirical
  1734. 1:26:41Network
  1735. 1:26:42then presumably this is because there is
  1736. 1:26:45a process behind it which is a linear
  1737. 1:26:50preferential attachment process
  1738. 1:26:55okay
  1739. 1:26:57so
  1740. 1:27:00this is um
  1741. 1:27:04what I wanted to tell you about
  1742. 1:27:08Networks
  1743. 1:27:11I mean
  1744. 1:27:12about the construction of networks so
  1745. 1:27:14two very different constructions of
  1746. 1:27:16course I'm not exhausting all the
  1747. 1:27:19possible ways to build networks I'm only
  1748. 1:27:21giving you two extreme cases
  1749. 1:27:24which leads to personal distribution of
  1750. 1:27:27degrees and is a the the classical uh
  1751. 1:27:31Network model and the Barabbas the
  1752. 1:27:33Albert model which gives the parallel
  1753. 1:27:36distribution of degrees
  1754. 1:27:37but you can invent many other ways to
  1755. 1:27:39build uh networks and they have to be
  1756. 1:27:43analyzed on the case-by-case basis but
  1757. 1:27:46what is important from a technical point
  1758. 1:27:48of view is and I encourage you to think
  1759. 1:27:51about this more if you haven't followed
  1760. 1:27:54all the steps but
  1761. 1:27:56you know behind all these models there
  1762. 1:28:00is often
  1763. 1:28:01a master equation an equation an
  1764. 1:28:03evolution equation like this and so this
  1765. 1:28:06is this is really from a technical point
  1766. 1:28:08of view the the main message of these
  1767. 1:28:09lectures
  1768. 1:28:12okay
  1769. 1:28:19so let me now talk about
  1770. 1:28:23um
  1771. 1:28:24a giant component
  1772. 1:28:37foreign
  1773. 1:28:43of
  1774. 1:28:46a giant component
  1775. 1:28:58so I've already insisted on why it's
  1776. 1:29:00important to know whether in your
  1777. 1:29:03network there is a giant component or
  1778. 1:29:05not
  1779. 1:29:07so what tools do we have to answer that
  1780. 1:29:10question I have a a given Network
  1781. 1:29:15how can I know
  1782. 1:29:16analytically
  1783. 1:29:18from a theoretical point of view whether
  1784. 1:29:21or not I have a giant component
  1785. 1:29:24that is whether or not my white will be
  1786. 1:29:27solid or liquid or whether or not my
  1787. 1:29:30epidemic will propagate among a social
  1788. 1:29:34network
  1789. 1:29:35and so on or whether a crisis will
  1790. 1:29:38propagate across a firm Network and
  1791. 1:29:41invade the whole economy or be localized
  1792. 1:29:44in some subparts of the economy okay so
  1793. 1:29:48this is a very important question indeed
  1794. 1:29:52so what I'm going to give you as a tool
  1795. 1:29:56to answer that question
  1796. 1:29:58is a little bit of a hand waving
  1797. 1:30:00argument which relies on everything
  1798. 1:30:03we've understood about branching
  1799. 1:30:05processes
  1800. 1:30:08um
  1801. 1:30:09it's it's going to be actually
  1802. 1:30:12restricted to some
  1803. 1:30:16some types of graph
  1804. 1:30:18which are what one called tree light
  1805. 1:30:21graph
  1806. 1:30:29so I'm going to explain in a minute what
  1807. 1:30:32the tree line graph but you can think of
  1808. 1:30:35it as an approximation for graph or
  1809. 1:30:39arbitrary graph to treat these graphs as
  1810. 1:30:42if they were trees but some graphs are
  1811. 1:30:45really
  1812. 1:30:46very close to being trees and for which
  1813. 1:30:49the approximation I'm going to talk
  1814. 1:30:51about actually is exact
  1815. 1:30:54and
  1816. 1:30:55what I'm going to derive for you is the
  1817. 1:30:58so-called Molloy read Criterion
  1818. 1:31:02so this is going to be called the Molloy
  1819. 1:31:06read Criterion
  1820. 1:31:08for the existence of a giant component
  1821. 1:31:15but the way I'm going to present this
  1822. 1:31:16Mallory Criterion is a little bit hand
  1823. 1:31:19waving
  1824. 1:31:21if you want to have a more mathematical
  1825. 1:31:24proof of the Molloy read Criterion
  1826. 1:31:27I'm going to if I have time give you a
  1827. 1:31:30hint of that
  1828. 1:31:31later on otherwise
  1829. 1:31:34um you will find it in in the notes that
  1830. 1:31:38I'm currently writing or actually in the
  1831. 1:31:41acculturally technique
  1832. 1:31:43um
  1833. 1:31:45lecture notes
  1834. 1:31:48but the way I'm going to present it I
  1835. 1:31:50think is nice because it emphasizes
  1836. 1:31:52um
  1837. 1:31:54the relation with what we've seen
  1838. 1:31:55already branching processes and I think
  1839. 1:31:59it's it's a very nice way to see things
  1840. 1:32:01okay so what's a tree
  1841. 1:32:05uh so a tree
  1842. 1:32:09is a graph with no loops
  1843. 1:32:19so for example
  1844. 1:32:26this is a regular tree
  1845. 1:32:28and you see I can continue that to
  1846. 1:32:31Infinity it has no loot
  1847. 1:32:36sometimes I have loops
  1848. 1:32:39in My Graph but the loops are are not
  1849. 1:32:43small Loops they're they're long loose
  1850. 1:32:45so maybe for example I continue the
  1851. 1:32:48construction here
  1852. 1:32:49and at this point
  1853. 1:32:52these two points merge together
  1854. 1:32:55so there's a loop in my graph
  1855. 1:32:58but the loop
  1856. 1:32:59here it's not that big but you can
  1857. 1:33:01imagine that if these Loops are big
  1858. 1:33:04enough
  1859. 1:33:05you know so it means that in a sense
  1860. 1:33:07they're rare enough
  1861. 1:33:09I can view locally the graph as a tree
  1862. 1:33:14and and so
  1863. 1:33:16if you look at for example the others
  1864. 1:33:18ready graph
  1865. 1:33:20well
  1866. 1:33:22in the limit where close to the giant
  1867. 1:33:25the appearance of the design component
  1868. 1:33:27the very large clusters in a in an
  1869. 1:33:31address many graph they're in a proper
  1870. 1:33:34mathematical sense tree-like there are
  1871. 1:33:37some Loops but they're somehow uh very
  1872. 1:33:40large compared to to one the the the
  1873. 1:33:43size of the loop is much larger than uh
  1874. 1:33:48than one so for example it grows like
  1875. 1:33:51the log of the number of
  1876. 1:33:53of sites so in these in some cases you
  1877. 1:33:57can really justify the approximation
  1878. 1:33:59what I'm that I'm going to present to
  1879. 1:34:00you in other cases the graph is really a
  1880. 1:34:04tree
  1881. 1:34:04so it's exact
  1882. 1:34:07and in still other cases it's just an
  1883. 1:34:10approximation so for example let me give
  1884. 1:34:12you a graph that's another tree
  1885. 1:34:15so if you take a euclidean lattice like
  1886. 1:34:17this
  1887. 1:34:18then you see that there's no real
  1888. 1:34:21meaning in saying that it's a tree
  1889. 1:34:23because even at the shortest length
  1890. 1:34:25scale there are Loops okay so this is
  1891. 1:34:28not a tree
  1892. 1:34:33but even even if it's not a tree you can
  1893. 1:34:36you know deem it as a tree treat it as a
  1894. 1:34:38tree and and it what I'm going to tell
  1895. 1:34:41you about is just an approximation which
  1896. 1:34:43has no reason to be good but uh you can
  1897. 1:34:47try it and in some cases it's a very
  1898. 1:34:49good approximation in other cases It's
  1899. 1:34:52actually an exact uh
  1900. 1:34:55treatment an exact argument okay
  1901. 1:34:59so my argument is about three-digraphs
  1902. 1:35:10so if I have a
  1903. 1:35:12cluster that's a tree
  1904. 1:35:18or a tree like object
  1905. 1:35:20I can always think of this tree as a
  1906. 1:35:24genealogical tree okay
  1907. 1:35:27of course it has nothing to do with the
  1908. 1:35:29population growth but I can think of the
  1909. 1:35:31tree
  1910. 1:35:32as something that has some temporal
  1911. 1:35:36structure where I choose a node
  1912. 1:35:39arbitrarily This Is The Answer ancestor
  1913. 1:35:45and then these guys are the child the
  1914. 1:35:47children of the first ancestor and these
  1915. 1:35:50guys are the children of the children
  1916. 1:35:51and so on okay so I'm just thinking of a
  1917. 1:35:55tree like a genealogical tree
  1918. 1:35:58so you see that if I have loops it it
  1919. 1:36:00doesn't mean anything because if I have
  1920. 1:36:02loops it means that I can beat a child
  1921. 1:36:04of my
  1922. 1:36:06um of my children
  1923. 1:36:08but if these Loops are rare enough I can
  1924. 1:36:12forget these
  1925. 1:36:13um these these anomalies and think of
  1926. 1:36:17that as a genealogical tree
  1927. 1:36:22and so what I know is that my general
  1928. 1:36:24genealogical tree
  1929. 1:36:28is growing so this tree
  1930. 1:36:32is
  1931. 1:36:34a finite size
  1932. 1:36:41so the family
  1933. 1:36:43that as this guy as an ancestor as a
  1934. 1:36:48finite spies if the reproduction rate of
  1935. 1:36:50zero is less than one
  1936. 1:36:53and it can be of infinite size
  1937. 1:37:04if a zero
  1938. 1:37:06is greater than one
  1939. 1:37:09okay and r0 equal one is this strange
  1940. 1:37:12critical thing that is in between
  1941. 1:37:16so if I want to know whether there's a
  1942. 1:37:19giant component
  1943. 1:37:20I want to know whether there can be
  1944. 1:37:22infinite size clusters in my in my graph
  1945. 1:37:26right that's the same question
  1946. 1:37:29so I have to answer the question in
  1947. 1:37:31terms of population growth
  1948. 1:37:34is whether the reproduction rate in this
  1949. 1:37:39fictitious tree in the sixth genological
  1950. 1:37:43tree is this uh genealogic is this
  1951. 1:37:46reproduction rate greater than one or
  1952. 1:37:49less than one okay so this is the
  1953. 1:37:51question that I'm going to try to
  1954. 1:37:52address
  1955. 1:37:53and it's going to lead to the Malloy
  1956. 1:37:56read criteria
  1957. 1:38:02so what I'm going to need
  1958. 1:38:07is
  1959. 1:38:09to describe my tree
  1960. 1:38:12in terms of
  1961. 1:38:14the probability of the degree
  1962. 1:38:17distribution
  1963. 1:38:26so the only ingredient I'm going to need
  1964. 1:38:32is that
  1965. 1:38:35is this object T of K
  1966. 1:38:38this is the unconditional
  1967. 1:38:44degree distribution
  1968. 1:38:54and I'm insisting on unconditional here
  1969. 1:38:56which means that I have my my My Graph
  1970. 1:39:01my network
  1971. 1:39:03oh maybe it looks like like this okay
  1972. 1:39:09and what unconditional means is that you
  1973. 1:39:11know I'm picking at random
  1974. 1:39:13this node and asking what is the
  1975. 1:39:16probability that this node has
  1976. 1:39:18degree k this is pfk
  1977. 1:39:22and you'll see in a second
  1978. 1:39:24another degree distribution which is
  1979. 1:39:26going to be conditioned and which is not
  1980. 1:39:28going to be the same as P of K and which
  1981. 1:39:30is going to play a crucial role
  1982. 1:39:34so I'm assuming that each node has
  1983. 1:39:37an independent degree and each of these
  1984. 1:39:41degrees is drawn according to pfk okay
  1985. 1:39:47nodes
  1986. 1:39:49have
  1987. 1:39:52Independence
  1988. 1:40:01so ID if you want
  1989. 1:40:05cross nodes
  1990. 1:40:12so there are no correlation between the
  1991. 1:40:15degrees it's not because this one has a
  1992. 1:40:17high degree that its neighbor will have
  1993. 1:40:19a high degree
  1994. 1:40:22okay so this is TFK now you know you
  1995. 1:40:25should pay attention because I'm going
  1996. 1:40:27to introduce
  1997. 1:40:29um and unfortunately of course as usual
  1998. 1:40:31I won't have time to finish today that's
  1999. 1:40:33too bad
  2000. 1:40:34but let me at least go until the Malloy
  2001. 1:40:37read Criterion
  2002. 1:40:39so
  2003. 1:40:41what I'm claiming is now that I'm going
  2004. 1:40:45to do another construction to uh to
  2005. 1:40:48introduce another degree distribution
  2006. 1:40:51which is the following
  2007. 1:40:53I'm going to take
  2008. 1:40:55a note at random like before this one
  2009. 1:40:59and then take an edge out which is
  2010. 1:41:02outgoing from that node
  2011. 1:41:04and Target another
  2012. 1:41:07node okay so I've taken this node in at
  2013. 1:41:10random I've chosen this particular
  2014. 1:41:13Edge
  2015. 1:41:15and I'm I'm landing on the second node
  2016. 1:41:17so this if you want is i0 which is the
  2017. 1:41:20node I chose at random the degree of
  2018. 1:41:23that node is distributed according to
  2019. 1:41:25pfk
  2020. 1:41:26and now I'm
  2021. 1:41:29looking at another node which is a
  2022. 1:41:31neighbor of mine and I'm asking what's
  2023. 1:41:33the distribution the degree distribution
  2024. 1:41:35of this guy J okay
  2025. 1:41:38so think of it in terms of your friends
  2026. 1:41:41in a social network
  2027. 1:41:43I'm taking one guy at random on a social
  2028. 1:41:45network and I'm counting the number of
  2029. 1:41:47friends this is distributed according to
  2030. 1:41:50pfk
  2031. 1:41:51now I'm taking one friend of this guy
  2032. 1:41:54and I'm asking what is the degree
  2033. 1:41:57distribution of that guy okay
  2034. 1:42:00and what I'm going to say is that this
  2035. 1:42:04degree distribution is what I'm going to
  2036. 1:42:06call Q of K
  2037. 1:42:08so it's the degree
  2038. 1:42:11distribution
  2039. 1:42:15of a neighbor
  2040. 1:42:18of a friend
  2041. 1:42:24and what I'm claiming is that Q of K is
  2042. 1:42:26not equal to pfk
  2043. 1:42:28and there's a clear reason already for
  2044. 1:42:31that to be the case which is that
  2045. 1:42:34you see that this node here has zero
  2046. 1:42:38Neighbors
  2047. 1:42:40so if I choose at random a site in my
  2048. 1:42:42network I I have a sudden probability to
  2049. 1:42:45find that P of k equals 0
  2050. 1:42:47is non-zero I mean I have a probability
  2051. 1:42:49to find a node with now with without any
  2052. 1:42:52neighbors so because P of k equals 0 is
  2053. 1:42:55not zero these are the guys that I'm
  2054. 1:42:58going to choose but this guy has
  2055. 1:43:01absolutely no chance of being chosen as
  2056. 1:43:03a friend because he has no friends
  2057. 1:43:06and if you think about this
  2058. 1:43:09this process of choosing a friend is
  2059. 1:43:12going to select preferentially friends
  2060. 1:43:14who have a large number of friends
  2061. 1:43:17because the more friends they have the
  2062. 1:43:19more likely it is that you are one of
  2063. 1:43:22his friends and the more likely it is
  2064. 1:43:24that you're going to choose him in your
  2065. 1:43:26selection process
  2066. 1:43:28so you can make this argument precise by
  2067. 1:43:32using base theorem for example and what
  2068. 1:43:35you find is that Q of K
  2069. 1:43:40is K times larger than TFK
  2070. 1:43:44because of this amplification effect
  2071. 1:43:46because there are k
  2072. 1:43:48ways of choosing a neighbor with a large
  2073. 1:43:52degree is going to be chosen more often
  2074. 1:43:55through this process okay
  2075. 1:43:58so
  2076. 1:44:03if you want to have a normalized
  2077. 1:44:05distribution
  2078. 1:44:07I should divide
  2079. 1:44:09k p of K by the expectation the average
  2080. 1:44:13value of K in p
  2081. 1:44:16so I've defined
  2082. 1:44:19EP of K
  2083. 1:44:21as the sum
  2084. 1:44:25from k equals 0 to Infinity of K
  2085. 1:44:28times P of K
  2086. 1:44:31such that the sum over o k of Q of K is
  2087. 1:44:35equal to one okay
  2088. 1:44:38and now something strange happens which
  2089. 1:44:41in a sense is contained in my argument
  2090. 1:44:43is that if I compute
  2091. 1:44:45the average value of the number of
  2092. 1:44:48friends of my friends
  2093. 1:44:49which is EQ of K
  2094. 1:44:53this is equal to sum over k
  2095. 1:44:57of K squared P of K
  2096. 1:45:00over p p of K
  2097. 1:45:06which is e t of K squared
  2098. 1:45:10divided by ep
  2099. 1:45:12of K
  2100. 1:45:15and I guess that I shouldn't go
  2101. 1:45:18other than that and this is larger or
  2102. 1:45:20equal than e key okay
  2103. 1:45:26so the average number of your friends is
  2104. 1:45:29larger than your average number of
  2105. 1:45:31friends so this is called the the
  2106. 1:45:34Friendship Paradox in Networks
  2107. 1:45:36which means it's very frustrating but it
  2108. 1:45:39means that uh
  2109. 1:45:40that's this uh selection bias the fact
  2110. 1:45:44that your friends are you know by by
  2111. 1:45:48making
  2112. 1:45:50you know mechanistic mechanistical way
  2113. 1:45:53uh more uh have more friends than you on
  2114. 1:45:57average means that they uh they're more
  2115. 1:46:00popular
  2116. 1:46:02okay
  2117. 1:46:03so this is going to have a very
  2118. 1:46:06important consequence for vaccination
  2119. 1:46:08campaigns but let me come back to what I
  2120. 1:46:13was interested in which is the existence
  2121. 1:46:15of a giant component
  2122. 1:46:21so what I'm claiming here
  2123. 1:46:23and I'll be done in five minutes and
  2124. 1:46:27then
  2125. 1:46:28unfortunately then next week is vacation
  2126. 1:46:30so
  2127. 1:46:34there will be a two-week Gap
  2128. 1:46:36for me to come back
  2129. 1:46:38on the last little thing that I wanted
  2130. 1:46:41to talk about but it's I I don't think I
  2131. 1:46:43should do that today it takes me too
  2132. 1:46:45long
  2133. 1:46:46um so what I'm saying is that you know
  2134. 1:46:50these children
  2135. 1:46:52by construction they are children of an
  2136. 1:46:54ancestor and so they are they are in my
  2137. 1:46:58analogy they are friends of a guy
  2138. 1:47:01and so if I want to know the
  2139. 1:47:04distribution of degrees of these
  2140. 1:47:07children I have to use Q of K and not P
  2141. 1:47:10of K
  2142. 1:47:12and so what happens is that r0
  2143. 1:47:17is equal to the average number of
  2144. 1:47:22children
  2145. 1:47:24which is
  2146. 1:47:26the expectation of K the average degree
  2147. 1:47:29on the Q
  2148. 1:47:31because again these are not random
  2149. 1:47:34people there are people selected as
  2150. 1:47:37being the child of someone
  2151. 1:47:39or the friend of someone minus one
  2152. 1:47:42because one of the links is the one that
  2153. 1:47:45defines their uh their ancestry okay
  2154. 1:47:50and so the multi read Criterion
  2155. 1:47:53is that r0 should be greater than one
  2156. 1:47:57which translates into
  2157. 1:48:00uh
  2158. 1:48:01EP of K squared
  2159. 1:48:06so EQ of K I said it's e p of K Square
  2160. 1:48:09divided by etfk so here I have EQ of K
  2161. 1:48:14must be greater than two so EPF K Square
  2162. 1:48:16must be greater than two times
  2163. 1:48:19EP
  2164. 1:48:21of K
  2165. 1:48:26so that exists
  2166. 1:48:29a giant component
  2167. 1:48:31if and only if
  2168. 1:48:33this Criterion holds okay
  2169. 1:48:37so that's that's what I wanted to arrive
  2170. 1:48:41at so you see that
  2171. 1:48:43I've I've been very hand waving here
  2172. 1:48:45I've used this uh General genealogical
  2173. 1:48:49tree analogy and I've relied on the
  2174. 1:48:52branching process on the on what we saw
  2175. 1:48:55last week about uh the Galton Watson
  2176. 1:48:58model
  2177. 1:48:59but I assure you that there's a better
  2178. 1:49:01way to do all this
  2179. 1:49:03which involves more mathematics and so I
  2180. 1:49:05didn't want to go into the mathematics
  2181. 1:49:08but you can certainly have a go in the
  2182. 1:49:11lecture note to see how you do this a
  2183. 1:49:14little better
  2184. 1:49:15anyway
  2185. 1:49:17um
  2186. 1:49:19let's let's do the elders ready case
  2187. 1:49:25ER is Elder shreni
  2188. 1:49:29um
  2189. 1:49:30other shreni means that P is a personal
  2190. 1:49:32distribution
  2191. 1:49:35so the question distribution is such
  2192. 1:49:37that EP is K squared
  2193. 1:49:41is equal to p squared plus p
  2194. 1:49:46why because the variance of K is p so
  2195. 1:49:51the variance is the average of K squared
  2196. 1:49:53minus the average of K the whole thing
  2197. 1:49:56squared that's what I get t squared plus
  2198. 1:49:59p and the average
  2199. 1:50:02of K is p so I have that this must be
  2200. 1:50:05larger than twice
  2201. 1:50:07and 2p
  2202. 1:50:09which means that P must be greater than
  2203. 1:50:13one
  2204. 1:50:14and so we recover what was anticipated
  2205. 1:50:17by
  2206. 1:50:18some in the room that if p is greater
  2207. 1:50:20than one in the others raining graph you
  2208. 1:50:23have a giant component
  2209. 1:50:27let's see what happens in the barability
  2210. 1:50:29Albert model
  2211. 1:50:31you remember the Albert
  2212. 1:50:35we had that pfk
  2213. 1:50:38was decaying as one over K Cube
  2214. 1:50:41which means formally that the average
  2215. 1:50:44value of K squared is infinite
  2216. 1:50:47so for Barbara Albert
  2217. 1:50:50there exists a giant component
  2218. 1:50:54and the reason is that
  2219. 1:50:57you know because of these hubs because
  2220. 1:50:59there are nodes that are so connected to
  2221. 1:51:01many others
  2222. 1:51:03then different parts of the subgraph
  2223. 1:51:06will likely be connected together
  2224. 1:51:08through these highly connected nodes
  2225. 1:51:11okay
  2226. 1:51:13so in again in the epidemic analogy
  2227. 1:51:17these are super spreaders
  2228. 1:51:18and because of their existence the the
  2229. 1:51:22disease is going to spread very quickly
  2230. 1:51:24in the population but at a formal level
  2231. 1:51:27we see that the Molloy read Criterion
  2232. 1:51:30tells you immediately that biology
  2233. 1:51:32output graphs are have a giant component
  2234. 1:51:37okay so what I wanted to tell you about
  2235. 1:51:42is okay there is a giant component
  2236. 1:51:46catastrophe
  2237. 1:51:48the epidemic is the propagating
  2238. 1:51:52what can I do to uh
  2239. 1:51:55to prevent it to cut
  2240. 1:51:58the uh the spread of of the disease and
  2241. 1:52:03this translates into how robust is this
  2242. 1:52:06giant component if I start
  2243. 1:52:08removing some links so imagine that
  2244. 1:52:11through vaccination
  2245. 1:52:12I'm removing some of the links of the of
  2246. 1:52:15that Network how many links should I
  2247. 1:52:17remove
  2248. 1:52:18to remove to kill the giant component to
  2249. 1:52:21to make such that the giant component
  2250. 1:52:25disintegrates and there are only finite
  2251. 1:52:27clusters
  2252. 1:52:29so this is a question that we can very
  2253. 1:52:31easily answer with the
  2254. 1:52:34formalism I've given you up to now
  2255. 1:52:37but um I think I have to stop at this
  2256. 1:52:39point unfortunately
  2257. 1:52:42so that's that's that's me for today
  2258. 1:52:46uh I don't know if there are questions
  2259. 1:52:52I have a question
  2260. 1:52:53yes uh can you explain again the
  2261. 1:52:56expression of Q of K uh
  2262. 1:52:59On The Other Board why I don't really
  2263. 1:53:02understand why the it's equal to K not
  2264. 1:53:05care over the expectation
  2265. 1:53:07okay so you know the proper way is to
  2266. 1:53:10use the base argument
  2267. 1:53:13but intuitively it means that
  2268. 1:53:17as I said if Jay has a large number of
  2269. 1:53:20Neighbors
  2270. 1:53:21okay it's highly probable that you will
  2271. 1:53:25be one of them
  2272. 1:53:27so the more Jay has neighbors the more
  2273. 1:53:31probable it is that it's going to be
  2274. 1:53:33selected through this mean that I
  2275. 1:53:36explained that is I first choose i0 at
  2276. 1:53:40random
  2277. 1:53:41and then I choose J as a friend of i0
  2278. 1:53:44but if J is a friend of I zero it means
  2279. 1:53:47that I zero is a friend of J and because
  2280. 1:53:50Jay had many friends is going to be much
  2281. 1:53:52more likely to choose J if J as many
  2282. 1:53:55friends than if J has a few friends and
  2283. 1:53:58in the extreme you see that if Jay has
  2284. 1:54:01no friend there's no way to select J
  2285. 1:54:04using this procedure and that's exactly
  2286. 1:54:06what you find here when K is 0 Q of Q of
  2287. 1:54:100 is 0 there's no way to choose a
  2288. 1:54:13neighbor with zero neighbor with with
  2289. 1:54:16yeah it's impossible to choose J if J is
  2290. 1:54:19no friends so this is an extreme case
  2291. 1:54:22but you can intuitively understand that
  2292. 1:54:26the you know the more K the larger K the
  2293. 1:54:30more probable it is to choose the
  2294. 1:54:31southern J and as I said I didn't do the
  2295. 1:54:35argument in a in a rigorous way but if
  2296. 1:54:38you want to do it in a rigorous way you
  2297. 1:54:40can think of it in in the biased fashion
  2298. 1:54:44okay okay thanks
  2299. 1:54:56my theorem
  2300. 1:55:00so what is the probability that I'm
  2301. 1:55:02chosen knowing that I have K Neighbors
  2302. 1:55:05and it's the probability that I have K
  2303. 1:55:07Neighbors times the probability time
  2304. 1:55:09chosen but the probability that I am
  2305. 1:55:11chosen is proportional to k okay
  2306. 1:55:14okay
  2307. 1:55:19other questions
  2308. 1:55:25can you explain again how you obtained
  2309. 1:55:28the Criterion
  2310. 1:55:32so what I'm saying is that
  2311. 1:55:36these guys they're they're threads they
  2312. 1:55:40are selected as I've explained here so
  2313. 1:55:42the degree distribution of these people
  2314. 1:55:45is Q of K
  2315. 1:55:47and because the degree distribution of Q
  2316. 1:55:49is Q of K the average number of children
  2317. 1:55:53is the average degree minus one because
  2318. 1:55:56there was one link that comes from the
  2319. 1:55:59ancestor from the parent so the number
  2320. 1:56:02of outgoing links here minus the one
  2321. 1:56:05that makes him or her a child is the
  2322. 1:56:11expected value of K called in queue
  2323. 1:56:14because I have to use q and not P minus
  2324. 1:56:171.
  2325. 1:56:19and the minus one here counts away the
  2326. 1:56:23ancestor
  2327. 1:56:25is the new length
  2328. 1:56:27coming out of the selected child
  2329. 1:56:36but you know make no mistake I I'm I'm I
  2330. 1:56:39know that this is a this is a rough
  2331. 1:56:41argument this is a kind of hand waving
  2332. 1:56:43argument
  2333. 1:56:44but I thought that it was uh maybe more
  2334. 1:56:48interesting to present this in this way
  2335. 1:56:51for you to understand the Deep analogy
  2336. 1:56:53between the existence of a giant
  2337. 1:56:55component and uh the criticality of
  2338. 1:56:58branching processes which we've seen
  2339. 1:57:00last time rather than to give you a more
  2340. 1:57:03formal uh way to think about this this
  2341. 1:57:06this problem
  2342. 1:57:09as I said there is there's a way and
  2343. 1:57:11you'll see them this these calculation
  2344. 1:57:14in the notes there's a way to be much
  2345. 1:57:17more precise than this and in particular
  2346. 1:57:19to compute uh the probability for a node
  2347. 1:57:23to belong to the infinite cluster so
  2348. 1:57:26what I call P Infinity
  2349. 1:57:29you see here I have no way of computing
  2350. 1:57:32P Infinity it's just it's just an
  2351. 1:57:34existence Criterion
  2352. 1:57:36but it doesn't tell me what the
  2353. 1:57:38probability to belong to the giant
  2354. 1:57:40cluster is
  2355. 1:57:41whereas the more technical approach to
  2356. 1:57:45this problem gives you an answer for p
  2357. 1:57:47infinity and of course it gives you that
  2358. 1:57:49P Infinity is not zero when
  2359. 1:57:53e of Q is greater than 2.
  2360. 1:57:58thank you
  2361. 1:58:05okay
  2362. 1:58:09well have a good vacation week and um
  2363. 1:58:12we'll see each other
  2364. 1:58:14quotes and quotes
  2365. 1:58:16first week of March
  2366. 1:58:24thank you
  2367. 1:58:27thanks bye this conference will now be
  2368. 1:58:31recorded
  2369. 1:58:32okay great so let's start with this uh
  2370. 1:58:36last day before of uh the holidays so as
  2371. 1:58:40you see we uh kind of catched up with a
  2372. 1:58:43lecture because this today is about hoax
  2373. 1:58:45processes that have been discussed
  2374. 1:58:48during the lecture today
  2375. 1:58:49but it is a little bit long so what
  2376. 1:58:52we're gonna do is to split it into two
  2377. 1:58:55so today we will do only the first part
  2378. 1:58:57which is a little bit connected to what
  2379. 1:59:02was discussed in the lectures in
  2380. 1:59:03particular it focuses on linear hoax
  2381. 1:59:06processes and then the second part which
  2382. 1:59:09is about non-linear hoax processes and
  2383. 1:59:11meta stability this will be postponed to
  2384. 1:59:14the 10th of March at this point
  2385. 1:59:18and inside what we can do in the
  2386. 1:59:21remaining time today for those who are
  2387. 1:59:23interested is to go back to uh what we
  2388. 1:59:26left behind from the three which was the
  2389. 1:59:28derivation of soccer plan for a
  2390. 1:59:30multiplicative noise and I just want to
  2391. 1:59:32sketch how you derive it both in detail
  2392. 1:59:35and in the set on which prescription and
  2393. 1:59:37just to tell you how to compute
  2394. 1:59:39stationary states which is uh pretty
  2395. 1:59:42easy
  2396. 1:59:43uh okay a comment so unfortunately I
  2397. 1:59:46realized that the notation of the today
  2398. 1:59:48and one of the lectures are totally
  2399. 1:59:50messed up so what I will do is this
  2400. 1:59:54afternoon to somehow modify that a day
  2401. 1:59:56in such a way that we stick to the
  2402. 1:59:58notation of the lectures so I will
  2403. 2:00:00upload a version with the solutions
  2404. 2:00:02which is compatible with the lecture but
  2405. 2:00:05uh in here since I gave you the text
  2406. 2:00:07already I think it's better to speak to
  2407. 2:00:11the notation that we have in the text so
  2408. 2:00:13I wanted to be a little bit elastic so
  2409. 2:00:15what I did is to call the kernel that in
  2410. 2:00:18the lecture was K and now I call it high
  2411. 2:00:21then what was called row 0 as you will
  2412. 2:00:23see and becomes alcine here the average
  2413. 2:00:27uh let's say rate that was Lambda bar I
  2414. 2:00:32will call it g infinity infinity because
  2415. 2:00:34because of this ergodicity you can also
  2416. 2:00:37relate it to uh how the stationary value
  2417. 2:00:40of
  2418. 2:00:42of Lambda and then we will be working
  2419. 2:00:45today with exponential clearness so in
  2420. 2:00:47the lecture the uh let's say
  2421. 2:00:51Decay time was one over Alpha here since
  2422. 2:00:53we use Alpha instead of r0 I will
  2423. 2:00:57introduce beta so forgive me for this
  2424. 2:01:00annotational issue but keep in mind that
  2425. 2:01:03somehow we are talking about the same
  2426. 2:01:04things
  2427. 2:01:06okay so let's go to
  2428. 2:01:08then exercise one so let me recall the
  2429. 2:01:12expression for this conditional
  2430. 2:01:14intensity of the Oaks process that I
  2431. 2:01:17call Lambda tip so this is given by some
  2432. 2:01:21background intensity Lambda 0 which was
  2433. 2:01:23mu in the lecture and then you have the
  2434. 2:01:26term uh with the kernel that as I say I
  2435. 2:01:29write it as Alpha sum over all the
  2436. 2:01:33events that happened before the
  2437. 2:01:35particular time T that we are looking at
  2438. 2:01:37of some kernel
  2439. 2:01:39at T minus TI and as it was said in the
  2440. 2:01:43lecture already we can rewrite this
  2441. 2:01:46discrete sum in the following form so as
  2442. 2:01:50an integral from time let me say zero to
  2443. 2:01:53time t 0 minus infinity it doesn't
  2444. 2:01:56change much of the kernel so as of
  2445. 2:02:01P minus Tau and then you have the
  2446. 2:02:03differential of your stochastic process
  2447. 2:02:06that counts how many events you have at
  2448. 2:02:10times out to help you uh Tau plus beta
  2449. 2:02:14that I denote in this way here
  2450. 2:02:17and let me stress that this is a
  2451. 2:02:19condition and intensity because it is
  2452. 2:02:21conditioned to the history of the
  2453. 2:02:23process so you assume that you know what
  2454. 2:02:26is the history up to time T so uh which
  2455. 2:02:29events occurred and at which times and
  2456. 2:02:32then once you know this you can write
  2457. 2:02:34down what is if you want the probability
  2458. 2:02:36to have an event at a later time D plus
  2459. 2:02:39DT that is controlled by this Lambda
  2460. 2:02:42team
  2461. 2:02:44okay then there were several things that
  2462. 2:02:46were already introduced so in particular
  2463. 2:02:50what we are gonna look at in here is the
  2464. 2:02:53clustering ratio so in the lecture it
  2465. 2:02:56was discussed the value of the
  2466. 2:02:58clustering ratio sometimes somehow at
  2467. 2:03:00infinite time so the stationary value
  2468. 2:03:03but here let me introduce some
  2469. 2:03:06more General time dependent row of T
  2470. 2:03:09that we are going to compute and let me
  2471. 2:03:12Define this
  2472. 2:03:13similarly to the lecture as the variance
  2473. 2:03:16by this V I mean variance
  2474. 2:03:19of the number of events at times t plus
  2475. 2:03:23now minus
  2476. 2:03:24the number of events next time p
  2477. 2:03:28yes
  2478. 2:03:31there was a question
  2479. 2:03:32okay
  2480. 2:03:34divided by the average of uh of this
  2481. 2:03:38difference and you see that what I have
  2482. 2:03:41on the right hand side is something
  2483. 2:03:42which in principle depends on T but I'm
  2484. 2:03:46assuming that this the clustering ratio
  2485. 2:03:49only depends on the time difference and
  2486. 2:03:51this is some Assumption of stationarity
  2487. 2:03:53that holds in the phase and we will see
  2488. 2:03:57whenever Alpha is smaller than one so
  2489. 2:04:00whenever you have the process is
  2490. 2:04:02eventually ergotic
  2491. 2:04:04so this is the
  2492. 2:04:07clustering
  2493. 2:04:09ratio
  2494. 2:04:12and what we're going to do in here is to
  2495. 2:04:14compute this classing ratio for any
  2496. 2:04:16value of time Tau for one specific
  2497. 2:04:20kernel that was already introduced in
  2498. 2:04:22the lecture which is the exponential
  2499. 2:04:25kernel so in here
  2500. 2:04:27we are going to focus on a kernel that
  2501. 2:04:30is of the form beta e to the minus
  2502. 2:04:35and we're going to compute this through
  2503. 2:04:37uh an equation which relates the
  2504. 2:04:40clustering ratio to correlation
  2505. 2:04:42functions so that gives you the
  2506. 2:04:45correlation between the number of events
  2507. 2:04:47at different times and this is something
  2508. 2:04:49that is defined in the today in equation
  2509. 2:04:53four I think so let me not rewrite
  2510. 2:04:56equation for an equation five but this
  2511. 2:04:58is what we are going to use to compute
  2512. 2:05:00this object in here
  2513. 2:05:03and so just as a comment
  2514. 2:05:07actually uh let me introduce another
  2515. 2:05:09quantity first
  2516. 2:05:11so uh we are gonna first of all compute
  2517. 2:05:14uh what I call in the CB G of t
  2518. 2:05:19and G of T is defined so as it was
  2519. 2:05:22stressed already in the lecture this
  2520. 2:05:24quantity this conditional rate is a
  2521. 2:05:27random variable itself and it is a
  2522. 2:05:29random variable because it depends on
  2523. 2:05:31the history of the process so once you
  2524. 2:05:33know these three you know what is Lambda
  2525. 2:05:35of T but in principle the history is a
  2526. 2:05:38stochastic process so you have
  2527. 2:05:40fluctuations depending on the different
  2528. 2:05:42realizations and what we're going to
  2529. 2:05:44introduce is the average of this
  2530. 2:05:46quantity with respect to
  2531. 2:05:48um
  2532. 2:05:49to these histories or if you want the
  2533. 2:05:52Ensemble leverage
  2534. 2:05:53each of this conditional
  2535. 2:05:57rate Lambda t
  2536. 2:06:00and we're going to solve the equation
  2537. 2:06:01for this G of T and what was discussed
  2538. 2:06:05uh in the lecture was essentially the
  2539. 2:06:08solution of this equation in the long
  2540. 2:06:10time limit so the quantity Lambda bar
  2541. 2:06:13was
  2542. 2:06:14what I call G Infinity so it's the limit
  2543. 2:06:18D go into Infinity of this G of t
  2544. 2:06:23and it was given a self-consistent
  2545. 2:06:25equation for this Lambda Barrow or G
  2546. 2:06:27infinity and we will recover uh in here
  2547. 2:06:30the results for these uh which is of the
  2548. 2:06:32form so if you remember the infinity
  2549. 2:06:34will be equal to in this notation Lambda
  2550. 2:06:370 over 1 over alpha or in the notation
  2551. 2:06:40of the lecture it was uh divided by 1
  2552. 2:06:44minus
  2553. 2:06:46r0 yes
  2554. 2:06:50no okay
  2555. 2:06:53uh good
  2556. 2:06:56and the other quantity that was given in
  2557. 2:06:58the lecture was the infinite time limit
  2558. 2:07:00of this clustering ratio that was in our
  2559. 2:07:04rotation 1 over 1 minus Alpha to the
  2560. 2:07:07power 2 and this is something that we
  2561. 2:07:08will derive uh right now
  2562. 2:07:11for the exponential curve
  2563. 2:07:14okay so let's do it so the first point
  2564. 2:07:17we see this yes
  2565. 2:07:20uh the first point is to use so this is
  2566. 2:07:23going to be an exercise on a Laplace
  2567. 2:07:25transforms basically
  2568. 2:07:27and what we have to do is to solve the
  2569. 2:07:29equation for this G of T and the
  2570. 2:07:32equation reads as follows so I can
  2571. 2:07:34directly derive it from up there
  2572. 2:07:39hopefully yeah
  2573. 2:07:41so if you see I have the equation for
  2574. 2:07:43Lambda T up there and what I can do is
  2575. 2:07:45to take the expectation value on the
  2576. 2:07:48left hand side and then I take the
  2577. 2:07:50expectation value on the right hand side
  2578. 2:07:52and this I bring the expectation into
  2579. 2:07:54inside the integral there and I will
  2580. 2:07:57have the expectation value of the
  2581. 2:07:59differential of my stochastic process
  2582. 2:08:02and then I remember that Lambda of T was
  2583. 2:08:06defined uh so that if you want the
  2584. 2:08:08proper definition of Lambda T is of a
  2585. 2:08:11conditional expectation value of
  2586. 2:08:16having events in a small interval TD
  2587. 2:08:19plus BT conditions to the history of the
  2588. 2:08:22process up to time T that I will denote
  2589. 2:08:26as h of t
  2590. 2:08:28okay so if I have this Lambda T and then
  2591. 2:08:32I take also the expectation with respect
  2592. 2:08:34to the to the history what I get out is
  2593. 2:08:38is simply The Ensemble average now
  2594. 2:08:40averaging over all times of my ideas
  2595. 2:08:43that is what will appear in the right
  2596. 2:08:46hand side if I take the expectation of
  2597. 2:08:49of this equation so these were many
  2598. 2:08:51words but somehow you can easily realize
  2599. 2:08:54that the equation for this
  2600. 2:08:56GLT is nothing but Lambda 0 Plus
  2601. 2:09:00integral there was an alpha in front
  2602. 2:09:03integrated from 0 to T in the Tau
  2603. 2:09:07of
  2604. 2:09:08PSI of T minus Tau times
  2605. 2:09:11the very same function G of Tau
  2606. 2:09:15so this is a self-consistent equation an
  2607. 2:09:18integral equation for G that we want to
  2608. 2:09:20solve
  2609. 2:09:21and as you see in this equation what you
  2610. 2:09:25have on the right hand side is a
  2611. 2:09:26convolution which is
  2612. 2:09:28uh
  2613. 2:09:30some sort of convolution
  2614. 2:09:34so there is a Theta of
  2615. 2:09:38so you're asking here that tau is
  2616. 2:09:40smaller than T so there is a Theta of uh
  2617. 2:09:42T mining style so I can rewrite this
  2618. 2:09:45if you prefer
  2619. 2:09:47in this way
  2620. 2:09:49and then you recognize that we have a
  2621. 2:09:51convolution
  2622. 2:09:52and we know what we have to do when we
  2623. 2:09:55have convolutions so there is a very
  2624. 2:09:57useful instrument or trick that we can
  2625. 2:10:02use to solve this type of equation and
  2626. 2:10:04this is either Fourier or or Laplace
  2627. 2:10:07transforms so in here I will use Laplace
  2628. 2:10:10transforms and I will integrate only
  2629. 2:10:12over positive times
  2630. 2:10:15and Laplace transforms are useful
  2631. 2:10:16because anytime you have a convolution
  2632. 2:10:18they allow you to somehow rewrite name
  2633. 2:10:22in terms of Laplace transform the
  2634. 2:10:24equation in terms of a product so let me
  2635. 2:10:26introduce the notation first
  2636. 2:10:29so the Laplace transform
  2637. 2:10:32of a function G
  2638. 2:10:34that will be a function of s now is
  2639. 2:10:37simply
  2640. 2:10:38the integral from 0 to Infinity in DT e
  2641. 2:10:43to the minus s t times
  2642. 2:10:46High function G of t
  2643. 2:10:50and so if I take the Laplace transform
  2644. 2:10:52of this equation here so now we will
  2645. 2:10:54call this G hat
  2646. 2:10:57of s this is a function of s let me
  2647. 2:11:01apply a such a transform to this
  2648. 2:11:03equation and if you do this
  2649. 2:11:05you will realize that this gives you G
  2650. 2:11:08hat of s equal to
  2651. 2:11:10the Laplace transform of a constant that
  2652. 2:11:14we I will compute in a minute that's
  2653. 2:11:16very simple
  2654. 2:11:17plus as I said so this is an exercise
  2655. 2:11:20that if if you want we can do at the end
  2656. 2:11:23if you have questions but it's very easy
  2657. 2:11:25to say to see that here you will end up
  2658. 2:11:27with a product of the Laplace transforms
  2659. 2:11:30of these two quantities uh in here so
  2660. 2:11:35I will simply have
  2661. 2:11:37the Laplace transform of my kernel
  2662. 2:11:40evaluated at s times
  2663. 2:11:44my function transforms evaluated
  2664. 2:11:48foreign
  2665. 2:11:52and this is nice because now this is
  2666. 2:11:54just an algebraic equation for my
  2667. 2:11:56function in LaPlace space so what I have
  2668. 2:11:59to do is to compute these two terms that
  2669. 2:12:03I have in here so the first one is the
  2670. 2:12:05Laplace transform of a constant but this
  2671. 2:12:07is very easy so if you just put a
  2672. 2:12:09constant in here and you integrate the
  2673. 2:12:12exponential you just get a factor of 1
  2674. 2:12:14over s
  2675. 2:12:15times the constant so this means
  2676. 2:12:18that this is number 0 over s
  2677. 2:12:22plus Alpha
  2678. 2:12:24jihat of Ash
  2679. 2:12:26and then we plug our assumption that the
  2680. 2:12:30kernel is exponential so let me compute
  2681. 2:12:33uh this c bar
  2682. 2:12:36that's assuming that Phi as the form up
  2683. 2:12:40there so this is again just an
  2684. 2:12:42exponential integral so this will be the
  2685. 2:12:45integral from 0 to Infinity
  2686. 2:12:49of e to the minus s t times my function
  2687. 2:12:53P which is e to the minus beta
  2688. 2:12:56t okay
  2689. 2:12:59and so you see that again doing the same
  2690. 2:13:02exponentially integral you have B
  2691. 2:13:05divided this time
  2692. 2:13:07by a factor B plus s
  2693. 2:13:10so I plug it in here so I have beta
  2694. 2:13:13sorry not B but beta divided by beta
  2695. 2:13:17plus s
  2696. 2:13:20okay and now let me solve for a G of s
  2697. 2:13:25I hope that you see yes
  2698. 2:13:28so then I I have this G of s
  2699. 2:13:32I collect all of the terms so I will
  2700. 2:13:34have one minus alphabeta over
  2701. 2:13:38beta plus s this is equal to
  2702. 2:13:41Lambda 0 over s
  2703. 2:13:44and therefore
  2704. 2:13:48G hat of s
  2705. 2:13:50is now very simple it's number zero
  2706. 2:13:53times
  2707. 2:13:54beta plus s
  2708. 2:13:56divided by S times
  2709. 2:14:00uh bit I have beta minus Alpha Beta plus
  2710. 2:14:03s so I can write this as beta
  2711. 2:14:071 minus Alpha plus s
  2712. 2:14:12okay so this is the solution
  2713. 2:14:14in terms of Laplace transforms
  2714. 2:14:19and now of course once we have this what
  2715. 2:14:22we have to do is to do the inverse
  2716. 2:14:24Laplace transform to get the solution as
  2717. 2:14:28a function of time
  2718. 2:14:29so let me briefly recall how you do or
  2719. 2:14:32how you define the inverse transform and
  2720. 2:14:36what is the usual trick to compute it
  2721. 2:14:39which is the residue CRM so uh first of
  2722. 2:14:43all what is the definition of the
  2723. 2:14:44inverse
  2724. 2:14:46applied
  2725. 2:14:48to my function G hat of my laplacians 4
  2726. 2:14:51so this will be a function of t
  2727. 2:14:54again
  2728. 2:14:56and this is
  2729. 2:14:57defined as you have a factor of 1 over 2
  2730. 2:15:02pi I
  2731. 2:15:03and then you have to perform an integral
  2732. 2:15:05in general in the complex plane
  2733. 2:15:08a longer Contour which is usually called
  2734. 2:15:11the Bromwich Contour
  2735. 2:15:14then I will just write and then I will
  2736. 2:15:16comment so it's an integral along a
  2737. 2:15:19vertical axis in my complex plane where
  2738. 2:15:22the real part is equal to some constant
  2739. 2:15:24gamma and then I integrate over all the
  2740. 2:15:27axis so from gamma minus I Infinity to
  2741. 2:15:30gamma Plus
  2742. 2:15:31I Infinity
  2743. 2:15:33of what while the integral is in DS now
  2744. 2:15:37Ash is a complex variable in general and
  2745. 2:15:40then I have e to the HT so the
  2746. 2:15:43reciprocal of the factor that I had in
  2747. 2:15:46the direct transform times G hat
  2748. 2:15:49avash
  2749. 2:15:52now how do you choose gamma well you can
  2750. 2:15:55choose it more or less arbitrarily but
  2751. 2:15:58with a constraint that if you are doing
  2752. 2:16:01the inverse transform of a function
  2753. 2:16:03which has some singularities on the
  2754. 2:16:05complex plane you have to choose gamma
  2755. 2:16:08in such a way that you are always at the
  2756. 2:16:10right of the singularity so let me give
  2757. 2:16:12an example so now this is my complex
  2758. 2:16:15plane for the variable s real and
  2759. 2:16:18imaginary part
  2760. 2:16:20and let me assume that we want to do the
  2761. 2:16:22inverse transform of some function which
  2762. 2:16:24has some pole poles or singularities on
  2763. 2:16:28the complex plane so for instance let's
  2764. 2:16:30go back to the function that we have as
  2765. 2:16:32you see you have two simple poles of
  2766. 2:16:35this function one at s equal to zero so
  2767. 2:16:38you will have one pole here and another
  2768. 2:16:41one at s equal to minus beta times 1
  2769. 2:16:45minus Alpha that we assume uh
  2770. 2:16:49but you can take arbitrary sign but in
  2771. 2:16:52the drawing let me assume that one minus
  2772. 2:16:54size is positive so that the pole is is
  2773. 2:16:58negative so you have two singularities
  2774. 2:17:00and you have to choose gamma to the
  2775. 2:17:02right of this Singularity so whatever
  2776. 2:17:04vertical line
  2777. 2:17:06that is to the right of zero in this
  2778. 2:17:08example would be a good contour for me
  2779. 2:17:11to do to perform this integral and since
  2780. 2:17:13the function is analytic I can move it
  2781. 2:17:15back and forth provided that I do not
  2782. 2:17:19hit any singularity
  2783. 2:17:22and then once I have this Contour the
  2784. 2:17:25usual trick to to perform this
  2785. 2:17:28integration is to close the Contour
  2786. 2:17:31or one way if you want to perform the
  2787. 2:17:34integration is to close the Contour at
  2788. 2:17:36Infinity
  2789. 2:17:37and this is good because it allows me to
  2790. 2:17:40use the so-called residue theorem which
  2791. 2:17:43tells me how to compute
  2792. 2:17:45integrass over close Contours on the
  2793. 2:17:48complex plane by summing the residues of
  2794. 2:17:52the function add to the singularities
  2795. 2:17:54which are inside the Contour so first
  2796. 2:17:57let me comment why it is it's not
  2797. 2:18:00dangerous to close the Contour at
  2798. 2:18:02Infinity well this is so whenever you
  2799. 2:18:04have a function which decays
  2800. 2:18:06sufficiently fast at Infinity so in this
  2801. 2:18:09case you have a Decay that is one over s
  2802. 2:18:11Square so you know that the contribution
  2803. 2:18:13along this big circle will go to
  2804. 2:18:16Infinity if I send a will go to zero
  2805. 2:18:18sorry if I send the radius of the
  2806. 2:18:21Contour to Infinity so these pieces of
  2807. 2:18:24the controller will not eventually
  2808. 2:18:26contribute but they allow me to close my
  2809. 2:18:29my Contour of integration and then I can
  2810. 2:18:33use this residue
  2811. 2:18:35formula that I'm sure you know so
  2812. 2:18:37suppose that I want to compute an
  2813. 2:18:40integral over a closed Contour
  2814. 2:18:42that I call now Capital gamma of a
  2815. 2:18:44function f of z d z
  2816. 2:18:49so this residue theorem tells me that
  2817. 2:18:52what I have to do is to sum over all the
  2818. 2:18:54singularities that I have inside the
  2819. 2:18:56Contour the residues of the function at
  2820. 2:18:59those singularities so I will get
  2821. 2:19:03there is a factor of 2 pi I which I'm
  2822. 2:19:05happy about because it will cancel this
  2823. 2:19:08one and then I have a sum overall The
  2824. 2:19:11Singularity that I call
  2825. 2:19:13zadai
  2826. 2:19:16so for instance that I are eventually
  2827. 2:19:18the poles of my function f of Z
  2828. 2:19:22of the residue
  2829. 2:19:25of the function f
  2830. 2:19:27at the point that I
  2831. 2:19:32so if you have never seen this before
  2832. 2:19:35just let me know but otherwise
  2833. 2:19:38uh let me just remind you so if you have
  2834. 2:19:41a simple pulse like in here Computing
  2835. 2:19:44the residues is very very simple so what
  2836. 2:19:46you have to do is uh essentially to so
  2837. 2:19:50if you see in here I have a poet s equal
  2838. 2:19:52to zero so the residue of this function
  2839. 2:19:55will be given by you multiply the
  2840. 2:19:58function by S minus the value at the
  2841. 2:20:01pole so in this case it would be just s
  2842. 2:20:03and then you compute what remains
  2843. 2:20:05exactly at the pole so okay let me write
  2844. 2:20:09a formula
  2845. 2:20:10just to be concrete
  2846. 2:20:16here
  2847. 2:20:28so if you have a simple Pole
  2848. 2:20:33this means that your function will be of
  2849. 2:20:35the form let me say G of Z
  2850. 2:20:39divided by Z minus z i which is the pole
  2851. 2:20:44and this is my f of Z
  2852. 2:20:48and then the residue
  2853. 2:20:51of s at I
  2854. 2:20:54is
  2855. 2:20:56where space
  2856. 2:20:58the limit without going to the die
  2857. 2:21:02of Z minus z i times
  2858. 2:21:05F of Z
  2859. 2:21:08so it is just essentially the value of
  2860. 2:21:10what I call Gene here computed that said
  2861. 2:21:13I
  2862. 2:21:15okay so let's use this then to compute
  2863. 2:21:18the inverse Laplace transform of my
  2864. 2:21:21function G hat
  2865. 2:21:26see this
  2866. 2:21:28yeah
  2867. 2:21:30yes
  2868. 2:21:33okay so what will be G of t
  2869. 2:21:37so I will have a factor of 1 over 2 pi I
  2870. 2:21:41which I cancel with the 2 pi I coming
  2871. 2:21:44from the residue theorem and then I have
  2872. 2:21:46the sum over my two singularities
  2873. 2:21:52as I so s i is either 0 or minus beta
  2874. 2:21:56times 1 minus Alpha
  2875. 2:21:59of the residue now what is the function
  2876. 2:22:02of which I have to compute the residue
  2877. 2:22:04so if you see
  2878. 2:22:05from up there I have G hat times the
  2879. 2:22:08exponential factor which I don't have to
  2880. 2:22:10forget which G hat
  2881. 2:22:13of s e to the SP
  2882. 2:22:17at the point h i
  2883. 2:22:21okay
  2884. 2:22:22so for our examples
  2885. 2:22:24example up there so as I say the first
  2886. 2:22:27poll is at s equal to zero so if I
  2887. 2:22:31compute the residues there I just get
  2888. 2:22:34Lambda 0 times beta from the numerator
  2889. 2:22:38the exponential computed at s equal to 0
  2890. 2:22:40gives me one
  2891. 2:22:42and then below I have beta
  2892. 2:22:46times 1 minus Alpha
  2893. 2:22:48because X is equal to zero
  2894. 2:22:51plus the contribution of the second pole
  2895. 2:22:54so the second pole is at minus beta
  2896. 2:22:571 minus Alpha so I will have at the
  2897. 2:23:00denominator just
  2898. 2:23:02beta times 1 minus Alpha
  2899. 2:23:05which comes from the factor one whereas
  2900. 2:23:07and then I have up here Lambda 0 then I
  2901. 2:23:11have beta Plus
  2902. 2:23:13uh s computed as a pole so this gives me
  2903. 2:23:16beta minus beta
  2904. 2:23:18so this is just Alpha
  2905. 2:23:22I think and then the exponential which
  2906. 2:23:25this time is no zero is e to the minus
  2907. 2:23:29Alpha times t
  2908. 2:23:31okay
  2909. 2:23:35so beta here simplifies so let me write
  2910. 2:23:39it as Lambda 0 1 minus Alpha and then I
  2911. 2:23:43have 1 minus
  2912. 2:23:44Alpha times this exponential Factor
  2913. 2:23:51okay
  2914. 2:23:53and this gives me for any time the
  2915. 2:23:57average value
  2916. 2:23:58of of the condition and intensity
  2917. 2:24:03so from here you can now connect with
  2918. 2:24:06what was said already in the lecture so
  2919. 2:24:09the first thing that you can see is that
  2920. 2:24:13uh for this simple case of the
  2921. 2:24:15exponential kernel
  2922. 2:24:17you have so let's assume now that one
  2923. 2:24:20minus five is positive so Alpha is
  2924. 2:24:22smaller than one
  2925. 2:24:23and remember that Alpha was row zero I
  2926. 2:24:27think in the lecture so in this case the
  2927. 2:24:30process is uh stationary and it will be
  2928. 2:24:33ergotic this factor in the long time
  2929. 2:24:36limit will Decay to zero and you will
  2930. 2:24:38find that the value at infinite time of
  2931. 2:24:42this G is nothing but Lambda 0 divided
  2932. 2:24:44by 1 minus Alpha which is precisely the
  2933. 2:24:48Lambda bar that was defined in the
  2934. 2:24:51lecture so we recover this this first
  2935. 2:24:54result and we also know how you Decay to
  2936. 2:24:57this particular stationary value so you
  2937. 2:25:00Decay with a relaxation time that is of
  2938. 2:25:03the form beta times 1 minus Alpha which
  2939. 2:25:07is also related to
  2940. 2:25:09um to the comments in the lecture so you
  2941. 2:25:11see that as soon as you have Alpha which
  2942. 2:25:13is smaller than one everything is fine
  2943. 2:25:15as you approach this critical value
  2944. 2:25:18Alpha being equal to one you have two
  2945. 2:25:20divergences so you have one Divergence
  2946. 2:25:23of the stationary rate in here and you
  2947. 2:25:26also have the Divergence of these
  2948. 2:25:29relaxation time and this tells you that
  2949. 2:25:32you are approaching a regime for this
  2950. 2:25:34point process which is unstable and
  2951. 2:25:38indeed if you choose Alpha larger than
  2952. 2:25:39one the processes is non-fictionary it
  2953. 2:25:42is not well designed if you want and you
  2954. 2:25:45see it from the fact that you have an
  2955. 2:25:46intensity which explodes exponentially
  2956. 2:25:49over time so if you have time to look at
  2957. 2:25:52the homework
  2958. 2:25:54on work five there there is a simple
  2959. 2:25:57code or a code to implement this hoax
  2960. 2:26:01process with the exponential kernel and
  2961. 2:26:04you can play around with this parameter
  2962. 2:26:07Alpha and you can really see what
  2963. 2:26:08happens if you choose Alpha uh becoming
  2964. 2:26:12closer and closer to one so you see that
  2965. 2:26:13the number of events start
  2966. 2:26:17increasing in a way that is somehow
  2967. 2:26:20uncontrolled as you expect from here
  2968. 2:26:23okay so this was the first point
  2969. 2:26:27now let me do another comment which is
  2970. 2:26:30good for the next exercise so we solve
  2971. 2:26:34let me go back to the equation where it
  2972. 2:26:36is
  2973. 2:26:37I I erased it so we had an equation for
  2974. 2:26:40G of T which was uh this convolution so
  2975. 2:26:44GST is a constant I know it's up there
  2976. 2:26:51okay
  2977. 2:26:54so you see it's a constant Plus this
  2978. 2:26:58convolution between the kernel and the
  2979. 2:27:00constant and the function itself
  2980. 2:27:02and we are saying that we want to choose
  2981. 2:27:04a kernel that is exponential and we can
  2982. 2:27:07solve the equation uh by Laplace
  2983. 2:27:09transform and this is what you should do
  2984. 2:27:11for any arbitrary kernel
  2985. 2:27:13but if you have a kernel that is
  2986. 2:27:15exponential you can immediately guess
  2987. 2:27:17what is the form of your function G of T
  2988. 2:27:20that is by the way this form in here
  2989. 2:27:23that is you can guess that the function
  2990. 2:27:26is itself an exponential and this is
  2991. 2:27:28because if you look at the right hand
  2992. 2:27:30side you have an integral of Phi which
  2993. 2:27:33is an exponential function and if you
  2994. 2:27:35assume that g is itself an exponential
  2995. 2:27:37function the integral of the product of
  2996. 2:27:40two exponentials will give you back
  2997. 2:27:42another exponential so by adjusting the
  2998. 2:27:45coefficient you can match the right hand
  2999. 2:27:47side to the left hand side and see that
  3000. 2:27:49any exponential answer is a good
  3001. 2:27:51solution for for the equation up there
  3002. 2:27:54so this was another possible way to uh
  3003. 2:27:58to proceed and this is what we are using
  3004. 2:27:59now to uh to solve another equation that
  3005. 2:28:02is the point two
  3006. 2:28:04of the exercise that is now the equation
  3007. 2:28:07yes
  3008. 2:28:09I have a question about the solution we
  3009. 2:28:12just found so does this mean if we
  3010. 2:28:14choose Alpha equals to one oh sorry can
  3011. 2:28:16you hear me
  3012. 2:28:17yes it is it's always bad but so far yes
  3013. 2:28:22okay sorry
  3014. 2:28:23um if we choose Alpha equals to one does
  3015. 2:28:26that mean that we reduce the problem
  3016. 2:28:27back to a poisson process
  3017. 2:28:30in here you should know actually it's
  3018. 2:28:34the limit Alpha going to zero that gives
  3019. 2:28:36you the percent so the question is uh
  3020. 2:28:39somehow for which Alpha I go back to a
  3021. 2:28:40person process
  3022. 2:28:42and the idea is that uh the limit of the
  3023. 2:28:45poisson process is given by
  3024. 2:28:48having no uh memory kernel if you want
  3025. 2:28:51in your process so what happens in in a
  3026. 2:28:54personal process is that uh the the
  3027. 2:28:57probability to have
  3028. 2:28:59a certain number of events in a given
  3029. 2:29:01small interval is uh independent with
  3030. 2:29:05respect to uh to the previous history of
  3031. 2:29:07the process so to the to the number of
  3032. 2:29:09events that you had before reaching that
  3033. 2:29:11interval and this is something that you
  3034. 2:29:14would recover setting Alpha equal to
  3035. 2:29:15zero in here so killing this memory term
  3036. 2:29:18that that carries memory about uh the
  3037. 2:29:22previous uh realization of the process
  3038. 2:29:25and indeed in the poisson case you just
  3039. 2:29:28have that the rate that controls whether
  3040. 2:29:32you have an event or not in a small
  3041. 2:29:34interval DP is a constant rate so this
  3042. 2:29:36would be poisson
  3043. 2:29:40and now that we are going to compute
  3044. 2:29:41this we are uh we will be able to check
  3045. 2:29:45that indeed that the ratio the
  3046. 2:29:48clustering ratio of the postman process
  3047. 2:29:50which is equal to one is recovered for
  3048. 2:29:53uh Alpha equal to zero
  3049. 2:29:56is it fine
  3050. 2:29:59uh yes thank you very much okay
  3051. 2:30:05so let's do that
  3052. 2:30:08and to do that we have to
  3053. 2:30:12let's say accept another equation which
  3054. 2:30:15is another integral equation this time
  3055. 2:30:18for the
  3056. 2:30:19correlation function
  3057. 2:30:25that I am not deriving in here but I
  3058. 2:30:28think you find
  3059. 2:30:30some derivation in the lecture notes
  3060. 2:30:34in in the last chapter that was given of
  3061. 2:30:36the lecture notes
  3062. 2:30:39and this equation has a name it is
  3063. 2:30:42called
  3064. 2:30:45this fold
  3065. 2:30:49there's a name that I forgot so let me
  3066. 2:30:53what is it you'll Walker equation
  3067. 2:31:01okay
  3068. 2:31:02and it is quite similar to the equation
  3069. 2:31:04we had for G so the idea is that you get
  3070. 2:31:08the correlation between the number of
  3071. 2:31:11events in two interval in two times if
  3072. 2:31:14you want separated by uh by a Time shift
  3073. 2:31:17Tau
  3074. 2:31:19this is equal to Alpha divided by
  3075. 2:31:23G Infinity so G Infinity maybe I didn't
  3076. 2:31:25Define it but it is
  3077. 2:31:30simply the limit of what we just
  3078. 2:31:33computed at large times
  3079. 2:31:35so for the explanation
  3080. 2:31:37currently it was just Lambda 0 1 minus
  3081. 2:31:41Alpha so this was Lambda bar in the
  3082. 2:31:43lecture
  3083. 2:31:46so this is what appears uh in here then
  3084. 2:31:49you have your kernel
  3085. 2:31:52I'm rewriting equation eight if you're
  3086. 2:31:55looking at it today
  3087. 2:31:58and then we have another
  3088. 2:32:01convolution again between
  3089. 2:32:04your kernel and the correlation function
  3090. 2:32:06itself
  3091. 2:32:09and this correlation function is assumed
  3092. 2:32:11to be symmetric
  3093. 2:32:15with respect to this
  3094. 2:32:17time difference now
  3095. 2:32:21okay now what we can do so why we want
  3096. 2:32:23to compute this because as you see from
  3097. 2:32:25that today there is an equation which
  3098. 2:32:28relates our clustering ratio that is uh
  3099. 2:32:32naturally related to a correlation
  3100. 2:32:34function because you see that it has two
  3101. 2:32:36times appearing when you compute this
  3102. 2:32:39variance so there is an explicit
  3103. 2:32:41equation which relates this quantity to
  3104. 2:32:44this correlation function so what we are
  3105. 2:32:46going to do is to compute this and then
  3106. 2:32:48use the result again for the exponential
  3107. 2:32:50kernel to get the clustering ratio
  3108. 2:32:54and we can proceed exactly as before so
  3109. 2:32:56we can do the Laplace transform of this
  3110. 2:32:59equation and solve it and this is what
  3111. 2:33:01you find in the lecture notes or we can
  3112. 2:33:05use this idea that I just mentioned that
  3113. 2:33:07if Phi is an exponential then we should
  3114. 2:33:10expect some sort of exponential form uh
  3115. 2:33:14also for the function C so it is
  3116. 2:33:16consistent to assume and this is what
  3117. 2:33:18I'm gonna do in here that our sea of Tau
  3118. 2:33:23has an explonation form so it is some
  3119. 2:33:26constant capital c
  3120. 2:33:28times e to the minus some exponents that
  3121. 2:33:32we have to determine that I call gamma
  3122. 2:33:34in here
  3123. 2:33:35and then I I put an absolute value of
  3124. 2:33:38Tau and I put an absolute value because
  3125. 2:33:40I want uh to preserve a symmetry of the
  3126. 2:33:43correlation function
  3127. 2:33:46okay so this is an answer
  3128. 2:33:51so what I can do is I take these assets
  3129. 2:33:53and I plug it into into our equations
  3130. 2:33:56and then I use the equation to determine
  3131. 2:33:59what is the expression for C and what is
  3132. 2:34:02the expression for gamma
  3133. 2:34:04so the left-hand side is easy so I get c
  3134. 2:34:07e to the minus gamma so now let's assume
  3135. 2:34:09that tau is positive
  3136. 2:34:14so I have c e to the minus gamma Tau
  3137. 2:34:17then on the right hand side I have my
  3138. 2:34:20exponential kernel beta e to the minus
  3139. 2:34:23beta Tau
  3140. 2:34:25and then I have this convolution to
  3141. 2:34:28compute so this is the integral from 0
  3142. 2:34:30to Infinity in the U
  3143. 2:34:33Alpha Beta e to the minus beta U
  3144. 2:34:37which is my fear of you
  3145. 2:34:39and then C and C is what is capital c e
  3146. 2:34:43to the minus gamma and now here I have
  3147. 2:34:45to keep the absolute value because uh
  3148. 2:34:49you as you see I'm integrating over U
  3149. 2:34:51from 0 to Infinity so this can be both
  3150. 2:34:54larger or smaller with respect to Tau so
  3151. 2:34:56I have to split
  3152. 2:34:59these two cases
  3153. 2:35:02so let's split these two cases
  3154. 2:35:05just a bit of algebra
  3155. 2:35:07so I have alphabeta over
  3156. 2:35:10G Infinity to the minus beta Tau
  3157. 2:35:14plus Alpha Beta capital c
  3158. 2:35:19and then
  3159. 2:35:20I assume first so I do first the
  3160. 2:35:23integration from zero to Tau which I
  3161. 2:35:26assume to be positive
  3162. 2:35:28so if I integrate from 0 to Tau I have e
  3163. 2:35:31to the minus beta U
  3164. 2:35:33and then U is smaller than Tau so this
  3165. 2:35:35is positive so this is minus
  3166. 2:35:38gamma Tau Plus
  3167. 2:35:41gamma U
  3168. 2:35:44okay
  3169. 2:35:45and then in the remaining
  3170. 2:35:48parts of the domain from Tau to Infinity
  3171. 2:35:50I still have e to the minus beta U and
  3172. 2:35:53then I have to flip the sign so this
  3173. 2:35:55gives me minus gamma U Plus
  3174. 2:35:59gamma Tau
  3175. 2:36:02okay
  3176. 2:36:04now where should I go maybe on the other
  3177. 2:36:07side
  3178. 2:36:10now I have
  3179. 2:36:13to do simple exponentially integrals
  3180. 2:36:16over you
  3181. 2:36:27this will be equal to so this is the
  3182. 2:36:30same as this
  3183. 2:36:33alpha beta version Infinity to the minus
  3184. 2:36:36beta u n o Tau
  3185. 2:36:39Plus
  3186. 2:36:41foreign
  3187. 2:36:46so from here what do I get so I have a
  3188. 2:36:49factor of e to the minus gamma Tau that
  3189. 2:36:52I can bring outside the Integra
  3190. 2:36:58and then I have the integral of e to the
  3191. 2:37:00minus
  3192. 2:37:02beta between brackets beta minus gamma
  3193. 2:37:05times U which gives me uh well let me
  3194. 2:37:09write this compactly this will be 1
  3195. 2:37:11minus E to the minus
  3196. 2:37:13beta minus gamma Tau
  3197. 2:37:16divided by
  3198. 2:37:18beta minus gamma
  3199. 2:37:23plus then I have the second term
  3200. 2:37:26uh let me write it here sorry that there
  3201. 2:37:31is a little bit of confusion with the
  3202. 2:37:33space so now in this case I have to take
  3203. 2:37:36out a factor of e to the gamma Tau
  3204. 2:37:40and then I have the integral
  3205. 2:37:42of e to the minus this time between
  3206. 2:37:44brackets beta plus gamma times U
  3207. 2:37:48between infinity and Tau so this will
  3208. 2:37:50give me e to the minus
  3209. 2:37:53beta plus gamma Tau divided by
  3210. 2:37:56beta plus gamma
  3211. 2:37:58hopefully
  3212. 2:38:00okay
  3213. 2:38:03and so let me now collect all of the
  3214. 2:38:07terms which have the same exponential in
  3215. 2:38:09front
  3216. 2:38:10so there are some terms which have a
  3217. 2:38:12factor of e to the minus
  3218. 2:38:15beta Tau in front
  3219. 2:38:17so we have one here this is just Alpha
  3220. 2:38:20Beta divided by
  3221. 2:38:21Gene Trinity
  3222. 2:38:23and then you see that if I multiply this
  3223. 2:38:25times this the factor of gamma conscious
  3224. 2:38:28and I just get the factor of e to the
  3225. 2:38:30minus beta Tau so this will contribute
  3226. 2:38:32with minus
  3227. 2:38:34Alpha Beta t
  3228. 2:38:37divided by
  3229. 2:38:38beta minus gamma and the same from here
  3230. 2:38:42so this is Plus
  3231. 2:38:44Alpha Beta C divided by Beta plus gamma
  3232. 2:38:50and then I have a unique term which
  3233. 2:38:53depends
  3234. 2:38:54at the exponents only on gamma which is
  3235. 2:38:57the term that I get
  3236. 2:38:59from this product so when I'm left with
  3237. 2:39:04alphabetashi
  3238. 2:39:06divided by Beta minus gamma
  3239. 2:39:09e to the minus gamma Tau
  3240. 2:39:13okay
  3241. 2:39:15and I'm rewriting this in this way
  3242. 2:39:16because now you see that I have an
  3243. 2:39:19expression on the right hand side that I
  3244. 2:39:20have to match with what we had on the
  3245. 2:39:23left hand side and on the left hand side
  3246. 2:39:26we only add the dependence on gamma
  3247. 2:39:29so uh what this means is that I have to
  3248. 2:39:32kill the factor which depends on e to
  3249. 2:39:34the minus gamma Tau so I have to set to
  3250. 2:39:36zero
  3251. 2:39:38what is in parenthesis in here and this
  3252. 2:39:41will give me an equation for C
  3253. 2:39:44if I solve this and then I have to match
  3254. 2:39:47the prefactoring here with the prefactor
  3255. 2:39:51that I have on the left hand side which
  3256. 2:39:52is just the constant C
  3257. 2:39:55and this immediately tells me that I
  3258. 2:39:57need
  3259. 2:39:58alphabeta divided by Beta minus gamma to
  3260. 2:40:02be equal to 1.
  3261. 2:40:04okay so from here I can read
  3262. 2:40:08that gamma similarly to the Decay that
  3263. 2:40:12we had above
  3264. 2:40:14must be equal to Beta times
  3265. 2:40:161 minus Alpha
  3266. 2:40:20and then plug in this expression from
  3267. 2:40:22gamma in here and setting this to zero I
  3268. 2:40:25get out an expression for C that I will
  3269. 2:40:28directly give you
  3270. 2:40:31in a minute
  3271. 2:40:33and you can do it by yourself
  3272. 2:40:37so with this matching condition
  3273. 2:40:47I recover the full correlation function
  3274. 2:40:50for the exponential kernel
  3275. 2:41:09foreign
  3276. 2:41:16is
  3277. 2:41:17of the following form so now I use the
  3278. 2:41:20expression that you can derive for the
  3279. 2:41:22constant C which is
  3280. 2:41:25Alpha Beta
  3281. 2:41:29over two
  3282. 2:41:31there is
  3283. 2:41:332 minus Alpha divided 1 minus Alpha
  3284. 2:41:381 over G Infinity that we know what it
  3285. 2:41:41is so this is Lambda 0 divided by 1
  3286. 2:41:43minus Alpha so you can plug it in if you
  3287. 2:41:46want and then I have e to the minus
  3288. 2:41:48beta 1 minus Alpha times
  3289. 2:41:52absolute value of Tau so above I assume
  3290. 2:41:56that I was positive if you assume it
  3291. 2:41:57negative you get a very similar
  3292. 2:42:00um
  3293. 2:42:01results that gives you this final
  3294. 2:42:04expression
  3295. 2:42:06okay and now finally
  3296. 2:42:09and perhaps I'm not doing this
  3297. 2:42:11explicitly but once we have the
  3298. 2:42:14correlation we can plug this
  3299. 2:42:16expression into the form
  3300. 2:42:18or the equation for
  3301. 2:42:20rope so they clustering ratio
  3302. 2:42:30so this requires doing other
  3303. 2:42:33exponential integrals but that those are
  3304. 2:42:36straightforwards so I will just
  3305. 2:42:38comment on what you get in the end
  3306. 2:42:41so from equation five uh in the today
  3307. 2:42:44where row is called r
  3308. 2:42:50you know that this will be 1 plus 2 this
  3309. 2:42:54G Infinity integral from 0 to Tau in the
  3310. 2:42:58U
  3311. 2:42:591 minus U over Tau times the function of
  3312. 2:43:03C that we just determined
  3313. 2:43:05so C is an exponential so if you
  3314. 2:43:07integrate this term will give you an
  3315. 2:43:10exponential and the second integral is
  3316. 2:43:12just an exponential times U so the
  3317. 2:43:15fastest way to do this if you have the
  3318. 2:43:17integral of x e to the minus alpha x is
  3319. 2:43:21to write it as minus the derivative over
  3320. 2:43:24a or Alpha of the integral
  3321. 2:43:27of e to the minus ax so you just have to
  3322. 2:43:31compute exponential integers and then
  3323. 2:43:33eventually derive it
  3324. 2:43:35with respect to the to the exponent so
  3325. 2:43:38you can do this in here and you get out
  3326. 2:43:40the following that now we can
  3327. 2:43:43comment
  3328. 2:43:46so we have a factor of 1 over
  3329. 2:43:491 minus Alpha Square
  3330. 2:43:52and then we have a factor that depends
  3331. 2:43:55that contains 1 over Tau which comes
  3332. 2:43:58from here
  3333. 2:44:00some numbers to minus Alpha over Alpha
  3334. 2:44:04so these are coming from the constant C
  3335. 2:44:06in the correlation function
  3336. 2:44:10okay
  3337. 2:44:11and then we have exponentials coming
  3338. 2:44:14from the integral with
  3339. 2:44:16this gamma exponent
  3340. 2:44:20that is beta times one minus Alpha
  3341. 2:44:26okay so again what you see so now this
  3342. 2:44:30is an expression for arbitrary times Tau
  3343. 2:44:34so what we can do is to study
  3344. 2:44:36the two limits of this Expressions so
  3345. 2:44:39first we assume so we have a relaxation
  3346. 2:44:41time uh in here let me call it Tau
  3347. 2:44:44relaxation that is
  3348. 2:44:471 over beta
  3349. 2:44:50times one minus Alpha
  3350. 2:44:53so this tells me that if I choose times
  3351. 2:44:57which are small with respect to this
  3352. 2:44:59relaxation times I can approximate this
  3353. 2:45:02function uh rasi by I can do the linear
  3354. 2:45:04expansion of the exponential and if
  3355. 2:45:06instead I'm looking at very large times
  3356. 2:45:08I can approximate be exponential with
  3357. 2:45:10with zero essentially and this will give
  3358. 2:45:13me the two limits so for sure times
  3359. 2:45:21meaning shorter than the relaxation
  3360. 2:45:24times I expand linearly this exponential
  3361. 2:45:27and what I get is that
  3362. 2:45:30row of tau is approximately
  3363. 2:45:34well the same factor of 1 over
  3364. 2:45:371 minus Alpha Square
  3365. 2:45:39and then I have so let me copy this to
  3366. 2:45:42minus
  3367. 2:45:44Alpha
  3368. 2:45:462 minus Alpha
  3369. 2:45:481 minus Alpha cubed
  3370. 2:45:51and then you see if I expand this this
  3371. 2:45:53will give me
  3372. 2:45:541 minus Tau which cancels so the one
  3373. 2:45:58will cancel and the Tau coming from the
  3374. 2:46:01linear term will cancel with this
  3375. 2:46:03there is a factor of beta that will
  3376. 2:46:05cancel with this and then there is a
  3377. 2:46:06factor of 1 minus Alpha that will cancel
  3378. 2:46:08with one of these Powers so if you do
  3379. 2:46:10this
  3380. 2:46:11you just get this
  3381. 2:46:14and you see that what you have in the in
  3382. 2:46:17the numerator is 1 minus two alpha plus
  3383. 2:46:20Alpha Square so this is precisely
  3384. 2:46:22y minus Alpha to the power 2 so you see
  3385. 2:46:25that in this short time limit
  3386. 2:46:27your clustering ratio is essentially
  3387. 2:46:31equal to one in particular in the in the
  3388. 2:46:33limit Tau going to zero this is uh well
  3389. 2:46:35no
  3390. 2:46:37you have this Singularity yes in the
  3391. 2:46:39limit Tau equal to zero this is exactly
  3392. 2:46:41equal to one because you cancel this
  3393. 2:46:44Singularity with this linearized
  3394. 2:46:46function
  3395. 2:46:47and what is one well what is one is the
  3396. 2:46:50poisson
  3397. 2:46:59and why do you get the personal ratio
  3398. 2:47:01well one way to to understand it
  3399. 2:47:03intuitively so remember that we said
  3400. 2:47:07that our Lambda
  3401. 2:47:11was Lambda 0 that is what you would get
  3402. 2:47:14if you just had a personal process plus
  3403. 2:47:17your kernel
  3404. 2:47:19and your kernel was an integral over
  3405. 2:47:22time and so what you can expect is that
  3406. 2:47:25in order for this kernel to be important
  3407. 2:47:28you have to allow your process to uh to
  3408. 2:47:32run a little bit because the process has
  3409. 2:47:34to realize that there are some events at
  3410. 2:47:37previous times and has to be excited by
  3411. 2:47:40this previous event and therefore if you
  3412. 2:47:43just look at very short times you
  3413. 2:47:44basically don't see the aspect of this
  3414. 2:47:47excitation kernel and you just recover
  3415. 2:47:49the poisson result
  3416. 2:47:51on the other hand if you've got a very
  3417. 2:47:52long time or large times
  3418. 2:48:00then you can eliminate this exponential
  3419. 2:48:04you also have a factor of one over Tau
  3420. 2:48:06that kills completely uh this second
  3421. 2:48:09term uh on the right and so you see that
  3422. 2:48:12your profile goes asymptotically as one
  3423. 2:48:16over
  3424. 2:48:17one minus Alpha Square
  3425. 2:48:20which is what was given in the lecture
  3426. 2:48:22foreign
  3427. 2:48:29larger than one because Alpha is
  3428. 2:48:32positive so the denominator is smaller
  3429. 2:48:34than one
  3430. 2:48:35so again just to have an example in the
  3431. 2:48:37arm work if you really do the simulation
  3432. 2:48:41of of the hoax process you can compute
  3433. 2:48:45this clustering ratio and you do this
  3434. 2:48:47taking the ratio of the variance with
  3435. 2:48:49respect to the expectation value and as
  3436. 2:48:52a function of Tau you should see
  3437. 2:48:54this you can see in the solution
  3438. 2:48:56something like this so you see that at
  3439. 2:48:59zero time it starts from one and then it
  3440. 2:49:01converges to some value that now we know
  3441. 2:49:04it has to be equal to one minus Alpha to
  3442. 2:49:07the power two so you can choose a value
  3443. 2:49:09of Alpha and then you can check that
  3444. 2:49:11this is the case and this is number five
  3445. 2:49:15point four
  3446. 2:49:17I think
  3447. 2:49:21okay
  3448. 2:49:22uh
  3449. 2:49:24what else well maybe just one finite
  3450. 2:49:27comment final which is related to
  3451. 2:49:31[Music]
  3452. 2:49:32um
  3453. 2:49:33uh to to to
  3454. 2:49:35the third point of exercise one that we
  3455. 2:49:38are not doing in detail but I will just
  3456. 2:49:40comment
  3457. 2:49:42so in the end what uh what do we derive
  3458. 2:49:45so we derive
  3459. 2:49:46in particular this expression
  3460. 2:49:49for the relaxation time
  3461. 2:49:52and for the asymptotic
  3462. 2:49:54uh
  3463. 2:49:55average rate which is
  3464. 2:49:58Lambda 0 1 minus Alpha
  3465. 2:50:05and I just want to point out that you
  3466. 2:50:07really see the aspect of this excitation
  3467. 2:50:10currentness so on one end
  3468. 2:50:13you see the effect because whenever
  3469. 2:50:15Alpha so when Alpha is equal to zero you
  3470. 2:50:16recover uh question whenever Alpha is
  3471. 2:50:20different from zero you have a value of
  3472. 2:50:22G which is larger so you have more
  3473. 2:50:24events than what you would expect in an
  3474. 2:50:26independent question process and this is
  3475. 2:50:28because as soon as you have one event
  3476. 2:50:30your excitation kernels promotes uh new
  3477. 2:50:33events uh in your process and this is
  3478. 2:50:36what you read out from from this and
  3479. 2:50:39also you have a relaxation time
  3480. 2:50:41which is again larger than what you
  3481. 2:50:45would have in absence of the current so
  3482. 2:50:47when Alpha is equal to zero because
  3483. 2:50:52so if you uh or actually this is larger
  3484. 2:50:55than what you would have somehow
  3485. 2:50:58if you just so this beta is what
  3486. 2:51:00controls the decay of the kernel here
  3487. 2:51:02right so this was
  3488. 2:51:05the kernel times
  3489. 2:51:07uh G of Tau itself
  3490. 2:51:11so we have a natural scale at which this
  3491. 2:51:14kernel decays which is one over beta in
  3492. 2:51:17our exponential example and this tells
  3493. 2:51:20you that if you have a mother event so
  3494. 2:51:22one point which occurs then this will
  3495. 2:51:26influence the future history up to times
  3496. 2:51:29which are of the order of one over beta
  3497. 2:51:32naively
  3498. 2:51:33but then the fact that you have this
  3499. 2:51:35self-excitation it tells you that
  3500. 2:51:37actually the influence goes over to
  3501. 2:51:39times which are larger than 1 over beta
  3502. 2:51:41by a factor of uh one times uh one over
  3503. 2:51:45one minus Alpha and this is again an
  3504. 2:51:48effect of an effect of self-excitation
  3505. 2:51:50so what happens is that you have a
  3506. 2:51:52mother event
  3507. 2:51:53this of course will influence all the
  3508. 2:51:55history in the future but if the mother
  3509. 2:51:58event gives rise to one son so think
  3510. 2:52:01again in terms of this uh Carlton Watson
  3511. 2:52:05birth processes the sun itself will
  3512. 2:52:09influence the future I will increase the
  3513. 2:52:12probability to to have more events and
  3514. 2:52:15and this is what is measured by this
  3515. 2:52:17factor of one over one minus Alpha and
  3516. 2:52:19in particular in the third part of the
  3517. 2:52:22exercise if you think about this as a
  3518. 2:52:26person that actually birth process what
  3519. 2:52:28you realize is that one over beta is
  3520. 2:52:31like the fertility of of the mother so
  3521. 2:52:34time scale over which the mother can
  3522. 2:52:36make songs but this is increased by a
  3523. 2:52:39factor of one over one minus Alpha which
  3524. 2:52:41is the average size of the family
  3525. 2:52:43generated by the mother and this
  3526. 2:52:46accounts for the fact that the mother
  3527. 2:52:48can generate many sounds and each of
  3528. 2:52:51these phones will increase the
  3529. 2:52:52probability to future events and this is
  3530. 2:52:55what eventually will increase if you
  3531. 2:52:57want the influence of the mother event
  3532. 2:53:00by this factor of one over one minus
  3533. 2:53:02Alpha so to make this a bit more precise
  3534. 2:53:04you can go and have a look at the third
  3535. 2:53:07exercise but somehow the idea is is what
  3536. 2:53:12I just sketched
  3537. 2:53:14okay so this was
  3538. 2:53:16for what concerns hoax
  3539. 2:53:18and now
  3540. 2:53:21we don't have much time
  3541. 2:53:23I just wanted so for those of you who
  3542. 2:53:26want to pay
  3543. 2:53:28maybe to sketch very briefly
  3544. 2:53:33um
  3545. 2:53:38this idea of Poker plank
  3546. 2:53:41with multiplicative noise
  3547. 2:53:44so if you
  3548. 2:53:46had time to go back to the tedda 3 and
  3549. 2:53:49the solutions you have seen how to
  3550. 2:53:51derive soccer planks for instance
  3551. 2:53:54in the case of additive noise and I
  3552. 2:53:56think this is also discussed in other
  3553. 2:53:58courses
  3554. 2:54:00so the only thing I wanted to point out
  3555. 2:54:02is that whenever you have multiplicative
  3556. 2:54:04noise again
  3557. 2:54:06you have to always specify the
  3558. 2:54:08prescription of this critization that
  3559. 2:54:10you use
  3560. 2:54:11so whether it's Ito or shatanovic
  3561. 2:54:15and you get two different forms if you
  3562. 2:54:18remember of the focal Planck equation
  3563. 2:54:22so now this is let's say soccer plank
  3564. 2:54:27I'll try to be short
  3565. 2:54:30and just to give the main ideas
  3566. 2:54:33so photo plan came from launch event
  3567. 2:54:37so in one dimension you have the X where
  3568. 2:54:40DT equal to some drift term
  3569. 2:54:43F of t plus
  3570. 2:54:45our noise
  3571. 2:54:48and remember that we could discretize
  3572. 2:54:54these equations so we can say that over
  3573. 2:54:57a small interval DT
  3574. 2:54:59we increment
  3575. 2:55:01so the value of the process at the time
  3576. 2:55:03t plus DTS is related to the value at a
  3577. 2:55:06time t
  3578. 2:55:09by this F evaluated
  3579. 2:55:13at some point
  3580. 2:55:15within let me call it X bar of T of
  3581. 2:55:19course this is
  3582. 2:55:21NX
  3583. 2:55:23these are functions of the process
  3584. 2:55:26so this was a point to be chosen
  3585. 2:55:29properly inside the interval TD plus BT
  3586. 2:55:33and then we have the same
  3587. 2:55:38times the noise in the interval times DT
  3588. 2:55:42and remember that the noise is of order
  3589. 2:55:44one over square root of DT so what we
  3590. 2:55:47have in here
  3591. 2:55:48is of order
  3592. 2:55:50square root of DT
  3593. 2:55:54so we can rewrite it and this is useful
  3594. 2:55:57to derive the plank as
  3595. 2:56:02so we can call this
  3596. 2:56:05as each scale
  3597. 2:56:09sorry now I the D is I call it capital B
  3598. 2:56:16assuming that then I will take the limit
  3599. 2:56:17delta T going to zero so this is our
  3600. 2:56:20order capital d t so I can rewrite it as
  3601. 2:56:23the order of magnitudes which is square
  3602. 2:56:25root of DT times
  3603. 2:56:27some random variable which is of order
  3604. 2:56:29one and which is gaussian and which
  3605. 2:56:32reproduces the statistics of uh of the
  3606. 2:56:35White Noise which means essentially that
  3607. 2:56:38is it a square has to be equal to Sigma
  3608. 2:56:41Square where Sigma is is the variance of
  3609. 2:56:45the noise at equal time
  3610. 2:56:47so if you want Z is the little bit of
  3611. 2:56:50noise which Acts in the interval t t
  3612. 2:56:53plus DT rescaled by square root of pt
  3613. 2:56:58okay and now this is essentially one
  3614. 2:57:02what you
  3615. 2:57:03mean
  3616. 2:57:04to inject or a useful way to think about
  3617. 2:57:08the problem when you want to derive
  3618. 2:57:10differential equations like the soccer
  3619. 2:57:12Planck equation
  3620. 2:57:14so the soccer plant equation is an
  3621. 2:57:16equation for a quantity
  3622. 2:57:18p
  3623. 2:57:22of x t given
  3624. 2:57:25x 0 to 0. so what is this this is the
  3625. 2:57:28probability in our average overall
  3626. 2:57:30possible trajectories so the role
  3627. 2:57:32possible realization
  3628. 2:57:33of the noise
  3629. 2:57:35to be
  3630. 2:57:37X time T given that
  3631. 2:57:40of time t 0
  3632. 2:57:42I was
  3633. 2:57:44in a given position at zero
  3634. 2:57:47and if you remember the structure of the
  3635. 2:57:50equation for this P was different
  3636. 2:57:52depending on whether when you uh Vito or
  3637. 2:57:56the statino which convention
  3638. 2:57:58so let me give you the form for uh one
  3639. 2:58:02of each
  3640. 2:58:04so we as we introduce
  3641. 2:58:08this B of X is just
  3642. 2:58:11it must put over 2 times 3 of X which is
  3643. 2:58:13the function which multiplies the noise
  3644. 2:58:15in the large of an equation and then
  3645. 2:58:17from strathanovic
  3646. 2:58:21the form of the equation was as follows
  3647. 2:58:23so now I will drop the dependence on the
  3648. 2:58:25argument
  3649. 2:58:26because of the form DP over DT
  3650. 2:58:29equals to minus
  3651. 2:58:32the derivative over X of f
  3652. 2:58:35which is the function appearing in the
  3653. 2:58:38larger one equation times p
  3654. 2:58:40Plus
  3655. 2:58:43the derivative over X of D of x times
  3656. 2:58:47the derivative over X
  3657. 2:58:50of B times
  3658. 2:58:54so there was a first there is this
  3659. 2:58:56metric structure that appears in the
  3660. 2:58:59second derivative whereas if you derive
  3661. 2:59:01the focal plants for Ito if you remember
  3662. 2:59:04you just have a double derivative in
  3663. 2:59:06here of uh
  3664. 2:59:08of the Square Times p
  3665. 2:59:11uh square root
  3666. 2:59:15I think
  3667. 2:59:16No it should be fine
  3668. 2:59:21yes
  3669. 2:59:23okay
  3670. 2:59:35okay
  3671. 2:59:37and now given that we have not much time
  3672. 2:59:40I would just uh perhaps uh tell you
  3673. 2:59:45the starting point or the main ideas of
  3674. 2:59:48the derivation so how do you derive an
  3675. 2:59:51equation for these
  3676. 2:59:52so you can start from one identity which
  3677. 2:59:55is in general true
  3678. 2:59:58for probabilities that is that is just
  3679. 3:00:01what is the probability to be at the
  3680. 3:00:03point x
  3681. 3:00:04time t plus DT given that your FX 0x
  3682. 3:00:11times is zero
  3683. 3:00:13what you can do is to take any time
  3684. 3:00:15between Type P0 and t plus TT and
  3685. 3:00:19write the this is equal to the
  3686. 3:00:21probability
  3687. 3:00:22that you were at a given value of y at
  3688. 3:00:25that time so it's being
  3689. 3:00:28let me write it directly and I recommend
  3690. 3:00:31so the probabilities that you reach X as
  3691. 3:00:34time C plus DT given that you were at Y
  3692. 3:00:36at the previous time p and then you have
  3693. 3:00:39the probability that you were at Y at
  3694. 3:00:42time T given that you were at x 0 x 9 t
  3695. 3:00:450 and you have to integrate overall
  3696. 3:00:48possible conditions or positions that
  3697. 3:00:51you reaches time t
  3698. 3:00:53so this is a very general identity of
  3699. 3:00:55conditional probabilities if you want
  3700. 3:00:59and then once you have this identity
  3701. 3:01:01what you do is you take uh both the
  3702. 3:01:05right and the left hand side you choose
  3703. 3:01:07a function s
  3704. 3:01:09arbitrary
  3705. 3:01:12and smooth
  3706. 3:01:17you multiply both the right and the left
  3707. 3:01:20hand side by this function f and then
  3708. 3:01:21you integrate over X
  3709. 3:01:24so on the left hand side you will the
  3710. 3:01:26left hand side is Trivial you just have
  3711. 3:01:28the integral over DX so
  3712. 3:01:32f of x times
  3713. 3:01:34C of x
  3714. 3:01:37slash DT
  3715. 3:01:39even
  3716. 3:01:42x 0 x 0.
  3717. 3:01:46and on the right hand side you have a
  3718. 3:01:47double integral
  3719. 3:01:51right and what you can do in this double
  3720. 3:01:54integral is
  3721. 3:01:56so let me
  3722. 3:01:58write it in the following ways so
  3723. 3:02:01or just to be short so you have a double
  3724. 3:02:03integral where you have to integrate f
  3725. 3:02:05of x in the X
  3726. 3:02:08and now f of x you assume it to be
  3727. 3:02:11smooth so this means that you can
  3728. 3:02:13approximate
  3729. 3:02:15f of x
  3730. 3:02:16as
  3731. 3:02:18F of Y so assuming that Y is the point
  3732. 3:02:22where you are at the previous time and
  3733. 3:02:24the time difference between the times
  3734. 3:02:27Associated to X and the one Associated
  3735. 3:02:29to Y is small then you can expand this F
  3736. 3:02:32and you can write this as as Prime of Y
  3737. 3:02:36times
  3738. 3:02:37y Plus
  3739. 3:02:39the second derivative evaluated that's
  3740. 3:02:42why over 2 times x minus y square and so
  3741. 3:02:46on
  3742. 3:02:47so now what I do in the left hand side
  3743. 3:02:49is to do the integration over DX f of x
  3744. 3:02:52and then I replace f of x with the X
  3745. 3:02:55function around Y and I will get
  3746. 3:02:59different terms so let me write the
  3747. 3:03:01first one
  3748. 3:03:03so let me exchange the integration of Y
  3749. 3:03:06and X so let me
  3750. 3:03:09take first this first contribution which
  3751. 3:03:12depends on why so we'll have integral
  3752. 3:03:15over d y of f y then I have this second
  3753. 3:03:19probability which depends on your why so
  3754. 3:03:21I will put it here
  3755. 3:03:23and now I will drop the dependence on on
  3756. 3:03:27the previous condition on X Sub 0 and d0
  3757. 3:03:30and then in this case I just have the
  3758. 3:03:32integral over X of this
  3759. 3:03:35so P of x e plus BT given that I was at
  3760. 3:03:40Y at time t
  3761. 3:03:43then I have the term which contains the
  3762. 3:03:47first derivative of the function f
  3763. 3:03:49so I will like integral over the Y of X
  3764. 3:03:53Prime of Y
  3765. 3:03:55B of y t
  3766. 3:03:59and now inside the integral depending on
  3767. 3:04:01x
  3768. 3:04:03I have an extra term because you see
  3769. 3:04:04that I have this x minus y so this
  3770. 3:04:08increment which depends on X so let me
  3771. 3:04:11write it here
  3772. 3:04:13e of x
  3773. 3:04:15e plus BT
  3774. 3:04:17Y2
  3775. 3:04:20okay
  3776. 3:04:21plus I will have a term coming
  3777. 3:04:24containing the second derivative which
  3778. 3:04:26is also important and then I have higher
  3779. 3:04:28order
  3780. 3:04:30so now let me introduce three quantities
  3781. 3:04:32I'm going to leave you so uh the first
  3782. 3:04:34quantity the three quantities correspond
  3783. 3:04:36to the integrals over X which I find at
  3784. 3:04:39each order in the expansion so the order
  3785. 3:04:42zero if you see is just the
  3786. 3:04:44integral of this probability so this
  3787. 3:04:47tells you what is the probability that
  3788. 3:04:48you start at Y at time speed and you end
  3789. 3:04:51up somewhere at times t plus BT well if
  3790. 3:04:54you integrate over the final State this
  3791. 3:04:57probability is simply equal to one
  3792. 3:04:58because you know that you will end up
  3793. 3:05:01somewhere at arbitrary time and if you
  3794. 3:05:04impose no conditions that the
  3795. 3:05:05probability has to be equal to one
  3796. 3:05:08this quantity here inside it is not
  3797. 3:05:10equal to one it depends on Y and I will
  3798. 3:05:14call it i1
  3799. 3:05:16of white
  3800. 3:05:17and you will have an analogous term
  3801. 3:05:19coming from the second order expansion
  3802. 3:05:22so in the end
  3803. 3:05:27the important things that you have to
  3804. 3:05:29compute
  3805. 3:05:31and with this maybe it will stop
  3806. 3:05:35are
  3807. 3:05:37i1 and I2
  3808. 3:05:39foreign
  3809. 3:05:41is what I just defined
  3810. 3:05:44so this is the integral of a small
  3811. 3:05:47increment
  3812. 3:05:50with respect to the uh
  3813. 3:05:53the probability of your process
  3814. 3:05:59you can go smaller
  3815. 3:06:03over y
  3816. 3:06:05EP
  3817. 3:06:07so this is an average increment so you
  3818. 3:06:09assume that you start at Y and you ask
  3819. 3:06:11what is the average
  3820. 3:06:13increments that I do over a small
  3821. 3:06:15intervalitative and what is also
  3822. 3:06:18important that will appear in the second
  3823. 3:06:20order term is
  3824. 3:06:23is he Imaging
  3825. 3:06:25the fluctuations of this
  3826. 3:06:29increments
  3827. 3:06:31that are just obtained taking the power
  3828. 3:06:33to
  3829. 3:06:35okay
  3830. 3:06:37and now this is what uh you have to
  3831. 3:06:40compute and this is where to compute
  3832. 3:06:42this quantities where you have to be
  3833. 3:06:44careful about the discretization so we
  3834. 3:06:48will probably go back to this but let me
  3835. 3:06:50just comment to all of these details in
  3836. 3:06:53the three
  3837. 3:06:55exercise three
  3838. 3:06:58and if you do the calculation properly
  3839. 3:07:00assuming either versus
  3840. 3:07:02what you should find is that this term
  3841. 3:07:07I2 is actually the same for both e to
  3842. 3:07:10instructions
  3843. 3:07:18and it's easy
  3844. 3:07:20to compute
  3845. 3:07:22whereas this average increment is what
  3846. 3:07:24is tricky so this is what will take
  3847. 3:07:26different form
  3848. 3:07:29foreign
  3849. 3:07:39on the type of discretization that you
  3850. 3:07:43choose and so this is what you have to
  3851. 3:07:45be careful about in particular if you do
  3852. 3:07:47the satanovic prescription and this is
  3853. 3:07:50what in the end we'll give you two
  3854. 3:07:53different forms of your pocket blank
  3855. 3:07:56equation depending on how you choose to
  3856. 3:07:58discretize your process
  3857. 3:07:59so I don't think we have time now it
  3858. 3:08:03to uh to go through this but you can
  3859. 3:08:05check it uh in the today and if there
  3860. 3:08:07are questions as I say there will be the
  3861. 3:08:10seven where we are gonna discuss an
  3862. 3:08:13example of this and there we can go back
  3863. 3:08:15to the details uh if there are doubts
  3864. 3:08:19okay
  3865. 3:08:20so I think
  3866. 3:08:22we can stop
  3867. 3:08:24if there are no questions
  3868. 3:08:30then I wish you a happy holiday week
  3869. 3:08:34and we will see each other's theme
  3870. 3:08:38three weeks I think and I will write an
  3871. 3:08:41email with all the information on this
  3872. 3:08:42schedule
  3873. 3:08:44okay
  3874. 3:08:49thank you thank you very much

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