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Lecture 9: The Phillips Curve and Inflation — Transcript

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  1. 0:16So, today I'm going to talk about the
  2. 0:18Phillips curve and inflation. Um
  3. 0:22Now, as I said in the previous lecture,
  4. 0:24uh
  5. 0:25the material that is specific to this
  6. 0:27lecture will not enter this quiz.
  7. 0:30It's the beginning of what is perhaps
  8. 0:31the most important model you'll see in
  9. 0:33the in in this in this uh class, but
  10. 0:37it will take us uh three or four
  11. 0:38lectures to to develop. So, I'm going to
  12. 0:42say things that certainly will
  13. 0:44um
  14. 0:45may help you understand a little better
  15. 0:46the previous lecture, and so
  16. 0:49if you're only concerned about the next
  17. 0:51quiz,
  18. 0:52uh there will be a sort of uh small
  19. 0:55review of the previous lecture here. Uh
  20. 0:57but again, anything that's specific to
  21. 1:00this lecture and was not in the previous
  22. 1:02one
  23. 1:03won't be part of of this quiz.
  24. 1:06So, what is this Phillips curve? Well,
  25. 1:08in in uh
  26. 1:10in 1958, an an economist uh at LSE, the
  27. 1:14London School of Economics,
  28. 1:16came up with some just an empirical
  29. 1:17relationship. This is A.W. Phillips. He
  30. 1:20found that using historical data
  31. 1:24uh for the US, I think he did it. Um
  32. 1:28uh there was a negative relation up to
  33. 1:30sort of the '50s, I think. Uh
  34. 1:33the there was a negative relation
  35. 1:35between uh the unemployment rate and the
  36. 1:37rate of inflation.
  37. 1:39And then our very own Paul Samuelson and
  38. 1:42Robert Solow
  39. 1:44labeled this relationship the Phillips
  40. 1:46curve in honor of uh
  41. 1:48A.W. Phillips.
  42. 1:49And nowadays it's sort of is a central
  43. 1:52concept uh in macroeconomics, and
  44. 1:55uh and uh it's certainly very, very
  45. 1:58relevant to understand what is going on
  46. 2:00uh right now in not only in the US
  47. 2:02economy, but in most economies around
  48. 2:04the world.
  49. 2:06So, let me
  50. 2:07show you sort of this is not the one
  51. 2:08that uh
  52. 2:10that Phillips uh plotted. I think this
  53. 2:12is the one that uh
  54. 2:14uh
  55. 2:15Samuelson and Solow plotted for data
  56. 2:17from between 1900 and 1960 uh
  57. 2:20for the US, you found you find sort of
  58. 2:23this sort of negative correlation. I
  59. 2:25think it's reasonable.
  60. 2:27Uh
  61. 2:28um
  62. 2:29there's negative correlation between
  63. 2:31uh the unemployment rate and inflation
  64. 2:34rate, no? At very low levels of
  65. 2:36unemployment, you typically see very
  66. 2:37high levels of inflation.
  67. 2:39Conversely, sort of at very high levels
  68. 2:41of unemployment, you tend to receive low
  69. 2:44levels of inflation or even deflation.
  70. 2:46In fact, this period includes the the
  71. 2:49Great Depression, for example.
  72. 2:52So,
  73. 2:53that's sort of the data. And and again,
  74. 2:56this was just an empirical regularity.
  75. 2:59But we can build some theory about this
  76. 3:00relationship using the ingredients most
  77. 3:03of the ingredients that
  78. 3:05I mean, essentially we can build a
  79. 3:07relationship that is downward sloping
  80. 3:10from the ingredients we already have.
  81. 3:13And this is the part that is a little
  82. 3:14bit of a review
  83. 3:15of the previous lecture.
  84. 3:17Remember that we had um um
  85. 3:20actually the previous two lectures. We
  86. 3:22had a wage setting equation
  87. 3:25W equal expected prices
  88. 3:28and then a decreasing function of
  89. 3:29unemployment and an increasing function
  90. 3:31of uh these labor market supporting
  91. 3:34institutions or
  92. 3:36worker supporting institutions, that
  93. 3:38institutional variables, I should say.
  94. 3:40And um and then we had a price setting
  95. 3:43equation, which was simply the wage uh
  96. 3:46marked up.
  97. 3:48M is a positive constant. So, let me
  98. 3:50start from these two what So, what I'm
  99. 3:53trying to do is derive a Phillips curve.
  100. 3:55Again, this was only an empirical
  101. 3:57relationship, but it turns out that even
  102. 3:59with theory we knew by the time of, you
  103. 4:01know, Samuelson and and and Solow, we
  104. 4:03could sort of come up with a with a
  105. 4:05theory of that relationship. And that
  106. 4:07theory builds on the ingredients we have
  107. 4:09been looking at. So, these are the price
  108. 4:11set the wage setting equation, the price
  109. 4:12setting equation. I'm going to just
  110. 4:14simplify things and assume that this
  111. 4:16this relationship here, this function f
  112. 4:19of u z, is some linear function, at
  113. 4:22least locally linear function, uh which
  114. 4:24is decreasing in unemployment and
  115. 4:26increasing in z.
  116. 4:28Why is it decreasing in unemployment?
  117. 4:35This says, no, that that if unemployment
  118. 4:37goes up,
  119. 4:39for any given expected price,
  120. 4:41wage demand is lower.
  121. 4:43Okay? And that's essentially because uh
  122. 4:46for the worker is is sort of is a
  123. 4:49becoming unemployed is a scary
  124. 4:50situation.
  125. 4:52Conversely, for firms it's higher it's
  126. 4:54easier to find uh
  127. 4:56uh
  128. 4:56a worker and and uh
  129. 4:59and uh So, as we said, a worker is
  130. 5:01scared for two reasons. One is that it's
  131. 5:04more likely it gets fired when
  132. 5:05unemployment is high, typically that's a
  133. 5:07recession. It's also likely they know
  134. 5:10that that worker knows that if she were
  135. 5:13to fall into the unemployment pool, it
  136. 5:15would take a longer time to get out of
  137. 5:17it. Okay? And the firms are seeing the
  138. 5:19opposite side. It's pretty easy for them
  139. 5:21to replace a worker if they were to
  140. 5:24dismiss a worker because there's lots of
  141. 5:26available workers in unemployment. Okay?
  142. 5:28So, that's the reason that's negative.
  143. 5:30So, I'm going to stick this function
  144. 5:32back in here.
  145. 5:34And then I'm going to replace this W
  146. 5:37with this function in there in the price
  147. 5:39setting equation, and I end up with an
  148. 5:42equation for P. Okay? So, this says that
  149. 5:46the price, given the expected price,
  150. 5:50is decreasing in unemployment and
  151. 5:52increasing in z and increasing in the
  152. 5:54markup.
  153. 5:55So, again, why is this price decreasing
  154. 5:58in unemployment?
  155. 6:02This is the part that is review of the
  156. 6:04previous lecture.
  157. 6:05Previous today. Because
  158. 6:07the wages go down and then the labor uh
  159. 6:09factors of production are cheaper. Okay,
  160. 6:10perfect. Because wages go down, since uh
  161. 6:14our firm needs one worker to produce one
  162. 6:16unit of a good, then the cost of
  163. 6:17production of one unit goes down with
  164. 6:19the wage, and and therefore the price
  165. 6:22goes down. Because the firm is asking
  166. 6:24for a constant markup over that wage,
  167. 6:26the wage declines, and the price drops.
  168. 6:31Good. So, that's all review. So,
  169. 6:35this equation you had seen just without
  170. 6:37an explicit functional form here. What I
  171. 6:39want to do is to go from here. This is
  172. 6:42still not the Phillips curve. Remember,
  173. 6:43the Phillips curve was a relationship
  174. 6:44between inflation
  175. 6:46and unemployment. Here we have a
  176. 6:48relationship between the price level
  177. 6:51and unemployment. Okay? So, we want to
  178. 6:53take one
  179. 6:55one derivative higher. We want to go to
  180. 6:57relation between
  181. 6:58inflation and unemployment. And
  182. 7:00inflation is is the rate of change of P.
  183. 7:03No?
  184. 7:04It's not it's not a level of P.
  185. 7:07So, to do that, all that we'll do is So,
  186. 7:09this when I don't have a subscript here,
  187. 7:11I mean
  188. 7:12the price at time t.
  189. 7:14Okay? And this is the expected price for
  190. 7:16next period, that's what we have.
  191. 7:18Uh
  192. 7:18but today for next period.
  193. 7:21What I'm going to do, I'm going to
  194. 7:22divide both sides by P minus 1. By that,
  195. 7:25I mean the price in the previous period.
  196. 7:27Okay? So, both sides. I'm going to
  197. 7:29divide this side by P minus 1.
  198. 7:32And and and this one by P minus 1.
  199. 7:34So, I get that expression. Okay? That's
  200. 7:36exactly the same equation we had before.
  201. 7:39All that I did is I divided by P minus
  202. 7:411. Remember remember what this means.
  203. 7:44So, if this is the price for the
  204. 7:46beginning for January 2023,
  205. 7:49uh
  206. 7:50this is the price for, say, where we're
  207. 7:51using annual data, for January 2022.
  208. 7:54Okay? So, I'm dividing by the price of
  209. 7:56January 2022 both sides.
  210. 8:00Now, notice that remember that I can
  211. 8:03that P over P minus 1 is equal to 1 plus
  212. 8:06the inflation rate. Remember where
  213. 8:08inflation rate is just
  214. 8:10P minus P minus 1 over P minus 1. So,
  215. 8:14this is just straightforward algebra,
  216. 8:16no?
  217. 8:17Remember our definition of inflation.
  218. 8:33That's P minus that's inflation. Okay?
  219. 8:36So, 1 plus pi is just
  220. 8:39P minus uh
  221. 8:41over P minus 1. Okay? And that's what
  222. 8:43you have there.
  223. 8:44I can do the same for expected
  224. 8:45inflation.
  225. 8:48Notice that
  226. 8:53sometimes people get confused, but
  227. 8:56expected inflation
  228. 8:58is equal to P
  229. 9:00expected
  230. 9:02not minus P expected minus 1. It's P
  231. 9:05minus 1.
  232. 9:07P minus 1.
  233. 9:10And the reason I'm not subtracting the
  234. 9:12expectation here is because at time t,
  235. 9:15which is when you're forming that
  236. 9:16expectation, you already know what
  237. 9:18happened at t minus 1.
  238. 9:21Okay? So, that's the reason this is
  239. 9:22expected inflation. I don't I don't need
  240. 9:25uh uh
  241. 9:26um
  242. 9:28to put expectations in here. Okay? So,
  243. 9:31that's pi e.
  244. 9:33And so, what we get is
  245. 9:35uh I can replace
  246. 9:37this guy here for 1 plus pi, this guy
  247. 9:40here for 1 plus pi e,
  248. 9:42and I get the following relationship.
  249. 9:45Okay?
  250. 9:47All that I've done is substituting this
  251. 9:49for that, that for that.
  252. 9:52So, that's our price setting equation
  253. 9:54now expressed in terms of inflation rate
  254. 9:58unexpected inflation rate
  255. 10:00and now you know
  256. 10:02if not we're not in Argentina we're in
  257. 10:04the US
  258. 10:05inflation if expected inflation is a
  259. 10:07small numbers
  260. 10:09and the log of 1 plus a small number is
  261. 10:11approximately that number
  262. 10:15so
  263. 10:17I'm going to use this approximation
  264. 10:19which again is valid for X small
  265. 10:23and and so I can replace this 1 plus pi
  266. 10:26for pi and this 1 plus pi e for pi e
  267. 10:30this 1 plus m for m
  268. 10:33plus no and this term here if these
  269. 10:36numbers are not too large again plus
  270. 10:39minus alpha u
  271. 10:41plus z
  272. 10:43and that I do all that and I end up with
  273. 10:45this expression
  274. 10:51all that I've done is I took logs of
  275. 10:53this so I get log of 1 plus pi equal to
  276. 10:56log of 1 plus pi e plus log of 1 plus m
  277. 10:59plus log of 1 minus alpha u plus alpha z
  278. 11:02I'm saying if pi pi e m alpha u plus z
  279. 11:07are not very large numbers which we're
  280. 11:09going to assume then this is
  281. 11:11approximately right so I can rewrite
  282. 11:13that expression as that
  283. 11:16approximately I should have put an
  284. 11:17approximately
  285. 11:22okay so now we have something that looks
  286. 11:23a lot more than like the empirical
  287. 11:25relationship we were talking about we
  288. 11:27have a relationship between inflation
  289. 11:29and unemployment so this says that
  290. 11:32for any given expected inflation and
  291. 11:34markups and and labor market
  292. 11:35institutions
  293. 11:37higher unemployment means lower
  294. 11:39inflation
  295. 11:40why is that
  296. 11:43so that curve tells you that's a
  297. 11:44negative relation we wanted no it says
  298. 11:47higher unemployment lower inflation
  299. 11:53why is that
  300. 12:02look you had it very clear when we talk
  301. 12:04about this no
  302. 12:05you you understood very clearly why an
  303. 12:07increase in unemployment lower the wage
  304. 12:10you understood very clearly why
  305. 12:13therefore an increase in unemployment
  306. 12:15lower the price
  307. 12:18I haven't done anything but algebra in
  308. 12:20the two steps so the same economics
  309. 12:22behind the explanations that you had
  310. 12:23before apply to this curve here
  311. 12:26so the reason inflation will be lower
  312. 12:29when you unemployment is higher given
  313. 12:31all the rest
  314. 12:33is because there's really less wage wage
  315. 12:35pressure workers will demand lower wages
  316. 12:38that means lower prices and therefore
  317. 12:39inflation will be lower the economics
  318. 12:41hasn't changed at all I only I only
  319. 12:43divided both sides
  320. 12:45by p minus 1 and I took the logs and I
  321. 12:47approximated so so the economics has not
  322. 12:49changed
  323. 12:50it just did a little bit of
  324. 12:53basic math okay
  325. 12:55so all the what I'm trying to say is all
  326. 12:57the intuitions that you can already you
  327. 12:59already had from the wage setting price
  328. 13:02setting equations and so on you can
  329. 13:03apply to the Phillips curve as well
  330. 13:06okay
  331. 13:08good so now we have something that
  332. 13:11in principle could explain the type of
  333. 13:13relationship that Phillips
  334. 13:16found and then Samuelson Solo
  335. 13:17corroborated with extended data
  336. 13:23so
  337. 13:26let's let's see how do we get to
  338. 13:27something that looks like what
  339. 13:30these people run as a
  340. 13:31they run a regression essentially
  341. 13:34or they correlated and inflation
  342. 13:38inflation with unemployment
  343. 13:40and they found a downward sloping
  344. 13:42relationship
  345. 13:44well
  346. 13:45look what if that happens here suppose
  347. 13:47that
  348. 13:48that we assume that expected inflation
  349. 13:51is equal to some constant
  350. 13:54in in economics we say when that's the
  351. 13:56case
  352. 13:58and especially if pi is a low number
  353. 14:00inflation expectations are well anchored
  354. 14:03meaning you know any single year they
  355. 14:06can be a price of oil is high or
  356. 14:07something happens and inflation will
  357. 14:09deviate from that
  358. 14:10but people are all the time expecting
  359. 14:12for inflation sort of to go back to the
  360. 14:15what is a normal level
  361. 14:17nowadays
  362. 14:18or at least
  363. 14:19a few years ago in the US the normal
  364. 14:22level was around 2% say okay so people
  365. 14:25say well this year inflation was 1.8 but
  366. 14:28we expect next year 2% the next year we
  367. 14:31got surprises on the upside price of
  368. 14:33food went up something like that we got
  369. 14:35inflation of 2.3% but you ask people how
  370. 14:38do you what much do you expect for next
  371. 14:40year they say well 2%
  372. 14:42so so that's what a model of expectation
  373. 14:45like this means is that you know you're
  374. 14:47always expecting something which is
  375. 14:49some historical value on that we have
  376. 14:51agreed is a reasonable level for our
  377. 14:54economy or something like that okay
  378. 14:56so you see that if I replace expected
  379. 14:58inflation for a constant here pi bar
  380. 15:01then I have then my Phillips curve is
  381. 15:04really this is inflation then I have a
  382. 15:06constant minus alpha u
  383. 15:09that's the simplest of the
  384. 15:11downward sloping relationship I can have
  385. 15:12that case is a line downward sloping
  386. 15:14line no that's it
  387. 15:17of course you know it could be
  388. 15:19non-linear and so on but but this
  389. 15:20captures the essence so that's the
  390. 15:22theory for why
  391. 15:24Phillips was finding what he was finding
  392. 15:27our theory of the
  393. 15:29wage of the labor market if you will and
  394. 15:31the price setting
  395. 15:33behavior of firms gives us a Phillips
  396. 15:35curve of the kind that he had in mind
  397. 15:39and if you look in the 60s in the US
  398. 15:43then you see this negative relationship
  399. 15:45that eventually become sort of became a
  400. 15:47steeper it wasn't linear like this it
  401. 15:49was a little convex but but it's
  402. 15:51downward sloping
  403. 15:53and in fact
  404. 15:55to some extent
  405. 15:58our own very our very own Bob Solo and
  406. 16:02Paul Samuelson
  407. 16:04were advising the US government at the
  408. 16:06time and they said well you know let's
  409. 16:08exploit this stuff a little
  410. 16:10we like to have lower unemployment we
  411. 16:13can live with a little less more
  412. 16:14inflation but we know there's a negative
  413. 16:16trade-off there's a negative trade-off
  414. 16:18between these two things okay so
  415. 16:20if we like to lower unemployment it's
  416. 16:22fine we get a little more of inflation
  417. 16:24and initially the deal was very good
  418. 16:26because this curve was very flat
  419. 16:29you see you could cut him unemployment a
  420. 16:31lot you can see the dates here cutting
  421. 16:33unemployment a lot and you're not
  422. 16:35getting a lot of inflation
  423. 16:37eventually the deal the deal turned into
  424. 16:39a much rather deal much more rather deal
  425. 16:41because
  426. 16:42then to lower a little bit more
  427. 16:43unemployment we start getting a lot more
  428. 16:45of inflation okay so people for a while
  429. 16:48you know were okay with this model
  430. 16:50assuming that inflation was low but when
  431. 16:53they realized that this thing was being
  432. 16:54exploited then they began to sort of
  433. 16:57change the expectations they made I
  434. 16:59think that's what we had here but but
  435. 17:01the the reason held pretty well
  436. 17:03during this time and again it became
  437. 17:05steeper and steeper as we
  438. 17:07pushed it more and more towards sort of
  439. 17:09very low levels of unemployment
  440. 17:12so that's the story but again there is
  441. 17:14your model of the Phillips curve and
  442. 17:15that
  443. 17:17it's a very very good model for the
  444. 17:18times where Phillips also estimated his
  445. 17:21his Phillips curve
  446. 17:23now
  447. 17:25if you sort of turn the page and look at
  448. 17:27the same data in the 70s
  449. 17:30look how it looks
  450. 17:32okay
  451. 17:33so from 1970 to 1995 that's the data you
  452. 17:36have there there's no negative
  453. 17:37relationship thing is all over the place
  454. 17:40okay
  455. 17:41so had Mr. Phillips been born a few
  456. 17:43years
  457. 17:44few decades later and had he estimated
  458. 17:47his regression he would have found
  459. 17:49nothing
  460. 17:50there would be no curve in his honor at
  461. 17:52least if he had run that same regression
  462. 17:54maybe he would have run a different
  463. 17:55regression but
  464. 17:56nothing
  465. 17:57okay so what happened
  466. 18:00well our theory can explain as well what
  467. 18:03happened there
  468. 18:04remember the theory is not that
  469. 18:07inflation is equal to a constant minus
  470. 18:09the
  471. 18:11minus
  472. 18:13alpha u
  473. 18:14the theory says
  474. 18:16this is a constant only if
  475. 18:18the model of expectation is this
  476. 18:20constant
  477. 18:21but if expectation is moving around
  478. 18:24or if anything in this constant is
  479. 18:26moving around then then there's another
  480. 18:29source of variation
  481. 18:31okay for example what happens suppose
  482. 18:34that you're here in 1965 and all of the
  483. 18:36sudden you get a the price of oil goes
  484. 18:39up a lot and I'm telling you capture the
  485. 18:41price of oil with an increase in m firms
  486. 18:43need to sort of mark up things more in
  487. 18:44order to cover higher energy energy
  488. 18:46costs
  489. 18:48well look at what m does m says that for
  490. 18:50any given level of unemployment now I
  491. 18:52get higher inflation that's what an oil
  492. 18:54shock does no you get an oil shock then
  493. 18:57for any given level of unemployment now
  494. 18:58you get find yourself with more
  495. 18:59inflation
  496. 19:00so that moves you in the opposite
  497. 19:02direction moves you up there and that's
  498. 19:04one of the reasons
  499. 19:06for these points around here
  500. 19:08we got lots of inflation because we got
  501. 19:10massive oil shocks
  502. 19:12during the 70s and early 80s okay
  503. 19:18we had wars in the Middle East and so on
  504. 19:20that that led to to those shocks so that
  505. 19:23so that was one of the reasons
  506. 19:25we got shocks here
  507. 19:27to this term here
  508. 19:29and that sort of
  509. 19:31muddied the relationship
  510. 19:33but the other reason which is more
  511. 19:35interesting I think and that you already
  512. 19:37began to see that something was
  513. 19:38happening here
  514. 19:40is that
  515. 19:41as inflation went up
  516. 19:44people sort of stopped believing in this
  517. 19:45model so the expectation formation
  518. 19:48mechanism changed
  519. 19:52okay so this guy
  520. 19:54began to react
  521. 19:56to
  522. 19:57endogenous variables. And I'm going to
  523. 19:58explain more precisely what So, that's
  524. 20:01what we mean by expected inflation
  525. 20:03became the anchor. It was no longer
  526. 20:06anchored around this constant of 2%
  527. 20:09but but but it became the anchor. It
  528. 20:11began to follow the data. So, if if the
  529. 20:13data came with more inflation, then
  530. 20:15people believed that next year we would
  531. 20:17have more inflation as well. Okay, not
  532. 20:19back to 2% but if we got 5% inflation
  533. 20:22today, people began to say, "Well, okay,
  534. 20:24I don't think that next year my best
  535. 20:26estimate is 2% is probably closer to
  536. 20:285%." Okay, that's what it means
  537. 20:30de-anchoring. That's what has the Fed
  538. 20:33and most central banks around the world
  539. 20:34terrified today.
  540. 20:36Inflation is very is much higher than 2%
  541. 20:39and they're very worried about this guy
  542. 20:42becoming
  543. 20:43the anchor or an anchor. Okay.
  544. 20:46I'll get back to that in a second.
  545. 20:48Anyway, so but let me let me explain
  546. 20:50this
  547. 20:51how this expected inflation term work
  548. 20:53here.
  549. 20:54So, let me replace the model of
  550. 20:56expected inflation
  551. 20:59for something which is some weighted
  552. 21:00average of a constant.
  553. 21:02That's
  554. 21:03and
  555. 21:05the most recent inflation.
  556. 21:07Okay. So, this model says, "What is my
  557. 21:09expected inflation for next year? Well,
  558. 21:12it's an average of this long-run target
  559. 21:13that we have,
  560. 21:15say 2%,
  561. 21:17and whatever was the most recent
  562. 21:18inflation."
  563. 21:20If theta in the model I showed you
  564. 21:22before, the one that applied to the '60s
  565. 21:24and so on,
  566. 21:25up to the '60s, had essentially theta
  567. 21:28equal to zero.
  568. 21:30So, this guy didn't show up there
  569. 21:32and and expected inflation was very well
  570. 21:35anchored.
  571. 21:36What we began to happen
  572. 21:39as we began to move that way
  573. 21:41and then we got hit by oil shocks so we
  574. 21:43So, people began to see much higher
  575. 21:45inflation numbers than they were used
  576. 21:46to,
  577. 21:48then this theta
  578. 21:50began to
  579. 21:51increase. Okay. So, people began to sort
  580. 21:54of change the model of expectation and
  581. 21:55began to think that
  582. 21:57inflation was going to be more
  583. 21:58persistent than they used to think in
  584. 22:00the past. So, in high inflation today
  585. 22:02means high inflation tomorrow. That's
  586. 22:03what it means more persistent. In the
  587. 22:05past was high inflation today was was a
  588. 22:07back draw, we'll go back to sort of the
  589. 22:10normal long-run average. Now, that's no
  590. 22:12longer the case. And so, if I replace
  591. 22:15this more general model of expected
  592. 22:16inflation
  593. 22:18here in the Phillips curve, I get this
  594. 22:20expression which now has this extra
  595. 22:22term.
  596. 22:23So, the
  597. 22:24we used to have theta equal to zero but
  598. 22:26during the '70s and '80s and even early
  599. 22:29'90s, actually that theta got to be very
  600. 22:31close to one.
  601. 22:33Okay, if you estimate these models, you
  602. 22:35get that theta was very close to one.
  603. 22:37And look at what happens when theta gets
  604. 22:39very close to one.
  605. 22:41So, when theta is is one literally, then
  606. 22:43the best forecast for inflation is the
  607. 22:45previous inflation.
  608. 22:47Okay, so this year is 5% and I think
  609. 22:49next year is 5%, not 2%, 5%.
  610. 22:53If this year is 7%, I think next year is
  611. 22:557% again.
  612. 22:57And so, if you do that, then my expected
  613. 23:00inflation becomes lag inflation pi t
  614. 23:02minus one. So, if I stick in replace the
  615. 23:04expected inflation for pi t minus one, I
  616. 23:07get to this Phillips curve
  617. 23:09which I can rewrite
  618. 23:11as the change in inflation in relation
  619. 23:14as as a relationship between the change
  620. 23:16in inflation and the level of
  621. 23:18unemployment.
  622. 23:20So, now what you have is that if
  623. 23:22unemployment is very low, then inflation
  624. 23:25is is picking up, you know, it's going
  625. 23:28there. So, if inflation if unemployment
  626. 23:30is very low, not only inflation is high,
  627. 23:33but it's also growing
  628. 23:34over time.
  629. 23:36Okay.
  630. 23:37That's the reason sometimes people refer
  631. 23:39to this formulation of the Phillips
  632. 23:41curve as the accelerationist Phillips
  633. 23:44curve because now there's a relation
  634. 23:45between unemployment and the change in
  635. 23:47inflation. And if you estimate
  636. 23:50this Phillips curve, this
  637. 23:51accelerationist Phillips curve on the
  638. 23:54data I just showed you of the '70s and
  639. 23:57'80s, you get a much better
  640. 23:59relationship. Okay, you still have the
  641. 24:00oil shocks that messed things up
  642. 24:03but but you can start seeing recovering
  643. 24:05this negative relationship. But again,
  644. 24:07it's between the change in inflation and
  645. 24:09the level of unemployment. And that's a
  646. 24:10very scary situation for a central bank
  647. 24:12to find itself in because it's very easy
  648. 24:14to for things to escalate.
  649. 24:19Okay.
  650. 24:22So, by the mid-'90s,
  651. 24:25we had re-anchored expectations. There
  652. 24:27was a sort of very aggressive
  653. 24:30policy to control inflation by Paul
  654. 24:32Volcker
  655. 24:33in the US and it was imitated around the
  656. 24:37world with some lag,
  657. 24:39but but inflation became re-anchored.
  658. 24:41So, we went back to this theta equal to
  659. 24:43zero type model. The expected inflation
  660. 24:46in the US, the target inflation of the
  661. 24:48central bank was around 2% that became
  662. 24:51what people expected for the next year
  663. 24:53and and that re-anchored. So, we went
  664. 24:56back in other words
  665. 25:00to that sort of Phillips curve.
  666. 25:03Okay, and that's what central banks want
  667. 25:04to be at. They want to have inflation
  668. 25:06expectation very well anchored.
  669. 25:09And they were very successful after the
  670. 25:10'90s. And so, we got
  671. 25:12into again now Look, I'm I'm now I'm not
  672. 25:15running the accelerations. I'm again
  673. 25:17running inflation against unemployment
  674. 25:19and you again can see this downward
  675. 25:21sloping relationship. Okay.
  676. 25:24So, that was very good news. Was great
  677. 25:26success of monetary policy
  678. 25:28during the '90s and later was the
  679. 25:31re-anchoring of expected inflation again
  680. 25:34all around the developed world and many
  681. 25:36of the include even
  682. 25:37Latin America, many economies in Latin
  683. 25:39America saw re-anchored expectation,
  684. 25:41Asia and so on. So,
  685. 25:43so it was a good time for central banks.
  686. 25:51Okay.
  687. 25:59So, the next
  688. 26:00thing I want to do, this will connect
  689. 26:01more with the with the the previous
  690. 26:03lecture. This is the last thing I want
  691. 26:05to say
  692. 26:07for this lecture then I'm I may start
  693. 26:10the review afterwards.
  694. 26:12Um
  695. 26:13is that I want to connect now this
  696. 26:16Phillips curve with something we
  697. 26:17discussed in the previous lecture which
  698. 26:19is the natural rate of unemployment
  699. 26:20because that's the way
  700. 26:22you'll typically see the Phillips curve
  701. 26:23written and and that's
  702. 26:26also the way
  703. 26:27that sort of uh you know, when Chairman
  704. 26:30Powell is talking about the labor market
  705. 26:32tightness and so on, he's not talking
  706. 26:34relative to M and Z and things like
  707. 26:37that, he's talking relative to what is
  708. 26:38called the natural rate of unemployment.
  709. 26:39So, I want to go from a Phillips curve
  710. 26:42that looks like that,
  711. 26:46you know, like that, to one that has the
  712. 26:48natural rate of unemployment in there.
  713. 26:50And so, that's the last step
  714. 26:53in this lecture.
  715. 26:54So,
  716. 26:55remember the definition of the natural
  717. 26:57rate of unemployment. What was the
  718. 26:59definition of the natural rate of
  719. 27:00unemployment?
  720. 27:04Was it the unemployment rate that God
  721. 27:07gave us?
  722. 27:10Any God?
  723. 27:15No.
  724. 27:17It had a very precise meaning for us.
  725. 27:24And remember, we used exactly that model
  726. 27:27to figure it out.
  727. 27:30Remember?
  728. 27:34We we solved the Actually, we solved the
  729. 27:36natural rate of unemployment from
  730. 27:38something like this. I think we had the
  731. 27:39function still generic function f of U
  732. 27:41Z. But we solved from an expression like
  733. 27:44this.
  734. 27:46We said,
  735. 27:47"Under one assumption,
  736. 27:50we can call this
  737. 27:51U
  738. 27:52U N, the natural rate of unemployment.
  739. 27:55What was that assumption?"
  740. 27:57And that's the only thing
  741. 27:59Expected price Okay, expected price is
  742. 28:01equal to the actual price. Okay, so we
  743. 28:03said if this is equal to that, then you
  744. 28:05solve out that's the natural rate of
  745. 28:07unemployment. And that's the only thing
  746. 28:08that that it that means that that that
  747. 28:12natural rate of unemployment means
  748. 28:14simply that when when the
  749. 28:15when the price is equal to the expected
  750. 28:17price.
  751. 28:20But if the price
  752. 28:23is equal to the expected price,
  753. 28:26what else is equal?
  754. 28:33I pointed at the right expressions
  755. 28:35there.
  756. 28:37Inflation is equal to expected
  757. 28:39inflation.
  758. 28:41So, I can use the same logic I used here
  759. 28:44for the natural rate of unemployment
  760. 28:45using the Phillips curve.
  761. 28:47I can say, "Okay,
  762. 28:49my I can solve out for the natural rate
  763. 28:51of unemployment here simply by setting
  764. 28:53the expected inflation equal to actual
  765. 28:55inflation."
  766. 28:58Okay.
  767. 28:59And if I do this, I can solve for the
  768. 29:01natural rate of unemployment from here.
  769. 29:04U N.
  770. 29:05I mean, I'm going to give I'm going to
  771. 29:06put the superscript N here when I when
  772. 29:08you let me replace pi e for pi. That's a
  773. 29:11That's what I
  774. 29:12That's what I
  775. 29:13The fact that I replace this pi e for pi
  776. 29:16is what allows me to put the superscript
  777. 29:17N there. Call it the natural rate of
  778. 29:19unemployment. And now I can solve it.
  779. 29:21Well, obviously that cancels with that
  780. 29:22and I can solve the natural rate of
  781. 29:23unemployment and it's equal to this
  782. 29:25function here.
  783. 29:28So, why is the natural rate of
  784. 29:30unemployment increasing in M?
  785. 29:33A question like that can come up in the
  786. 29:35quiz.
  787. 29:38I'm not going to use the Phillips curve
  788. 29:39to ask you if I ask you about that, but
  789. 29:41I can ask you that. What
  790. 29:42What happens to the natural rate of
  791. 29:43unemployment if M goes up?
  792. 29:47You know that.
  793. 29:49UN will go up, but what is the
  794. 29:50mechanism?
  795. 29:59So, why does the natural rate of
  796. 30:00unemployment go up when
  797. 30:02the markup goes up?
  798. 30:06Yep. If the real cost is constant, wages
  799. 30:08have to go down, right?
  800. 30:10I mean, another way of saying it is that
  801. 30:12the firms are not willing to pay they
  802. 30:14want to pay a lower real wage.
  803. 30:16At the original level of unemployment
  804. 30:19before the change in M,
  805. 30:22workers would not take that lower real
  806. 30:24wage.
  807. 30:26No, it's not an equilibrium real wage
  808. 30:27because workers say, "No, no, at this
  809. 30:29level of unemployment we need a higher
  810. 30:31real wage."
  811. 30:32So, the only way to restore equilibrium
  812. 30:34in that model we had was to increase
  813. 30:37unemployment because that will lower the
  814. 30:39bargaining power of workers and they
  815. 30:40will end up accepting the lower real
  816. 30:42wage that firms are willing to offer
  817. 30:44now. Okay.
  818. 30:46So, that's the reason
  819. 30:48uh we get this this markup effect.
  820. 30:53Z is
  821. 30:55same logic. It's a little easier to see
  822. 30:57it there, but Z means, well, at any
  823. 31:00given level of unemployment
  824. 31:02an increase in Z means workers want a
  825. 31:04higher real wage.
  826. 31:06Firms are not willing to pay a higher
  827. 31:07real wage,
  828. 31:09so you have to bring down the real wage
  829. 31:11that workers demand and the only way
  830. 31:13that can happen is with a higher
  831. 31:14unemployment.
  832. 31:15Okay. That's the reason the natural rate
  833. 31:17of unemployment is also increasing in Z.
  834. 31:23Okay.
  835. 31:24And now the last step.
  836. 31:26The last step is to
  837. 31:29You see, I can go back to my Phillips
  838. 31:31curve.
  839. 31:34Say that.
  840. 31:36And I'm going to replace M plus Z
  841. 31:40for alpha UN. I can do that, you see?
  842. 31:45I can replace this M plus C Z for alpha
  843. 31:48times UN.
  844. 31:52How do I know that? Well, M plus C Z is
  845. 31:55equal to UN times alpha.
  846. 31:58I can replace in the Phillips curve
  847. 32:01M plus C by alpha UN and I can re
  848. 32:04I can therefore
  849. 32:06rewrite the Phillips curve in the
  850. 32:08following form.
  851. 32:10Inflation is equal to expected inflation
  852. 32:12minus alpha times the gap between the
  853. 32:16unemployment rate and the natural rate
  854. 32:18of unemployment.
  855. 32:20Okay. So,
  856. 32:22so
  857. 32:23when
  858. 32:25Chairman Powell is worried about labor
  859. 32:27market being very tight, what he's
  860. 32:29saying is, well, unemployment is likely
  861. 32:31to be below the natural rate of
  862. 32:33unemployment.
  863. 32:34Because if unemployment is below the
  864. 32:36natural rate of unemployment, that's
  865. 32:37putting upward pressure on inflation.
  866. 32:41Okay.
  867. 32:44So, that's a
  868. 32:45So, that's what it means. This gap is
  869. 32:47very important uh for macroeconomists
  870. 32:50and certainly for central bankers that
  871. 32:52are very worried about inflation. Okay?
  872. 32:54That gap here.
  873. 32:55Problem is is this this is a difficult
  874. 32:58object to estimate, so you have to have
  875. 32:59estimates as
  876. 33:02The truth is that it's very difficult to
  877. 33:04know what it is, although there are
  878. 33:05estimates out there and I'm going to
  879. 33:06show you one.
  880. 33:09You notice that something is wrong when
  881. 33:10this guy starts picking up. It's a It's
  882. 33:12a little bit the other way around, you
  883. 33:14know?
  884. 33:15Uh uh
  885. 33:16the US in fact had a the opposite
  886. 33:18problem
  887. 33:20um
  888. 33:21before COVID. It's a somehow
  889. 33:23unemployment was very low relative to
  890. 33:25historical levels, but inflation was not
  891. 33:27picking up.
  892. 33:28So, that was implicitly telling us that
  893. 33:30for some reason, not fully understood,
  894. 33:33the natural rate of unemployment was
  895. 33:34declining.
  896. 33:36Okay.
  897. 33:38So, here is one picture that looks
  898. 33:40is one estimate uh again, I I don't
  899. 33:43trust any particular estimate, but
  900. 33:45it tells a story. That's one particular
  901. 33:48estimate of the natural rate of
  902. 33:49unemployment in the US, that blue line.
  903. 33:52And what you see in red the red is the
  904. 33:54actual rate of unemployment in the US.
  905. 33:57So,
  906. 33:58what happens when when in situations
  907. 34:00like these?
  908. 34:04So, what do you think what's happening
  909. 34:05to inflation in in this episode, which
  910. 34:08is right after the global financial
  911. 34:09crisis or the great recession?
  912. 34:15So, what what what do you need to read
  913. 34:17here? Well,
  914. 34:18the unemployment rate was a lot higher
  915. 34:19than the
  916. 34:21natural rate of unemployment.
  917. 34:24Does that put upward or downward
  918. 34:25pressure on inflation?
  919. 34:28Downward pressure on inflation. No,
  920. 34:29unemployment is very high relative to
  921. 34:30natural rate of unemployment. It's minus
  922. 34:32alpha times U minus UN.
  923. 34:34So, and that's what happened. We had
  924. 34:36lots of problem with inflation.
  925. 34:37Inflation was going very low. We even
  926. 34:39had negative inflation there, a little
  927. 34:41deflation for a while.
  928. 34:43Okay. So, that was a problem.
  929. 34:46Here is the period that they described
  930. 34:48before is a little mysterious because we
  931. 34:49went unemployment went below what we
  932. 34:51thought it was a natural rate of
  933. 34:52unemployment and inflation wasn't really
  934. 34:54picking up a lot. At the end began to
  935. 34:55pick up a little, but it wasn't picking
  936. 34:57up a lot and that was a little bit of a
  937. 34:59mystery.
  938. 35:00Now, we're in this situation here,
  939. 35:03which
  940. 35:04we have extremely low unemployment
  941. 35:07and very high inflation. So, so this I
  942. 35:10think this captures well the situation
  943. 35:12right now. We have a
  944. 35:13negative gap between unemployment and
  945. 35:15the natural rate of unemployment and
  946. 35:17that's the reason that's putting a lot
  947. 35:18of pressure on inflation.
  948. 35:20We also have other things that are
  949. 35:22putting pressure on inflation that come
  950. 35:23from the supply side of the economy and
  951. 35:25so on.
  952. 35:26So, that combination is pretty bad for
  953. 35:29for the
  954. 35:31inflation outcomes and outlook
  955. 35:35as well.
  956. 35:36Okay.
  957. 35:38So, that's where we're at.
  958. 35:40We're going to talk a lot more about
  959. 35:41this because this is what is going on
  960. 35:43right now.
  961. 35:45Any questions about that? Otherwise, I
  962. 35:47want to start sort of reviewing things,
  963. 35:48although I don't know.
  964. 35:51Any question about this? Yep.
  965. 35:54Is correction to increase unemployment?
  966. 35:57Sorry? Is the only way to fix, I guess,
  967. 35:59the inflationary expectations? Well,
  968. 36:01that's a very good question.
  969. 36:03That's a very good question.
  970. 36:09I'm I'm trying to decide what to
  971. 36:14answer what with what do we have.
  972. 36:17Um
  973. 36:23There are two views
  974. 36:24at this moment.
  975. 36:27There's one view
  976. 36:29that says there's no way around that.
  977. 36:32They just look at these curves and say,
  978. 36:33"Look,
  979. 36:34there's no way around that. That's the
  980. 36:35reason we need a recession."
  981. 36:38Okay.
  982. 36:38Because otherwise we were not going to
  983. 36:40control inflation.
  984. 36:43And a recession means high unemployment.
  985. 36:45Okay, that's one view.
  986. 36:47At this moment, it's becoming the
  987. 36:50dominant view.
  988. 36:51It has gone in cycles, but at this
  989. 36:53moment it's the dominant view.
  990. 36:57There is a another view,
  991. 36:59which is the one that the central bank
  992. 37:01the Fed adopted for a while,
  993. 37:04that said, "Well, this is not the only
  994. 37:06indicator of tightness of the labor
  995. 37:08market. There is other things as well."
  996. 37:11And those indicators are moving in the
  997. 37:13right direction.
  998. 37:14And so, we may be able not to create a
  999. 37:16big mess here because these other
  1000. 37:18factors are moving in the right right
  1001. 37:21direction.
  1002. 37:22Some of those factors are as I said,
  1003. 37:24other measures of of labor market
  1004. 37:26tightness and and hiring, the flows.
  1005. 37:28Remember I showed you flows between
  1006. 37:29employment and unemployment, out of
  1007. 37:31employment and so on. Those flows look
  1008. 37:33extremely tight and now they're
  1009. 37:35improving. So, the gaps in those
  1010. 37:36dimensions are better. And the other one
  1011. 37:38is the what's a big cost push component,
  1012. 37:40which is what I said before, the supply
  1013. 37:42chains and so on created extra
  1014. 37:44inflation, abnormal inflation like
  1015. 37:46increasing markups, like M was very
  1016. 37:48high.
  1017. 37:49And some of that is subsiding as well.
  1018. 37:50So, so there are dynamics that suggest
  1019. 37:53that inflation is declining even without
  1020. 37:54unemployment.
  1021. 37:56But, I would say
  1022. 37:58the medium voter
  1023. 38:00in this space of, you know, forecast of
  1024. 38:02inflation and so on,
  1025. 38:04thinks that that that we will need some
  1026. 38:06some adjustment through this this part
  1027. 38:08as well. Okay.
  1028. 38:11My main concern I I think that
  1029. 38:15the the Fed the the path the Fed is
  1030. 38:17forecasting is feasible,
  1031. 38:19but a very narrow path. I mean, it may
  1032. 38:21happen.
  1033. 38:22And and to me, whether it they're
  1034. 38:24successful at not creating a big mess
  1035. 38:26here, I mean, bringing unemployment very
  1036. 38:29high in order to bring inflation down,
  1037. 38:31has a lot to do with whether
  1038. 38:34somehow we manage to keep expected
  1039. 38:35inflation anchored.
  1040. 38:37And there there was some evidence, I
  1041. 38:39think I said that a few lectures ago,
  1042. 38:41there was some evidence that in the
  1043. 38:42summer of
  1044. 38:45uh summer of 2022, I'm from the southern
  1045. 38:49hemisphere, so I get always confused
  1046. 38:50with summers and and so on.
  1047. 38:52So, the in in the summer of 2022, US
  1048. 38:55summer of 2022, inflation was becoming
  1049. 38:57very unanchored. This guy
  1050. 38:59one year expected inflation was creeping
  1051. 39:01up to 6% and that was very scary. Okay?
  1052. 39:04Because think what happened. If if if
  1053. 39:07you get expected inflation at 6%,
  1054. 39:10then it's not enough to bring
  1055. 39:12unemployment to the natural rate of
  1056. 39:13unemployment to get inflation back to
  1057. 39:15the 2% we like because you need to bring
  1058. 39:17expected inflation down now. And that
  1059. 39:19means you need to sort of bring the
  1060. 39:22unemployment rate very very high in
  1061. 39:24order to re-anchor expectations. So,
  1062. 39:26that's a very scary situation. They were
  1063. 39:28very persuasive though at the end of the
  1064. 39:29summer with very hawkish speeches and so
  1065. 39:32on
  1066. 39:33and they managed to re-anchor expected
  1067. 39:35inflation. So, expected inflation very
  1068. 39:37quickly came down to two two and a half
  1069. 39:38percent one year out to
  1070. 39:41But, now it been picking up again and
  1071. 39:43now we are around 3% again, so it's a
  1072. 39:44little bit scary for where we are. So,
  1073. 39:47to me this is going to be very important
  1074. 39:49in that. So,
  1075. 39:51if inflation keeps lingering around 6%
  1076. 39:53and so on, and eventually the expected
  1077. 39:55inflation becomes an anchor, then
  1078. 39:57there's almost no way around but to have
  1079. 39:59a recession to get out of that.
  1080. 40:02If that doesn't happen, if they succeed
  1081. 40:04convincing a ton of people that that,
  1082. 40:06you know, they're very serious about
  1083. 40:07about this stuff and they they re-anchor
  1084. 40:09expectation expected inflation, then we
  1085. 40:11don't need to create a large recession.
  1086. 40:14Still they may create it, cause it
  1087. 40:15because, you know, accidents happen, but
  1088. 40:17but but but they don't need to.
  1089. 40:20But they will need to if this guy gets
  1090. 40:22an anchor.
  1091. 40:24Actually, maybe I can use even this
  1092. 40:26expression here
  1093. 40:28to explain what I'm trying to say and I
  1094. 40:30realize that this is again, this is
  1095. 40:31material really for
  1096. 40:33for the next lecture.
  1097. 40:35What I'm trying to say is that if they
  1098. 40:36manage
  1099. 40:38to keep this theta very close to zero,
  1100. 40:42okay?
  1101. 40:43Then, in order to bring inflation back
  1102. 40:46to their target of pi bar, 2% or so,
  1103. 40:50all that they really need to do is to
  1104. 40:52sort of bring unemployment to the
  1105. 40:53natural rate of unemployment. So, they
  1106. 40:55only need to really
  1107. 40:57uh
  1108. 40:59fix this gap.
  1109. 41:01Okay? They need to raise unemployment so
  1110. 41:03so it closes that gap. But it's a small
  1111. 41:05change.
  1112. 41:06That's if they succeed keeping expected
  1113. 41:09inflation at around 2%.
  1114. 41:12If they don't,
  1115. 41:16say suppose that that
  1116. 41:18that
  1117. 41:19theta becomes very far from from zero,
  1118. 41:24then we have a problem because then
  1119. 41:25expected inflation is above the target,
  1120. 41:28no? Because we have 6%, so suppose theta
  1121. 41:30is equal to one, we have 6%, then
  1122. 41:32expected inflation
  1123. 41:33is 6%.
  1124. 41:35That means that if you if your expected
  1125. 41:38inflation
  1126. 41:40is
  1127. 41:416%,
  1128. 41:43then in order to bring bring the
  1129. 41:44inflation if you bring unemployment just
  1130. 41:47to the natural rate of unemployment, so
  1131. 41:48the red line to the blue line, you
  1132. 41:50haven't made a lot of progress. All that
  1133. 41:52you have done is
  1134. 41:53you have brought down inflation
  1135. 41:55to 6%, which is expected inflation.
  1136. 41:58So, if you are have expected inflation
  1137. 42:00of 6%, you need to bring unemployment
  1138. 42:03much higher than the natural rate of
  1139. 42:05unemployment in order to bring inflation
  1140. 42:07back to the target of 2%.
  1141. 42:10That's the reason I say
  1142. 42:11to me
  1143. 42:13the fight will be
  1144. 42:15the battle will be won or lost
  1145. 42:18on that term there.
  1146. 42:21Yep.
  1147. 42:23How much
  1148. 42:24of this current like inflationary
  1149. 42:26pressure is caused by unemployment? How
  1150. 42:28much of it is caused on the supply side?
  1151. 42:30Cuz it feels like a lot of this stuff
  1152. 42:31like CPI going up, energy prices going
  1153. 42:33up, it's like how much can the Fed keep
  1154. 42:35control of something like Well, it
  1155. 42:36varies a little from different
  1156. 42:40This is around the world, but but in the
  1157. 42:41US,
  1158. 42:42uh for a while a big component of
  1159. 42:44inflation was all that stuff.
  1160. 42:47Uh you know, bottlenecks in the ports
  1161. 42:49and and stuff like that.
  1162. 42:51That's almost all gone.
  1163. 42:52There's very little of that left. So,
  1164. 42:54now is
  1165. 42:56is aggregate demand. People feel very
  1166. 42:57rich
  1167. 42:59for a variety of reasons, they're
  1168. 43:00spending a lot and that's the reason
  1169. 43:01unemployment is very low.
  1170. 43:04It's not unemployment per se, it's just
  1171. 43:05the aggregate demand is very high.
  1172. 43:07You know?
  1173. 43:09Uh and that translates into very low
  1174. 43:10unemployment and that feeds into
  1175. 43:12inflation this way
  1176. 43:13through wages and so on.
  1177. 43:15But
  1178. 43:17in the US, the component of aggregate
  1179. 43:18demand is much larger than in Europe. In
  1180. 43:20Europe, those supply side factors are
  1181. 43:22much more important. So,
  1182. 43:25you know, around the
  1183. 43:29Yeah, the summer of 2022, you could say
  1184. 43:33both both Europe and the US had about
  1185. 43:36the same amount of excess inflation.
  1186. 43:37They were all with about 10% inflation.
  1187. 43:41But in the US was 2/3 excess aggregate
  1188. 43:44demand,
  1189. 43:45while in Europe was 2/3 problems on the
  1190. 43:48supply side, especially because of the
  1191. 43:49war and stuff like that.
  1192. 43:51Okay?
  1193. 43:51So,
  1194. 43:52so but it for the US today is mostly an
  1195. 43:54aggregate demand problem. We're not
  1196. 43:56going to get a lot of
  1197. 43:57Obviously, if the war stops, that's
  1198. 43:59going to help,
  1199. 44:01but it's not going to be enough. We we
  1200. 44:02we need to
  1201. 44:04just the economy is too hot. It's too
  1202. 44:05much aggregate demand out there.
  1203. 44:07That's the that's the fundamental
  1204. 44:09problem. Yeah.
  1205. 44:11Can you explain again why an increase in
  1206. 44:13Z would increase the natural rate of
  1207. 44:16unemployment? An increase in Z? Yeah.
  1208. 44:19So,
  1209. 44:20uh
  1210. 44:21um
  1211. 44:23for that the basis the previous slide
  1212. 44:25diagram, but remember what Z does.
  1213. 44:27Actually, let me go to
  1214. 44:30this equation here.
  1215. 44:34So, we can figure out in this in this
  1216. 44:36two equations here. If Z goes up, that
  1217. 44:39means for any given level of
  1218. 44:40unemployment
  1219. 44:42and expected inflation,
  1220. 44:45wages go up. Workers demand higher wage.
  1221. 44:50But
  1222. 44:51remember that that the firms
  1223. 44:55uh
  1224. 44:56So, so let me let me let me we're
  1225. 44:58talking about the natural rate of
  1226. 44:58unemployment, so let me replace this PE
  1227. 45:00for P first of all.
  1228. 45:02Okay?
  1229. 45:03So, I'm going to divide
  1230. 45:05W by P both sides. So, I get
  1231. 45:09if if Z goes up, the workers want a
  1232. 45:12higher real wage.
  1233. 45:14No? If because
  1234. 45:17if Z goes up, then W over P, I'm
  1235. 45:20dividing by P both sides, goes up.
  1236. 45:23Workers demand a higher wage.
  1237. 45:25But the firms, from here you can see
  1238. 45:27that I can divide by P both sides, W
  1239. 45:29over P that the firms offer is equal to
  1240. 45:321 over 1 + M.
  1241. 45:35Okay? So, the the firms are not going to
  1242. 45:37offer a higher real wage. The workers
  1243. 45:40want a higher real wage.
  1244. 45:42The only thing that can restore
  1245. 45:43equilibrium that the workers end up
  1246. 45:45demanding the same real wage as the
  1247. 45:47firms are willing to pay
  1248. 45:49is that somehow the hands of the worker
  1249. 45:51gets weakened. And the only variable
  1250. 45:53here that can weaken their hand is a
  1251. 45:56higher unemployment.
  1252. 45:58Okay?
  1253. 45:59So,
  1254. 46:00let me put it all in
  1255. 46:05So, at the natural rate,
  1256. 46:07I know that PE is equal to P.
  1257. 46:10So, that means the wage setting equation
  1258. 46:13the wage setting equation implies
  1259. 46:16W over P
  1260. 46:19equal F U Z.
  1261. 46:22Okay?
  1262. 46:24From the price setting equation,
  1263. 46:28I have that
  1264. 46:29W over P
  1265. 46:32is equal to 1 over 1 + M.
  1266. 46:35So, in this very simple model, this is
  1267. 46:37given.
  1268. 46:38If this guy goes up,
  1269. 46:40these guys want a higher real wage, but
  1270. 46:42that cannot happen because that would be
  1271. 46:43inconsistent with the price setting, so
  1272. 46:45you need to bring down this guy down.
  1273. 46:48The only thing that can bring it down is
  1274. 46:49for unemployment to go up.
  1275. 46:52And that's at P, we call that the
  1276. 46:54natural rate of unemployment.
  1277. 46:56Okay.
  1278. 46:59Yeah.
  1279. 47:01So, like last lecture we talked about
  1280. 47:03the labor force participation rate. Um
  1281. 47:07is there like any reason to try and like
  1282. 47:10increase that to increase Oh,
  1283. 47:12fantastic. Yes.
  1284. 47:16Well, I mean
  1285. 47:19there are sort of negative policies as
  1286. 47:21well.
  1287. 47:22You know, Z reduction in a sense does
  1288. 47:24that because
  1289. 47:25the the was a emergency unemployment
  1290. 47:28benefits and emergency
  1291. 47:30income supplements and so on as a result
  1292. 47:32of the pandemic that are disappearing
  1293. 47:34slowly. And that's very naturally so
  1294. 47:36it's it's going to bring
  1295. 47:39uh participation back up and it is
  1296. 47:41beginning to pick up. So,
  1297. 47:43so yeah, you need to incentivize return
  1298. 47:46to work. And now there are some people
  1299. 47:48that
  1300. 47:48there's nothing that
  1301. 47:50they've retired essentially or, you
  1302. 47:52know, they have health problems and they
  1303. 47:54they just cannot return. We lost that.
  1304. 47:57And the other margin which is very
  1305. 47:58important is immigration. So, that's a
  1306. 48:00big issue
  1307. 48:01because immigration obviously that we
  1308. 48:03lost I think in the US, I'm not a labor
  1309. 48:05economist, but we lost
  1310. 48:07I think a flow of the order of the order
  1311. 48:09of 500,000 people a year
  1312. 48:11during COVID.
  1313. 48:13And and and that's that's a big chunk of
  1314. 48:15the decline in
  1315. 48:17in the labor No, what you need is more
  1316. 48:19employment. That's going to that puts
  1317. 48:21downward pressure on wages for the same
  1318. 48:23amount of aggregate demand.
  1319. 48:25And that's what you need, but but
  1320. 48:28Yeah, we're taking that's a very good
  1321. 48:29point. We're taking all that as given
  1322. 48:31here. Remember, we're fixing all that,
  1323. 48:33but but if you don't, then then you
  1324. 48:36other terms will start appearing in this
  1325. 48:38expression and so on.
  1326. 48:40Good.
  1327. 48:42Obviously, I'm not going to start the
  1328. 48:43review. We have only 1 minute, but so in
  1329. 48:45the next lecture I I'll just review
  1330. 48:48uh the material for the quiz.

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