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The Structure of Time and Space | Stephen Wolfram — Transcript

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  1. 0:00The notion of time is the progression of
  2. 0:03computation. So something we say this
  3. 0:06event happens and this other event can
  4. 0:09only happen after that first event later
  5. 0:12in time than that first event because
  6. 0:14that second event is using the output
  7. 0:16from the first event. It's consuming the
  8. 0:19kind of atoms of space that were created
  9. 0:21in that first event.
  10. 0:25[Music]
  11. 0:30Welcome to Closer to Truth. I'm speaking
  12. 0:33with Steven Wolfrram, the distinguished
  13. 0:35physicist, computer scientist, and
  14. 0:37software entrepreneur. We're discussing
  15. 0:39in depth the Wolfrram physics project.
  16. 0:42Steven's grand indeed radical vision of
  17. 0:44a new kind of science in which
  18. 0:46computation via simple rules is the
  19. 0:49foundation of physical reality. The Wolf
  20. 0:51from Physics Project is a closer to
  21. 0:53truth multi-part series. This is part
  22. 0:55three on a path to a fundamental theory
  23. 1:00of physics. Stephen, let's start by
  24. 1:02giving a quick overview of the physic
  25. 1:05the wolf from physics project itself and
  26. 1:08then we'll get into how you get to this
  27. 1:11path to a fundamental theory of physics.
  28. 1:14>> So the the question is what's the
  29. 1:17universe made of?
  30. 1:18>> And our physics project basically says
  31. 1:21the answer is it's computation all the
  32. 1:23way down.
  33. 1:25And so let's see what that means.
  34. 1:28Essentially the one sort of historical
  35. 1:31path we can take is back in antiquity
  36. 1:34people were sort of wondering what's the
  37. 1:36universe made of? Is it made of atomic
  38. 1:38discrete things? Is it made of kind of
  39. 1:40continuous flowing things or what? By
  40. 1:44the end of the 19th century partly that
  41. 1:46was answered. Matter is discrete. It's
  42. 1:48made of discrete molecules. Little bit
  43. 1:50later, you can think of light as being
  44. 1:52made of discrete photons. At the
  45. 1:54beginning of the 20th century, a lot of
  46. 1:56physicists assumed that space would be
  47. 1:58discreet as well, but they couldn't
  48. 2:00figure out how to make that work. In
  49. 2:02fact, they published very little about
  50. 2:03it. It's only very recently that I
  51. 2:05learned that all the greats basically at
  52. 2:07that time thought that space was
  53. 2:09discreet. And even like Einstein made
  54. 2:11comments like in the end, it will turn
  55. 2:12out that space is discreet, but we don't
  56. 2:14have the the appropriate tools to see
  57. 2:16how that works yet. Well, 100 years
  58. 2:19later, I think we do. And uh the sort of
  59. 2:22beginning of a project is to think about
  60. 2:26what's what's the universe made of and
  61. 2:29what is space made of. We don't usually
  62. 2:31think of space as being made of
  63. 2:33something. We just usually think of
  64. 2:34space as being this background where we
  65. 2:37can put things here or there or or
  66. 2:39anywhere. Um but like a fluid like water
  67. 2:43we now know is made of molecules. So we
  68. 2:46think of space as being made of discrete
  69. 2:49atoms of space, not atoms in the in the
  70. 2:52sense of of material atoms, but these
  71. 2:55indivisible points that uh we can think
  72. 2:58of as sort of the raw material of space.
  73. 3:01And kind of the the starting point for
  74. 3:03thinking about what the universe is made
  75. 3:05of is to think it's it's this giant
  76. 3:08collection of atoms of space where the
  77. 3:10only thing we know about atoms of space
  78. 3:12is how they're related to each other.
  79. 3:14sort of what the friends of one atom of
  80. 3:16space are. And so we can represent that
  81. 3:19at a sort of mathematical level as a
  82. 3:21graph or actually more in the way that
  83. 3:24we set it up as a hyperraph. Uh a
  84. 3:26hyperraph is just something where you're
  85. 3:28saying we have these these points these
  86. 3:31nodes and have these hyper edges in
  87. 3:34which we associate we relate some number
  88. 3:37of nodes together. So an ordinary graph
  89. 3:39we'd always be relating pairs of nodes.
  90. 3:41In a hyperraph we can relate any number
  91. 3:43of nodes with a hyper edge so to speak.
  92. 3:46So
  93. 3:47>> and so this is a key point using
  94. 3:49hyperraph which is uh a a a
  95. 3:53representation of a computation to
  96. 3:55represent space. This is the is this
  97. 3:58kind of the first step in the path to
  98. 4:00the fundamental theory of physics.
  99. 4:01>> It's not representing a computation. The
  100. 4:03hypograph is just it's kind of like if
  101. 4:06you're a computer person it's it's a
  102. 4:08data structure. It's the data structure
  103. 4:10of the universe so to speak. Um so it is
  104. 4:13it is just that is the structure of
  105. 4:15space and everything in it. So another
  106. 4:17feature of of of our model is that
  107. 4:22there's there's nothing in the universe
  108. 4:23other than space. Everything that we
  109. 4:25know the electrons the photons us and so
  110. 4:28on. It's all just features of space. So
  111. 4:31it's like we if we were dealing with a
  112. 4:33fluid like water we would say well
  113. 4:35there's this eddy that goes through the
  114. 4:37water. That eddy is ultimately made of
  115. 4:40molecules just like any other feature of
  116. 4:42the fluid. But the eddi has some some
  117. 4:44independent identity to it. And that's
  118. 4:46kind of the way we imagine something
  119. 4:48like an electron works in in in space
  120. 4:51where the space is built up from this
  121. 4:53hypograph. What at the bottom everything
  122. 4:56is just represented as this hypograph.
  123. 4:58And that's that that everything about
  124. 5:01the universe is represented in the
  125. 5:04structure of that hypograph. When you
  126. 5:06say represented, do you mean represented
  127. 5:08in a modeling sense or in some ways as
  128. 5:11as of the reality itself?
  129. 5:15>> Well, you know, usually we're used in
  130. 5:17science to saying we make models of
  131. 5:19things, which means we're making an
  132. 5:21approximation to how something works,
  133. 5:22right?
  134. 5:23>> Where we say we capture some features
  135. 5:25and ignore other features. This is the
  136. 5:27unique case where we're trying to nail
  137. 5:29it. This is you know this is the
  138. 5:32ultimate model because this is this
  139. 5:34there is no approximation we're talking
  140. 5:36about this the idea is that this is what
  141. 5:40a representation of the way the universe
  142. 5:43works now I say representation because
  143. 5:46it's it is what is what is the nature of
  144. 5:49a model a model is or is is something
  145. 5:53which is trying to translate between
  146. 5:55what the universe is actually doing and
  147. 5:58what we can understand with our minds.
  148. 6:01So when I say it's represented as a
  149. 6:04hypograph, that's the way that we can
  150. 6:06conceptualize what's going on. If we say
  151. 6:09in some sense what is actually there,
  152. 6:13it's that that's that's that's sort of
  153. 6:16that's a different kind of thing. That's
  154. 6:18not it. It's like saying we have uh
  155. 6:21Newtonian you know the the equations of
  156. 6:24mechanics uh from you know the calculus
  157. 6:27equations that that Newton produced and
  158. 6:29we say you know the earth is moving
  159. 6:31according to this law of gravity and so
  160. 6:34on. We don't imagine that the earth has
  161. 6:38a computer inside it that is you know
  162. 6:40solving those equations. We imagine that
  163. 6:42those equations are representing what
  164. 6:44the earth does. And and this is the same
  165. 6:46kind of thing with the with the
  166. 6:48difference that instead of saying this
  167. 6:50is an approximation to what's going on,
  168. 6:52we're saying this is the whole story of
  169. 6:55what's going on. And so you know the the
  170. 6:59the the first step is to think about
  171. 7:02sort of the structure of space and
  172. 7:03everything in space. The next question
  173. 7:06is so what happens with this? How does
  174. 7:08time work? This is the static structure
  175. 7:11of space. How does this progress through
  176. 7:13time? And the idea is that this network,
  177. 7:18this hyperraph at every moment pieces of
  178. 7:21that hyperraph are being rewritten into
  179. 7:23other pieces of hypograph. So the basic
  180. 7:26thing is that there are rules that say
  181. 7:27if you see a piece of hypograph that
  182. 7:29looks like this, it will be rewritten as
  183. 7:31a piece of hypograph that looks like
  184. 7:33that. And that's happening all the time.
  185. 7:35That is the progress of time is the the
  186. 7:39progressive rewriting of this hypograph.
  187. 7:42And that's that's kind of the story of
  188. 7:44of what the universe is and what it does
  189. 7:48is the hypograph and the rewriting of
  190. 7:50this hypograph.
  191. 7:51>> Okay. So that's this is a very uh
  192. 7:54powerful idea. It it's actually quite
  193. 7:57easy to understand the way you just
  194. 7:58described it. um as the the the space is
  195. 8:03the hypograph and the rewriting of the
  196. 8:06hypograph into new structures is the
  197. 8:08progressive of time and what we see as
  198. 8:10uh as events whether they're molec micro
  199. 8:14or or macro. just to get a sense of
  200. 8:16orders of magnitude if if this is at all
  201. 8:19uh possible of uh how you would describe
  202. 8:23I mean we know the size of the
  203. 8:25observable universe at least I don't
  204. 8:27know 10^ the 26 m or whatever uh we know
  205. 8:31plank a plankton plank lengths um and
  206. 8:36plank times 10us 43rd or 10us 27th
  207. 8:39various elements that we think are the
  208. 8:42simple so putting this together. What
  209. 8:45kind of orders of magnitude can you
  210. 8:46describe in terms of uh the actual
  211. 8:50hyperraph of the universe if to
  212. 8:53represent it using
  213. 8:55>> in your sense and uh the number of rules
  214. 9:00order of magnitude that you would need
  215. 9:02in order to make all the transformations
  216. 9:04necessary.
  217. 9:06So okay in terms of you know what is the
  218. 9:09elementary length if we were to convert
  219. 9:12kind of the the kind of one edge of a
  220. 9:16hyperraph into meters how many meters
  221. 9:18would it be right
  222. 9:19>> we don't know there's there's in our
  223. 9:22model there's one parameter you can it's
  224. 9:24the elementary length the elementary
  225. 9:26time the elementary energy it's also
  226. 9:28related to a thing we call the maximum
  227. 9:29entanglement speed which we'll get on to
  228. 9:31when we talk about quantum mechanics but
  229. 9:33the we don't know the value of
  230. 9:35I have a a very vague estimate that it
  231. 9:38might be around 10us 100 m. That the
  232. 9:41elementary length might be around 10 -
  233. 9:43100 m. It's much smaller than the plank
  234. 9:45scale.
  235. 9:46>> Much smaller than the plank line.
  236. 9:47>> Right. And it kind of resolves a a a bit
  237. 9:50of a mystery which is the plank energy
  238. 9:52is actually quite macroscopic in the
  239. 9:54usual setup. Our elementary energy is
  240. 9:56also microscopic which is kind of the
  241. 9:59way you would expect it to be. So, you
  242. 10:02know, there's a question of will we be
  243. 10:04lucky enough that there's an experiment
  244. 10:06that we can do or that even has been
  245. 10:08done that will detect the elementary
  246. 10:11length.
  247. 10:11>> Yeah, that that sounds very improbable.
  248. 10:14>> Well, let me explain why it's not quite
  249. 10:16so improbable. Okay. So, I think people
  250. 10:19were really lucky in at at the beginning
  251. 10:22of the 20th century that molecules were
  252. 10:24as big as they are relative to the kinds
  253. 10:27of equipment that existed to make
  254. 10:29measurements at the time. Yeah.
  255. 10:30>> But even despite that actually they
  256. 10:33could have known molecules existed
  257. 10:34earlier because Brownian motion which
  258. 10:36was the thing that kind of clinched the
  259. 10:37whole story that was discovered in 1827.
  260. 10:41So all the time that people like
  261. 10:42Boltzman were worrying about do
  262. 10:44molecules exist or not actually there
  263. 10:46was already evidence that they existed.
  264. 10:48It's just it wasn't interpreted right. I
  265. 10:50will be I I think it is very likely that
  266. 10:53there was already data in astrophysics
  267. 10:56in various areas of of of quantum
  268. 10:58mechanics that already is a clue that
  269. 11:02there's discreetness to space but it
  270. 11:05hasn't been interpreted yet. And that's
  271. 11:06a that's an interesting project to try
  272. 11:08and sort of mine the literature before
  273. 11:11you spend tens of billions of dollars
  274. 11:13building experiments to to look for the
  275. 11:15next thing. But what happens is that
  276. 11:18there are some effects that are
  277. 11:21predicted by a kind of model that are
  278. 11:24very different from what's been seen
  279. 11:25before. So here's an example of one. So
  280. 11:28when you have this big hypograph uh it
  281. 11:32it does not define what the
  282. 11:33dimensionality of space is. We normally
  283. 11:36think space is this thing that we can
  284. 11:38describe with three coordinates and it's
  285. 11:40three dimensions and so on. But this
  286. 11:43hyperraph it doesn't have any fixed set
  287. 11:45of coordinates. It's what emerges when
  288. 11:49you have a big enough hypograph is
  289. 11:51something which can approximate space.
  290. 11:52But at the beginning it's not defined
  291. 11:55whether that space is is two-dimensional
  292. 11:57or threedimensional or 3.1dimensional
  293. 12:00or infinite dimensional or whatever
  294. 12:01else. And so it's one of the things that
  295. 12:05we expect are dimension fluctuations
  296. 12:08where the dimensionality of space is not
  297. 12:10exactly three. That's a bizarre
  298. 12:12phenomenon. It's mathematical analysis
  299. 12:14is difficult. I mean people study, you
  300. 12:16know, they study calculus of one
  301. 12:18variable. They study calculus of two or
  302. 12:19three variables. They don't study
  303. 12:21calculus of 2.7 variables because nobody
  304. 12:24knows how that works. And we have to
  305. 12:26build kind of we're kind of trying to
  306. 12:27rebuild the sort of the whole tower of
  307. 12:30geometry and calculus and so on when for
  308. 12:34for what you build on top of on top of
  309. 12:35these hypographs rather than on top of
  310. 12:38kind of Uklid's version of space.
  311. 12:40>> Okay, let's go then get back to what you
  312. 12:42said. Give you your 10 to the minus
  313. 12:44100th is the is the ultimate
  314. 12:48point structure of space. Nice round
  315. 12:50number we can we can easily remember. uh
  316. 12:53what are the implications of that given
  317. 12:55the size of the known universe in terms
  318. 12:58of a hypographic representation?
  319. 13:01>> Well, I mean it it's
  320. 13:04the first question is when you have this
  321. 13:05hypograph and it's sort of doing its
  322. 13:07thing at this discrete level, what what
  323. 13:11does it do on the scale of of human
  324. 13:14experience, so to speak, or on the scale
  325. 13:15of of astronomy? It's a similar question
  326. 13:18to asking if you have a fluid that's
  327. 13:20made of a bunch of molecules, you've got
  328. 13:22all these molecules bouncing around.
  329. 13:24What is the large scale aggregate
  330. 13:26behavior of the fluid? What we know in
  331. 13:28that case is that the large scale
  332. 13:29aggregate behavior follows the equations
  333. 13:31of fluid mechanics. And so one question
  334. 13:34is well what is the large scale
  335. 13:36aggregate behavior that we see from this
  336. 13:38hyperraph doing all its rewriting at
  337. 13:40this very small scale? The answer is
  338. 13:43Einstein's equations for the structure
  339. 13:44of spaceime. So what is in the case of
  340. 13:47fluid mechanics from molecular dynamics
  341. 13:49we can derive the Navia Stokes equations
  342. 13:51of fluid flow from this hyperraph
  343. 13:53rewriting we can derive and when I say
  344. 13:56derive mathematicians will say there are
  345. 13:58many many footnotes there's a century
  346. 14:00worth of footnotes that still has to be
  347. 14:02filled in to see how that derivation
  348. 14:03works by the way the same is even true
  349. 14:06for fluid mechanics the derivation of
  350. 14:08fluid mechanics from molecular dynamics
  351. 14:10has never been done in a mathematically
  352. 14:11rigorous way but we can you know one of
  353. 14:14the great advantages that I've had
  354. 14:16methodologically in the things that I've
  355. 14:18done is that there is both the
  356. 14:20mathematics side of analyzing things but
  357. 14:22also there's computer experiments and
  358. 14:24you can see a lot of what's true from
  359. 14:26computer experiments even though you
  360. 14:28can't necessarily say here's how I can
  361. 14:31give the full sort of mathematical
  362. 14:32narrative for how this works but so the
  363. 14:35first thing to say is that the the kind
  364. 14:37of largecale behavior of spaceime is
  365. 14:42that you get from this underlying
  366. 14:44hypography writing
  367. 14:45follows the Einstein equations but it
  368. 14:47has some deviations like these dimension
  369. 14:50fluctuations and so on.
  370. 14:51>> The other thing that happens is that a
  371. 14:53lot of features of physics that one has
  372. 14:56just had to say oh well you follow the
  373. 14:59equations you solve the equations then
  374. 15:01you work out how things will work. A lot
  375. 15:03of features of physics now become things
  376. 15:05that you can kind of almost mechanically
  377. 15:07explain. Let me give an example. So in
  378. 15:10relativity one of the sort of classic
  379. 15:12phenomena is time dilation. when things
  380. 15:15move more quickly, time seems to run
  381. 15:17slower for them. Well, in our physics
  382. 15:21project, we can really see quite
  383. 15:22mechanically why that happens. So, if
  384. 15:24you have a thing like an electron, let's
  385. 15:26say, and it's represented by some
  386. 15:28structure in the hypograph and it is
  387. 15:31progressively uh kind of uh it is it is
  388. 15:34it continues to exist because as the
  389. 15:37hypograph gets rewritten that electron
  390. 15:40structure is preserved by the successive
  391. 15:42rewritings. it's it's recreated at every
  392. 15:45moment in time um by by this hypograph
  393. 15:48rewriting process. Now we say let's have
  394. 15:51the electron move from here to there.
  395. 15:53What happens is some of its sort of
  396. 15:55computation budget if it's moving has to
  397. 15:58be used in kind of recreating the
  398. 16:00electron at different places in space.
  399. 16:02So if it's using some of its computation
  400. 16:04budget to recreate itself at different
  401. 16:06places in space, it has less computation
  402. 16:09budget to just sort of be continuing
  403. 16:12through time. So in effect of in effect
  404. 16:15it is it's used up its computation
  405. 16:17budget on motion. So its time has to run
  406. 16:20slower for it. It has less computation
  407. 16:22budget to sort of run itself forward in
  408. 16:25time.
  409. 16:25>> And that that assumes there's a there's
  410. 16:27a finite computation budget.
  411. 16:30>> Yes. But that but the the whole point is
  412. 16:32that the the whole notion of time is
  413. 16:35that time is associated with the
  414. 16:37progressive doing of computation. our
  415. 16:41what what happens in the universe in a
  416. 16:44sense we experience time because
  417. 16:47computations are going on in us and we
  418. 16:50are but if if you were to just look from
  419. 16:52outside the universe you could say well
  420. 16:56you know I'm just not going to do the
  421. 16:57next step of computation then the
  422. 16:59universe is frozen but so are we we we
  423. 17:01our perception of the passage of time
  424. 17:04>> is a is a consequence of of the fact
  425. 17:06that these computations are going on in
  426. 17:08us as in the rest of the universe
  427. 17:10The fact that there is a sort of
  428. 17:11uniformity to that computation both
  429. 17:14inside us and in the universe at large
  430. 17:17is why there is a sort of invariant
  431. 17:18notion of time. It could be the case
  432. 17:21that time is was was very different for
  433. 17:24different kinds of entities. But the
  434. 17:26fact is that in a sense it's it's it
  435. 17:29comes back to the principle of
  436. 17:30computational equivalence actually that
  437. 17:32there is a a sort of uniform notion of
  438. 17:34time that applies both to our experience
  439. 17:37of time and to what happens in time in
  440. 17:39in in the universe at large. Let's take
  441. 17:41a a simpler example from classical
  442. 17:45physics energy and momentum um which are
  443. 17:49have been thought to be understandable
  444. 17:52in Newtonian physics um how would those
  445. 17:55represent to get to to see how the the
  446. 17:58hyperraph system works for physics in in
  447. 18:01a simple way
  448. 18:02>> right so well I didn't think energy was
  449. 18:05going to be simple actually I thought we
  450. 18:06were going to have to understand
  451. 18:07particles in order to understand energy
  452. 18:09I was wrong turns out that we can think
  453. 18:12about energy as a bulk phenomenon and
  454. 18:15roughly energy is the density of
  455. 18:17activity in the hypograph. So roughly
  456. 18:20the um and momentum so so put a little
  457. 18:23bit more precisely the way that one
  458. 18:26thinks about things is every rewriting
  459. 18:29event is this is this is an it's an
  460. 18:32event and you think about all these
  461. 18:34different rewriting events and they all
  462. 18:37they have a certain network of causal
  463. 18:40relationships. So one rewriting event uh
  464. 18:43has to have happened before another one
  465. 18:45can happen because the next one is going
  466. 18:48to use the output from the first one and
  467. 18:50that builds one up this kind of causal
  468. 18:53graph of causal connections between
  469. 18:55these rewriting events.
  470. 18:57>> And so put a little bit more formally
  471. 18:59energy is essentially the flux of causal
  472. 19:02edges through what we can call
  473. 19:04space-like hypersurfaces. So in in um
  474. 19:07it's kind of like the the way that um
  475. 19:11This is this is one of the tricky things
  476. 19:13which which was not known when people
  477. 19:16were thinking about sort of discrete
  478. 19:18space in the early part of the 20th
  479. 19:20century. What was not known uh people
  480. 19:23were imagining that space would have to
  481. 19:25be some sort of discrete lattice or
  482. 19:27something. What emerges in the physics
  483. 19:29project is that the key thing to look at
  484. 19:32is this causal graph of the causal
  485. 19:35relationships between different events.
  486. 19:37And it's it's invariances of that causal
  487. 19:40graph that lead to relativity.
  488. 19:42>> Um that lead to the fact that you uh
  489. 19:45well the notion of time is the
  490. 19:48progression of computation. So something
  491. 19:52we say this event happens and this other
  492. 19:54event can only happen after that first
  493. 19:57event later in time than that first
  494. 19:59event because that second event is using
  495. 20:02the output from the first event. It's
  496. 20:04consuming the kind of atoms of space
  497. 20:06that were created in that first event.
  498. 20:09Now what can happen is there are all
  499. 20:10these events taking place and you can
  500. 20:13say well which events can we think of as
  501. 20:16simultaneous and this is very similar to
  502. 20:17the kind of way one thinks about
  503. 20:19relativity. One says what what events
  504. 20:21can one think of as a space-like surface
  505. 20:24as events that can be thought of as just
  506. 20:26laid out in space all at the same time.
  507. 20:29And there are many different possible
  508. 20:31choices of space-like surfaces, many
  509. 20:33different choices of simultaneity
  510. 20:35surfaces. That's the same kind of thing
  511. 20:37that happens in relativity, but it
  512. 20:38happens very directly in our models. And
  513. 20:40it's it's um uh and it's it's that um
  514. 20:44and and the sort of the the key thing
  515. 20:45that one's looking at is this is this
  516. 20:47causal graph. Energy turns out to be the
  517. 20:49flux of causal edges through space-like
  518. 20:51hypersurfaces. Momentum is a flux
  519. 20:54through timelike hypersurfaces. Those
  520. 20:56are sort of the formal statements. I
  521. 20:58would say that one of the things that
  522. 20:59was a mystery for a long time is why in
  523. 21:01relativity theory the transformation
  524. 21:04rules for space and time have the same
  525. 21:06mathematical form as the transformation
  526. 21:08rules for energy and momentum
  527. 21:10>> in our model that's it's obvious why
  528. 21:12that's the case from what I just said
  529. 21:15it's not so obvious
  530. 21:16>> that's an interesting point because that
  531. 21:17that is the case I mean in your model
  532. 21:19they're both related to the same kind of
  533. 21:21structure so it's it's it's it's not
  534. 21:25it's almost trivial because they're both
  535. 21:27caused by the same transformations of
  536. 21:30hypograph as as opposed to two radically
  537. 21:32different kinds of things.
  538. 21:35>> Let me go back to an ear earlier
  539. 21:36question. So we we we we got an order of
  540. 21:39magnitude of the nature of the hypograph
  541. 21:42by 10 the minus 100th and we know the
  542. 21:44size of the universe
  543. 21:46at least observable universe. Let's go
  544. 21:48to the the the order of magnitude of the
  545. 21:51number or kinds of transformations or
  546. 21:54rule the rules that cause these
  547. 21:57transformations in the hyperraph which
  548. 22:00generates the the physics that we know.
  549. 22:02How many different kinds of rules do you
  550. 22:05need?
  551. 22:06>> Okay, we're we're now about to descend
  552. 22:09into the deeper parts of the rabbit hole
  553. 22:11because the that's ultimately the story
  554. 22:14of the rouad.
  555. 22:16>> All right. Well, we're going to do the
  556. 22:17rouad in another completely.
  557. 22:19>> I think I think we should not let me
  558. 22:21just say that for our there are many
  559. 22:25different rules that we can use to
  560. 22:30describe how a universe works and they
  561. 22:32are all ultimately equivalent in terms
  562. 22:36of the things that we observe about the
  563. 22:38universe. And let me give a a a way to
  564. 22:41sort of see why that might work that
  565. 22:44way. It relates again to fluid
  566. 22:46mechanics. If we look at the equations
  567. 22:48of fluid mechanics, it's the same
  568. 22:50equations for water and for air. Even
  569. 22:53though the molecules that make up water
  570. 22:54and air are quite different, right?
  571. 22:56>> And it's it's um but it is a bit more
  572. 22:59complicated in the in the full case of
  573. 23:00the universe because we are observers
  574. 23:03embedded within the thing that is the
  575. 23:06universe. And so if we're the that when
  576. 23:09we say we are thinking about the
  577. 23:11universe in this way in terms of these
  578. 23:13rules but we are also made into made of
  579. 23:16those rules and it turns out that it we
  580. 23:19can we can attribute sort of the
  581. 23:21behavior of the universe to different
  582. 23:23rules and end up coming to the same
  583. 23:25conclusions about the aspects of the
  584. 23:27universe that are observable. So the the
  585. 23:30you know the the I think the the way to
  586. 23:32answer that is to say there actually can
  587. 23:34be just one rule that uh or you know a
  588. 23:38very small number of rules that we can
  589. 23:41we can run those rules and get what is
  590. 23:45at our observable to us as what happens
  591. 23:48in the universe. So let me give an
  592. 23:50example of that. I mean so so we have
  593. 23:52simulations now of things like black
  594. 23:54hole mergers in our models and the you
  595. 23:58can use a whole range of different
  596. 24:00possible rules and you'll always get the
  597. 24:03same kind of behavior at the scale you
  598. 24:06know if you look at the absolutely
  599. 24:07microscopic scale you'll see different
  600. 24:09things going on but if you look at a at
  601. 24:12a sort of zoomed out scale you'll see
  602. 24:14these black holes merging and some
  603. 24:15gravitational waves produced and so on
  604. 24:18and uh it's uh So that's it's it's a
  605. 24:22slightly it's a slightly weird thing
  606. 24:23because it's a little different from the
  607. 24:25way that one's thought about physical
  608. 24:26theories before and that that will tell
  609. 24:28us that will take us into into the story
  610. 24:30of the rouad.
  611. 24:32>> Okay. Well rullad's coming coming soon.
  612. 24:34Uh so this is this is great. Uh viewers
  613. 24:37can watch all the videos in closer to
  614. 24:38truth the wolf from physics project on
  615. 24:40the closer truth website and YouTube
  616. 24:43channel and including the rouad which is
  617. 24:45coming which is going to be I think my
  618. 24:47favorite. Thanks for joining us.
  619. 24:51Thank you for watching. If you like this
  620. 24:53video, please like and comment below.
  621. 24:56You can support Closer to Truth by
  622. 24:58subscribing.
  623. 25:00Closer to Truth is now accepting your
  624. 25:02taxexempt donations. Please come to
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  627. 25:12and thanks for watching.

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