The Structure of Time and Space | Stephen Wolfram — Transcript
Full transcript
- 0:00The notion of time is the progression of
- 0:03computation. So something we say this
- 0:06event happens and this other event can
- 0:09only happen after that first event later
- 0:12in time than that first event because
- 0:14that second event is using the output
- 0:16from the first event. It's consuming the
- 0:19kind of atoms of space that were created
- 0:21in that first event.
- 0:25[Music]
- 0:30Welcome to Closer to Truth. I'm speaking
- 0:33with Steven Wolfrram, the distinguished
- 0:35physicist, computer scientist, and
- 0:37software entrepreneur. We're discussing
- 0:39in depth the Wolfrram physics project.
- 0:42Steven's grand indeed radical vision of
- 0:44a new kind of science in which
- 0:46computation via simple rules is the
- 0:49foundation of physical reality. The Wolf
- 0:51from Physics Project is a closer to
- 0:53truth multi-part series. This is part
- 0:55three on a path to a fundamental theory
- 1:00of physics. Stephen, let's start by
- 1:02giving a quick overview of the physic
- 1:05the wolf from physics project itself and
- 1:08then we'll get into how you get to this
- 1:11path to a fundamental theory of physics.
- 1:14>> So the the question is what's the
- 1:17universe made of?
- 1:18>> And our physics project basically says
- 1:21the answer is it's computation all the
- 1:23way down.
- 1:25And so let's see what that means.
- 1:28Essentially the one sort of historical
- 1:31path we can take is back in antiquity
- 1:34people were sort of wondering what's the
- 1:36universe made of? Is it made of atomic
- 1:38discrete things? Is it made of kind of
- 1:40continuous flowing things or what? By
- 1:44the end of the 19th century partly that
- 1:46was answered. Matter is discrete. It's
- 1:48made of discrete molecules. Little bit
- 1:50later, you can think of light as being
- 1:52made of discrete photons. At the
- 1:54beginning of the 20th century, a lot of
- 1:56physicists assumed that space would be
- 1:58discreet as well, but they couldn't
- 2:00figure out how to make that work. In
- 2:02fact, they published very little about
- 2:03it. It's only very recently that I
- 2:05learned that all the greats basically at
- 2:07that time thought that space was
- 2:09discreet. And even like Einstein made
- 2:11comments like in the end, it will turn
- 2:12out that space is discreet, but we don't
- 2:14have the the appropriate tools to see
- 2:16how that works yet. Well, 100 years
- 2:19later, I think we do. And uh the sort of
- 2:22beginning of a project is to think about
- 2:26what's what's the universe made of and
- 2:29what is space made of. We don't usually
- 2:31think of space as being made of
- 2:33something. We just usually think of
- 2:34space as being this background where we
- 2:37can put things here or there or or
- 2:39anywhere. Um but like a fluid like water
- 2:43we now know is made of molecules. So we
- 2:46think of space as being made of discrete
- 2:49atoms of space, not atoms in the in the
- 2:52sense of of material atoms, but these
- 2:55indivisible points that uh we can think
- 2:58of as sort of the raw material of space.
- 3:01And kind of the the starting point for
- 3:03thinking about what the universe is made
- 3:05of is to think it's it's this giant
- 3:08collection of atoms of space where the
- 3:10only thing we know about atoms of space
- 3:12is how they're related to each other.
- 3:14sort of what the friends of one atom of
- 3:16space are. And so we can represent that
- 3:19at a sort of mathematical level as a
- 3:21graph or actually more in the way that
- 3:24we set it up as a hyperraph. Uh a
- 3:26hyperraph is just something where you're
- 3:28saying we have these these points these
- 3:31nodes and have these hyper edges in
- 3:34which we associate we relate some number
- 3:37of nodes together. So an ordinary graph
- 3:39we'd always be relating pairs of nodes.
- 3:41In a hyperraph we can relate any number
- 3:43of nodes with a hyper edge so to speak.
- 3:46So
- 3:47>> and so this is a key point using
- 3:49hyperraph which is uh a a a
- 3:53representation of a computation to
- 3:55represent space. This is the is this
- 3:58kind of the first step in the path to
- 4:00the fundamental theory of physics.
- 4:01>> It's not representing a computation. The
- 4:03hypograph is just it's kind of like if
- 4:06you're a computer person it's it's a
- 4:08data structure. It's the data structure
- 4:10of the universe so to speak. Um so it is
- 4:13it is just that is the structure of
- 4:15space and everything in it. So another
- 4:17feature of of of our model is that
- 4:22there's there's nothing in the universe
- 4:23other than space. Everything that we
- 4:25know the electrons the photons us and so
- 4:28on. It's all just features of space. So
- 4:31it's like we if we were dealing with a
- 4:33fluid like water we would say well
- 4:35there's this eddy that goes through the
- 4:37water. That eddy is ultimately made of
- 4:40molecules just like any other feature of
- 4:42the fluid. But the eddi has some some
- 4:44independent identity to it. And that's
- 4:46kind of the way we imagine something
- 4:48like an electron works in in in space
- 4:51where the space is built up from this
- 4:53hypograph. What at the bottom everything
- 4:56is just represented as this hypograph.
- 4:58And that's that that everything about
- 5:01the universe is represented in the
- 5:04structure of that hypograph. When you
- 5:06say represented, do you mean represented
- 5:08in a modeling sense or in some ways as
- 5:11as of the reality itself?
- 5:15>> Well, you know, usually we're used in
- 5:17science to saying we make models of
- 5:19things, which means we're making an
- 5:21approximation to how something works,
- 5:22right?
- 5:23>> Where we say we capture some features
- 5:25and ignore other features. This is the
- 5:27unique case where we're trying to nail
- 5:29it. This is you know this is the
- 5:32ultimate model because this is this
- 5:34there is no approximation we're talking
- 5:36about this the idea is that this is what
- 5:40a representation of the way the universe
- 5:43works now I say representation because
- 5:46it's it is what is what is the nature of
- 5:49a model a model is or is is something
- 5:53which is trying to translate between
- 5:55what the universe is actually doing and
- 5:58what we can understand with our minds.
- 6:01So when I say it's represented as a
- 6:04hypograph, that's the way that we can
- 6:06conceptualize what's going on. If we say
- 6:09in some sense what is actually there,
- 6:13it's that that's that's that's sort of
- 6:16that's a different kind of thing. That's
- 6:18not it. It's like saying we have uh
- 6:21Newtonian you know the the equations of
- 6:24mechanics uh from you know the calculus
- 6:27equations that that Newton produced and
- 6:29we say you know the earth is moving
- 6:31according to this law of gravity and so
- 6:34on. We don't imagine that the earth has
- 6:38a computer inside it that is you know
- 6:40solving those equations. We imagine that
- 6:42those equations are representing what
- 6:44the earth does. And and this is the same
- 6:46kind of thing with the with the
- 6:48difference that instead of saying this
- 6:50is an approximation to what's going on,
- 6:52we're saying this is the whole story of
- 6:55what's going on. And so you know the the
- 6:59the the first step is to think about
- 7:02sort of the structure of space and
- 7:03everything in space. The next question
- 7:06is so what happens with this? How does
- 7:08time work? This is the static structure
- 7:11of space. How does this progress through
- 7:13time? And the idea is that this network,
- 7:18this hyperraph at every moment pieces of
- 7:21that hyperraph are being rewritten into
- 7:23other pieces of hypograph. So the basic
- 7:26thing is that there are rules that say
- 7:27if you see a piece of hypograph that
- 7:29looks like this, it will be rewritten as
- 7:31a piece of hypograph that looks like
- 7:33that. And that's happening all the time.
- 7:35That is the progress of time is the the
- 7:39progressive rewriting of this hypograph.
- 7:42And that's that's kind of the story of
- 7:44of what the universe is and what it does
- 7:48is the hypograph and the rewriting of
- 7:50this hypograph.
- 7:51>> Okay. So that's this is a very uh
- 7:54powerful idea. It it's actually quite
- 7:57easy to understand the way you just
- 7:58described it. um as the the the space is
- 8:03the hypograph and the rewriting of the
- 8:06hypograph into new structures is the
- 8:08progressive of time and what we see as
- 8:10uh as events whether they're molec micro
- 8:14or or macro. just to get a sense of
- 8:16orders of magnitude if if this is at all
- 8:19uh possible of uh how you would describe
- 8:23I mean we know the size of the
- 8:25observable universe at least I don't
- 8:27know 10^ the 26 m or whatever uh we know
- 8:31plank a plankton plank lengths um and
- 8:36plank times 10us 43rd or 10us 27th
- 8:39various elements that we think are the
- 8:42simple so putting this together. What
- 8:45kind of orders of magnitude can you
- 8:46describe in terms of uh the actual
- 8:50hyperraph of the universe if to
- 8:53represent it using
- 8:55>> in your sense and uh the number of rules
- 9:00order of magnitude that you would need
- 9:02in order to make all the transformations
- 9:04necessary.
- 9:06So okay in terms of you know what is the
- 9:09elementary length if we were to convert
- 9:12kind of the the kind of one edge of a
- 9:16hyperraph into meters how many meters
- 9:18would it be right
- 9:19>> we don't know there's there's in our
- 9:22model there's one parameter you can it's
- 9:24the elementary length the elementary
- 9:26time the elementary energy it's also
- 9:28related to a thing we call the maximum
- 9:29entanglement speed which we'll get on to
- 9:31when we talk about quantum mechanics but
- 9:33the we don't know the value of
- 9:35I have a a very vague estimate that it
- 9:38might be around 10us 100 m. That the
- 9:41elementary length might be around 10 -
- 9:43100 m. It's much smaller than the plank
- 9:45scale.
- 9:46>> Much smaller than the plank line.
- 9:47>> Right. And it kind of resolves a a a bit
- 9:50of a mystery which is the plank energy
- 9:52is actually quite macroscopic in the
- 9:54usual setup. Our elementary energy is
- 9:56also microscopic which is kind of the
- 9:59way you would expect it to be. So, you
- 10:02know, there's a question of will we be
- 10:04lucky enough that there's an experiment
- 10:06that we can do or that even has been
- 10:08done that will detect the elementary
- 10:11length.
- 10:11>> Yeah, that that sounds very improbable.
- 10:14>> Well, let me explain why it's not quite
- 10:16so improbable. Okay. So, I think people
- 10:19were really lucky in at at the beginning
- 10:22of the 20th century that molecules were
- 10:24as big as they are relative to the kinds
- 10:27of equipment that existed to make
- 10:29measurements at the time. Yeah.
- 10:30>> But even despite that actually they
- 10:33could have known molecules existed
- 10:34earlier because Brownian motion which
- 10:36was the thing that kind of clinched the
- 10:37whole story that was discovered in 1827.
- 10:41So all the time that people like
- 10:42Boltzman were worrying about do
- 10:44molecules exist or not actually there
- 10:46was already evidence that they existed.
- 10:48It's just it wasn't interpreted right. I
- 10:50will be I I think it is very likely that
- 10:53there was already data in astrophysics
- 10:56in various areas of of of quantum
- 10:58mechanics that already is a clue that
- 11:02there's discreetness to space but it
- 11:05hasn't been interpreted yet. And that's
- 11:06a that's an interesting project to try
- 11:08and sort of mine the literature before
- 11:11you spend tens of billions of dollars
- 11:13building experiments to to look for the
- 11:15next thing. But what happens is that
- 11:18there are some effects that are
- 11:21predicted by a kind of model that are
- 11:24very different from what's been seen
- 11:25before. So here's an example of one. So
- 11:28when you have this big hypograph uh it
- 11:32it does not define what the
- 11:33dimensionality of space is. We normally
- 11:36think space is this thing that we can
- 11:38describe with three coordinates and it's
- 11:40three dimensions and so on. But this
- 11:43hyperraph it doesn't have any fixed set
- 11:45of coordinates. It's what emerges when
- 11:49you have a big enough hypograph is
- 11:51something which can approximate space.
- 11:52But at the beginning it's not defined
- 11:55whether that space is is two-dimensional
- 11:57or threedimensional or 3.1dimensional
- 12:00or infinite dimensional or whatever
- 12:01else. And so it's one of the things that
- 12:05we expect are dimension fluctuations
- 12:08where the dimensionality of space is not
- 12:10exactly three. That's a bizarre
- 12:12phenomenon. It's mathematical analysis
- 12:14is difficult. I mean people study, you
- 12:16know, they study calculus of one
- 12:18variable. They study calculus of two or
- 12:19three variables. They don't study
- 12:21calculus of 2.7 variables because nobody
- 12:24knows how that works. And we have to
- 12:26build kind of we're kind of trying to
- 12:27rebuild the sort of the whole tower of
- 12:30geometry and calculus and so on when for
- 12:34for what you build on top of on top of
- 12:35these hypographs rather than on top of
- 12:38kind of Uklid's version of space.
- 12:40>> Okay, let's go then get back to what you
- 12:42said. Give you your 10 to the minus
- 12:44100th is the is the ultimate
- 12:48point structure of space. Nice round
- 12:50number we can we can easily remember. uh
- 12:53what are the implications of that given
- 12:55the size of the known universe in terms
- 12:58of a hypographic representation?
- 13:01>> Well, I mean it it's
- 13:04the first question is when you have this
- 13:05hypograph and it's sort of doing its
- 13:07thing at this discrete level, what what
- 13:11does it do on the scale of of human
- 13:14experience, so to speak, or on the scale
- 13:15of of astronomy? It's a similar question
- 13:18to asking if you have a fluid that's
- 13:20made of a bunch of molecules, you've got
- 13:22all these molecules bouncing around.
- 13:24What is the large scale aggregate
- 13:26behavior of the fluid? What we know in
- 13:28that case is that the large scale
- 13:29aggregate behavior follows the equations
- 13:31of fluid mechanics. And so one question
- 13:34is well what is the large scale
- 13:36aggregate behavior that we see from this
- 13:38hyperraph doing all its rewriting at
- 13:40this very small scale? The answer is
- 13:43Einstein's equations for the structure
- 13:44of spaceime. So what is in the case of
- 13:47fluid mechanics from molecular dynamics
- 13:49we can derive the Navia Stokes equations
- 13:51of fluid flow from this hyperraph
- 13:53rewriting we can derive and when I say
- 13:56derive mathematicians will say there are
- 13:58many many footnotes there's a century
- 14:00worth of footnotes that still has to be
- 14:02filled in to see how that derivation
- 14:03works by the way the same is even true
- 14:06for fluid mechanics the derivation of
- 14:08fluid mechanics from molecular dynamics
- 14:10has never been done in a mathematically
- 14:11rigorous way but we can you know one of
- 14:14the great advantages that I've had
- 14:16methodologically in the things that I've
- 14:18done is that there is both the
- 14:20mathematics side of analyzing things but
- 14:22also there's computer experiments and
- 14:24you can see a lot of what's true from
- 14:26computer experiments even though you
- 14:28can't necessarily say here's how I can
- 14:31give the full sort of mathematical
- 14:32narrative for how this works but so the
- 14:35first thing to say is that the the kind
- 14:37of largecale behavior of spaceime is
- 14:42that you get from this underlying
- 14:44hypography writing
- 14:45follows the Einstein equations but it
- 14:47has some deviations like these dimension
- 14:50fluctuations and so on.
- 14:51>> The other thing that happens is that a
- 14:53lot of features of physics that one has
- 14:56just had to say oh well you follow the
- 14:59equations you solve the equations then
- 15:01you work out how things will work. A lot
- 15:03of features of physics now become things
- 15:05that you can kind of almost mechanically
- 15:07explain. Let me give an example. So in
- 15:10relativity one of the sort of classic
- 15:12phenomena is time dilation. when things
- 15:15move more quickly, time seems to run
- 15:17slower for them. Well, in our physics
- 15:21project, we can really see quite
- 15:22mechanically why that happens. So, if
- 15:24you have a thing like an electron, let's
- 15:26say, and it's represented by some
- 15:28structure in the hypograph and it is
- 15:31progressively uh kind of uh it is it is
- 15:34it continues to exist because as the
- 15:37hypograph gets rewritten that electron
- 15:40structure is preserved by the successive
- 15:42rewritings. it's it's recreated at every
- 15:45moment in time um by by this hypograph
- 15:48rewriting process. Now we say let's have
- 15:51the electron move from here to there.
- 15:53What happens is some of its sort of
- 15:55computation budget if it's moving has to
- 15:58be used in kind of recreating the
- 16:00electron at different places in space.
- 16:02So if it's using some of its computation
- 16:04budget to recreate itself at different
- 16:06places in space, it has less computation
- 16:09budget to just sort of be continuing
- 16:12through time. So in effect of in effect
- 16:15it is it's used up its computation
- 16:17budget on motion. So its time has to run
- 16:20slower for it. It has less computation
- 16:22budget to sort of run itself forward in
- 16:25time.
- 16:25>> And that that assumes there's a there's
- 16:27a finite computation budget.
- 16:30>> Yes. But that but the the whole point is
- 16:32that the the whole notion of time is
- 16:35that time is associated with the
- 16:37progressive doing of computation. our
- 16:41what what happens in the universe in a
- 16:44sense we experience time because
- 16:47computations are going on in us and we
- 16:50are but if if you were to just look from
- 16:52outside the universe you could say well
- 16:56you know I'm just not going to do the
- 16:57next step of computation then the
- 16:59universe is frozen but so are we we we
- 17:01our perception of the passage of time
- 17:04>> is a is a consequence of of the fact
- 17:06that these computations are going on in
- 17:08us as in the rest of the universe
- 17:10The fact that there is a sort of
- 17:11uniformity to that computation both
- 17:14inside us and in the universe at large
- 17:17is why there is a sort of invariant
- 17:18notion of time. It could be the case
- 17:21that time is was was very different for
- 17:24different kinds of entities. But the
- 17:26fact is that in a sense it's it's it
- 17:29comes back to the principle of
- 17:30computational equivalence actually that
- 17:32there is a a sort of uniform notion of
- 17:34time that applies both to our experience
- 17:37of time and to what happens in time in
- 17:39in in the universe at large. Let's take
- 17:41a a simpler example from classical
- 17:45physics energy and momentum um which are
- 17:49have been thought to be understandable
- 17:52in Newtonian physics um how would those
- 17:55represent to get to to see how the the
- 17:58hyperraph system works for physics in in
- 18:01a simple way
- 18:02>> right so well I didn't think energy was
- 18:05going to be simple actually I thought we
- 18:06were going to have to understand
- 18:07particles in order to understand energy
- 18:09I was wrong turns out that we can think
- 18:12about energy as a bulk phenomenon and
- 18:15roughly energy is the density of
- 18:17activity in the hypograph. So roughly
- 18:20the um and momentum so so put a little
- 18:23bit more precisely the way that one
- 18:26thinks about things is every rewriting
- 18:29event is this is this is an it's an
- 18:32event and you think about all these
- 18:34different rewriting events and they all
- 18:37they have a certain network of causal
- 18:40relationships. So one rewriting event uh
- 18:43has to have happened before another one
- 18:45can happen because the next one is going
- 18:48to use the output from the first one and
- 18:50that builds one up this kind of causal
- 18:53graph of causal connections between
- 18:55these rewriting events.
- 18:57>> And so put a little bit more formally
- 18:59energy is essentially the flux of causal
- 19:02edges through what we can call
- 19:04space-like hypersurfaces. So in in um
- 19:07it's kind of like the the way that um
- 19:11This is this is one of the tricky things
- 19:13which which was not known when people
- 19:16were thinking about sort of discrete
- 19:18space in the early part of the 20th
- 19:20century. What was not known uh people
- 19:23were imagining that space would have to
- 19:25be some sort of discrete lattice or
- 19:27something. What emerges in the physics
- 19:29project is that the key thing to look at
- 19:32is this causal graph of the causal
- 19:35relationships between different events.
- 19:37And it's it's invariances of that causal
- 19:40graph that lead to relativity.
- 19:42>> Um that lead to the fact that you uh
- 19:45well the notion of time is the
- 19:48progression of computation. So something
- 19:52we say this event happens and this other
- 19:54event can only happen after that first
- 19:57event later in time than that first
- 19:59event because that second event is using
- 20:02the output from the first event. It's
- 20:04consuming the kind of atoms of space
- 20:06that were created in that first event.
- 20:09Now what can happen is there are all
- 20:10these events taking place and you can
- 20:13say well which events can we think of as
- 20:16simultaneous and this is very similar to
- 20:17the kind of way one thinks about
- 20:19relativity. One says what what events
- 20:21can one think of as a space-like surface
- 20:24as events that can be thought of as just
- 20:26laid out in space all at the same time.
- 20:29And there are many different possible
- 20:31choices of space-like surfaces, many
- 20:33different choices of simultaneity
- 20:35surfaces. That's the same kind of thing
- 20:37that happens in relativity, but it
- 20:38happens very directly in our models. And
- 20:40it's it's um uh and it's it's that um
- 20:44and and the sort of the the key thing
- 20:45that one's looking at is this is this
- 20:47causal graph. Energy turns out to be the
- 20:49flux of causal edges through space-like
- 20:51hypersurfaces. Momentum is a flux
- 20:54through timelike hypersurfaces. Those
- 20:56are sort of the formal statements. I
- 20:58would say that one of the things that
- 20:59was a mystery for a long time is why in
- 21:01relativity theory the transformation
- 21:04rules for space and time have the same
- 21:06mathematical form as the transformation
- 21:08rules for energy and momentum
- 21:10>> in our model that's it's obvious why
- 21:12that's the case from what I just said
- 21:15it's not so obvious
- 21:16>> that's an interesting point because that
- 21:17that is the case I mean in your model
- 21:19they're both related to the same kind of
- 21:21structure so it's it's it's it's not
- 21:25it's almost trivial because they're both
- 21:27caused by the same transformations of
- 21:30hypograph as as opposed to two radically
- 21:32different kinds of things.
- 21:35>> Let me go back to an ear earlier
- 21:36question. So we we we we got an order of
- 21:39magnitude of the nature of the hypograph
- 21:42by 10 the minus 100th and we know the
- 21:44size of the universe
- 21:46at least observable universe. Let's go
- 21:48to the the the order of magnitude of the
- 21:51number or kinds of transformations or
- 21:54rule the rules that cause these
- 21:57transformations in the hyperraph which
- 22:00generates the the physics that we know.
- 22:02How many different kinds of rules do you
- 22:05need?
- 22:06>> Okay, we're we're now about to descend
- 22:09into the deeper parts of the rabbit hole
- 22:11because the that's ultimately the story
- 22:14of the rouad.
- 22:16>> All right. Well, we're going to do the
- 22:17rouad in another completely.
- 22:19>> I think I think we should not let me
- 22:21just say that for our there are many
- 22:25different rules that we can use to
- 22:30describe how a universe works and they
- 22:32are all ultimately equivalent in terms
- 22:36of the things that we observe about the
- 22:38universe. And let me give a a a way to
- 22:41sort of see why that might work that
- 22:44way. It relates again to fluid
- 22:46mechanics. If we look at the equations
- 22:48of fluid mechanics, it's the same
- 22:50equations for water and for air. Even
- 22:53though the molecules that make up water
- 22:54and air are quite different, right?
- 22:56>> And it's it's um but it is a bit more
- 22:59complicated in the in the full case of
- 23:00the universe because we are observers
- 23:03embedded within the thing that is the
- 23:06universe. And so if we're the that when
- 23:09we say we are thinking about the
- 23:11universe in this way in terms of these
- 23:13rules but we are also made into made of
- 23:16those rules and it turns out that it we
- 23:19can we can attribute sort of the
- 23:21behavior of the universe to different
- 23:23rules and end up coming to the same
- 23:25conclusions about the aspects of the
- 23:27universe that are observable. So the the
- 23:30you know the the I think the the way to
- 23:32answer that is to say there actually can
- 23:34be just one rule that uh or you know a
- 23:38very small number of rules that we can
- 23:41we can run those rules and get what is
- 23:45at our observable to us as what happens
- 23:48in the universe. So let me give an
- 23:50example of that. I mean so so we have
- 23:52simulations now of things like black
- 23:54hole mergers in our models and the you
- 23:58can use a whole range of different
- 24:00possible rules and you'll always get the
- 24:03same kind of behavior at the scale you
- 24:06know if you look at the absolutely
- 24:07microscopic scale you'll see different
- 24:09things going on but if you look at a at
- 24:12a sort of zoomed out scale you'll see
- 24:14these black holes merging and some
- 24:15gravitational waves produced and so on
- 24:18and uh it's uh So that's it's it's a
- 24:22slightly it's a slightly weird thing
- 24:23because it's a little different from the
- 24:25way that one's thought about physical
- 24:26theories before and that that will tell
- 24:28us that will take us into into the story
- 24:30of the rouad.
- 24:32>> Okay. Well rullad's coming coming soon.
- 24:34Uh so this is this is great. Uh viewers
- 24:37can watch all the videos in closer to
- 24:38truth the wolf from physics project on
- 24:40the closer truth website and YouTube
- 24:43channel and including the rouad which is
- 24:45coming which is going to be I think my
- 24:47favorite. Thanks for joining us.
- 24:51Thank you for watching. If you like this
- 24:53video, please like and comment below.
- 24:56You can support Closer to Truth by
- 24:58subscribing.
- 25:00Closer to Truth is now accepting your
- 25:02taxexempt donations. Please come to
- 25:06closerto.com/donate.
- 25:10Thank you very much for supporting us
- 25:12and thanks for watching.
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