08/05/2021
What is Matter? with Bryan Cheong
A conversation with Bryan Cheong about the laws of thermodynamics. Bryan Cheong received his Bachelor of Science from Stanford University, with a degree in applied and computational mathematics. He then went on to receive a Masters degree in Materials Science, also from Stanford. Outro Song: “Pick Up The Pieces” by The Average White Band
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This is KZSU Stanford.
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Welcome to entitled opinions.
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My name is Robert Harrison and we're coming to you from the Stanford campus.
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The average white band with pickup the pieces.
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That's all we have in the end, pieces.
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That's all we have in the beginning too.
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The subatomic particles that form atoms, the atoms that form molecules,
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the molecules that form elements, entities, and organisms.
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The star systems that form galaxies, and the black holes that devour them eventually.
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It's all in the pieces and no one knows whether there's a hole to which they belong
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or whether the material world is just parts outside of parts, outside of parts.
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Practice X-appatus as medieval scholasticism used to define matter.
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Thank you.
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[Music]
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Barrowing from Alan Lightman, the credo of the scientific view of the world can be stated as follows.
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The universe is made of matter and nothing more.
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It is governed exclusively by a small number of fundamental forces and laws,
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and all composite things in the world, including humans and stars,
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eventually disintegrate and return to their component parts.
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Now even though the phenomenologist in me objects to nothing but philosophies,
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I can live with the idea that the universe is made of matter and nothing more.
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Matter after all isn't what it used to be.
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We're starting to understand that matter can in fact think and feel,
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that under some conditions it can self-transcend, and that spirit is a rare,
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maybe the rarest form of sublimated matter.
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So if matter indeed contains the potentiality of spirit,
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if it can glint or glow in someone's eye, and if it can even ask what matter itself is,
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as my guest and I will be doing shortly, then yes I'm happy to call myself a materialist,
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in the most scopious sense of the term.
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There's a word you haven't heard me use before on entitled opinions,
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scopious, having a wide scope, spacious, first known use, 1599,
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in Thomas Middleton's Microcynecon.
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I quote, "streams ER barred their course swelled with more rage and far more greater force,
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until their full stuffed gorge of passage makes into the wide maws of more scopious lakes."
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Scopious indeed is our theme today. I'm joined by Stanford Graduate Brian Chong to discuss
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some of the more basic laws of the material world above all those of thermodynamics.
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Brian received his Bachelor of Science with a degree in applied and computational mathematics
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here at Stanford. He then went on to receive a Master's degree in material science,
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also from Stanford, and I'm delighted he's here today to help us think through some
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fundamental aspects of what we call matter. Brian, welcome to entitled opinions.
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Thank you Robert, the pleasure is entirely mine to be here.
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So Brian, I mentioned earlier that matter is not what it used to be, meaning that our conceptions
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of it, of matter, and of the laws that govern it have changed quite a bit in the past few centuries.
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Why don't we start with the basic question like what are some of the significant transformations
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in our understanding since the 1700s? Well, thank you. In many ways the 1700s and the 1800s were
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very special time in science and our understanding of matter. It was a time when, after the discovery
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of Newton's laws and the invention of many types of scientific apparatus that was able to describe
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the expansion of air and heat. Many of the thinkers in Europe started to move towards a very
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deterministic and mechanistic view of the universe of a clockwork universe where all of motion
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is mediated through fluids and cogs and rods and all of these very fixed and rigid mechanisms.
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And that is the deterministic universe of the 18th and 19th centuries, while the universe of our
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current conception is one that's a bit more dynamical, more probabilistic. And because these
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phenomena are probabilistic, we think of these universal phenomena in terms of statistics. What
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is statistics? It is the science of treating probabilistic phenomena when something is not
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deterministic. When you don't know what is going to happen in the future, the art of predicting
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that and the art of predicting the distribution of outcomes is statistics. And because our
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conception of matter is now very much dynamical and probabilistic, statistics is the tool with which
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we rely on in order to come up with the ways that we describe matter. And a very good example of
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that would be from the evolution of our understanding of heat in the 18th and 19th centuries,
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people thought of heat as a sort of fluid in, if it was, it would mean like a substance.
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It's indeed an actual fluidic substance like a liquid. When it was producing combustion, they
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called it floriston, and when it's being transferred from a hot to cold object, they called it
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caloric and it's called the caloric theory of heat. We now know that in material objects,
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these things are not actual liquids. Anyway, we think of heat instead as the kinetic energy of
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particles. It is the average speed at which particles move about if it's in it. These would be
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subatomic particles. No, these are atoms and molecules. So if it's in a gas, they would be moving
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about in space. And if they're in a solid, they usually just vibrating really quickly. And the speed
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of this movement and vibration is what we call heat. There's no fluid to mediate the transfer of heat
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at all. And when you have a particle that moves really quickly, and that's a, they are really hot,
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if your particles move very slowly, they're really cold. And a transfer of heat from a hot object to
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cold object is nothing more than a really fast moving particle knocking against slow moving particles
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and transferring some of their speed. So famously, second law of thermodynamics, we'll get into it
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more in detail later. Heat can only go from a hot to cold. Why can't they go from cold to hot?
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It can. So James Clerk Maxwell, who was a very famous physicist, described how the second law
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of thermodynamics is a statistical law. It's not a purely mathematical one. It can be violated when it's,
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you have very small collection of particles and on very, like, local areas. But when you have a lot
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of particles has a whole, the law is violated because of the law of large numbers. And this law is
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defined as, well, there's different formulations of it. And I know of it as the law of entropy,
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but maybe you can give a more formal definition of the second law of thermodynamics. We're going
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to speak a lot about that. Sure. And there are many different ways of formulating that this second law
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of thermodynamics. And one of the earliest ones is from Sadif Garneau. He actually thought of heat
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in terms of the caloric theory. He thought of heat as a fluid, but he was able to come up with the
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second law of thermodynamics by thinking of what an ideal engine looked like, an ideal engine that's
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powered by no more than a difference in temperature between a hot object and cold object. And the first
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earliest statement of the second law is that there exists a maximally efficient engine. Another
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system. It means that you, there's only a maximum amount of work that you can get from a different
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in temperature. So engines derive from differences in temperature. You have a hot thing and a cold
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thing and then you try to derive work by this difference. You don't have to think of it in terms of
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heat. You can think of it in terms of say a fountain or a dam where a turbine is being driven by
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something as a very high water level versus something as a very low water level. And a difference is what
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drives turbines and same with heat as well. So given two different water levels in terms of heat,
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there's only a maximum amount of work that you can derive from it.
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So why not call this energy rather than the transfers from hot to colders? That's how we understand
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energy. Well, energy is something, well, we have to go back to the first law for that as well.
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Energy is something that cannot be created and destroyed. And that's the first law of thermodynamics.
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That's right. Conservation of energy. That's right. And the second law is about how the form,
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it's governs the forms that this energy can take. Your turning heat energy into movement
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energy or work energy. That is a transfer or transformation of energy. But it's a difference in
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terms of you're not really creating energy along this way. So it'll be incorrect to say that
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you're creating energy from an engine. Yeah, well, that's a very subtle distinction that I will
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have to keep in mind because I think that if you put coal into the steam engine, you are
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generating energy or what you're allowing for the second law of thermodynamics to do its thing,
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I guess you would put it that way, right? I'll say that you are putting the chemical energy of coal
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inside a engine. And that's the whole thing. You're transforming that chemical energy into
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heat and then the heat into work energy. Okay, so, so, Brian, between the 16, 17,
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1800s and now the real shift in thinking is that we've gone from a mechanical deterministic
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view of matter to one where now matter is composed of particles. That's right. Small bits.
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And heat, for example, is the speed at which these particles interact. That's right.
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The faster the hotter the slower the colder. That's right. And therefore, we need a statistical
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understanding of matter rather than let's say a mechanical one because at the quantum level or at
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the molecular atomic level, it's only a huge amount of particles that will give patterns of order
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that then can be measured only statistically rather than exactly. So, there are two things to think
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about here right now. The first is the law of large numbers. This is a statistical law that governs
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when you have a lot of things versus very few things. And the law is things tend to the expected value,
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the more you have of them. So, if you flip two coins, the expected value of the number of heads you
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get is one. But if you flip just any two coins, you might get both tails or both heads. But if you
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flip this coin, these pair of coins many trillions of times, the final expected value from many of
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these flips will be one. So, is that what's called equilibrium in the final analysis?
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That is not an equilibrium. The second thing I have to talk about because when I say that
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heat is the average speed of particles, a hot object can have very slow particles as well as very
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fast particles. So, these slow particles are considered cold but how can cold particles exist in a
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hot object? It's because particles form a distribution of cold and hot particles inside a single body.
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And usually if it's sort of an ideal gas, this distribution is known as a Maxwell-Boltzmann distribution.
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And very often you encounter these sort of distributions and statistics as well because these
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distributions basically tell you how you, if you have something that is probabilistic,
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what is the probability of finding it in a cold as a cold particle or a hot particle? And the
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distribution describes that probability. And the main theorists of this new kind of statistical
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understanding of matter would, I mean you mentioned the Maxwell, you've told me about the Maxwell-Boltzmann
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distribution. So, Boltzmann is another figure here. I mentioned Boltzmann and I think one way to
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illustrate this distribution would be to think of one of Boltzmann's own thought experiments.
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Boltzmann in particular, the theory called H theory. And to think of how a Maxwell-Boltzmann
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distribution of particles of slow and fast particles can arise naturally, just think of a box of particles
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with even speeds. Imagine you have lots of particles on a box, they all trapped inside and they all
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have the same speed. This is actually very unnatural. It has very low entropy and a system
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obstacle to a place where fire entropy, wise that the case. Because when you have two particles of
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even speeds hitting on each other, one will speed up and one will slow down. And eventually,
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as faster particles are more likely to hit other particles, while the slow particles are less likely
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to hit other particles. And so at some point, the rate at which fast particles get slowed down by
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hitting another particle and the rate at which slow particles speed up by being hit by another
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particle becomes even and that's an equilibrium. That is what is called a fine balance. And once
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this condition is reached, you realize that a Maxwell-Boltzmann distribution of particles emerges
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where there's a lot of slow particles and some really, really fast particles. But then when they
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even are and they reach equilibrium, that's almost like a death. It means that nothing happens anymore.
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It's still a dynamical system. That's why I still describe it as a dynamical system. Particles
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are still slowing down and speeding up all the time is just that the proportion of them
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will forever remain the same if they're in our particles in that box unless something from outside
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the box intervenes. Right. So here we're talking about closed systems. That's right. Okay.
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Does this theory of particles and their constant, you call it speed, you say their motion and
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interaction, their relations? Does this theory proceed the quantum mechanics, the thinking of
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quantum mechanics? Because it seems like quantum mechanics is also predicated upon very much of the
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same notion of a dynamical systems where you have probabilistic knowledge of where, for example,
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electron will be and so forth. But it sounds to me like the laws of thermodynamics are
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independent of quantum mechanics. Very much so. These sorts of things are entirely of a statistical
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description. And in some ways, it's even more fundamental than a quantum mechanical one.
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If you go to a physicist and tell them that you have observed something, something that breaks
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the standard model of quantum mechanics, they might believe you. If you go to them and say,
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I found something that violates the second law of thermodynamics, they'll laugh you out of the
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the room, because it's that fundamental. So if matter were to be in the same conception as
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Epicurus, where they would just rigid balls or rigid objects rather than a quantum mechanical
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system, they will still behave in the same way and they will still reach the same equilibrium,
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just entirely from this statistical principle of how this distribution can arise from the
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fine balance. What about irreversible ability? Because the second law of thermodynamics is very
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famously associated with the concept of things that are irreversible. And we were reading Carlow
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Ruhveli, the quantum theorist who has written some really magnificent books, especially for
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people like me who don't follow the equations. But he has a book called The Order of Time,
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in which he claims that the only law in the universe, which can account for the fact that time
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moves from past to the future is the second law of thermodynamics, because it's the only law
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about that has to do with the irreversibility and things. And time itself is being irreversible.
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How does the irreversibility of time relate to the second law of thermodynamics?
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That's a very good point. So one of the things that a purely deterministic universe has
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is if you took the arrow of every single part of the universe and the direction that
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moving in and flipped it, the world would be as it is. That's obviously not the case. If you film something
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and you do it in reverse, you can tell quite obviously that there is an arrow of time. And the second
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law is that arrow. Because when you think the difference between the present and the past and the
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future and the present is that the future will always have more entropy, as long as there's some sort
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of irreversible process. So in order to approach this concept, let's think of, let's try to define
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what entropy is. Yes, let's do that. So one common understanding of entropy is that it is disorder.
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But disorder is not something that you can really quantify, right? If you break a plate,
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the pieces of the plate is more disorderly. But the universe doesn't care if it played as whole,
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or if it is in many pieces. No, but we say entropy negative because you can go from the plate to
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the pieces. Now we're going back to the average white band song, pick up the pieces. But you cannot
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go from the pieces of the broken plate and it will not reform naturally the plate.
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So I don't like calling entropy sort of negative thing. And no, I don't either. That's why I want
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to hear a few. I want to, I'm strong, a pologee as the Latin say for entropy as being utterly vital.
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So when you think of entropy, think instead of it as a measure of degrees of freedom. So
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the entropy of a crystal is very low because the particles in a crystal, the atoms are fixed in
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position and they can move at all. They can only vibrate in place. The entropy of a gas is very high
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because the particles are free to go all over the place and take the form of wind and breeze and so on.
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So the entropy of particles in a very restricted place is really low, well, if you expand that space
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and give them more states of freedom, what a physicist called microstates, then the entropy becomes
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higher. And one restatement of entropy is that it is the measure of the degrees of freedom
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and a restatement of the second law is that the degrees of freedom once given cannot be taken back.
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And I'd like to say that it's like the material arc of the universe bends towards freedom as it
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well, because once you give freedom to these particles, these forms of matter, you can take it back
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anymore. And that's what irreversibility means, things that are free, you can capture them back.
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So for me, that sounds like a highly radical revolutionary understanding of entropy as something that
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is the condition for the creation of the universe, for the origins of life, for all sorts of things
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that come into being, that emerge into forms that what I don't understand is things emerge into order.
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And this idea that everything is a kind of irreversible directionality towards a disorder,
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which is another word for entropy in the common understanding of entropy. I don't understand how we
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get new forms of order created, except perhaps by creating more entropy elsewhere than within the
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systems that are ordered spontaneously. So we can think of the universe as moving through arcs of complexity.
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The very young universe, everything was all put together, there weren't too many big galaxies,
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there weren't any, there wasn't any life and that had very low entropy. And I think one way of
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thinking about it is that entropy is like the weights of a grandfather clock, where you're able to,
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the beginning of the universe is a very low entropy place. And...
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Well, excuse me, but how can I be low entropy when you have all this extraordinary creation of
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stars and galaxies and the expansion of space, that sounds to me like the utmost arena freedom
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and freedom for work to take place. That's precisely that when you say expansion of space,
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you're using the same words I did to describe it increase in entropy. And that increase in freedom
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of universal freedom is the very first breath, the very first fiat looks of the increase of entropy.
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And the young universe was a really hot, really localized, very compact sort of place, where all
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the stars are close to get, all of the matter was very close together. And now it's
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freer to take all different forms. When you think of entropy and transfer of entropy,
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or rather the transfer of free energy, you think of the increase of entropy in the heart of the sun.
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And that gives earth a free gift of free energy and under the do our work and create our own
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complexities of life. Entropy is not just an increase in the degrees of freedom, it's also,
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the freedom arises in terms of complexity. When you have a more complex system, it's often
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something that is more entropic in nature. And so when you want to think of a future universe,
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think of future Earth, think of even more complex, more, I don't like what messy,
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but you know, messy sort of place. So I have a question about life, if one imagines that life
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is one of the most complex dynamical systems of matter that we know of. Then how does one
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understand the entropic condition of possibility for life? And is life by virtue of it's being
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alive and remaining alive and thriving in its animate form? Is it creating all sorts of disorder
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outside of itself by virtue of itself perpetuation? This is certainly the theory of some biologist,
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Lynn Margulis and others, even Schrodinger, who wrote a book called What Is Life claims that
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this extraordinary complexity that life is creates a great deal of entropic disorder outside of itself
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in order to maintain itself in being. So I want to think of life as a sort of entropy itself is
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like life, right? Because life is the process of being far away from an equilibrium process. You
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are constantly creating irreversible changes to the world around you and inside you. And being
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in this state of constant irreversible processes, you are constantly increasing entropy. But
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it's hard to think of it as creating disorder outside yourself because let's go by all the way to
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what powers life, right? How does life get this potentiality to actualize into the forms that it takes?
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For that we need to first think of what is free energy. So I mentioned before that energy cannot
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be created or destroyed, it can only be transformed. Well, there are some forms of energy that
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can be transformed to others, but not the other way around because of the increase of entropy
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from one form to the other. And the free energy that powers life and comes from mostly the sun,
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the sun gives us light and the light hits an electron in the leaf of a plant.
|
00:25:08.400 |
The electron, this single subatomic particle leaves from one molecule, one jumps from one atom to
|
00:25:15.600 |
the other, and that small gap, that tiny little jump is what powers most of the life forms that you
|
00:25:22.960 |
see. You're describing photosynthesis. I am describing photosynthesis. And how does it work
|
00:25:27.280 |
exactly? It's a decoupling of an electron from it's nucleus. So it is indeed you
|
00:25:33.600 |
some ultraviolet light hits an electron and the electron makes a small jump. And that tiny
|
00:25:40.480 |
subatomic jump is like the lifting of a weight of an old grandfather clock. The way you
|
00:25:45.840 |
usually power it is that you would lift a weight hung on a chain on a grandfather clock and then
|
00:25:51.040 |
over the course of a day or even two days that the weight would slowly descend as it powers the
|
00:25:56.000 |
rotation of the hands of the clock. Well, that single jump of a single subatomic electron is
|
00:26:02.000 |
like lifting the weight of a grandfather clock. And that electron is passed from molecule to
|
00:26:06.960 |
molecule within the chloroplasts or the green powerhouses of a plant, making us very slow
|
00:26:14.480 |
energetic descent so that you are squeezing every bit of free energy you can from that single
|
00:26:19.600 |
jump of an electron. And when animals and humans ingest plants, we take into ourselves the potentiality
|
00:26:27.760 |
powered by that free energy given by the sun. And so in ways we are increasing entropy, but the cost
|
00:26:35.360 |
has already been incurred in the heart of the sun by some hydrogen has already combined possibly
|
00:26:40.800 |
thousands of years ago. I like to think of it as a big drama of things between the sun and the
|
00:26:46.480 |
earth and everything that lives on the earth. It's not necessarily that we are just engines of disorder,
|
00:26:51.760 |
just generating disorder all the time from ourselves. It is this big system that spans our entire
|
00:26:57.760 |
solar system. Yeah, well, I did a show on the sun. I think last year it was a solo show called
|
00:27:03.680 |
the heart of the sun. I went to the very heart of the sun to look at the kind of processes that
|
00:27:08.960 |
take place in terms of nuclear fusion. Yes indeed, you also remind me that the earth has its own
|
00:27:19.120 |
molten core which itself at the heart of our planet, there is a great deal of heat that is coming
|
00:27:26.320 |
from radioactive decay and that is also another condition for the possibility of life in so far as
|
00:27:33.760 |
if only because it gives us the magnetic shield that protects our atmosphere from burning away
|
00:27:41.760 |
thanks to the heat that's generated at the heart of the heart of the earth itself.
|
00:27:48.000 |
So there are sort of heat-loving bacteria that never touched the light of the sun and they are
|
00:27:53.520 |
indeed powered entirely by the heat in the earth. So there are three forms of energy that humanity
|
00:28:00.720 |
has captured. One is the common source of most energetic life forms, whether it's organic life forms like
|
00:28:08.880 |
plants and animals or what I want to call inorganic life forms like the breeze and the ocean waves.
|
00:28:15.520 |
Those are all powered by the light of the sun. The light of the sun is also what is found in
|
00:28:20.800 |
petroleum and in coal and everything else. Of course, those have got fossil fuels because they
|
00:28:26.720 |
are fossilized sunlight. The light of sun created those plants, the plants become fossilized and then we
|
00:28:32.480 |
release the energy once more. That's the bulk of the energy that humanity uses to power our
|
00:28:37.840 |
modern industries and also our living bodies. The second form is as you described from the earth.
|
00:28:44.160 |
Most of the heat of the earth, the center of the earth comes from the breakdown of radioactive
|
00:28:48.880 |
particles, of radioactive elements like uranium and because the earth is so thick, it's like a
|
00:28:54.160 |
safe blanket that traps most of this heat inside. So nuclear reactors and geothermal stations use the
|
00:29:00.160 |
same power which is the breakdown of uranium. The third form of energy that we tap into is the
|
00:29:07.200 |
rotation of the earth. The only way I can think of that really manifesting itself in the
|
00:29:15.280 |
non-organic living systems of earth is in tidal energy. The tides are powered by the rotation of the
|
00:29:22.880 |
earth. Not only are the tides powered by it, the tides give a bit of the energy away to the moon and so
|
00:29:28.480 |
the moon is actually inching slowly away from earth, powered by that rotation. Those are the three
|
00:29:33.440 |
forms of energy that power all the free energy activity on earth. All of these forms of energy,
|
00:29:40.880 |
not only here on our earth and solar system, but the entire universe, are governed by
|
00:29:48.000 |
these fundamental laws. One is the conservation of energy and the second law of thermodynamics,
|
00:29:55.360 |
you say for every action there's a reaction, remember that? That's a law of motion,
|
00:30:01.600 |
Newton's a third law. Motion. So for every action there's a reaction, is the old understanding
|
00:30:09.440 |
of a kind of symmetry. You do this and then you get that. But we are living in a very different
|
00:30:14.720 |
conception of matter where we don't have that kind of equivalence because there's this irreversible
|
00:30:23.280 |
process at work in forms of energy. I think we want to be more precise in nuance here. There is no
|
00:30:30.320 |
contradiction between every action has a reaction and the second law of thermodynamics. In fact,
|
00:30:36.880 |
the thing that powers the second law is that every action has a reaction when I mentioned the
|
00:30:42.320 |
particles in a box hitting each other. The reason why energy is transferred is because of Newton's
|
00:30:48.800 |
third law of motion that every reaction, every action has a reaction. Let's think of matter
|
00:30:55.920 |
statistically now. Let's conceive of a balloon. What is forcing a balloon to hold its shape?
|
00:31:01.920 |
It's the air inside. But I told you that air has loads of particles moving around all the time.
|
00:31:07.520 |
So how do these particles maintain shape? It is because of collisions. On average, there are enough
|
00:31:14.160 |
particles colliding with the side of the balloon both from the outside and the inside to even out
|
00:31:19.920 |
at that point of that balloon to how have it maintained its shape. The shape of the balloon,
|
00:31:25.280 |
and in fact the shape of anything that is maintained by pressure and fluidic dynamics,
|
00:31:30.240 |
is from the energy of particles colliding against its side and balancing itself out.
|
00:31:36.880 |
So this third law is about that transfer of energy that happens when you have that collision.
|
00:31:42.480 |
And when you think of it statistically, think of it in terms of the law of large numbers,
|
00:31:47.280 |
there is in a, let's say you have a balloon that's about a liter inside. Then there are about,
|
00:31:53.760 |
I think I'm going to get the order of magnitude wrong and you're going to get angry emails. They're
|
00:31:57.680 |
about several tens of trillion trillion particles in that balloon. Some of them are slow and they'll
|
00:32:03.600 |
never hit the side of it. Some of them are really fast and they're hit really hard,
|
00:32:06.720 |
disproportionately hard. But on average, when you have so many particles in the same place,
|
00:32:12.080 |
they are very predictable. You tend towards having this particular pressure applied by these
|
00:32:17.520 |
number of particles. And that's the nature of how the third law of motion relates to the second law
|
00:32:23.680 |
and how the world is maintained by many of these fine balances happening.
|
00:32:28.720 |
Well, that's very interesting because I'm preparing for the show and also having read
|
00:32:33.760 |
Cardinal Ravelli, I've been plunged in quantum mechanics of late. And also having done a show
|
00:32:42.400 |
with Mark Taylor, philosopher, we're talking about relational ontologies where
|
00:32:48.560 |
for Ravelli too, he thinks that the essence of quantum mechanics that everything is in
|
00:32:54.160 |
relation that there are not substances, but that there are almost events and these events are the way
|
00:33:00.080 |
things act and interact with each other. And that's fine and there's relations. But
|
00:33:06.080 |
in preparation for this show, I realize that even more fundamental than relationality is
|
00:33:12.240 |
collision. It's extraordinary how much of the very motor and agency of all of matter depends on
|
00:33:19.440 |
collision and things smashing into each other. And this is also what we experience in our
|
00:33:28.080 |
lives in everyday lives and in moments of heightened activity or conflict and things that
|
00:33:39.840 |
collision, contact, it's such a mystery to me because it just means that all of matter seen,
|
00:33:48.400 |
it's all conspired to not just interact with each other, but to collide and sometimes annihilate
|
00:33:55.600 |
the other particles and so forth. This is a very violent view of matter, wouldn't you say?
|
00:34:03.200 |
I'd say let's think of it in certain ways, in certain ways, in a certain way,
|
00:34:07.920 |
why don't we think of in terms of serendipity? These are all serendipitous meetings and the sum of
|
00:34:13.600 |
all these serendipities create the properties of the things we see around this. But if they didn't
|
00:34:18.320 |
collide, there wouldn't be any activity, there wouldn't be any, as you said, the slow particles
|
00:34:24.000 |
are hit by fast particles and they get faster and the other ones get slower, but without
|
00:34:29.680 |
collision, nothing happens. That's true. And even with collision, nothing can happen.
|
00:34:36.480 |
And that's sort of the cursive entropy. You can, if you, if the number of collisions that you have
|
00:34:42.880 |
doesn't change on average, on a macroscopic level, nothing happens. And in that way, you can have a very
|
00:34:48.480 |
tip at universe with a very large as many collisions as you have now. So I think that it's
|
00:34:55.520 |
this sort of like fundamental violence that's happening beneath the surface of macroscopic properties
|
00:35:02.320 |
happens regardless of whether we have a creative, beautiful, complex universe, or one that's really
|
00:35:09.840 |
tepid and really informative. And it is just that the particles themselves don't think of it
|
00:35:17.280 |
in terms of violence. They think of it in terms of this is the way that we manifest our energies
|
00:35:22.880 |
and we transfer energies. It's by giving and receiving and sometimes like giving and receiving
|
00:35:27.760 |
is a bit faster than we on our very slow macroscopic levels. I used to.
|
00:35:32.560 |
So you mentioned the word tepid. So I want to ask two big questions for the, you know, the remainder of
|
00:35:41.280 |
the show. One is because the word tepid reminds me, and I know it reminds you of a passage in St. John's
|
00:35:48.320 |
Revelation. That's right. Which is related to the revelation is the vision of the end of time.
|
00:35:56.160 |
And we could call it the end of the universe. And there's something there where John speaks
|
00:36:02.240 |
about the lukewarm. Can you relate that moment in St. John's Revelation to the vision of the
|
00:36:11.600 |
end of a universe where the entropy gets to the point where we are in this kind of neither
|
00:36:17.360 |
cotton or coal, but a kind of lukewarm tepid equilibrium state. So
|
00:36:23.440 |
entropy is irreversible in the sense that you lose potential energy, right? Things that are hot,
|
00:36:32.640 |
one of the other restatements of the second law of thermodynamics by Lord Kelvin is you cannot
|
00:36:37.760 |
spontaneously transfer heat from a cold object to a hot one. And so eventually the heat of the
|
00:36:44.240 |
universe will be so even things will be so sit it still on average, same-ish, that no more changes
|
00:36:51.520 |
will happen. And finally, the universal region equilibrium point from which you'll never depart.
|
00:36:57.200 |
And that is the lukewarm universe. In reality, it might be about four degrees above absolute
|
00:37:01.440 |
zero or five depending. So it's not necessarily, it's not exactly a lukewarm day. It's quite cold by
|
00:37:09.040 |
human standards. But really, this is, again, this I don't want to be unfair to the notion of
|
00:37:15.040 |
entropy because the way that we have put it, it sounds like entropy is the bringer of the eschaton,
|
00:37:19.520 |
it's the coming of the end times. When in reality, entropy is really just the whole process of
|
00:37:24.560 |
life and living. I know, and that's great, it's a very important corrective to the normal
|
00:37:32.160 |
connotation of entropy. However, life, the condition of life which requires a lot of energy and
|
00:37:40.880 |
mobilizes, creates it. So it's also death. And so it's no devaluation of life to say that it ends in
|
00:37:49.920 |
death because without death, you wouldn't have life, as we know it, at least most forms of life that
|
00:37:56.960 |
we know. So in that sense, maybe a kind of eschaton or death is a price you pay for a miracle,
|
00:38:07.600 |
such as this higher form organization of matter which we call the not only life, but the spirit of
|
00:38:16.720 |
life too. Well, let's think, let's go all the way back to Sadhi
|
00:38:23.360 |
Gahunoh's engine. If you want a state of the universe that will never, that will never
|
00:38:28.640 |
approach entropy, but still changes, you can always have this perfect engine that's constantly
|
00:38:34.480 |
being powered. You can run for ever because it is always lubricated. The problem with it is,
|
00:38:39.920 |
the calf no engine needs to run infinitely slowly, become infinitely isolated, and be infinitely
|
00:38:47.440 |
lubricated. And can you imagine a universe of only that sort of thing? Well, I can not only
|
00:38:53.520 |
imagine, but I can even be nostalgic for one, it ends when I'm in certain moods because when I think
|
00:38:59.440 |
of our moment in history and the kind of aggravated modernity that we are living in, that we are
|
00:39:08.080 |
so overheated at a cultural, you know, socio-political level that there is so much going on,
|
00:39:16.480 |
and the transformations are so rapid and disorienting that I can understand the nostalgia of
|
00:39:24.160 |
cultures that are anti-motor where they would like to go back to a much slower homeostatic
|
00:39:35.840 |
condition where every year you don't have to completely reorientate your understanding of the world
|
00:39:43.760 |
you live in because things are changing at a much slower pace. I can understand the desire to
|
00:39:51.040 |
cool things down at historically speaking. So yes, I wouldn't want to have the kind of
|
00:39:59.440 |
engine where it's kind of frozen to death, but do you think that we live historically in a very
|
00:40:06.640 |
overheated moment? I do not. And the two things to say about that, what you've said just now,
|
00:40:12.640 |
homeostasis, you want to, you mentioned that this is a homeostatic, you want to have a nostalgia
|
00:40:18.720 |
for homeostatic. Well, homeostasis is the process of maintaining something far from equilibrium,
|
00:40:25.840 |
your body's maintaining your body temperature and life through homeostasis in a system that doesn't
|
00:40:31.840 |
want to go down all the way to equilibrium. So you've already described a very irreversible
|
00:40:36.240 |
process over there. And the second thing is that it's not how life works. Perhaps what I meant to
|
00:40:42.400 |
say is that the historical conditions of our reality are completely non-homeostatic.
|
00:40:49.920 |
Well, there are two ways to look at it, right? Because the way that the variety of life has
|
00:40:55.440 |
arisen, the way that evolution has arisen is by many of these shocking changes and by introduction
|
00:41:01.120 |
on random changes. And we, this is not, this is a false nostalgia because life has never been like
|
00:41:08.640 |
this. Life has taken many forms and moves and transforms even when there's nothing, we think you
|
00:41:15.120 |
are an isolated island of the Galapagos. Life will always find a way to specialize and change in
|
00:41:22.080 |
its conditions and compete with each other. And I think it's a false nostalgia thing that you can
|
00:41:27.200 |
always have this sort of stasis. Well, we can leave nostalgia out of it. We can talk about the,
|
00:41:33.440 |
what Freud called the death drive. And it's a very compelling Freudian notion that
|
00:41:42.560 |
all of matter was universally and originally inanimate. And that in order to move from, to jump from
|
00:41:50.480 |
the inanimate into an anima state, it took a tremendous traumatic shock of transition and that
|
00:41:57.920 |
therefore in everything alive, there is even more fundamental and deeper than the pleasure
|
00:42:04.960 |
principle or the reproduction is a death drive that wants to return invariably to this inanimate
|
00:42:12.880 |
static state that preceded the emergence into organic living being. And that is true because
|
00:42:20.800 |
the only way that these irreversible processes is powered is because there is an ultimate end
|
00:42:25.680 |
of that equilibrium state. I mentioned the grandfather clock being powered by life,
|
00:42:31.920 |
that equilibrium state that the universe is. The, when that weight on that grandfather clock that
|
00:42:37.280 |
was lifted just once by the fiat looks of Genesis finally hits its bottom and there's nowhere else to go
|
00:42:44.560 |
and the clock stops ticking. That however is going to take tens of trillions of years and I think it
|
00:42:50.720 |
takes a cosmic level of bad faith to think of that particular end when there's so much more
|
00:42:57.120 |
drama and so much more story to happen between now and then. Oh yeah, but I'm not particularly
|
00:43:02.320 |
concerned with the grand finale of the whole thing. I'm just more concerned with what it means to
|
00:43:08.480 |
be an embodied life form in this particular moment that I'm living in and the way in which
|
00:43:16.080 |
entropy works for me, for you, for our society, the way the death drive may covertly be sponsoring
|
00:43:26.400 |
all sorts of destructive behavior that history is made of. You can say that that destructive
|
00:43:32.000 |
behavior is part of the entropic processes that create life. It's funny, but I think that we,
|
00:43:37.760 |
we deny the implacability of the death drive at our own peril. So that's, we can close that
|
00:43:45.200 |
little parentheses now about that because I want in the time remaining the few minutes we
|
00:43:50.720 |
made to ask you about your specialty, which is statistical mathematics and analysis and you spoke
|
00:43:56.960 |
about the the large numbers, the big numbers, but this whole thing also is related to what we are
|
00:44:03.680 |
living culturally as an era of big data and how big data this compilation of statistical
|
00:44:12.080 |
probabilities and averages has an almost predictive power of how we are going to behave as
|
00:44:17.840 |
individuals, right? That's right. So the reason why the second law, it's so absolute,
|
00:44:24.960 |
is because we are unable to track the location of every single particle in the trillions of
|
00:44:30.960 |
trillions of particles that are around us. James Fluck Maxwell had this hypothetical thought
|
00:44:36.880 |
experiment of a demon that is able to track every single particle in a box and it has control
|
00:44:43.280 |
over a gate. And so Maxwell's demon will open the gate only for hard particles and close the
|
00:44:49.120 |
gate for cold particles. And so by just using this gate without changing any of the behavior of
|
00:44:55.120 |
the other particles, you're able to aggregate all the hot particles on one side of the gate and
|
00:44:59.840 |
cold ones on the other side. And so you're spontaneously violated the second law as the
|
00:45:05.360 |
Lord Kelvin statement of the second law. You cannot spontaneously create a hot and cold body
|
00:45:09.840 |
and separated out like that. And that's only possible only because this demon is omniscient,
|
00:45:16.240 |
is able to track and measure the speed of all these particles about actually creating
|
00:45:20.160 |
any new change or any new entropy around it. And that's an impossibility because there's no such
|
00:45:27.920 |
way of creating this omniscient demon. Every measurement for particle will create disorder as well.
|
00:45:33.280 |
And in that way, omniscience, this impossible omniscience implies omnipotence because it empowers
|
00:45:39.440 |
you to reverse the second law of thermodynamics and time itself and the laws of the universe itself.
|
00:45:46.320 |
But while you are unable to track the individual motion of particles, you can track the motion of
|
00:45:54.720 |
individual humans. So we can't make meaningful predictions of individual humans. We have this
|
00:46:02.240 |
freedom to choose as we want to. Sociologists and social scientists are able to make meaningful
|
00:46:08.080 |
descriptions of humans in the large when you have a large collection of people in the society,
|
00:46:13.680 |
you can make meaningful predictions about how they would behave in certain circumstances and so on.
|
00:46:17.760 |
It's just that we're beginning to live in an era where we collect enough data to construct
|
00:46:24.880 |
lots of little Maxwell demons for each person. We are able to track our location, now preferences,
|
00:46:30.240 |
where we go, what we listen to, who our friends are. And so the people who possess these data
|
00:46:35.520 |
can become more than chosen than Facebook. Well, I'm not going to name anyone because I am
|
00:46:40.560 |
a native of Silicon Valley and so these people are my lords and masters and one I will not speak
|
00:46:48.800 |
against my betters. But they are able to construct certain amounts of Maxwell demons. And I want
|
00:46:54.560 |
to think very carefully about the consequence of that without any individual changing their
|
00:47:00.640 |
behavior or knowing they are changing their behavior. You are able to separate the
|
00:47:05.520 |
hots from the colds, the lambs from the goats entirely just by the opening and closing of a gate.
|
00:47:13.200 |
And while we cannot be omnipotent when it comes to the particles of matter,
|
00:47:18.080 |
that omnipotence isn't necessarily out of our hands when it comes to human beings.
|
00:47:24.160 |
So are your lords and masters the lords and masters of me and everyone else at this point?
|
00:47:31.360 |
Well, not because they possess the big data. Not quite yet, there's not enough to do something like that.
|
00:47:37.680 |
We'll see how the world looks like in the future, whether we as human beings can follow the
|
00:47:43.760 |
material arc of the universe and find ourselves in an irreversible state of freedom.
|
00:47:49.360 |
Well said, Brian. We've been speaking with Brian Chung. I'm really proud to have had him as a
|
00:47:56.480 |
student of mine years ago in a freshman seminar and we've been in touch ever since and
|
00:48:01.840 |
delighted to have you come on the show and explain some things about the concept of matter as we
|
00:48:09.200 |
understand it today and it will continue to evolve. So thank you very much for coming on to
|
00:48:13.600 |
entitled opinions. I'm Robert Harrison. Stay tuned for our next show. Bye bye.
|
00:48:26.320 |
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