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We're making something that's called a thermopoltaic device.

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It's an alternative way to make power that doesn't use steam or turbines.

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It uses the fact that you can shape and scale the amount of energy that comes

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out of a flame uh as light and tune the PV cells that can absorb that

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light uh and turn it into electricity. And so people always ask, you know, how does

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this scale? you know, does it work well when it is really small?

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Does it work well when it's really big? And the crazy thing about it is it

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seems that the the physics does scale across like all the way down from a single

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sodium atom to uh imaginable Dyson sphere around Sagittarius uh a the super massive

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black hole in the center of our galaxy. So how does this work?

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Um so basically uh I I say that uh you can define a Dyson sphere as

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like you have a luminous object that has energy that is that is surrounded by

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hopefully an insulated set of solar cells or or a PV cells that photovoltaic cells

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rather that convert that light energy into useful electricity so you can do work

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and you start with the atom. So, this is actually a uh real time Schrodinger

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evolved. Let me see if I where's my where's my cursor?

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There it is. All right. This is actually a real time uh Schroinger equation for the

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sodium atom. And it's basically I had never seen this.

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This was not this was not available when I was a physicist physics student.

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Um but uh it's running in the browser. It can work in your phone.

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Uh all this stuff is going to be up on Dyson Sphere.

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FYI fyi. Um and uh basically sodium and all the alkali atoms are special because

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they have essentially they've got a full shell uh and the nucleus and that's all

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tight together and doesn't interact much you know full molecule and then on the

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outside you have an easily excited I like to call it an incel electron which can

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easily be knocked around and it turns out they're rather single-minded so they can

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very rapidly um they basically work as a dipole.

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The electron moves back and forth and then u and then the much heavier nucleus with

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all the cells has an opposite charge and so it moves back and forth and not

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only is it an extremely strong and so it emits this incredibly bright yellow light

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yellow jacket yellow light. This is this yellow uh sodium discharge.

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Uh it also they they work together. So we think that this is actually pushing into

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what's extremely interesting for me. Um you know people are like oh a lot of

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quantum things require low temperature. Uh so some of the there were a bunch of

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Nobel prizes won for Bose Einstein con condensates is extremely low temperature um

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which used this kind of atom an alkali atom and particularly sodium uh in order to

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show that there's collective effects. And this is the same as two subwoofers that

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are in a in a building in phase with each other.

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They couple together and they they they output more power and there's a it's not

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quite lazing, but it's something called super radiance, super absorption and super

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transfer that ends up dominating the radiation.

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Anyway, it's getting a little complicated.

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The point being, the sodium atom is incredibly bright.

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If you calculate out just how much energy once you've excited it, the rate of power

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that it can that it can put out, it's extreme.

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Like you can end up with megawws in a liter.

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And but what happens is it doesn't just go straight out.

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It also absorbs. It has a high resonance.

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It's like a really really really imagine the best possible acoustic resonator that

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might have a Q factor of like 20. This has a Q factor of thousands and

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thousands. So it it it also absorbs. So the radiation is trapped and so the

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question is how does it scale? Does it scale in a way that is good?

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So um starting from the sodium atom we can scale to what we've done in the

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lab. So um this is a the world's highest temperature type heat exchanger.

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Uh and we've developed it. It uses ceramic that is 3D printed in a kind of

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a a photo resin that uh you make into this kind of compound arch shape.

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It's called a triply periodic minimal surface.

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And what that means is because it has all this curvature, it's able to maintain the

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incredible temperature differences across um you know from from here where it's air

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coming in less than 100° to over here where the exhaust is coming out where it's

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it's it's nearly 1400° the boiling point of salt and salt is how we get this

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the the sodium in. So it's actually in a chemical loop.

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So it goes um salt first becomes mo molten and then it has a high surface

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tension and it wicks around all of the surfaces including uh the tube um and

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including all of the different uh surfaces inside the heat exchanger and that

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allows it to be continuously refreshed and act as a resonator while not being

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itself consumed. And the reason this works is because the sodium chloride has the

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strongest bond. It's the strongest bond energy because the one's on the left side

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of the periodic table, one's on the right side of the periodic table.

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This one's an extreme in cell. This one's extremely well, the molecule needs

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another member, and they connect. I They should teach chemistry this way.

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Anyway, um so, uh what that allows you to do is convert almost all of the

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energy into this single uh wavelength, almost this single wave.

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And what you get is if you can compare it.

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So this is wavelength and this is the amount of energy uh per and this is

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a log chart. So almost all of the energy is showing up uh right here.

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It's actually um this is actually uh measured uh from from our system.

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Um and the there are two kinds of silicon cells plotted here.

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This is the internal quantum efficiency of a silicon cell.

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And this is internal quantum efficiency of indium gallium phosphide, which is the

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the highest efficiency cell to match that yellow.

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And as you can see, we're much closer. So, so the way that solar cells work

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is um it's called the photoelectric effect.

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Not the only thing Einstein won the Nobel Prize for, but sure.

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Oh, sorry. Okay. Sure. Uh little closer.

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Hopefully some of the earlier can be fixed in post.

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Um so the amount of energy um that light transfers comes in discrete packets

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quantum mechanics photons. Uh if you have more energy than what's called the band

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gap of a PB cell that extra energy is wasted.

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If you have less energy then it can't absorb it at all.

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So ideally you want your PV cells to have a band gap that is like just

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underneath the uh exhausted power and that's that's here.

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So this is a much better light source than just a sing a sun.

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So as we scale the system however we can actually change it.

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It's a little fiddly here. We can actually change it and as uh hopefully this

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works. Uh so is it changing? No, it's not.

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All right. Unfortunately, uh my claude must have busted this.

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Uh immediately before, uh the fable was so great.

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Anyway, uh so all right. So, so what is yeah set back we have setback science

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by one week. Uh so um what happens when you have an increasing amount of power

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is because of this trapping you get an increased amount of energy in the excited

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states. And those excited states uh can still leak out energy in different ways to

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other uh luminous uh lines. And one in particular when you have two excited states

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and they collide they can do what's called a pooling reaction.

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get one of them up to an even higher state and then when that jumps down

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that's a near infrared which is right here.

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So what should it be happening when I'm scaling this uh is it will go up

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yeah go up a lot. So um and it actually the first thing that happens there

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is um yeah first thing that I don't know why it's fiddly uh but um actually

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it it it again this is logarithmic so there's quite a lot here but then this

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a secondary can be added in which you can convert um that excitation into uh even

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more infrared and even better match for silicon.

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Why is this relevant? Silicon is like by far the cheapest source of energy in the

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world. It's just only available when the sun is around.

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So if you can tap into this with this light source, you can produce power

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continuously. Um so what are the kind of scales that we're talking about?

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Well, we can first start talking about like the first thing that we kind of want

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to make is something that can power a Starlink Mini and your Mac Mini and so

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on. But um as a uh as you get larger and larger uh it starts to

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get more more and more interesting. So uh friend of mine uh makes private jet says

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you need about 1 megawatt to fly. Uh a lot of people are like hey Danielle

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how quickly can you produce 100 megawws forgetting how much it will cost um because

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we desperately need it. um can it scale to that?

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And uh one thing I find I found very useful to convince Claude about this uh

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because it would keep making simplifying assumptions that was less extreme.

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It's like well one of the things that's the highest power that we ever run is

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like a um a rocket launch. So, if you have a Starship Superheavy launch or a

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static fire when it stays on on the ground, the amount of power out is 330

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uh gawatt, which is an enormous amount of power.

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But if you've ever I don't know if you you've ever looked next time there's a

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rocket launch, notice how it's yellow when it's on the ground, when it's close to

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the ground, and then it turns white. Why does it do that?

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The reason is the tiny amount of trace sodium that's just from the sea salt comes

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out and lights up the whole thing. You you also saw the same thing when the

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Blue Origin rocket exploded. So what if you actually use this tech technique to

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make a system that can actually uh produce an enormous amount of of power in a

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single installation. So if you calculate it out uh the amount of total power that

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you're generating from from that amount of of of fuel you know which is like

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methane you know liquid natural gas and oxygen which you can just condense from the

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air um that is if you converted it approximately the amount of energy about 100

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amount of power about 100 gawatts of power in a single installation which is about

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the amount that is added to the electrical grid in the United States in a single

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So uh completely different kind of uh power plant.

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So extremely interesting. So what about building a Dyson sphere at an even greater

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scale? So there are kind of two branches here.

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Um one thing is in a a for an earth shade.

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So one thing people talk about is as you increase the amount of power that goes

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to AI even if it's green it increases the amount of waste heat on earth eventually

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we get cooked what do we do so uh one of the things that you can

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do is you can figure out okay how much anthropogenic global warming have we already

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cooked into this thing and uh let's put a Dyson swarm just you know for good

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weather put it in L1 which is the Lrange point in between Earth and the sun

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and it at 0.01% of a a a shade like a a planet shade that will

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cancel out all the global warming. It's also 200 terowatts of incoming power and on

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the on the order you know near near to 100 terowatts of power right um so

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that's a very interesting thing for uh AI especially if you can start producing the

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solar panels on the moon uh because the the the moon regalith itself contains

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silica contains all kinds of oxides and uh so you can make solar cells it's also

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dramatically easier to get something into lunar orbital velocity and once it's in

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lunar orbital velocity, it can slowly maneuver to wherever it needs to be with

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light um and uh electronic uh transport.

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Sorry, I know I know this is a small room and it seems like microphone it

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a whole lot, but it's crucial to just speak into it.

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this pretty directly just so sorry I'll try to have it locked here but maybe there

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should be a compressor somewhere um okay all right great um so if you have u

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if you have an earth shade then basically up to the design point of it is

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providing the amount of cooling that we want this is a great place to to get

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energy and it could be substantially cheaper than even earthborne energy if you can

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generate uh the satellites and send them and basically you can spin launch or or

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rail gun launch to lunar orbital velocity and use almost no energy compared to

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launching something from the earth's surface.

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So I think it's good for alignment if uh AI eventually gets power off of Earth

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because then we don't get cooked by the waste heat.

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Um in addition to the fact you know we're currently we're burning a lot of fuel.

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Um but then something it was once you get to really large scale.

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So you you you you basically you have heavy industry near Mercury, you start to

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disassemble it and you you you you can send stuff out, you know, into the ecliptic.

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There's so much extra power uh in the sun.

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You can actually change the direction that the energy is is going.

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You can have um this the sun has an enormous magnetic field and it's p it's

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moving through the milky way and so it's actually accreting gas and it's exhaust

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and exhausting gas and and photons at the same time.

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So if you change where the light is going out and you change where the exhaust

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is going out and you change where stuff is coming in, this is basically a busousard

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uh ramjet which is this idea where you actually make guess I see in the audience

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you make a fusion reactor that absorbs the interstellar gas and and moves around.

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So what can you do with this? I'm not saying it's easy thing to do but

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this is how a awesome way to make a generation ship.

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Over eons, the sun can scoot around throughout the Milky Way, visit other stars,

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and potentially find another star that can scoot around even more.

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which means that you can get to the final prize which is uh if you have

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energy uh if you have at the center of the Milky Way a super massive black

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hole the amount of extractable energy when you drop something into the accretion

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disc it's it's about 50% of the of the rest mass energy which is enormous which

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is like about 50 times the amount that you would get out if you fused everything.

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Okay. Um, and the amount of power that's available if you were to do that is

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of the order of 10 the 30 33 watts. Uh, which is like just so dramatically.

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I had a big argument with Elazar Yudkowski last night, you know, um, much respect.

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He's like, you know, they'll they can use you for energy and they can use you

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for mass. And it's like, well, there's like 10 to the very large number of of

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of more energy and mass out there in space.

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It's a big place and we don't necessarily have to set things up for resource

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conflict. We can use ideas to to get out of it.

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Um, so let me see if I can show a few other things that didn't quite

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make it into this this flow. Just one second.

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Uh and then we can probably discuss um well yeah sure sorry oh uh Dyson sphere.fyi

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which I I I hope is is up right now. Let's see if Claude managed it.

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Yeah. Unfortunately uh this part isn't working.

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So I have to fix that from my Cloudflare settings.

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But um yes uh it will it will be up and the intent is so I

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I I discovered um one of the things that people always ask is you know why

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didn't anybody ever oh why didn't anybody think of this before and there's usually

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a lot of reasons. I mean this is pretty esoteric.

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You need to know at least a few things sort of you know how sodium lights

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work or fireworks work, how PV cells work and and and light divides into different

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wavelengths. Um and you need to decide to build it which involves high temperature

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flames and designing that's all right. Um and uh you you need you need to do

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all these different things. But um I was like why why isn't there any study of

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this? Like there there were 20 different ways to do thermop photovoltaics and

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nobody decided to try uh adding sodium when this is known like this is demonstrated

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in high school physics class you know just just flame tests um and and and these

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are the most efficient lights in the world.

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These highress sodium lights are the most efficient um lights in the world.

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Uh let me just let me just move back here to where we at.

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Um yeah. So so this is a a one-dimensional uh simulation uh of how much uh

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energy gets out into each wavelength. So as you in you see it as you increase

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the amount of um this is in WM. If if you tell your AI to use

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WM everything gets incredibly fast. Uh okay.

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So as you increase this you get more and more of this um self-traed line and

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then you get uh more and more energy coming out in this um 819 this near

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uh near infant. Yes. Sorry. Sorry. All right.

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So this is this is the amount of pressure of the primary sodium and you can

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have a a secondary sodium that that that basically um traps it like it like an

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annulus of of of additional resonant material that's just trying to trap it.

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Um and uh this this will be up as well. What what I was trying to

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get to is um there is a code at Lawrence Liverour that does radiative transport and

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the reason you can't have it is because it's used for Hbombs, but I'm not going

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to use it for that. So, I'm making my own.

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Uh uh and and and it's going it's going to go up on our our website

240
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and and and up here and it just isn't uh integrated yet.

241
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Um so uh um another thing to say is that we there's sort of two really

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important questions in terms of the actual physics of how this works.

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One is is the emission actually coupled like a laser or like this so-called super

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radiance. If you click it on or off it well it can change a lot but

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apparently not with these these parameters.

246
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All right. Maybe it's maybe it's off. Hold on.

247
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No, it's not working. Okay. Formally, super radiance would make some difference,

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some degradation. Additionally, um the amount of energy uh and the amount of

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irreversibility that happens when you when you combust something, when you do a

250
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chemical reaction, um as you get to higher and higher temperatures and you drive it

251
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towards a steady state where that temperature is so high that the reaction products

252
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uh also thermodynamically um they thermalize uh and and split apart.

253
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And so the heat itself is keeping things apart.

254
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When things are that hot, the amount of energy that is available um to the system

255
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as you when you when you rack more, it doesn't create any uh entropy.

256
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It it's it's it's reversible. And the um the available bond energy we think is

257
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probably significantly excited beyond what would be the kinetic temperature.

258
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So the kinetic temperature is the temperature of all of the molecules and and atoms

259
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moving around. Um and you calculate calculate that.

260
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But when when a reaction first occurs, the energy is an excited states on the

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molecule and it can excite this uh light emission.

262
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Um, and we think that because of this, we can get much much higher emission

263
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densities than we previously had, which is exciting for the the highly tuned cells

264
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that we have because you can match the yellow much more exactly.

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And it's exciting because it means that there's more amount of energy that's in the

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the yellow light anyway and trapped. And that's what creates the near infrared

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light that matches silicon and gallium arsenide.

268
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Oh well. Uh yeah. So I have been kind of blowing through it.

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Maybe I can uh get some questions from the audience.

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Uh sure. Yes. Yeah, that's pretty much it.

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Sorry. Uh yeah. Uh sorry. Uh um to understand carefully uh it is uh we use

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the energy in heat to excite sodium which produces yellow light which can be

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converted efficiently. So yes. So um you did a transition from uh chemical chemical

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fuel systems to solo point um I wasn't clear on what was perhaps the chemical yeah

275
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it's a good question so the traditional Dyson sphere is you surround it you

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surround the sun but different suns are different colors And actually every

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astrophysical or a whole pile of astrophysical objects that we know actually have a

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corona that is bright in the sodium lines that is you know it's low density but

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it it's bright and the temperature if you measure it is like 10 million degrees.

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The sun is like this. It's not quite 10 million degrees in in the optical uh

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for Earth, but it is like that. The because stars are different colors, your

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optimization is going to be different for each different astrophysical option.

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Um blue, red giant star, but you can convert the energy using a kind of uh

284
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secondary. So one can imagine for the sun that you actually don't exactly know best

285
00:24:34,840 --> 00:24:41,360
way to do this but get more sodium into the um layers of the sun and

286
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it will emit uh it will emit light in that band.

287
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But probably for for for the sun it doesn't make a huge amount of sense to

288
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like engineer the whole thing to be emitting specifically at the extreme end when

289
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you have a small star you can add um or or or or like the sagittarius

290
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like if you have an accretion disc or something if you have sodium in the accretion

291
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disc when it's a moderate temperature it will emit incredibly brightly in the

292
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yellow um and then you can absorb Yes. Yeah.

293
00:25:16,940 --> 00:25:22,740
So, could you like have two layers? One which is just a block like a ghost

294
00:25:22,740 --> 00:25:27,220
block sodium that reriate or that would that be less activated?

295
00:25:27,220 --> 00:25:32,040
It it could be. There's there's long been ideas of like a they call it a

296
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mattressa Dyson sphere where you have multiple layers and the one of them radiates

297
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out and you you cover the other. But if it depending on where you put the

298
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atoms, you can pump more of the energy and use it and then recycle the rest.

299
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So if you had a cavity that was like a very good mirror um and then

300
00:25:54,960 --> 00:25:59,800
uh you you pick out only this uh part of the spectrum, then then that that's

301
00:25:59,800 --> 00:26:03,040
a way to do what we're doing. But astrophysically it's difficult.

302
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I mean mo most of the time when you're doing a Dyson sphere, you really are

303
00:26:06,640 --> 00:26:09,840
going to want to have a a swarm. you're not going to have a complete cavity.

304
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The energy is going to go back into the sun.

305
00:26:12,400 --> 00:26:17,920
But it is, but if you have a partial cavity and you like let light out

306
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or let exhaust products out in one direction, uh you can do all sorts of things

307
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including like like I said, scooting around the local neighborhood.

308
00:26:24,640 --> 00:26:43,560
take the first lickable right so um we're trying to make over the next couple of

309
00:26:43,560 --> 00:26:48,400
years both smallcale devices that are your general purpose utility provides power

310
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heat light water just condenses the chemically created water um at small scale and

311
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we think that this will be you know a general purpose sidearm everyone's going to

312
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want Um at large scale there's a huge demand for data center power and so we

313
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are trying to find hundreds of megawws or gigawatts of basically natural gas um and

314
00:27:15,800 --> 00:27:21,180
also at a place where you can generate a lot of hydrogen from excess solar and

315
00:27:21,180 --> 00:27:26,160
so you can you can switch between natural gas and hydrogen and hopefully mostly

316
00:27:26,160 --> 00:27:32,140
hydrogen um at at that much larger scale as we increase the amount of empirical

317
00:27:32,140 --> 00:27:38,380
data behind if you scale this can you get higher and higher efficiencies out with

318
00:27:38,560 --> 00:27:44,880
uh silicon cells with silicon cells and uh that could happen pretty fast but you

319
00:27:44,880 --> 00:27:52,400
know maybe two years from go when there's a whole pile of money um and then

320
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I think and people kept asking me hey Danielle why is Elon talking about a mass

321
00:27:58,100 --> 00:28:02,220
driver on the moon this is why I don't know when He's intending to do that,

322
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but it could happen quite quickly. Uh, Blue Origin has actually made solar cells

323
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from lunar regalith, and you know, you don't even need to throw it very fast to

324
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get into lunar orbit, although you need to do a little correction.

325
00:28:16,000 --> 00:28:26,800
Uh, Matt, so power generation generate way over 50.

326
00:28:28,220 --> 00:28:37,400
How does how does this stack up against the boats at its circuit recover?

327
00:28:37,940 --> 00:28:45,140
Yeah. So, we think that we can fairly beat what's called a simple cycle gas

328
00:28:45,140 --> 00:28:48,000
turbine, which is sort of 30% efficiency.

329
00:28:48,280 --> 00:28:53,920
So we think 30% plus, but we think that if you if you optimize everything, you

330
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can probably get to 60% or so what when everything is working in your favor.

331
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And you can also do what's called a combined cycle plant, which combines it with

332
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spinning things and boiling water. You know, maybe boiling boiling alcohol off of

333
00:29:11,760 --> 00:29:14,120
the back of the solar cells will will generate power.

334
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And uh you need you need a certain amount of air flowing through.

335
00:29:19,080 --> 00:29:21,460
So you can imagine a having a turbine on the on the back end.

336
00:29:21,660 --> 00:29:28,440
And so this is how the highest efficiency fuel um systems h uh have achieved uh

337
00:29:29,500 --> 00:29:33,240
a combined cycle and a steam plant over 60% efficiency.

338
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We think we can get over 70%. long term.

339
00:29:43,900 --> 00:29:48,780
Uh, good question. So, uh, well, um, at least ours.

340
00:29:49,120 --> 00:29:57,340
Um, so, so it's a very good this is one of the most costic environments imaginable,

341
00:29:57,440 --> 00:30:01,480
right? You have sodium chloride, which is also and extremely high temperatures.

342
00:30:01,480 --> 00:30:06,140
How are we hundreds of temperatures higher than you know MIT National Labs all

343
00:30:06,140 --> 00:30:08,220
that? The main thing is we're using ceramic.

344
00:30:08,740 --> 00:30:17,340
So um chemically aluminina uh aluminum aluminum 2 oxygen 3 is really difficult to

345
00:30:17,340 --> 00:30:21,220
react to anything else. It's such in such a a ground state basically.

346
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Um so it it it tolerates the salt and in fact the salt makes it stronger.

347
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it fills in all the pores and it distributes strain.

348
00:30:31,480 --> 00:30:36,140
Um the second thing is we have to use these.

349
00:30:36,320 --> 00:30:53,880
Um let me show you. Uh so not this. Okay.

350
00:30:54,240 --> 00:31:11,880
So sorry. Um so this shape um these kind of corugations solves the critical

351
00:31:11,880 --> 00:31:17,700
structural problem. So uh even though the thermal expansion coefficient of the

352
00:31:17,700 --> 00:31:23,780
ceramic isn't very high compared with steel, it's maybe one/ird, it's much much

353
00:31:23,780 --> 00:31:26,940
harder. It's actually like nine on the MO scale.

354
00:31:27,180 --> 00:31:30,720
It's like within a factor of four of diamond.

355
00:31:31,360 --> 00:31:35,640
So on one hand, the thermal stresses will become really great if everything holds

356
00:31:35,640 --> 00:31:39,960
together. But on the other hand, if you have a just a little bit of strain

357
00:31:39,960 --> 00:31:42,780
relief, then you can dissipate almost all that stress.

358
00:31:42,780 --> 00:31:44,080
So it's like the inverse of the problem.

359
00:31:44,280 --> 00:31:47,860
So the key is you have to make it curved in all of the different dimensions.

360
00:31:47,980 --> 00:31:52,340
And there's a mathematical shape called a triply periodic minimal surface.

361
00:31:52,420 --> 00:31:58,800
This one here is called a Schwarz diamond that divides the space into two different

362
00:31:58,800 --> 00:32:02,420
volumes. And so that's the perfect sort of building block for a heat exchanger, but

363
00:32:02,420 --> 00:32:04,780
also for all of the structure. So that's what we do.

364
00:32:05,100 --> 00:32:09,820
And it's similar to how, you know, how does a gas turbine or how does a

365
00:32:09,820 --> 00:32:17,040
a rocket nozzle survive even though the gas inside is much much much hotter than um

366
00:32:18,400 --> 00:32:22,660
the melting point even. Uh it it's you do regenerative cooling.

367
00:32:22,860 --> 00:32:25,820
So the amount of air that's coming in equals the amount of air that's going out,

368
00:32:26,080 --> 00:32:29,500
you know, plus the fuel. So it's it's cooling on the way in plus radiator.

369
00:32:32,360 --> 00:32:36,520
Yes. Yes. It's both. And you need both, but you can you you there's a fair

370
00:32:36,520 --> 00:32:42,980
amount of variation you can have. Yeah. Uh is there a nuclear reactor design that

371
00:32:42,980 --> 00:32:46,020
sodium in this? I am I I love this question.

372
00:32:46,020 --> 00:32:50,280
So many uh many nuclear reactors already use sodium as heat pipes.

373
00:32:50,580 --> 00:32:52,400
Um but it's a relatively lower temperature.

374
00:32:52,600 --> 00:32:57,120
It gets to vaporized um at about you know 600°.

375
00:32:58,180 --> 00:33:04,440
Um but many people have asked me hey is there any way to do this with

376
00:33:04,440 --> 00:33:06,520
nuclear? And there is there's a bunch of interesting ones.

377
00:33:06,700 --> 00:33:12,560
Um the main thing is it because it's heat that is is being recycled uh and

378
00:33:12,560 --> 00:33:16,880
it gets very bright that way then then you can use this this technique to both

379
00:33:16,880 --> 00:33:20,840
spectrally shape and also make sure that everything inside a chamber is about the

380
00:33:20,840 --> 00:33:26,760
same temperature. Same way that um heat pipes do except instead of heat pipes going

381
00:33:26,760 --> 00:33:30,740
out to another heat engine it's light going out a window.

382
00:33:31,260 --> 00:33:34,560
Now the thing is you have to redesign your nuclear reactor completely.

383
00:33:34,560 --> 00:33:41,360
I mean this works nonlinearly. Many people know that as the temperature increases

384
00:33:41,520 --> 00:33:44,660
the power increases as T 4th for black bodies.

385
00:33:44,800 --> 00:33:47,120
Well, it's even faster here. It's even faster.

386
00:33:47,240 --> 00:33:51,320
It's almost to the 10th power um at at these regimes.

387
00:33:51,520 --> 00:33:55,780
So what you would need is a nuclear fuel that is a ceramic that can tolerate

388
00:33:55,780 --> 00:33:59,380
the sodium, tolerate the salt uh and can tolerate the high temperature.

389
00:34:00,340 --> 00:34:06,840
So there is such a thing and actually the very best uh refractory oxides in the

390
00:34:06,840 --> 00:34:14,820
universe are is thorium oxide which is in addition to being a great nuclear fuel

391
00:34:15,040 --> 00:34:23,700
because it is it is breathable. Uh um the the uh it it you'll burn the

392
00:34:23,800 --> 00:34:29,400
the uranium in place. First it captures the neutron, becomes uranium, and then it

393
00:34:29,400 --> 00:34:33,080
burns the uranium. So when both of those things happen, you can solve

394
00:34:33,080 --> 00:34:37,880
proliferation. I I think although you know there's still some other edge cases like

395
00:34:37,880 --> 00:34:40,600
if you're if you have a neutron fluence, you can do you can do stuff with

396
00:34:40,600 --> 00:34:46,100
that. But um you can design a system that is an amplifier.

397
00:34:46,100 --> 00:34:49,960
This is my favorite where you you start with a seed fusion.

398
00:34:50,140 --> 00:34:54,660
The fusion doesn't generate much power uh versus how much you put out, but it does

399
00:34:54,660 --> 00:34:59,760
generate neutrons. the neutrons multiply in the nuke and you get about 16 times the

400
00:34:59,760 --> 00:35:08,220
energy out per fision and you get one over uh one minus k for multiplication.

401
00:35:08,220 --> 00:35:13,100
So you can get like 2,000 times as much energy out uh per per fusion which

402
00:35:13,100 --> 00:35:16,740
means that you can run fusion at much much lower than Q.

403
00:35:17,020 --> 00:35:18,740
Uh and so you can have a tiny little thing.

404
00:35:19,000 --> 00:35:23,840
You can imagine, you know, having a completely nuclearpowered propulsion system

405
00:35:23,840 --> 00:35:26,920
that you never need to refuel basically.

406
00:35:27,940 --> 00:35:36,400
And that's very interesting. Yeah. Um, let's say I'm a killer and I need a lot

407
00:35:38,760 --> 00:35:57,500
through like what? Uh, yeah. So, um, we think that we'll be able to get in

408
00:35:57,500 --> 00:36:02,440
a modular system about 10 megawatts, maybe more in a shipping container.

409
00:36:03,080 --> 00:36:07,720
Uh, I we might need to be more competitive than this because boom supersonic is

410
00:36:07,720 --> 00:36:12,000
saying 42 megawatts, although no one has ever demonstrated that within a factor

411
00:36:12,200 --> 00:36:18,660
within an order of magnitude. we but um those could just be stacked up at the

412
00:36:18,660 --> 00:36:23,240
larger scale where you're doing kind of a monolithic thing like the super heavy

413
00:36:23,240 --> 00:36:32,260
going into a salt bowl surrounded by a tower of uh like an giant cathedral tower

414
00:36:32,260 --> 00:36:39,040
of uh silicon cells where they're designed to handle not just one sun of intensity

415
00:36:39,200 --> 00:36:44,960
but maybe up to 20 suns of intensity. Um, it's like pretty big skyscraper type

416
00:36:44,960 --> 00:36:54,140
thing, but a single installation could equal the amount of electricity uh capacity

417
00:36:54,140 --> 00:36:57,980
added to to the electrical grid in the United States in in one installation.

418
00:36:57,980 --> 00:37:00,780
So, but it, you know, it's still a mega structure.

419
00:37:00,780 --> 00:37:05,960
It's like hundreds of meters tall, like been very large and very bright.

420
00:37:06,500 --> 00:37:09,260
Um, but you know, it's not like we haven't built those.

421
00:37:09,360 --> 00:37:14,700
I mean, literally the Starship Super Heavy 330 gawatt of fuel rate.

422
00:37:14,700 --> 00:37:18,860
And so we could probably convert, you know, a third of that up to a half

423
00:37:19,020 --> 00:37:32,120
that. Well, because it's so super linear, you Yeah, I mean, you can you can you

424
00:37:32,120 --> 00:37:36,780
can see it. Oh. Uh, what uh what temperature is necessary to see the night yellow

425
00:37:36,780 --> 00:37:41,380
light? So you can see it if you've got salt around on just like any open

426
00:37:41,380 --> 00:37:43,260
flame like natural gas flame or whatever.

427
00:37:43,300 --> 00:37:47,820
You can already see it. Um I've seen but it's super linear.

428
00:37:48,280 --> 00:37:50,780
It's like really really really to a high degree.

429
00:37:51,000 --> 00:37:55,640
Uh and so as you increase the temperatures so so for us the design point is

430
00:37:55,640 --> 00:38:00,340
you want the the flame plasma to be at least at the boiling temperature of salt

431
00:38:00,520 --> 00:38:07,480
which is 1400° C. And then I ideally you actually drive it so that the the

432
00:38:07,580 --> 00:38:10,880
the chemical reaction is held near 3,000° C.

433
00:38:11,100 --> 00:38:16,020
Uh yeah. Um with preheated air or oxygen and fuel.

434
00:38:16,680 --> 00:38:27,420
Yes. It's a good question. Um we should talk after uh there are a lot of

435
00:38:27,420 --> 00:38:30,140
things that you definitely want in a nuclear reactor.

436
00:38:30,460 --> 00:38:36,560
One is passive stability. So um not liquid but actually super critical.

437
00:38:36,840 --> 00:38:43,520
So if you have a moderator that is dutyium oxide and sodium chloride and super

438
00:38:43,520 --> 00:38:52,900
critical that works great. Uh we can talk about when you scale up uh IPS hall

439
00:38:53,000 --> 00:38:58,920
it will bench all the so does much bigger column or you more and more yeah

440
00:38:59,080 --> 00:39:04,080
I mean at some point it's it's the practical fabrication limit that's the that's

441
00:39:04,080 --> 00:39:08,180
the limit at the time. Uh one scale I like to think about is you know

442
00:39:08,260 --> 00:39:11,560
those backyard we've got I think there's a bunch of backyard heaters with a quartz

443
00:39:11,560 --> 00:39:14,060
tube. Those quartz tubes are mass-produced.

444
00:39:14,540 --> 00:39:15,900
They're so cheap. They're like 40 bucks.

445
00:39:15,900 --> 00:39:20,520
One of those things could probably handle about 100 kilowatts.

446
00:39:20,520 --> 00:39:25,320
So that is sort of the modular scale size where if you have a hundred of

447
00:39:25,320 --> 00:39:32,080
those, you know, 10 x 10 in a shipping container, that's 10 megawatts and that's uh

448
00:39:33,140 --> 00:39:38,900
pretty interesting. Um as you get larger and larger, you have to start doing

449
00:39:38,900 --> 00:39:43,080
construction that is tile based. This is the same thing with uh fusion reactors.

450
00:39:44,560 --> 00:39:46,220
See, you have to do something different.

451
00:39:46,420 --> 00:39:50,580
And instead of using a glass containment, you'll actually use the air itself.

452
00:39:51,660 --> 00:40:01,780
If you have um I mean you you you instead of having the wall be right

453
00:40:01,780 --> 00:40:06,900
up against this extremely high temperature thing, we have like a swirling column of

454
00:40:06,900 --> 00:40:11,120
air in inside the inside the tube. And that keeps it off of of the wall

455
00:40:11,120 --> 00:40:12,860
because it's it's heavier because it's colder.

456
00:40:13,380 --> 00:40:17,020
Um, so but you still need to get the energy out somehow.

457
00:40:17,020 --> 00:40:22,320
So there's there's there's got to be um so we're probably it's probably not ideal

458
00:40:22,320 --> 00:40:24,780
to do an an open system. You probably want a cavity.

459
00:40:24,780 --> 00:40:30,680
And we've experimented with basically quartz, which is great, but eventually gets

460
00:40:30,680 --> 00:40:36,760
corroded by the salt. Um sapphire, which is great, but but it can crack and you're

461
00:40:36,760 --> 00:40:44,220
terrified about it because it can build up strength uh stress and um amorphous

462
00:40:44,220 --> 00:40:51,020
aluminina which is which is pressed together in something called uh hipping uh uh

463
00:40:51,300 --> 00:40:56,080
which makes all the grains stick together and it makes it translucent but we don't

464
00:40:56,080 --> 00:40:58,540
use that as much for experiment because we can't see through the thing.

465
00:40:58,540 --> 00:41:03,040
So but that's what everybody uses for high pressure sodium lamps which have like

466
00:41:03,040 --> 00:41:07,100
75% radiative efficiency although not all of it is in light that you can see.

467
00:41:07,220 --> 00:41:14,380
Oh. Uh, looks like we're we got room for one more question.

468
00:41:14,620 --> 00:41:17,240
Uh, I think you you were going to ask something.

469
00:41:17,240 --> 00:41:34,300
No, nobody else. All right. Yes. Haha. Uh, you need you need special juice.

470
00:41:34,840 --> 00:41:41,460
Um, one thing is that we kind of call it, you know, fundraising by stunts.

471
00:41:41,600 --> 00:41:46,060
You know, we do all these kind of engineering things and we whatever scientific

472
00:41:46,060 --> 00:41:50,120
information we can gather, but also we try to show as many people as possible with

473
00:41:50,120 --> 00:41:54,180
their own eyes. I didn't bring it this this year, but last year we had a

474
00:41:54,180 --> 00:41:57,800
big uh light cell um operating in one of the gardens.

475
00:41:57,800 --> 00:42:01,680
It lit up the whole thing. Um, so that's one thing.

476
00:42:01,680 --> 00:42:06,260
I I had previously raised a bunch of money for my previous company, Light Sale

477
00:42:06,260 --> 00:42:08,400
Energy, which was compressed air energy storage.

478
00:42:09,140 --> 00:42:12,420
And so I had some reputation from that. So that made it easier.

479
00:42:12,860 --> 00:42:16,120
It didn't make it easy. And uh and we're still fundraising.

480
00:42:16,400 --> 00:42:21,880
So, you know, um it would probably be easier if I used all the AI stuff

481
00:42:21,880 --> 00:42:24,180
that I'm doing and be like, we're we're just an AI company.

482
00:42:24,180 --> 00:42:30,680
However, I insist that since it's energy to AI and this is the relevant durable

483
00:42:30,680 --> 00:42:37,320
constraint and that we're using the AI to understand you how to actually enact our

484
00:42:37,320 --> 00:42:41,960
our company h how how to build everything and it's a huge intuition pump for like

485
00:42:41,960 --> 00:42:47,200
pushing the AI to the limits and we're sitting in San Francisco that these things

486
00:42:47,200 --> 00:43:00,760
reinforce each other. Uh, and so that's how we keep raising money.

