Helion's approach uses a field-reversed configuration (FRC), where the plasma generates its own magnetic field and traps itself, rather than being trapped by external magnets like in a tokamak or stellarator.

(00:00:00) The following is a conversation with David Kirtley, a nuclear engineer, expert on nuclear fusion, and the CEO of Helion Energy, a company working on building nuclear fusion reactors and have made incredible progress in a short period of time that make it seem possible like we could actually get there as a civilization. (00:00:21) This is exciting because nuclear fusion, if achieved commercially, would solve most of our energy needs in a clean, safe way, providing virtually unlimited clean electricity. (00:00:33) The problem is that fusion is incredibly difficult to achieve. (00:00:36) You need to heat hydrogen to over 100 million degrees Celsius and contain it long enough for atoms to fuse. (00:00:44) That's why the joke in the past has been that fusion is 30 years away and always will be. (00:00:51) Just in case you're not familiar, let me clarify the difference between nuclear fusion and nuclear fission. (00:00:58) By the way, I believe according to the excellent sample size subreddit post by PM Goodbeer on this, the preferred pronunciation of the latter in US is nuclear fission, like vision, and in the UK and other countries is nuclear fission, like mission. (00:01:19) I prefer the nuclear fission pronunciation because America. (00:01:26) So today's nuclear power plants use nuclear fission. (00:01:30) They split apart heavy uranium atoms to release energy. (00:01:34) Fusion does the opposite. (00:01:36) It combines light hydrogen atoms together, the same reaction that powers the sun and the stars. (00:01:42) The result is that it's clean fuel from water, no long-lived radioactive waste, inherently safe because a fusion reactor can't melt down. (00:01:51) If something goes wrong, the reactor simply stops, and there's no carbon emissions. (00:01:57) On a more technical side, helene uses a different approach to fusion than has traditionally been done. (00:02:04) Most fusion efforts have used tokamaks, which are these giant donut-shaped magnetic containment chambers. (00:02:10) Helion uses pulsed magneto-inertial fusion. (00:02:13) David gets into the super-technical physics and engineering details in this episode, which was fun and fascinating. (00:02:22) I think it's important to remember that for all of human history, we have been limited by energy scarcity. (00:02:29) And every major leap in civilization, agriculture, industrialization, the information age, came in part from unlocking new energy sources. (00:02:39) If someone is able to solve commercial fusion, we would enter a new era of energy abundance that fundamentally changes what's possible for us humans. (00:02:51) I'm excited for the future and I'm excited for Super Technical Physics podcast episodes. (00:03:01) And now a quick few second mention of each sponsor. (00:03:03) Check them out in the description or at lexfriedman.com/sponsors. (00:03:07) It is the best way to support this podcast. (00:03:10) We got Uplift Desk for my favorite office desk that I'm behind right now, Finn for customer service AI agents, Miro for brainstorming ideas with your team, Element for electrolytes, BetterHelp for mental health, and Shopify for selling stuff online. (00:03:26) Choose wisely, my friends. (00:03:28) And now on to the full ad rates. (00:03:30) I try to make them interesting, but if you skip, please still check out the sponsors. (00:03:33) I enjoy their stuff. (00:03:34) Maybe you will too. (00:03:35) To get in touch with me for whatever reason, go to lexfreeman.com slash contact. (00:03:40) All right, let's go. (00:03:42) This episode is brought to you by Uplift Desk, my go-to for all office and podcast studio furniture. (00:03:50) If you go back across many years, many wonderful conversations, man, just even (00:03:57) accessing my memory for some of those conversations, I feel truly, truly lucky to get to do what I do, to get to be alive, to get to know so many incredible people, to get a chance to sit down with them. (00:04:11) Behind, by the way, a desk I love. (00:04:13) And I remember when I first came to Austin, I got this crappy folding tape, and I think I recorded a couple conversations. (00:04:21) I feel like I know I didn't have anything in that space. (00:04:26) And I don't think I yet got the Uplift desks in. (00:04:30) And I remember feeling like this just doesn't feel right. (00:04:32) And when I pretty quickly got the Uplift desks in, everything just locked into place just like it was before. (00:04:39) And then of course I got the desk for the computer and then for the robotics work I'm doing. (00:04:43) It's just Uplift desks everywhere. (00:04:46) You should go support them. (00:04:48) They're amazing. (00:04:48) I love them very much. (00:04:50) Go to upliftdesk.com slash Lex and use code Lex to get 4 free accessories. (00:04:55) free same-day shipping, free returns, a 15-year warranty, and an extra discount off your entire order. (00:05:01) That's UPLIFTDESK.com slash flex. (00:05:08) This episode is also brought to you by Finn, the number one AI agent for customer service. (00:05:14) This is the era of AI agents trying to find their niche and dominate. (00:05:19) This is the way you create a successful company. (00:05:22) It's not just waving hands and (00:05:24) saying AI agents are going to change everything. (00:05:27) You figure out problems that people have and create a system that solves those problems. (00:05:32) And FIN does that for customer service. (00:05:35) It has a 65% average resolution rate. (00:05:38) It's trusted by over 5,000 customer service leaders and top AI companies, including Anthropic. (00:05:44) FIN is powered by FIN AI Engine. (00:05:47) which is a continuously improving system that easily allows you to analyze, train, test, and deploy over and over, repeat that cycle as the system gets smarter and smarter and smarter and smarter. (00:05:56) That's kind of the thing that you need to have a system that operates in the real world. (00:06:02) It's built to handle complex multi-step queries like returns, exchanges, disputes, delivering high quality personalized answers just like your best human agent. (00:06:11) Go to fin.ai/lex to learn more about transforming your customer service and scaling your support team. (00:06:18) That's fin.ai/lex. (00:06:21) This episode is also brought to you by Miro, an online collaborative platform that enables teams to brainstorm, prototype, and iterate fast on their ideas. (00:06:32) It converts sticky notes, screenshots, all those kinds of things into actual diagrams and prototypes in minutes. (00:06:40) I spent the last several weeks back in the lab having intense, fascinating, epic conversations with graduate students, with researchers about ideas and machine learning and robotics, philosophy, all of it. (00:06:58) Some of the discussions were just behind the table together, maybe with a sheet of paper, but really those are inefficient because (00:07:04) You have a bunch of ideas that are flying around the place and they're not really archived to be built on in future meetings. (00:07:13) So it's really nice to have tooling that captures those ideas and allows us to then go back to our offices and sort of think over the things discussed and build on it and build on that across days, across weeks. (00:07:26) For that, Miro's excellent. (00:07:28) Help your teams develop great ideas into results with Miro. (00:07:32) Go to mirror.com to find out how, that's M-I-R-O.com. (00:07:38) This episode is also brought to you by Element, my daily zero sugar and delicious electrolyte mix that I'm drinking currently, that I'm drinking every single day, that I'm drinking a bunch of when I travel, that's the thing I bring with me to make me feel like a little bit of homeless with me. (00:07:55) I'm thinking of doing some insane travel coming up in the new year. (00:08:01) across places with just a backpack. (00:08:04) And there I'll have to decide if I want to bring some element, because really what you need is water and electrolytes. (00:08:12) But of course, you're extremely limited by the number of things you can bring with you when it's just a backpack. (00:08:18) But anyway, it is good for me physically, it is good for me mentally, but it is also just good spiritually in terms of it's a thing that gives me this foundation (00:08:29) of habit and making me feel like I have my shit together, especially when I'm doing crazy stuff physically. (00:08:36) Anyway, get a free ACON sample pack with any purchase. (00:08:39) Try it at drinkelement.com/lex. (00:08:43) This episode is also brought to you by Better Help, spelled H-E-L-P Help. (00:08:49) They figure out what you need and match you with a licensed therapist in under 48 hours. (00:08:55) Over 350 million messages in chat and phone and video sessions. (00:09:02) Over 34,000 licensed therapists. (00:09:04) Over 4.4 million people got help. (00:09:08) That's because the thing is easy, discreet, affordable, available everywhere. (00:09:15) It's a great first step into trying therapy, whether it's just therapy for you or... (00:09:23) Therapy for two, I apologize for rhyming that. (00:09:27) Couples therapy. (00:09:29) I think sometimes with these kinds of things, the hardest step is the first step to take. (00:09:34) So BetterHelp makes it easier to take the first step. (00:09:37) Check them out at betterhelp.com/lex and save in your first month. (00:09:40) That's betterhelp.com/lex. (00:09:44) And last but not least, our old friend Shopify. (00:09:49) A platform designed for anyone to sell anywhere with a great looking online store. (00:09:55) You could probably tell that I'm a little bit happy. (00:09:57) I'm not sure what kind of trajectory this is going to lead or how this work will materialize, but it's good to be putting in significant hours every single day on math, on programming, on being in contact with robots, robots all around me, and exploring different cutting edge ideas. (00:10:17) It's an exciting time for machine learning. (00:10:18) It's an exciting time for programming. (00:10:21) That excitement, by the way, is captured masterfully by the great, the powerful DHH, who I believe is on the board of Shopify, or at the very least is the ambassador of the technology stack that Shopify utilizes in order to deliver incredible services at scale, low latency. (00:10:42) It works. (00:10:43) It's stable. (00:10:44) huge number of transactions, just the insanity of what they have to pull off to know that underpinning it is beautiful code is wonderful to learn. (00:10:54) Anyway, sign up for a $1 per month trial period at shopify.com slash Lux. (00:10:59) That's all lowercase. (00:11:00) Go to shopify.com slash Lux to take your business to the next level today. (00:11:05) This is the Lex Friedman Podcast. (00:11:07) To support it, please check out our sponsors in the description, where you can also find links to contact me, ask questions, give feedback, and so on. (00:11:16) And now, dear friends, here's David Kirtley. (00:11:36) Let's start with a big picture. (00:11:38) What is nuclear fusion and maybe what is nuclear fission? (00:11:42) Let's lay out the basics. (00:11:44) So fusion is what powers the universe. (00:11:46) Fusion is what happens in stars and it's where the vast amount of energy that even that we use today here on Earth comes from the process of fusion. (00:11:57) It also is what powers plants, and those plants become oil, and those become fossil fuels that then powers the rest of human civilization for the last 100 years. (00:12:08) And so fusion really underpins a lot of what has enabled us as humans to go forward. (00:12:17) However, ironically, we don't do it actively here on Earth to make electricity yet. (00:12:23) And so fundamentally what fusion is, taking the most common elements in the universe, hydrogen and lightweight isotopes of hydrogen and helium, and fusing those together to make heavier elements. (00:12:35) In that process, as you combine atomic nuclei and form heavier nuclei, those nuclei are slightly lighter than the sum of the parts. (00:12:45) And that comes from a lot of the details of quantum mechanics and how those fundamental particles combine and interact. (00:12:52) We also talk about the strong nuclear force that holds the atomic nucleuses together as one of the fundamental forces involved in fusion. (00:13:00) But that mass defect, (00:13:03) E equals MC squared, we know from Einstein, is also energy. (00:13:07) And so in that process, a tremendous amount of energy is released. (00:13:11) And the actual reactions, I think, is a lot more interesting than simply, it's a little bit lighter, and therefore energy is released. (00:13:16) But that's the fundamental process in fusion, is you're bringing those lightweight atomic nuclei, those isotopes together. (00:13:24) Fission is the exact opposite, where you're taking the heaviest elements in the universe, uranium, plutonium, things that are so heavy and have so (00:13:33) many internal protons and neutrons and electrons that they're barely held together at all. (00:13:38) They're fundamentally unstable or radioactive. (00:13:41) And those elements are very close to falling apart. (00:13:45) And as they do that, if you take a uranium-235 or a plutonium-239 nucleus and you add something new, usually it's a neutron, a subatomic particle that's uncharged, that unstable, that very large nuclei will then break into pieces, many pieces, a whole spectrum of pieces. (00:14:01) But if you add up all of those pieces, they also have slightly less mass than the initial one did, the initial uranium or plutonium. (00:14:09) And in that process, again, E equals MC squared, a tremendous amount of energy is released. (00:14:15) There's a very famous curve in atomic physics, fusion or fission, looking at the periodic table, going from the lightest elements, hydrogen, to the heaviest elements, those uranium, plutonium, and others. (00:14:26) And fusion happens up to iron. (00:14:29) Iron is the magical point in between where lighter elements than iron fuse together and heavier elements (00:14:37) fizz or our fizzile and break apart and release energy. (00:14:41) I think about and I look at that process in stars, and that our star is fundamentally an early stage star that's burning just hydrogens. (00:14:52) But when it burns and does fusion, those hydrogens combine into heliums. (00:14:56) And later stage starts can then burn those heliums. (00:15:00) And they can fuse those together to form even heavier elements and carbons. (00:15:03) And those carbons can fuse together and form heavier elements. (00:15:07) And that whole stellar process is something that inspires us at Helion to think about what are fusion fuels, not just the simplest ones, but more advanced fusion fuels that we see in stars throughout the universe. (00:15:20) Okay, so there's a million things I want to say. (00:15:22) So first, maybe zooming out to the biggest possible picture. (00:15:25) If you look across hundreds of millions, billions of years, and all the, my opinion, alien civilizations that are out there, (00:15:33) they're going to be powered likely by fusion. (00:15:36) So our advanced intelligent civilization is powered by fusion in that the sun is our power plant. (00:15:44) Then the other thing is the physics. (00:15:46) Again, very basic, but you said E equals MC squared a couple times. (00:15:50) Can you explain this equation? (00:15:52) E equals MC squared is a fundamental relationship that a patent clerk, Einstein, discovered and unlocked an entire new realm (00:16:02) of physics and engineering and has shown us atomic physics, what happens inside the nucleus, and unlocked our understanding of the universe and paved the way for many of the physics advancements that came after that we think about mass as these particles. (00:16:19) But in reality, also at the same time, their energy. (00:16:23) And there's a direct quantitative relationship between how much energy is in all of that mass. (00:16:28) And in fact, all of the energy that is released (00:16:32) even by atomic physics, certainly in atomic reactions, is equals MC squared. (00:16:37) And that I think most people have heard of and are used to. (00:16:40) But also in chemistry and in chemical bonds, that in those chemical bonds, there is a change in mass. (00:16:46) When you take a hydrogen and an oxygen and you burn them and you combine them into water, there's a change in mass. (00:16:53) Now, that change per atom and per molecule is actually so small that it's extremely hard to measure. (00:17:00) But it's still there. (00:17:01) And that's the energy that is released. (00:17:03) And you can quantify that. (00:17:04) We use units of electron volts as a unit of what is the energy in atomic processes or chemical processes. (00:17:14) Can you also just speak to the different fuels that you mentioned, both on the fusion and the fission side? (00:17:20) So uranium, plutonium for the fission, and then hydrogen isotopes for the fusion. (00:17:26) So for fission, uranium and plutonium, we (00:17:29) don't make those nuclei. (00:17:32) Those right now for humanity, those have been made in the primordial universe through supernova and big bang and the initial formation of the universe where matter was created. (00:17:43) And so we dig those up. (00:17:45) We dig up uranium, plutonium out of the ground. (00:17:47) And in fact, most plutonium we make from uranium. (00:17:50) And we can talk about how to enrich uranium if we want to go down that road. (00:17:55) But that's how we get those (00:17:57) molecules and nuclei. (00:17:59) For fusion materials, hydrogenetic species, or hydrogens, are primordial in the universe. (00:18:05) Also, only the most common things that are in the universe. (00:18:09) The suns and stars are made-up of hydrogens and heliums. (00:18:14) And so the vast majority of atoms in the universe still are hydrogen. (00:18:18) So the basic fuel for fission is already in the ground, and then the basic fuel for fusion is everywhere. (00:18:24) everywhere. (00:18:25) And we particularly use a type of hydrogen called deuterium, which is a heavier isotope of hydrogen. (00:18:33) Hydrogen is typically one proton and one electron, atomic mass of 1. (00:18:37) Deuterium is an atomic mass of 2, which is a proton, which is a charged particle, and it has a neutron. (00:18:42) in its nucleus, which is an uncharged particle. (00:18:45) And so that's deuterium as the fuel. (00:18:47) Now, deuterium is also found in all water on Earth, in the water I'm drinking right now. (00:18:52) It's in my body. (00:18:52) It's in Coca-Cola. (00:18:54) It's everywhere. (00:18:58) And safe and clean and one of those fundamental particles that was born in the cosmos. (00:19:04) And we estimate that in seawater here on Earth, we have, if we powered at our current use of electricity, (00:19:12) all of humanity on fusion, somewhere between 100 million years and a billion years of fuel in hydrogen and deuterium here on Earth. (00:19:21) And how is that stored mostly? (00:19:23) And mostly that's just in water. (00:19:26) Mostly that it's a mix of, we call this actually heavy water, where you have normal water that you're used to. (00:19:32) We talk about, and you learn in school, is H2O, where there's two hydrogens and oxygen in (00:19:38) a nucleus in the molecule. (00:19:40) And deuterium or heavy water is D2O, 2 deuteriums and an oxygen. (00:19:45) In reality, it's actually an interesting mix where you have some HDO, so a mix of hydrogen and deuterium. (00:19:52) You also have other hydrogenic species. (00:19:54) Tritium is another one where you add a second neutron to that hydrogen and then you can have T2O, tritiated water. (00:20:02) And that's something that comes up and we need to talk about at some point. (00:20:07) And there's other, (00:20:08) As you go up the periodic table, you add 2 protons and you get helium. And so helium, the most common helium, is helium-4, which is 2 protons and two neutrons. And then we use an isotope of helium. The nucleus is called the helion, which is what we base the company after, which is 2 protons and one neutron. It's a light helium molecule. So the number you mentioned in terms of how much fuel is available, basically the takeaway there is it's a nearly endless resource. (00:20:38) in terms of fuel. Is that correct to say? That's correct to say at today's power level. I think what's interesting is the idea that as we deploy the same power source that powers the universe here on Earth as humans, can we do more? Can we have access to much more electricity and much more energy and do really interesting things with that? And still there's large amounts, millions and millions of years of power, even at much higher output power levels for humanity. Yeah, so the moment we start running (00:21:08) out of hydrogen and helium, where that means we're doing some pretty incredible things with our technology. And then that technology is probably going to allow us to propagate out into the universe and then discover other sources. Because you can also get it on other planets, whatever planets of water, and it looks more and more likely like a lot of them do. What an incredible future. Just out into the cosmos, nuclear power planets everywhere. (00:21:35) Yeah. Okay. So to linger on some of the technical stuff, you said strong nuclear force. So how exactly is the energy created? So how does the E equals MC squared, the M go to the E in fusion? (00:21:52) So in fusion, you take these lightweight isotopes like hydrogen and deuterium. And as you combine them and take these molecules and get them closer and closer together, some really interesting fundamental physics happens. So first, these atomic nuclei are charged. They have an electric charge. And they, like charges, repel. And I think everybody is familiar with that, where you take two positive charges and you try to push them together and the electromagnetic force between them repels them. (00:22:22) So you have a force that's actually pushing against them. So in fusion, you work to get your fuel very hot, very, very high temperatures, 100 million degree temperatures. And temperature really is kinetic energy. It's motion, it's velocity. So that these particles are moving so fast that even though they're coming together and there's this repulsive electromagnetic force, they can still come close enough that another force comes into play, which is the strong force. And then once you get within (00:22:49) a very close distance on the order of the scale of those nuclei themselves of those atomic nuclei. So the tiniest thing you could imagine and probably way smaller than that, these particles then are attracted to each other and they combine and they fuse together. At that point, you create heavier atomic nuclei that have a slightly less mass, slightly less total mass in the system. And that mass equals MC squared is energy. (00:23:16) So extremely high temperature, extremely high speed. Maybe that's one of the other differences also with fusion and fission is just the amount of temperature required for the reactions. Is that accurate to say? Yeah, and I think fundamentally it's that in a lot of ways, fusion is hard and fission is easy. Nuclear fission happens at room temperature, that this uranium and plutonium is so likely to break apart already that simply the adding of one of these neutrons, (00:23:46) one extra particle will then break it apart and release energy. And if you have a lot of them together, it will create a chain reaction. Fusion, that doesn't happen at all. Fusion is actually really hard to do. You have to overcome those electromagnetic forces to have a single fusion reaction happen. And so it takes things like in our sun, we have what is called gravitational confinement, where the gravity, literally the mass of the fuel itself is (00:24:13) pulling to the center of the sun and it's pulling in there. So there's a large force that's pulling all that fuel together and holding it and confining it together such that it gets close enough and hot enough for long enough that fusion happens. And then we have to figure out if we're building fusion reactors, we have to figure out how to do that confinement without the huge size gravity of the sun. (00:24:39) That's right. Obviously, the sun is vastly larger than Earth, and so we can't do that same process here on Earth. Yet. No, I'm just kidding. But we have other forces we get to use. We can use the electromagnetic force, which the sun doesn't get to do, to apply those forces. (00:24:56) And I actually want to take a pause right there and point out a word. Historically, we've used the word reactor around fusion, but I don't think that's right. And for me, we're really careful about this terminology. When we look to how that word is defined, and we can look to how the experts define it, doesn't really apply to fusion. So the Nuclear Regulatory Commission, the NRC, (00:25:20) defines reactor as, I have it right here. A nuclear reactor is an apparatus other than an atomic weapon designed or used to sustain nuclear fission in a self-supporting chain reaction. And there's two big parts to that. one, fission reaction, obviously fusion is not that, we've talked about why, but also the self-sustaining part. (00:25:43) in that a reactor is self-sustaining. You take your hands off of it and it keeps going. In fusion, that doesn't happen. And we know, because we have to do it every day and it's really hard to do. And so we actually use the word generator because we don't talk about, for instance, a natural gas reactor, is that if you stop putting in fuel, it turns off. And the same thing happens in fusion. (00:26:05) And so we're pretty careful about making sure we talk about that as a generator where you're putting in fuel, you're getting electricity out. And then when you stop putting in fuel, it just shuts off. And you can go even one step further and say, what am I going to do with this fusion that powers the universe? And what does humanity want out of this? And what we want is electricity. We don't simply want a set of reactions or even heat and energy. That's great, but what I really want is electricity. (00:26:33) And yeah, we'll talk about the technical details of one of the big benefits of the linear design of the approach that you do is you get to electricity directly, as quickly as possible. And some of the other alternatives have a intermediate step. And those, again, are technical details. But let me sort of still linger on the difference between fusion and fission. What are some advantages at a high level of nuclear fusion as a source of energy? Fundamentally, as a source of energy, (00:27:02) in fusion, you're taking these lightweight isotopes, you're bringing them together, you're releasing energy, and that energy is in the form of charged particles. It's already in the form of electricity. Fusion itself has electricity built into it without a lot of the steam or thermal system requirements. And so that's a really nice fundamental benefit of fusion itself. Also, (00:27:26) This reaction that's really hard to do turns itself off. So you end up with that fusion is fundamentally safe. And that's really a key requirement of any industrial system is that it turns itself off and it's safe. You turn the key off on your car, you know it's gonna turn off. I guess the flip side of that, just sort of stating the obvious, but it's nice to lay it out. For nuclear fission, it's a chain reaction, so it's hard to shut off. (00:27:53) and it works by boiling water into steam, which spins turbines and produces electricity. Can you talk through this process in a nuclear fission reactor? In a nuclear fission reactor, you put enough of this fissile material, uranium or plutonium together, such that as these unstable molecules, these unstable atoms crack open and break apart, they release heat, that the component parts of those are actually quite hot. (00:28:23) And so not only are the component parts that the uranium breaks into, and it's a whole spectrum of different atoms and atomic nuclei are hot, but it also releases neutrons. It also releases more of these uncharged particles. (00:28:36) And if you do it right, this fissile material will be next to other fissile material. And so that neutron will then go and bombard another uranium nucleus, again, opening that up and releasing more heat and more of these neutrons. And that's how you have those reactions of a self-supporting chain reaction. And that chain reaction then continues. (00:28:59) People design fission reactors such that you have just the right balance of enough neutrons are made such that the reaction is continuing, but not so many neutrons are made that it speeds up because you don't want it to speed up. And there's some kind of cooling mechanisms also, like that's part of the art. (00:29:16) and the engineering of it. And then the key is at the same time, you want to make sure that the whole thing is in water, is typically the cooling fluid. There's some more advanced fission reactors that have different cooling fluids, but water typically, where then that absorbs that both the heat and those extra neutrons. (00:29:34) And so you use the water and the fluid to then run a steam turbine to do traditional electricity generation and output electricity through your steam turbine. You end up with complicated systems of flowing liquids and flowing water, balancing the heat. A lot of fission reactor design comes from that thermal balance of keeping this reaction going, making sure it doesn't speed up, because that's an uncontrolled chain reaction, which you would not want. (00:30:04) and balancing the cooling and the output of getting the water out of it. So we should say that for reasons you already laid out, maybe you can speak to a bit more, is nuclear fusion is much safer. So there's no chain reaction going on. You can just shut it off. But it should also be said that as far as I understand, the current fission nuclear reactors are also very safe. (00:30:29) I think there's a perception that nuclear fission reactors are unsafe. They're dangerous. And if you just look empirically at the statistics, that the fear is not justified by the actual safety data. Can you just speak to that a little bit? Yeah, we've been talking about the reaction processes themselves, but I think fundamentally, let's take a step back and look a little broader and say, let's look at what we care about, which is the power plant, making electricity. And I look at this from a nuclear engineer's point of view. I spent a lot of years studying these systems. (00:31:00) And modern fission reactors, I believe, are engineered to be safe. They're engineered in ways where as those reactions maybe speed up and those systems get hotter, they actually are built to expand and cool down passively and natively. And there's protection systems in place that modern systems are quite safe from an engineering perspective. (00:31:24) And so I believe that we have figured out how to build nuclear fission reactors in a way where the engineering of the power plant is safe. I would say that I look back at the history of what we've built over time, and the challenge hasn't come to the engineering, actually. I believe the engineers have solved these problems. The problem comes from humans, and the problem comes from (00:31:47) other things around nuclear power. You have to enrich that uranium to put it in a plant, and the plant's safe, but you had to enrich that uranium, and that is some of the problem. Or a plant is designed to run for a certain number of decades safely, but do we run it longer than that? And so those are where I think the real challenges happen, is more with the humans around these systems than the engineering of the power plants themselves. Well, I have to ask then, what do you think happened in Chernobyl? (00:32:14) What lessons do we learn from Chernobyl nuclear disaster and maybe also Three Mile Island and Fukushima accidents? I think you're suggesting that it has to do with the humans a bit. So with Chernobyl and Fukushima, I actually put Three Mile Island in a different category. In fact, some of the recent news in the last year is that we're going to be restarting Three Mile Island. (00:32:35) because there's such a need for clean base load power. So that's actually a very interesting other topic we should talk about is why and how we're doing that. But more than that, going back to the accidents that did happen, in both of those systems, you can point to the human failure rather than the engineering failures of those systems. (00:32:57) that in Fukushima specifically, there were multiple nuclear fission reactors on the same site that successfully kept running through the tsunami, totally successfully, and were only later shut down for more political reasons. But the old one, the oldest of them that had been on site for long periods and maybe too long, I think some experts have looked at this in the past, was where some of the problems actually happened. (00:33:23) And so I look to that less as a failure of the engineering of the power plants and more of the humans and around those systems that if we that we should be operating these plants as designed and then I believe they're safe. (00:33:41) And that gets to some of the atomic weapons questions that I think are the other part around nuclear reactors and fission reactors that are concerning for me. Can you speak to those? So maybe this is a good place to also lay out the difference between nuclear fission power plants and nuclear fission weapons, and maybe also nuclear fusion power plants and nuclear fusion (00:34:11) weapons, like what are the differences here? Fusion power plants can't be used to make nuclear weapons. Fundamentally, that the processes in fusion aren't the same processes that happen in nuclear bombs and nuclear weapons. (00:34:28) And so it's actually one reason I started in fusion, and most of our team thinks about the mission of fusion of delivering clean, safe electricity, is that it also can't be used to make weapons. And I think that's a little bit of a distinction from traditional nuclear fission reactors, is that while I totally believe as a nuclear engineer, we build power plants now that are safe, that aren't going to have reactions, they use a fuel. (00:34:56) uranium and plutonium that can be used to make nuclear weapons. That we know that if you take enough fissile material together, enough uranium and plutonium, put it in a small volume, that it will not just create a reaction, but it will create a supercritical reaction that will then continue and grow and release a tremendous amount of energy all at once. (00:35:18) And that is a bomb. That is a bad situation. And that is what we want to avoid. A lot of the key is recognizing that even though there are things called fusion bombs, the H-bomb, the hydrogen bomb, the hydrogen bomb has uranium in it. It's still a fission bomb. And so how this fundamentally works is that you have a fission reaction, a primary, and that creates radiation that induces a fusion reaction (00:35:45) a small amount of fusion fuel that then boosts that uranium reaction again. And so most of the energy, in fact, 90% of the energy in an H-bomb is all still from the uranium reactions themselves. Yeah, I think people call it sort of the nuclear fusion bomb, hydrogen bomb, but really it's still a nuclear fission bomb. It's just that fusion is a part of the process to make it more powerful, but you still need, like you said, the uranium fuel. So it's not accurate to sort of think of it as a fusion bomb, really. And if you take (00:36:15) away that fissile material, that nuclear fission reaction, the fusion reaction doesn't happen at all. In fact, there's been researchers that have over the decades tried to make an all fusion bomb and been very unsuccessful at it. The physics and the engineering don't support it can ever happen with our understanding today. (00:36:37) The topic we're talking about is more broadly called proliferation. And this is the creation of nuclear weapons in the world and the distribution of those weapons. And something we know as physicists and engineers is that fusion can't be used to make nuclear weapons. We know that. But that is not sort of widely known. (00:36:59) And part of what we went out to do is work with the proliferation experts in the world, the people who work to prevent nuclear weapons from being made. (00:37:08) being created, being shared throughout the world, because the challenges, the geopolitical challenges that happen. And we went to those proliferation experts, and we were worried that they would have the sort of the same historical question of like, well, the word nuclear is in fusion, so therefore it must be related. And in fact, the total opposite happened. What they told us is, please, go develop fusion power plants absolutely as fast as possible. (00:37:36) The world needs this. And the proliferation experts were telling us that otherwise people would start enriching uranium throughout the world. And we'd be building enriched uranium power plants because we need the electricity that's clean and baseload. But in those processes, they'll be making fuel that could be one day used for atomic weapons, for nuclear weapons. And they were worried that the growth of this enriched uranium, think about the centrifuges, (00:38:04) that having a lot more centrifuges happening all over the world would lead to more weapons, at least the possibility of it. And so they are pushing us as fast as possible. Go build fusion generators and get them deployed everywhere. Not just in the United States, but all over the world so that we're building fusion power and that's meeting humanity's needs, not this other thing. And so I was really pleasantly surprised. We've written a number of papers and worked with those communities on this of what does it mean? How is (00:38:34) fusion power safe and can't be used for nuclear weapons. So this might be interesting to ask on the geopolitics side of things. I have the chance to interview a few world leaders coming up. By way of advice, what questions should I ask world leaders to figure out the geopolitics of nuclear, nuclear proliferation, nuclear weapons, nuclear fission, (00:39:00) power plants and nuclear fusion power plants. What's the interesting, intricate complexity there that you could maybe speak to? The question I would want to ask is, what would you do if we could deliver for you low cost, clean, industrial scale, 10s or hundreds of megawatts of fusion power that's low cost, clean, base load and doesn't have (00:39:29) the geopolitical consequences of uranium and plutonium, of fissile material. What would you do there? How would that change your view of the next 30 years? But also there's a lot of geopolitics connected to oil, natural gas, and other sources of energy, which I think are important in Saudi Arabia, in the Middle East, in Russia, (00:39:50) I mean, all across the world. And that's interesting, too. So do you think actually, if everybody has nuclear fusion power plants, that alleviates some of the geopolitical tension that have to do with energy, other energy sources? I certainly do. That the fuel is in seawater all over Earth. Everybody has deuterium. (00:40:10) And everybody has it. (00:40:11) And so you can't have a monopoly on the fuel. (00:40:14) And no one can control the fuel and no one can turn off the fuel. (00:40:17) No one can cut a pipeline. (00:40:19) That just cannot happen with fusion. (00:40:21) And so if we can deploy those plants and we can deploy them quickly, then it decouples the ability of anyone or any few countries to control energy. (00:40:33) Okay, so let's sort of return to the basic question. (00:40:36) We already mentioned it a little bit, but is nuclear fusion safe? (00:40:42) So the power plants that we're talking about, fusion power plants, are they safe? (00:40:47) Yes, fusion power is fundamentally safe. (00:40:51) The physics and the reactions of (00:40:54) the fusion system itself means you don't have runaways. (00:40:57) And so we've talked about some of the human factors around power plants and power systems and industrial scale systems. (00:41:04) And that's something that we build into the design of these from today. (00:41:10) We look at how these systems might fail. (00:41:15) And in fact, some of the analysis we do is we did this analysis for the Nuclear Regulatory Commission over the last few years, looking at how do you regulate fusion power. (00:41:26) As we're building the first fusion power plant, we need to make sure we're regulated safely. (00:41:31) And so we spent a lot of time doing the technical case and the political case in the United States of how to regulate fusion. (00:41:40) And so the analysis we did is assume you have a fusion power plant that's operating. (00:41:44) And then at any one time, a meteor strikes it. (00:41:47) The whole thing is vaporized. (00:41:49) What is the impact of that? (00:41:51) So this is worse than you could ever imagine an actual physical scenario, but let's start there. (00:41:57) And the answer is you don't need to evacuate the populace nearby the fusion power plant. (00:42:02) And one of the keys I think that I come to when I think about this is (00:42:09) the fuel. (00:42:10) In that in a fusion generator, you are continuously feeding in this hydrogen, these deuterium fuels. (00:42:19) And at any one time in a helion fusion system and most fusion systems, you have one second of fuel in that system. (00:42:28) And so what that means is if you stop turning on, if you stop putting fuel into that system, fusion just stops. (00:42:33) But what it also means is that if something really catastrophic happened and for whatever reason, you have all that fuel that's not in the system. (00:42:42) And fusion is so hard to make happen, you hit it with a meteor. (00:42:45) You do anything in that nature and fusion doesn't happen. (00:42:49) That hydrogen, that heavy water, that deuterium just goes back into the environment safely and cleanly without issue. (00:42:56) And so that's the fundamental safety mechanism of fusion. (00:43:00) And you can compare that with other types of power plants, oil or a coal power plant. (00:43:05) You might have a large pile of coal that then catches fire and burns. (00:43:09) And it's not catastrophic, but you have a large coal fire for a long time releasing toxic fumes that you may have to deal with. (00:43:15) And in nuclear power and a fission power plant, you may have several years of fuel sitting in the core. (00:43:21) And in that case, if something bad happened, you have all that potential energy for things to happen. (00:43:27) But in fusion, you have literally one second of fuel at any time in the system. (00:43:31) And having a tank of deuterium, which we have around all the time, can't do fusion by itself. (00:43:36) It needs that complex system. (00:43:39) I love that there's like a PowerPoint going on in a secret meeting about like what happens if a meteor hits a fusion power plant. (00:43:46) Okay, so that's really interesting. (00:43:48) What about the waste? (00:43:50) What kind of waste is there for fusion power plants? (00:43:53) So the fusion reaction itself is still fundamentally an atomic reaction. (00:43:57) And so during this reaction, you do create ionizing radiation. (00:44:01) You create x-rays, you create neutrons, and you create all these charged particles. (00:44:05) The church particles themselves for a fusion reaction are all contained in the fusion system. (00:44:11) And the X-ray is similar to, think about a dentist's office, although a lot more than that, but that type of same X-ray and X-ray energy is absorbed by the fusion system. (00:44:22) But the thing we do care about is those neutrons. (00:44:24) And so we do have in a fusion system activation. (00:44:27) During its operation, neutrons are made and leave. (00:44:30) And so we have to shield. (00:44:32) these fusion systems during their operation. (00:44:35) And so this is very similar. (00:44:36) And in fact, this is a lot of the work we did with the Nuclear Regulatory Commission over the last number of years, that there was a landmark agreement that happened for the NRC that then was codified into law last year called the Advance Act, which is really powerful because it says for the very first time how the US government leading the way on this, which I'm really proud of, (00:44:58) will regulate fusion. (00:44:59) And this gets into a little bit of the details, but the way the Nuclear Regulatory Commission regulates nuclear things in the United States is in these different sets of statutes. (00:45:10) And nuclear reactors are regulated under something what's called Part 50. (00:45:15) And there's a lot of variety of the regulatory language around that, but most of it is to handle special nuclear materials, uranium and plutonium. (00:45:23) But fusion is not. (00:45:25) Fusion is regulated under something called Part 30. (00:45:28) Part 30 is how hospitals are regulated, particle accelerators, other types of irradiators, where as they're operating, you have very high energy particles, ionizing radiation, and you have to protect operators from it, and you have to shield them. (00:45:41) And so we build concrete shields. (00:45:43) And if you came and visited Helion, you would see plastic, borated polyethylene, and concrete shielding to protect operators and equipment from the fusion reactions while they're happening. (00:45:54) But again, you turn them off and those fusion reactions stop. (00:45:58) And that's really the key. (00:46:00) There's a funny story related to that. (00:46:04) We've been building fusion systems that do fusion a long time. (00:46:10) And at some level, they got powerful enough, doing enough fusion, we started building these shields and shielding them like a particle accelerator. (00:46:18) And I went to (00:46:20) the regulatory bodies that regulate Part 30. (00:46:24) This is in Washington State. (00:46:25) It's the Department of Health. (00:46:26) And so I went to the Department of Health and said, here's an application for a fusion generator shielding permit as a particle accelerator. (00:46:35) And the very first question I got asked was, great, where do the patients go? (00:46:41) because the standard form had a patient as a hospital, the patient dose for the particle accelerator, and then the shielding. (00:46:48) And we talked all about the shielding and the operators, which is very similar for a helion system. (00:46:52) And we said, no, patients at all. (00:46:54) No one's inside this thing. (00:46:55) Our goal is to generate electricity one day. (00:46:57) This was a lot of years ago. (00:46:59) And we were able to go through and work with the state agencies to license these fusion particle accelerators. (00:47:06) We were, as far as we know, the first licensed fusion system (00:47:11) ever as a particle accelerator for those first systems. (00:47:16) First license we had was in 2020. (00:47:18) We then have gone on and now licensed several of our fusion systems that we've built that do fusion, both the shielding as well as some of the fuel processes. (00:47:29) So high level, what are the different ways to build a nuclear fusion power plant? (00:47:36) So, can you explain what a Tokamak is, what a Stylarator is, and what's the linear approach that Helion is using? (00:47:46) So there are a number of ways to do fusion. (00:47:50) And fundamentally, in all fusion approaches, you're trying to do the same fundamental physical process, which is take these lightweight isotopes, heat them up so that they can move at high velocity, over 100 million degrees, bring enough of them together, we call it density, enough of them together in a certain volume so that you have reactions happening at a higher rate, and keep them together long enough that they are able (00:48:16) collide into each other and do fusion and release energy. (00:48:21) That's the fundamental core. (00:48:22) Now, how you do that, how you bring those particles together, how you hold them together long enough, there's a wide range of technologies that as humans we've been exploring since the 1950s. (00:48:34) And I think about several main categories. (00:48:37) If you look at the fusion funding out there, government funding in the world, private funding actually has quite a different profile, which is (00:48:45) an interesting thing to talk about. (00:48:47) But in public funding and federal funding in the United States, there's two mainline programs called inertial fusion and magnetic fusion. (00:48:55) And in inertial fusion, what you're trying to do is bring together and push together by a variety of means, physical means, those particles, you push them together. (00:49:06) The most common is called laser inertial fusion. (00:49:09) Our colleagues at the National Ignition Facility did this really well and made world records in the last few years for being able to demonstrate you can do this and do it at scale, where you take very high power lasers and pulse them together to combine them to do fusion. (00:49:25) a pulse for a very short period of time, nanoseconds, billionths of a second. (00:49:30) The other extreme, and you mentioned tokamaks and stellarators. (00:49:35) Stellarators are actually my favorite, so we'll talk about those. (00:49:39) graduate student in fusion, the stellarator is the first thing you learn about. (00:49:43) Because there's a mathematical solution for a stellarator that solves perfectly. (00:49:48) And you can write it out and you can solve it. (00:49:51) And analytically, it's very simple. (00:49:53) Building one is very hard. (00:49:55) And so it's taken humanity a number of decades to be able to build stellarators. (00:50:01) And we can do it now. (00:50:02) With the Windelstein 7X that came online, (00:50:06) in the last few years being the premier stellarator in the world. (00:50:11) I should say, all the different ways to do fusion all just look so badass in terms of engineering, creating this containment, extremely high temperature, high density, everything's moving super fast. (00:50:26) Everything is happening super fast. (00:50:28) It's just fascinating that humans are able to do. (00:50:30) There's certain things, accelerators of that a little bit, but this is even cooler because you're generating energy that can power humanity with this machine. (00:50:40) Anyway, can you just speak a little bit more to the inertia and the magnetic fusion systems? (00:50:44) In a magnetic system, your goal is not to... (00:50:49) push together those particles as fast as possible. (00:50:52) Your goal is to hold on to them for as long as possible. (00:50:56) And to do that, we use magnetic fields. (00:50:58) So let's take a step back. (00:51:00) What is a magnetic field? (00:51:01) So in an electromagnet, there's a variety of ways to make a magnetic field. (00:51:07) One of the most famous, I think everyone is familiar with, is Earth itself. (00:51:10) Earth has what we call the magnetosphere, which is the magnetic protection that's generated actually by the core of the Earth. (00:51:19) But we have a magnetic field around the Earth. (00:51:22) And that magnetic field protects us from particles coming from (00:51:27) the galaxy, galactic cosmic rays and solar particles that would come to Earth. (00:51:32) That magnetic field, when you run a compass, you see the magnetic field from the Earth. (00:51:36) So we know it's happening. (00:51:37) It's all over. (00:51:38) But how we generate it with electric currents is a little bit different. (00:51:42) And what we do is that we have a loop of wire. (00:51:45) And the simplest way to think about it is literally (00:51:48) a round loop. (00:51:49) And in that loop, you have electrons. (00:51:51) You have an electrical current that's running. (00:51:53) And when electrical current, this is some of Maxwell's equations that we discovered in the 1800s, that when you have an electrical current and a wire, it generates a magnetic field inside that wire. (00:52:04) And so when you look at fusion systems, you always have these big magnetic coils with large amounts of current. (00:52:12) We don't run a little bit of current. (00:52:13) In our systems, we have hundreds of mega amps of current. (00:52:16) If you think about at your house (00:52:18) you have your breaker box with 200 amps, or maybe a 400 amp breaker box, and we run 100 million amps of electrical current. (00:52:28) So massive amounts of electrical current to be able to do this. (00:52:32) So that magnetic field that's generated inside that magnetic coil has some really special properties. (00:52:38) And we take advantage of those properties to do fusion. (00:52:42) And some of those properties are not intuitive. (00:52:45) So here's one of my favorites, (00:52:47) When you have an electromagnetic field, you have this coil with electricity going around it, and you have a magnetic field inside of it. (00:52:55) And then you have a test particle, a charged particle, an electron or an ion, which is, if you imagine, to generate this, I have a coil with electrons moving around it. (00:53:05) But if I put one in the middle of it, in this magnetic field, some really interesting things happen. (00:53:10) That (00:53:11) electron or that ion, that charged particle is what's called magnetized. (00:53:15) And what magnetized means is that it's trapped on that field line. (00:53:19) In fact, even really more interesting is that it oscillates around that field line. (00:53:25) And so the way I think about this is if you think about the Earth's magnetosphere again, and you think about the charged particles, the aurora, the northern lights, is a charged particle trapped in the Earth's magnetic field going around. (00:53:38) the Earth's magnetic field. (00:53:39) And in the same way in fusion, we do the same thing here on Earth, but in a smaller direction where we trap these particles on magnetic fields and they can go around and stay a trap to that magnetic field line. (00:53:51) How much of the physics at this scale is understood here, like how these systems behave when you trap the magnetic field in this way? (00:54:03) Is this fundamentally now an engineering problem or is there a new physics to be discovered about how the system is behaving? (00:54:10) In fusion, the physics we're using is actually quite old. (00:54:14) That the fundamental electromagnetic physics is 1800s physics. (00:54:18) The fundamental atomic physics is early 1900s. (00:54:21) And so the fundamental physics of how these work is very well understood. (00:54:27) Putting them all together into a power plant, that's hard. (00:54:30) And so you can do the math. (00:54:31) You can do the math. (00:54:32) Every introductory grad student does the math on a stellarator and say, this is all I need to do. (00:54:38) I just need to make a magnetic coil in this very complicated shape. (00:54:42) And then fusion will happen. (00:54:44) However, doing that in practice is actually quite challenging. (00:54:48) So maybe you could speak a little bit more. (00:54:50) So the stellarator and the Tokamak, what's the difference between those two? (00:54:54) They're both magnetic fusion systems. (00:54:57) And then what does Helion do? (00:54:59) The tokamak and the accelerator are both magnetic systems. (00:55:02) Their goal is to generate this magnetic field and hold on to the fusion fuel long enough. (00:55:10) Like I mentioned, these charged particles are trapped on the magnetic field. (00:55:13) In fact, they're oscillating. (00:55:14) We call that a gyro orbit as the radius that they oscillate around this magnetic field. (00:55:20) And we've been talking about atomic physics where everything is at this nano scale. (00:55:25) But gyro orbits are not. (00:55:26) Gyro orbits for these fusion particles are measured in inches. (00:55:30) And so they're on a scale that we can see and measure and understand really intuitively. (00:55:37) And in a magnetic system, your goal is to simply trap as many of these particles as you can for long enough and heat them so they're hot enough so that they bang into each other. (00:55:47) They collide enough that you're doing fusion. (00:55:49) And you're doing enough fusion to overcome as fast as you're losing those particles. (00:55:54) And so that's what (00:55:55) What happens when you put particles in a magnetic field and you try to hold on to it? (00:55:59) The challenge is, that's really hard to hold on to them long enough. (00:56:03) These particles are moving around, they're moving at very high velocity, millions of mph. (00:56:07) They're colliding with each other, and they're getting knocked off and getting knocked away. (00:56:12) So we've talked about inertial fusion, where you try to confine (00:56:18) a fusion plasma by crushing it as fast as possible. (00:56:21) And magnetic fusion, where you just simply have a magnetic field and your goal is to hold on to it for as long as possible. (00:56:28) But there's another way to do fusion. (00:56:30) And in some ways, it's one of the earliest approaches for fusion that was successful. (00:56:36) As scientists and engineers, maybe we're not too creative with the terminology, we call the technique that Helion uses magneto-inertial fusion, because it does a little bit of both. (00:56:47) So to understand that, we can actually go back in history a little bit and think about the evolution of some of these approaches to fusion. (00:56:54) And so from our perspective, we look at the technology that we use as built on physics experiments that were very successful in the 1950s. (00:57:04) And in those systems, the earliest pioneers of fusion said, (00:57:08) I know we understand the physics. (00:57:11) We have to take these gases, heat them to 100 million degrees, and then confine them, push them together so that fusion happens. (00:57:18) And so what is the best way to do that? (00:57:20) So some of the earliest programs, we call them the Theta Pinch. (00:57:24) And what those programs were, a linear topology, because we knew how to build these magnets. (00:57:29) It's called a solenoid, where you take a series of electric coils, you run electrical current through them, that generates a magnetic field. (00:57:36) Great. (00:57:37) So you have a magnetic field. (00:57:38) Now you add your fusion particles. (00:57:40) Okay. (00:57:40) So you've added fusion particles to this solenoid. (00:57:43) Here's the challenge. (00:57:45) Those particles, as they're sitting in that magnetic field, in this nice magnet, escape. (00:57:50) They leave out the ends, because there's nothing holding them in. (00:57:53) Great. (00:57:53) So that makes sense. (00:57:55) And so that doesn't work. (00:57:56) Okay. (00:57:57) So then the next approach is say, well, one branch of fusion said, okay, well, to solve that, why don't we take this solenoid and bend it around? (00:58:05) Let's just make it a big donut. (00:58:06) So as they're escaping, they go around and around in a circle. (00:58:09) Great. (00:58:10) That's a great approach. (00:58:11) And so one branch of fusion went down that direction. (00:58:15) And that became, that evolved into the stellarator and the tokamak. (00:58:19) Different ways of taking those solenoids and wrapping them around so that the plasmas go round and round in that magnetic field and those charged particles are held long enough that fusion happens. (00:58:30) But there's a different way to do it. (00:58:31) And so the theta pinch was what was born in the 1950s of take this magnetic field and oh, they're trying to escape. (00:58:38) Great. (00:58:39) Let's not let them escape. (00:58:40) Let's close the bottle. (00:58:42) Let's close the ends. (00:58:43) And so we make the magnetic field much stronger at the ends. (00:58:46) This one was called the mirror. (00:58:47) And so the idea was that the particles would bounce in between. (00:58:51) And that worked and they got hotter and hotter and hotter. (00:58:54) But guess what? (00:58:54) As you kind of would imagine, (00:58:56) As this mirror topology, this linear topology, the pressure increased inside. (00:59:02) The particle pressure, the particles tried to push back on the magnetic field. (00:59:06) They were trying to escape now. (00:59:08) They're trying, they're getting hotter and hotter. (00:59:09) And just as you imagine, hot gas in a balloon tries to get out the ends. (00:59:14) You could not hold it tight enough at the ends to keep those particles in. (00:59:17) And in fact, the problem is the hottest ones were the ones that would escape. (00:59:21) And so you do a good job of heating it and they'd all leave out the ends. (00:59:24) Okay? (00:59:25) So then the next iteration has said, (00:59:26) Okay, why don't we just not try to hold on to it very long? (00:59:29) Why don't we squeeze it? (00:59:31) And so rather than just holding it constantly, let's now crush it. (00:59:35) So we built this solenoid, we pinched the ends, and then we crushed it. (00:59:40) And what I mean by crushing it is not actually like crushed it. (00:59:44) crushing any magnets or changing the topology or moving any parts, but just rapidly increasing the magnetic field. (00:59:51) And so going from a magnetic field that's just holding it to now taking all those particles, if you imagine they were in a streaming around together, and then rapidly increasing the magnetic field so that those particles get closer and closer, closer together. (01:00:07) So you increase the density. (01:00:08) And now fusion starts to really happen. (01:00:12) But they ended up hitting a technological limit. (01:00:15) So this is the part that I look back and I look at the pioneers that in 1958, there was some pioneering work done. (01:00:24) And this was in California, what later became Livermore Labs. (01:00:28) There was also some work done at other national labs too. (01:00:32) These were all federally funded programs to explore this theta pinch topology of can you just squeeze the plasma down fast enough, hard enough? (01:00:41) because this was 1958, the transistor was sitting in the laboratory and they were commuting, they were turning on millions of amps of electrical current. (01:00:51) And they were doing it, we haven't talked about the time scales, but they were doing it in millionths of a second, microseconds, megahertz speeds. (01:01:00) And this was in 1958. (01:01:01) No transistor, no CPUs, and no electrical switches, none of the things that I take for granted every day. (01:01:09) And so they were able to show at that time the highest performing fusion systems. (01:01:13) They got to temperatures, they didn't get to 100 million degrees, not quite then, but they got to 50 million degrees. (01:01:19) They were outperforming everything else in fusion, but they reached a technical limit where they just could not build it anymore. (01:01:26) And so they, those pioneers, went in a different direction. (01:01:31) And they started down the laser inertial path of saying like, okay, well, we can't do these electromagnetic pinches, (01:01:38) But we now have, this new thing has invented the laser, which turns on in a nanosecond. (01:01:43) It's vast, it's interesting. (01:01:44) Let's go down that path. (01:01:46) And it's not, you have to fast forward a couple of decades to researchers found with some of these theta pinches, when they're operated in a very specific way, something else happened, something new happened. (01:01:58) And that these plasmas where before they squeezed them, (01:02:04) very hard. (01:02:05) And just like squeezing a tube of toothpaste, they squirted out the ends. (01:02:07) Now it didn't squirt out the ends. (01:02:09) It actually pushed back. (01:02:10) It stayed confined. (01:02:12) It stayed trapped inside that linear topology. (01:02:15) Even though the ends were open, the plasma didn't leave. (01:02:18) And so there was a large amount of programs of like, what is happening here? (01:02:22) This is an accidental discovery in plasma physics. (01:02:25) that something new is happening. (01:02:26) And what we discovered is we now call the field reverse configuration. (01:02:31) There's numerous programs of FRC, field reverse configuration programs, both at national labs. (01:02:38) There's actually a number of private companies now of people building field reverse configurations. (01:02:43) And they have some really unique properties. (01:02:45) But fundamentally, talking about the main difference, I described the solenoid with magnetic fields throughout the center of that volume and plasma trapped (01:02:54) going back and forth. (01:02:55) But some other things can happen, which is really interesting. (01:02:58) And what they discovered early is if they have field going in one direction, so the plasma, the electrical current is going around the loop, and the plasma is going back and forth along this magnetic field line inside that solenoid, inside that theta patch. (01:03:15) But then they change the direction of the magnetic field. (01:03:18) And this is what we call field reversal. (01:03:20) And this is really the key, is that you start with the plasma going in one direction, (01:03:24) And very rapidly, you change the direction. (01:03:27) You change the direction and reverse the direction of that field. (01:03:30) And something really interesting happens, which is the plasma, this fusion fuel, these charged particles, which are trapped on the magnetic field lines that are moving back and forth, you change the direction. (01:03:42) What that means is that you're trying to take that electrical current and that magnetic field and reverse its direction, flip it. (01:03:51) but it can't flip fast enough, that the plasma is sitting there and you can't move the particles. (01:03:58) And so what's really interesting is what happens is that because the particles can't move, but you've now flipped the direction of the magnetic field, you've inverted it, something really, really unique happens, which is that the plasma itself reconnects internally. (01:04:14) And so now what you're left with is an outside magnetic field, an electrical coil, and inside the plasma, where now it was, before it was moving along, it's now moving internally. (01:04:27) Rapidly reversing the magnetic field, plasma self-organizes into a closed field. (01:04:35) What? (01:04:36) Yep. (01:04:36) So it sounds wild. (01:04:39) It's, yeah. (01:04:40) So first of all, there's a lot of, there's a million questions I have. (01:04:43) So one of them, what's rapidly? (01:04:46) What time scale are we talking about here? (01:04:50) You have to reverse the electrical current faster than a million degree, which is a very hot gas particle can move. (01:04:58) And so that means we have to do it on the order of a millionth of a second. (01:05:02) We have to do it in a millionth of a second. (01:05:03) Wow. (01:05:05) And so in practice, this is hard. (01:05:08) And it's only, we can only do it now because of semiconductor switching. (01:05:14) Because we can move things, we can switch things like the transistor in every CPU in a computer switches at a gigahertz. (01:05:21) That means in a nanosecond, it's switching in a billionth of a second. (01:05:24) And so now, which we didn't in the 1950s when these theta pinches were invented, but now we have the semiconductors to be able to do that. (01:05:31) The self-organizing plasma, can you just speak to that? (01:05:35) What the heck is it doing? (01:05:37) How do we discover, how do we understand the self-organizing mechanism, the dynamics of the plasma that it's able to contain itself? (01:05:44) So what I like to do is use an analogy here of once you've made it, it's actually somewhat straightforward to understand. (01:05:54) Getting to it is tricky. (01:05:56) And how they discovered it the first time is absolutely amazing. (01:05:59) But once you've made it, (01:06:01) it's a lot more straightforward to understand. (01:06:04) So in a magnetic coil, when you have a round electrical coil, you have electrical current flowing in that coil. (01:06:13) And if you have a conductor, if you have another, a metal inside that coil, and this is called Linz's law in one of the Maxwell equations, is that as you have electrons and you have current flowing in that coil, (01:06:27) An equal and opposite electrical current is induced in a piece of metal nearby. (01:06:33) This is the same thing that happens in a transformer, where you have a primary on a transformer and you have electricity flowing it, and you have a secondary where electricity flows exactly the opposite direction. (01:06:42) We use this every day in our lives. (01:06:46) And so in this condition, you have a conductor, an electrical conductor, where current can flow, and you have an electrical current flowing on the outside, electrical current flows on the inside. (01:06:57) And in that case, now I've described two pieces of metal. (01:07:02) Now let's go one step further, and that inner conductor is not a piece of metal anymore. (01:07:06) It's one of these high temperature gases, this plasma, this charged particles. (01:07:10) So now you have current, electrical current flowing in the plasma. (01:07:15) And this is really, really interesting. (01:07:17) We talked about these charges moving back and forth. (01:07:20) Well, moving electrical charges is current. (01:07:22) So in every plasma condition we've talked about, the tokamak, the theta pinch, the stellarator, there's electrical current flowing in the plasma. (01:07:31) But in the field reverse configuration, you have a lot of electrical current flowing in the plasma, massive amounts of it. (01:07:37) And that's the key. (01:07:38) So you have the center core where electrical current is flowing in this transformer, if you want to think about it, primary and secondary. (01:07:45) And here's the craziest part of it. (01:07:48) This electrical current, how did I describe a magnet? (01:07:52) An electromagnet is a loop that has electrical current flowing in it that generates a magnetic field. (01:07:59) And for a theta pinch, and for a mirror, and for a tokamak, in that magnetic field, the plasma gets trapped. (01:08:07) But in an FRC, this electrical current is the plasma. (01:08:12) And that plasma then generates its own magnetic field. (01:08:16) And it's then trapped on its own magnetic field. (01:08:20) That's fascinating. (01:08:21) And that's the key. (01:08:22) And so in your tokamak, in your donut, and in your funky donut, your stellarator, you make the magnets and you trap your plasma in it. (01:08:31) In an FRC, you make the plasma, which makes the magnets, and it traps itself. (01:08:37) And the craziest part of this in my mind is that we actually see this in nature all the time. (01:08:43) If you look at the sun, we see solar flares. (01:08:46) And in a solar flare, we've all seen the pictures of the photosphere of the sun and this large arc of plasma coming out. (01:08:55) That plasma has current, electrical current flowing in it. (01:08:58) And then we see this solar flare (01:09:00) rip off of the sun. (01:09:02) And that solar flare then can flow throughout and continue into the solar system. (01:09:07) And for a little while anyway, it makes something called a plasmoid. (01:09:11) That plasmoid is in fact electrical current flowing in the plasma, generate a magnetic field and holding it for longer than it would otherwise. (01:09:20) And so we've observed these for 100 years. (01:09:22) And we've known about these plasmoids for a long time. (01:09:25) And there's researchers that have tried intentionally to make them. (01:09:28) But fundamentally, that's what we do every day is make one of these self-organized closed field plasmas. (01:09:36) In a more controlled way at this rapid rate of 1 millionth of a second and being able to make sure it's reliable and stable and all that kind of stuff. (01:09:45) So by the way, how do you keep the thing stable? (01:09:47) And there's the hard part, because I just described a solar flare. (01:09:51) And yes, we've seen the pictures of them, but we've also watched them and they appear, they fly away from the sun and then they go away. (01:09:58) And that's not what (01:09:58) We want infusion, right? (01:09:59) We want to be able to control this. (01:10:01) And so that's the hard part of the job. (01:10:04) And so that's what we've spent the last number of years learning how to do ourselves and others on these pulsed closed field FRC systems. (01:10:14) Let's first talk about how to make them, and then we'll talk about how to make them stable, because they're two different things, and we spent a lot of time on both. (01:10:21) So we talked about time scales. (01:10:23) So you have to reverse the field. (01:10:24) You have to change the electrical current in a millionth of a second. (01:10:28) And so how do you do that? (01:10:30) So I've described this system as you have a series of magnets. (01:10:33) You have a magnetic field on the outside. (01:10:37) And then on the inside of this, you have this donut, this FRC that has its own electrical current. (01:10:44) And we didn't talk about this yet, but it's generated a magnetic field. (01:10:47) And that magnetic field has pressure. (01:10:50) And this is the other thing that's really interesting. (01:10:52) So we talked about how this theta bench (01:10:54) compresses a magnetic field. (01:10:56) It applies a pressure on the outside. (01:11:00) But the plasma itself has a pressure on the inside. (01:11:03) And it has both the particle pressure, literally the particles bouncing, think about hot gas in a balloon, the particles expanding, the ideal gas law expanding and contracting inside a balloon, but they also have a magnetic pressure. (01:11:14) They have the electromagnetism is pushing back. (01:11:18) And so I like to think about this as the motor in a Tesla. (01:11:22) in your electric car, you have a motor, electric motor. (01:11:26) And what that motor has is a series of windings. (01:11:28) Those windings, you flow electrical current, in this case from a battery, hit the gas, electricity flows from the battery into the motor, into those windings, and it generates an electromagnetic force, a Lorentz force is what it's technically called. (01:11:41) This electromagnetic force (01:11:43) induces an electrical current on the armature, on the shaft. (01:11:48) And this is getting into the details, but in the armature of an electrical motor, that actually is what spins. (01:11:53) And so the outside of a motor doesn't spin. (01:11:56) You have flow electrical current through it, and the inside does spin. (01:11:59) That electromagnetic force is what is spinning that armature. (01:12:03) In our case, we're inducing an electrical force in that electromagnet, and that's putting electrical current, just like in the armature, (01:12:11) into that plasma, and we can use that force to do interesting things. (01:12:16) So that electromagnetic force can compress the fusion plasma, it can expand the fusion plasma, but here's the problem, it's unstable. (01:12:24) And so this is something you learn very early in your graduate work as a student in fusion, is you learn about plasmas that are called high beta plasmas. (01:12:35) So I keep seeing this (01:12:36) plasma beta thing everywhere. (01:12:38) What is this ratio of plasma field energy to confining magnetic field energy? (01:12:43) Please explain. (01:12:44) Plasma beta is the ratio of the magnetic pressure to the particle pressure. (01:12:48) And so what that fundamentally means is I talked about how you have a magnetic field. (01:12:53) And in that magnetic field, plasma is trapped on that magnetic field. (01:12:58) But (01:12:59) It's not very well trapped. (01:13:00) It can escape. (01:13:01) It can leave either down the ends, it can freely travel, or it can also travel across the magnetic field. (01:13:08) And so we have a term called plasma beta, which gives us an understanding of how well trapped that plasma is. (01:13:16) So as you apply a magnetic pressure, a magnetic field to this plasma, it pushes back. (01:13:22) And does it push back a little or does it push back a lot? (01:13:25) And for a field reverse configuration in one of our plasmas, beta is very close to 1, usually by definition, one at any point in the system, which means that every time I apply a magnetic force on this donut to compress it, the plasma particles on the inside push back. (01:13:44) And what's really interesting is you have an equation for magnetic pressure, which is B squared or 2 mu naught. (01:13:51) The magnetic field squared is the external magnetic pressure. (01:13:55) Any magnetic field anywhere generates this pressure. (01:13:58) But the plasma particles themselves also have a pressure. (01:14:02) This is the ideal gas law. (01:14:04) And we use the definition in KT, density, Boltzmann constant, and temperature for pressure. (01:14:11) And in high beta, they're the