Episode #485 from 13:14

Physics of E=mc^2

So in fusion, you take these lightweight isotopes like hydrogen and deuterium, and as you combine them and get these molecules closer and closer together, some really interesting fundamental physics happens. First, these atomic nuclei are charged. They have an electric charge, and like charges repel. 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. So you have a force that's actually pushing against them. 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 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. Once you get within a very close distance, on the order of the scale of those nuclei themselves—of those atomic nuclei, the tiniest thing you could imagine, and probably way smaller than that—these particles then are attracted to each other, and they combine and 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 MC² as energy.

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So in fusion, you take these lightweight isotopes like hydrogen and deuterium, and as you combine them and get these molecules closer and closer together, some really interesting fundamental physics happens. First, these atomic nuclei are charged. They have an electric charge, and like charges repel. 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. So you have a force that's actually pushing against them. 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 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. Once you get within a very close distance, on the order of the scale of those nuclei themselves—of those atomic nuclei, the tiniest thing you could imagine, and probably way smaller than that—these particles then are attracted to each other, and they combine and 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 MC² as energy.

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Physics of E=mc^2 chapter timestamp | David Kirtley: Nuclear Fusion, Plasma Physics, and the Future of Energy | EpisodeIndex