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Dennis Whyte

๐Ÿ‘ค Speaker
1833 total appearances

Appearances Over Time

Podcast Appearances

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

Those are high kinetic energy, but it's not a temperature.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

So it actually doesn't count as confinement.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

So we go through all of those.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

You have temperature.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

And then the other requirement, not too surprising, is actually that there has to be enough density of the fuel, right?

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

Enough, but not too much, yes.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

And so, in the end, the way that there's a fancy name for it, it's called the Lawson Criterion, because it was formulated by scientists in the United Kingdom about 1956 or 1957.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

And this was essentially the realization, oh, this is what it's going to take, regardless of the confinement method.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

These are, this is the basic, what it is actually, power balance.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

It just says, oh, there's a certain amount of heat coming in, which is coming from the fusion reaction itself, because the fusion reaction heats the fuel, versus how fast you would lose it.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

And it basically summarizes, it's summarized by those three parameters, which is fairly simple.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

So temperature, and then the reason we say 100 million degrees is because almost all in...

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

And for this kind of fusion, deuterium tritium fusion, the minimum in the density and the confinement time product is at about 100 million.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

So you almost always design your device around that minimum.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

And then you try to get it contained well enough, and you try to get enough density.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

So that temperature thing sounds crazy, right?

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

That's what we've actually achieved in the laboratory.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

Like our experiment here at MIT, when it ran its optimum configuration, it was at 100 million degrees.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

but it wasn't actually the product of the density in the confinement time wasn't sufficient that we were at a place that we were getting high net energy gain, but it was making fusion reactions.

Lex Fridman Podcast
#353 โ€“ Dennis Whyte: Nuclear Fusion and the Future of Energy

So this is the sequence that you go through.