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"Surely You're Joking, Mr. Feynman!" - unam.

"Surely You're Joking, Mr. Feynman!" - unam.

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pronouncing the words, knowing what not to include in a paper or a seminar, and<br />

detecting a weak technique in an experiment. But I love physics, and I love to go back to<br />

it.<br />

Monster Minds<br />

While I was still a graduate student at Princeton, I worked as a research assistant<br />

under John Wheeler. He gave me a problem to work on, and it got hard, and I wasn't<br />

getting anywhere. So I went back to an idea that I had had earlier, at MIT. The idea was<br />

that electrons don't act on themselves, they only act on other electrons.<br />

There was this problem: When you shake an electron, it radiates energy, and so<br />

there's a loss. That means there must be a force on it. And there must be a different force<br />

when it's charged than when it's not charged. (If the force were exactly the same when it<br />

was charged and not charged, in one case it would lose energy, and in the other it<br />

wouldn't. You can't have two different answers to the same problem.)<br />

The standard theory was that it was the electron acting on itself that made that<br />

force (called the force of radiation reaction), and I had only electrons acting on other<br />

electrons. So I was in some difficulty, I realized, by that time. (When I was at MIT, I got<br />

the idea without noticing the problem, but by the time I got to Princeton, I knew that<br />

problem.)<br />

What I thought was: I'll shake this electron. It will make some nearby electron<br />

shake, and the effect back from the nearby electron would be the origin of the force of<br />

radiation reaction. So I did some calculations and took them to Wheeler.<br />

Wheeler, right away, said, "Well, that isn't right because it varies inversely as the<br />

square of the distance of the other electrons, whereas it should not depend on any of these<br />

variables at all. It'll also depend inversely upon the mass of the other electron; it'll be<br />

proportional to the charge on the other electron."<br />

What bothered me was, I thought he must have done the calculation. I only<br />

realized later that a man like Wheeler could immediately see all that stuff when you give<br />

him the problem. I had to calculate, but he could see.<br />

Then he said, "And it'll be delayed ­­ the wave returns late ­­ so all you've<br />

described is reflected light."<br />

"Oh! Of course," I said.<br />

"But wait," he said. "Let's suppose it returns by advanced waves ­­ reactions<br />

backward in time ­­ so it comes back at the right time. We saw the effect varied inversely<br />

as the square of the distance, but suppose there are a lot of electrons, all over space: the<br />

number is proportional to the square of the distance. So maybe we can make it all<br />

compensate."<br />

We found out we could do that. It came out very nicely, and fit very well. It was a<br />

classical theory that could be right, even though it differed from Maxwell's standard, or<br />

Lorentz's standard theory. It didn't have any trouble with the infinity of self­action, and it<br />

was ingenious. It had actions and delays, forwards and backwards in time ­­ we called it<br />

"half­advanced and half­retarded potentials."<br />

Wheeler and I thought the next problem was to turn to the quantum theory of<br />

electrodynamics, which had difficulties (I thought) with the self­action of the electron.

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