If I'm understanding correctly, he's saying that if you put a hydrogen atom through a change in gravitational potential of ##\Delta\phi##, then this has a probability ##\sim (\Delta\phi/c)^2## of kicking it into the n=2 state. (This probability is multiplied by an energy ratio that I think is on the order of 1 for atomic hydrogen.)
This would be a pretty serious violation of the equivalence principle. He talks about a ##\Delta\phi## corresponding to the difference in potential between the Earth's surface and (I think) a large distance from the earth. But if we believe in the equivalence principle, then there should be no way to tell whether there is some other, stronger, uniform field superimposed on top of the earth's. In general it's just physically bizarre that he claims that the gravitational potential produces physically observable effects. The e.p. says that only the second derivative of the potential should be observable.
It would be interesting to get someone with good QM chops to look at this and see if it's just obviously wrong. That may be the case, and if so, then that would explain why he publishes this stuff in such obscure journals. Although his calculations are actually pretty simple, I think it takes someone with a very firm grasp on the fundamentals to sniff out a mistake in this kind of novel context.
It's not clear to me whether he's also in effect predicting nonconservation of energy here...??
DrClaude said:
If this was correct, wouldn't we have already noticed something in interstellar clouds?
Although I believe some of those clouds are very cold (so that the expected equilibrium thermal population of the n=2 states may be negligible), they're still exposed to an environment with a lot of hard radiation. Therefore I don't think they're really in a state of thermal equilibrium, are they? I imagine it wouldn't take a lot of ambient UV to produce a non-equilibrium population of 10^-16 in an n=2 state. A secondary issue is that these clouds would contain molecular hydrogen, not atomic hydrogen, but I assume that if his theory were right, it would also predict these anomalous transitions in molecular hydrogen.
greswd said:
What about conducting an experiment using a tank of hydrogen in free fall on Earth?
If I'm understanding him correctly, then there is no reason that it has to be in free fall. It could be in a moving elevator or contained in a spacecraft whose rockets were thrusting. I think the reason he talks about a spacecraft is that he wants to make a very large change in gravitational potential. (The effect is proportional to the square of that change.) If I'm understanding his prediction correctly, then it even implies that there should be an annual effect in a tabletop experiment, due to the Earth's motion in the sun's potential as it goes through its slightly elliptical orbit. Or maybe there would be an effect due to the solar system's motion through the potential due to the Milky Way.
I suppose a calculation is required in order to figure out the conditions of temperature and pressure that would be needed in order to keep a tank of atomic hydrogen gas in a condition where ##\lesssim 10^{-16}## of the atoms are in the n=2 state based on thermal equilibrium, and furthermore where interactions between atoms don't distort the wavefunctions by something on the order of this amount. In fact, this seems like the kind of estimate that Lebed should have done as part of these papers.
Looking back at his claimed result for the probability of a gravitationally induced change of state, he has an additional factor involving energies that I think is of order unity for hydrogen. Let's call this factor F. It's ##F=(V/\Delta E)^2##, where ##V## is something like the internal energy of the atom (average KE plus electrical PE), and ##\Delta E## is, in the case he discusses, the energy difference between the n=1 and n=2 states. This makes me wonder why he doesn't consider systems in which this energy ratio is large.
In H2, the rotational transitions are in the infrared, with energies on the order of 0.1 eV, so that I think his energy ratio would be on the order of 10^4, which is a lot better than hydrogen. Of course, it might be hard to prepare a sample of H2 cold enough to keep the first excited rotational state unpopulated -- you'd probably tend to make liquid H2 unless the pressure was very low.
Or what about nuclei? Odd-odd nuclei often have isomeric states with excitation energies on the order of 1 keV (possibly much less in some cases?). The internal energy of a heavy nucleus is ##V\sim10^6## keV or something, so it seems like F would be gigantic. If Lebed's theory is right, why don't we observe very strong anomalous emission of x-rays from odd-odd nuclei? It seems like with an F this large, it should be very easy to detect this in tabletop experiments, based on annual variations in the gravitational potential due to the sun.