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Take the hydrogen atom. It is easy to imagine that the gravitational pull it creates is smaller than the sum of those of the proton plus the electron, because a photon of 13.6 eV was created when the atom assembled, and has left the system. In other words, the binding energy between the proton and the electron has to be subtracted to the mass of the system.

But where does this appear in general relativity? How does it fit in the stress-energy tensor? I know how to define this tensor for one particle, or for an electromagnetic field, but I don't see how the binding energy fits.

fffred
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1 Answers1

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Generally we just fudge the issue and ignore the binding energy. It helps that gravity is negligable on the subatomic scale$^1$ so this isn't a problem. We just take measured mass of the (in this case) hydrogen atom and bung it in $T_{00}$.

If you start worrying about binging energies you risk walking the path to madness. The majority of an atom's mass is in the nucleus, and 99% of the mass of a nucleon is the QCD binding energy. So if you start worrying about how to describe the electrostatic binding energy in an atom you have a far worse problem trying to describe the binding energy in a nucleon.

Of possible interest is that the kinetic energy of subatomic particles should also go into the stress-energy tensor because it will produce non-zero contributions to all the entries in the stress-energy tensor. I note someone has even put a paper on the Arxiv about this.


$^1$ I'm assuming here that the LHC hasn't produced any black holes.

John Rennie
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