Well, I goofed. Energy conservation in GR turns out to be subtle, and it's certainly not right to flatly say energy is conserved. Quite a few people pointed this out. Here's a couple of samples, at different levels of explanation:https://twitter.com/johncarlosbaez/status/1191164917597917184 …
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And a nice discussion here (and in followups):https://twitter.com/the_happyproton/status/1191107133628207106 …
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It is, nonetheless, possible to make some sense of the notion of energy conservation in GR. Here's an overview: http://math.ucr.edu/home/baez/physics/Relativity/GR/energy_gr.html … (also by
@johncarlosbaez and collaborator).Show this thread -
There's also a set of ideas known as the ADM formalism, a so-called Hamiltonian formulation of GR. (The Hamiltonian is a sort of energy function). https://en.wikipedia.org/wiki/ADM_formalism …
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These caveats don't make my original statement correct! But they are useful context, a sense in which the notion of energy (or a Hamiltonian) is correct in general relativity.
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Another topic: some people are replying "Isn't this Noether's theorem?" But that misses the the point. Of course, once you're in Lagrangian mechanics & have time-translation invariance, conservation follows. And there's an analogous quantum argument...
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... but assuming all that structure begs the question.
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Energy is conserved in theories where 1) symmetries give conservation laws and 2) time translation is a symmetry. It's not conserved in the Big Bang cosmology, where 2) fails.
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one might argue that energy ought to be that which is conserved (by time evolution) by definition; you can sorta make this precise using noether's theorem, although that might be circular
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Noether's theorem is a consequence of Lagrangian mechanics, so it's sorta begging the question. In some sense, though, you can get energy conservation in both GR and NM this way, which I guess is a good point!
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