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Mar 4, 2021 at 20:06 comment added Shashaank @R.Rankin any simple reference for this ADM formalism for a beginner? My current knowledge in GR is till Black holes, Kerr metric etc and a bit of singularity theorems and I have never heard of this ADM formalism. Any book or notes for at a starting level?
Feb 28, 2021 at 8:35 history edited Shashaank CC BY-SA 4.0
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Feb 11, 2021 at 9:08 history edited Shashaank CC BY-SA 4.0
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Feb 11, 2021 at 7:22 history edited Shashaank CC BY-SA 4.0
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Feb 10, 2021 at 17:32 comment added R. Rankin Yes, energy is in fact still conserved, this is evidenced by taking the ADM energy. You find that while the gravitational energy is ill-defined locally, it still yields total covariant quantities when integrated over spacetime. This quantity changes when the E&M wave is included in closer proximity. This is where your missing photon energy goes
Feb 10, 2021 at 14:38 comment added Shashaank @R.Rankin But the Schwarzschild metric has a timeline killing vector field, yet energy is not conserved. Any comments?
Feb 10, 2021 at 8:32 comment added R. Rankin @Shashaank If our universe had a timelike Killing vector photon energy would indeed be conserved. Such spacetimes are known as stationary spacetimes. Ours is NOT one. This is because space is expanding over time, which rules out timelike Killing vectors. One can obtain a conformal Killing vector though.
Feb 10, 2021 at 7:32 history edited Shashaank CC BY-SA 4.0
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Jan 8, 2021 at 14:18 vote accept Shashaank
Jan 8, 2021 at 14:18 vote accept Shashaank
Jan 8, 2021 at 14:18
Jan 8, 2021 at 14:18 vote accept Shashaank
Jan 8, 2021 at 14:18
S Jan 7, 2021 at 22:36 history suggested jng224 CC BY-SA 4.0
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Jan 7, 2021 at 21:10 review Suggested edits
S Jan 7, 2021 at 22:36
Jan 7, 2021 at 21:05 history edited Shashaank CC BY-SA 4.0
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Jan 7, 2021 at 18:00 answer added Mike Serfas timeline score: 1
Jan 7, 2021 at 16:29 history edited Shashaank CC BY-SA 4.0
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Jan 7, 2021 at 16:06 answer added Andrew Steane timeline score: 15
Jan 7, 2021 at 15:20 answer added user284984 timeline score: 3
Jan 7, 2021 at 5:52 comment added Shashaank @RedGiant I understand that energy is conserved along a geodesic and for the reason please see the comment I have just made above.
Jan 7, 2021 at 5:51 comment added Shashaank @Eletie But Caroll says that though the geodesic eqn (or rather by just solving the Euler Lagrange eqn for the time coordinate) you have $(1-R/r) \dot{t} =constant$ and the constant is interpreted as the energy. So I understand that energy is conserved along a geodesic and hence the question of photon getting redshifted and loosing energy.
Jan 7, 2021 at 0:18 answer added stuffu timeline score: 1
Jan 6, 2021 at 23:20 review Close votes
Jan 11, 2021 at 3:04
Jan 6, 2021 at 23:02 comment added Eletie Does this answer your question? Are photon energies conserved in general relativity?
Jan 6, 2021 at 22:13 comment added RedGiant Do you know that energy conservation law does not hold in GR?
Jan 6, 2021 at 21:00 history asked Shashaank CC BY-SA 4.0