On energy for accelerating observers in black hole spacetimes
arXiv:2203.00085 · doi:10.1103/PhysRevD.105.104050
Abstract
Quasi-local energies for constantly accelerating observers in Bañados, Teitelboim, and Zanelli (BTZ), Schwarzschild and Schwarzschild-de Sitter spacetimes are derived. The energies are expressed in terms of acceleration, cosmological constant, and area, quantities measurable by the observers. Based on results from quantum fields in curved spacetime for the redshifted Hawking temperature, entropy and thermodynamic-like laws are briefly explored in the three spacetimes.
arXiv commentComments welcome. v2: description of the approach and derivation clarified. v3: updated referencing, typos corrected, close to published version
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