Energy Conservation and Hawking Radiation
classification
✦ hep-th
gr-qc
keywords
blackconservationenergyholeapplicableapproximatelycannotconsider
read the original abstract
The conservation of energy implies that an isolated radiating black hole cannot have an emission spectrum that is precisely thermal. Moreover, the no-hair theorem is only approximately applicable. We consider the implications for the black hole information puzzle.
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Forward citations
Cited by 2 Pith papers
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Spin effects on particle creation and evaporation in $f(R,T)$ gravity
Spin-dependent particle creation densities, greybody factors, absorption cross sections, and evaporation lifetimes are computed for scalar, vector, tensor, and spinorial modes around black holes in f(R,T) gravity.
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Particle production, absorption, scattering, and geodesics in a Schwarzschild-Hernquist black hole
Embedding a Schwarzschild black hole in a Hernquist dark matter halo suppresses particle creation rates, changes scattering cross sections, and alters null and timelike geodesics relative to the vacuum case.
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