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Energy Conservation and Hawking Radiation
classification
✦ hep-th
gr-qc
keywords
blackconservationenergyholeapplicableapproximatelycannotconsider
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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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Cited by 1 Pith paper
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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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