Energy Conservation and Hawking Radiation

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.

6 pages, LaTex; v2: references added

References in corpus (3)

• Radiation via Tunneling from a de Sitter Cosmological Horizon
• New Coordinates for de Sitter Space and de Sitter Radiation
• Semiclassical Corrections to the Bekenstein-Hawking entropy of the BTZ Black Hole via Self-Gravitation

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• Planck-scale nonthermal correlations in a noncommutative geometry inspired Vaidya black hole
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