Ingoing Eddington-Finkelstein Metric of an Evaporating Black Hole

We present an approximate time-dependent metric in ingoing Eddington-Finkelstein coordinates for an evaporating nonrotating black hole as a first-order perturbation of the Schwarzschild metric, using the linearized back reaction from a realistic approximation to the stress-energy tensor for the Hawk...

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Veröffentlicht in:	arXiv.org 2019-12
Hauptverfasser:	Abdolrahimi, Shohreh, Page, Don N, Tzounis, Christos
Format:	Artikel
Sprache:	eng
Schlagworte:	Black holes Hawking radiation Perturbation Physics - General Relativity and Quantum Cosmology Physics - High Energy Physics - Theory Schwarzschild metric Tensors Time dependence
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Zusammenfassung:	We present an approximate time-dependent metric in ingoing Eddington-Finkelstein coordinates for an evaporating nonrotating black hole as a first-order perturbation of the Schwarzschild metric, using the linearized back reaction from a realistic approximation to the stress-energy tensor for the Hawking radiation in the Unruh quantum state.
ISSN:	2331-8422
DOI:	10.48550/arxiv.1607.05280