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Ingoing Eddington-Finkelstein Metric of an Evaporating Black Hole

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arxiv 1607.05280 v4 pith:BTNF6TF2 submitted 2016-07-18 hep-th gr-qc

Shohreh Abdolrahimi , Don N. Page , Christos Tzounis This is my paper · ORCID
classification hep-thgr-qc
keywords metricblackeddington-finkelsteinevaporatingholeingoingapproximateapproximation
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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.

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  1. Evaporating universes

    hep-th 2025-07 conditional novelty 6.0 of 10

    A toy model using four-dimensional Brill-Lindquist wormholes reproduces the Page curve for black hole evaporation and shows Hawking-radiation decoding complexity falls to polynomial at late times.

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