Information recovery from evaporating black holes

Abstract

We show that the apparent horizon and the region near $r=0$ of an evaporating charged, rotating black hole are timelike. It then follows that for black holes in nature, which invariably have some rotation, have a channel, via which classical or quantum information can escape to the outside, while the black hole shrinks in size. We discuss implications for the information loss problem.

arXiv commentMinor typos corrected, version to match the published version in the International Journal of Modern Physics D

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• Quasinormal modes of anyons
• Hawking radiation of anyons