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arXiv · 1506.08075

Free fall onto evaporating black holes at the quantum limit

Maurice H. P. M. van Putten
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Abstract

Black hole space times evaporate in discrete steps due to remarkably slow Hawking radiation. We here identify evaporation with essentially extremal states at the limit of quantum computation, performing $2.7\times 10^{79}$ bit calculations per photon emission in a one solar mass black hole. During evaporation, particles in free fall co-evolve satisfying $EM=$constant, where $E$ and $M$ denote the total mass energy-at-infinity of the particle and, respectively, black hole. Particles are hereby increasingly entangled with the black hole space-time over the course of its evaporation.

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Maurice H. P. M. van Putten. 2015-06-25. Free fall onto evaporating black holes at the quantum limit. https://arxiv.org/abs/1506.08075

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