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The Persistence of the Large Volumes in Black Holes

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arxiv 1503.08245 v4 pith:DGN2LIC5 submitted 2015-03-27 gr-qc hep-th

Yen Chin Ong This is my paper · ORCID
classification gr-qchep-th
keywords blacklargevolumesextremalgrowholeholesinterior
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Classically, black holes admit maximal interior volumes that grow asymptotically linearly in time. We show that such volumes remain large when Hawking evaporation is taken into account. Even if a charged black hole approaches the extremal limit during this evolution, its volume continues to grow; although an exactly extremal black hole does not have a "large interior". We clarify this point and discuss the implications of our results to the information loss and firewall paradoxes.

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Cited by 1 Pith paper

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  1. Aspects of the Black Hole Interior Volume and Entropy

    gr-qc 2025-09 unverdicted novelty 2.0 of 10

    A doctoral thesis compiles and reproduces prior semiclassical results claiming the interior scalar-mode entropy of black holes is proportional to horizon entropy with a coefficient less than one.

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