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arXiv · 1211.4620

Black holes without firewalls

Klaus Larjo·David A. Lowe·Larus Thorlacius
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Abstract

The postulates of black hole complementarity do not imply a firewall for infalling observers at a black hole horizon. The dynamics of the stretched horizon, that scrambles and re-emits information, determines whether infalling observers experience anything out of the ordinary when entering a large black hole. In particular, there is no firewall if the stretched horizon degrees of freedom retain information for a time of order the black hole scrambling time.

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Klaus Larjo, David A. Lowe, Larus Thorlacius. 2013-06-21. Black holes without firewalls. https://doi.org/10.1103/physrevd.87.104018

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