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Black holes without firewalls · Around

2012

Black holes without firewalls

Larjo, Klaus, Lowe, David A., Thorlacius, Larus

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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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