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Black holes without firewalls
Stockholm University, Nordic Institute for Theoretical Physics (Nordita).
2013 (English)In: Physical Review D, ISSN 1550-7998, E-ISSN 1550-2368, Vol. 87, no 10, 104018- p.Article in journal (Refereed) Published
Abstract [en]

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 reemits 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 the order of the black hole scrambling time.

Place, publisher, year, edition, pages
2013. Vol. 87, no 10, 104018- p.
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-91191DOI: 10.1103/PhysRevD.87.104018ISI: 000319127500005OAI: oai:DiVA.org:su-91191DiVA: diva2:632111
Note

AuthorCount:3;

Available from: 2013-06-24 Created: 2013-06-24 Last updated: 2017-12-06Bibliographically approved

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