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Black holes without firewalls
KTH, Centres, 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
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-124041DOI: 10.1103/PhysRevD.87.104018ISI: 000319127500005Scopus ID: 2-s2.0-84877947319OAI: oai:DiVA.org:kth-124041DiVA: diva2:633616
Note

QC 20130627

Available from: 2013-06-27 Created: 2013-06-25 Last updated: 2017-12-06Bibliographically approved

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