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Pure states and black hole complementarity
KTH, Centres, Nordic Institute for Theoretical Physics NORDITA.
2013 (English)In: Physical Review D, ISSN 1550-7998, Vol. 88, no 4, 044012- p.Article in journal (Refereed) Published
Abstract [en]

The future apparent horizon of a black hole develops large stress energy due to quantum effects, unless the outgoing modes are in a thermal density matrix at the local Hawking temperature. It is shown for generic pure states that the deviation from thermality is so small that infalling observers will see no drama on their way to the stretched horizon, providing a derivation of black hole complementarity after the Page time. Atypical pure states, and atypical observers, may of course see surprises, but that is not surprising.

Place, publisher, year, edition, pages
2013. Vol. 88, no 4, 044012- p.
National Category
Physical Sciences
URN: urn:nbn:se:kth:diva-127750DOI: 10.1103/PhysRevD.88.044012ISI: 000322785700001ScopusID: 2-s2.0-84884825748OAI: diva2:646362

QC 20130909

Available from: 2013-09-09 Created: 2013-09-05 Last updated: 2013-09-09Bibliographically approved

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Thorlacius, Larus
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