Empty black holes, firewalls, and the origin of Bekenstein–Hawking entropy
DOI10.1142/S021827181443007XzbMath1314.83032arXiv1212.4176OpenAlexW2963708302WikidataQ60721041 ScholiaQ60721041MaRDI QIDQ5252778
Mehdi Saravani, Niayesh Afshordi, Robert B. Mann
Publication date: 3 June 2015
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1212.4176
Black holes (83C57) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Measures of information, entropy (94A17) Quantum information, communication, networks (quantum-theoretic aspects) (81P45)
Related Items (13)
Cites Work
- Black holes as incompressible fluids on the sphere
- Wilsonian approach to fluid/gravity duality
- Ten theses on black hole entropy
- Tunneling into fuzzball states
- Instability of the Kaluza-Klein vacuum
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- The information paradox: a pedagogical introduction
- HOW FAST CAN A BLACK HOLE RELEASE ITS INFORMATION?
- The cosmological constant problem
- The self-screening Hawking atmosphere -- a different approach to quantum black hole microstates
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