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Pure states don't wear black

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Publication:1384844
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DOI10.1023/A:1018855611972zbMath0900.83015arXivgr-qc/9705065MaRDI QIDQ1384844

D. Massart

Publication date: 25 May 1998

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9705065


zbMATH Keywords

black hole formationquantum coherenceinformation loss paradoxblack hole evaporation


Mathematics Subject Classification ID

Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47)


Related Items

Generalized uncertainty principle: implications for black hole complementarity ⋮ Generating asymptotically plane wave spacetimes ⋮ Evolution of holographic entanglement entropy after thermal and electromagnetic quenches ⋮ Probable ratio of the vacuum energy in a Schwarzschild-de Sitter space ⋮ A quantum Rosetta Stone for the information paradox ⋮ AdS/CFT in the infinite momentum frame ⋮ Gödel incompleteness and the Black hole information paradox ⋮ Search for quantum gravity



Cites Work

  • Particle creation by black holes
  • Microscopic origin of the Bekenstein-Hawking entropy
  • \(D\)-brane approach to black hole quantum mechanics
  • Comparing decay rates for black holes and D-branes
  • The four laws of black hole mechanics
  • Black Holes and Entropy
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