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Can black holes have Euclidean cores?

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Publication:2903557
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DOI10.1103/PhysRevD.68.044003zbMath1244.83020arXivhep-th/0303174MaRDI QIDQ2903557

Bob Holdom, Takayuki Hirayama

Publication date: 10 August 2012

Published in: Physical Review D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0303174

zbMATH Keywords

black holesEuclidean signature


Mathematics Subject Classification ID

Black holes (83C57)


Related Items

The tetralogy of Birkhoff theorems



Cites Work

  • Duality and the signature of space-time
  • Monopoles and the emergence of black hole entropy
  • The \(T\)-domain and extreme matter phases inside spherically symmetric black holes
  • Physically valid black hole interior models
  • No-go theorem for false vacuum black holes
  • Spacelike Brane Actions
  • Change of signature in classical relativity
  • Signature dynamics in general relativity
  • Cosmic Censorship: As Strong As Ever
  • TWILIGHT FOR THE ENERGY CONDITIONS?
  • Black holes, cosmological singularities and change of signature
  • Models of regular Schwarzschild black holes satisfying weak energy conditions
  • Classical Signature Change in the Black Hole Topology
  • Note on signature change and Colombeau theory
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