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Phase transition in Schwarzschild-de Sitter spacetime

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Publication:1008420
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DOI10.1007/s10509-008-9883-7zbMath1161.83375arXiv0903.0081OpenAlexW2143646042MaRDI QIDQ1008420

J. Martínez

Publication date: 27 March 2009

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0903.0081

zbMATH Keywords

gravitydark matterscalar fielddark energy


Mathematics Subject Classification ID

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


Related Items

A cosmology governed by a fractional differential equation and the generalized Kilbas-Saigo-Mittag-Leffler function, Inflation driven by \(q\)-de Sitter, A NOTE ON CONSTANT CURVATURE SOLUTIONS IN CYLINDRICALLY SYMMETRIC METRIC f(R) GRAVITY, EXACT SOLUTION FOR THE MASSLESS CYLINDRICALLY SYMMETRIC SCALAR FIELD IN GENERAL RELATIVITY, WITH COSMOLOGICAL CONSTANT



Cites Work

  • Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
  • On the spherical collapse model in dark energy cosmologies
  • Galactic collapse of scalar field dark matter
  • Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
  • Hessence: a new view of quintom dark energy
  • An alternative to quintessence
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