Spherically symmetric space-time with two cosmological constants.

DOI10.1023/A:1026619228583zbMath1047.83505OpenAlexW31742024MaRDI QIDQ1807311

I. G. Dymnikova, B. Sołtysek

Publication date: 18 November 1999

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

Full work available at URL: https://doi.org/10.1023/a:1026619228583

Mathematics Subject Classification ID

Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (13)

DE-DM unification based on space-time symmetry ⋮ A new regular black hole ⋮ Lemaître dark energy model singled out by the holographic principle ⋮ Thermodynamics of horizons in a globally regular spherically symmetric spacetime ⋮ Thermodynamics of regular cosmological black holes with the de Sitter interior ⋮ Graviatoms with de Sitter interior ⋮ Gravastar: An alternative to black hole ⋮ Thermodynamics of regular cosmological black holes with de Sitter interior ⋮ Vacuum solitons with a de Sitter center as dark matter candidates ⋮ Possibilities and surprises of vacuum dark fluid ⋮ Geodesic portrait of de Sitter-Schwarzschild space-time ⋮ Hawking radiation as a possible probe for the interior structure of regular black holes ⋮ TRIPLE-HORIZON SPHERICALLY SYMMETRIC SPACETIME AND HOLOGRAPHIC PRINCIPLE

Cites Work

• Physics of black holes. Transl. from the Russian by V. I. Kisin and E. M. Yankovsky
• General Relativity
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