Geodesic portrait of de Sitter-Schwarzschild space-time

DOI10.1134/S0202289308030092zbMath1153.83356MaRDI QIDQ954177

B. Sołtysek, A. Poszwa, I. G. Dymnikova

Publication date: 10 November 2008

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Mathematics Subject Classification ID

Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (2)

Vacuum solitons with a de Sitter center as dark matter candidates ⋮ COMPARISON OF GENERAL RELATIVISTIC AND PSEUDO-NEWTONIAN DESCRIPTION OF MAGELLANIC-CLOUDS MOTION IN THE FIELD OF MILKY WAY

Cites Work

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• Vacuum dark fluid
• Effects of a positive cosmological constant on circular orbits in the Reissner-Nordstroem, Schwarzschild, and Kerr fields
• Stability of the vacuum non-singular black hole.
• Spherically symmetric space-time with two cosmological constants.
• Regular electrically charged vacuum structures with de Sitter centre in nonlinear electrodynamics coupled to general relativity
• The cosmological term as a source of mass
• Nonsingular vacuum cosmologies with a variable cosmological term
• Stability of a vacuum non-singular black hole
• General Relativity
• The algebraic structure of a cosmological term in spherically symmetric solutions

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