PSEUDO-NEWTONIAN GRAVITATIONAL POTENTIAL FOR SCHWARZSCHILD–DE SITTER SPACE–TIMES

DOI10.1142/S021827180801373XzbMath1184.83010arXiv0803.3641OpenAlexW3099172785MaRDI QIDQ3631021

Jiří Kovář, Zdeněk Stuchlík

Publication date: 5 June 2009

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0803.3641

zbMATH Keywords

black holecosmological constanteffective potentialgravitational potentialbound orbitsorbital energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (6)

Planetary orbital precession in pseudo-Newtonian potentials: reproduction of the general relativity orbital effect ⋮ Neutrino trapping in extremely compact objects described by the internal Schwarzschild-(anti-)de Sitter spacetimes ⋮ Equatorial circular orbits in Kerr-anti-de Sitter spacetimes ⋮ COMPARISON OF GENERAL RELATIVISTIC AND PSEUDO-NEWTONIAN DESCRIPTION OF MAGELLANIC-CLOUDS MOTION IN THE FIELD OF MILKY WAY ⋮ Aspects of GRMHD in high-energy astrophysics: geometrically thick disks and tori agglomerates around spinning black holes ⋮ MOTION OF CHARGED PARTICLES ON THE REISSNER–NORDSTRÖM (ANTI)-DE SITTER BLACK HOLE SPACETIME

Cites Work

• Optical reference geometry for stationary and static dynamics
• Dynamics of thick discs around Schwarzschild-de Sitter black holes
• FORCES IN KERR SPACE–TIMES WITH A REPULSIVE COSMOLOGICAL CONSTANT
• Optical reference geometry and inertial forces in Kerr–de Sitter spacetimes
• DYNAMICS OF DARK ENERGY
• INFLUENCE OF THE RELICT COSMOLOGICAL CONSTANT ON ACCRETION DISCS
• Optical reference geometry for stationary and axially symmetric spacetimes
• Relativistic thick discs in the Kerr–de Sitter backgrounds

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