COMPARISON OF GENERAL RELATIVISTIC AND PSEUDO-NEWTONIAN DESCRIPTION OF MAGELLANIC-CLOUDS MOTION IN THE FIELD OF MILKY WAY

DOI10.1142/S0218271812500319zbMath1263.85015OpenAlexW1979910143MaRDI QIDQ4911485

Jan Schee, Zdeněk Stuchlík

Publication date: 15 March 2013

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

Full work available at URL: https://doi.org/10.1142/s0218271812500319

zbMATH Keywords

general relativityMilky Waypseudo-Newtonian potentialMagellanic Clouds

Mathematics Subject Classification ID

Black holes (83C57) 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 (4)

Supermassive black holes surrounded by dark matter modeled as anisotropic fluid: epicyclic oscillations and their fitting to observed QPOs ⋮ Equatorial circular orbits in Kerr-anti-de Sitter spacetimes ⋮ Gravitational lensing and frame dragging of light in the Kerr-Newman and the Kerr-Newman (anti) de Sitter black hole spacetimes ⋮ Multi-transonic spherical-type flows around massive black holes: galactic potential induced standing isothermal shocks

Cites Work

• A two-mass expanding exact space-time solution
• Geodesic portrait of de Sitter-Schwarzschild space-time
• Precise analytic treatment of Kerr and Kerr-(anti) de Sitter black holes as gravitational lenses
• Dynamics of thick discs around Schwarzschild-de Sitter black holes
• Frame dragging and bending of light in Kerr and Kerr–(anti) de Sitter spacetimes
• Periapsis and gravitomagnetic precessions of stellar orbits in Kerr and Kerr–de Sitter black hole spacetimes
• PSEUDO-NEWTONIAN GRAVITATIONAL POTENTIAL FOR SCHWARZSCHILD–DE SITTER SPACE–TIMES
• Pseudo-Newtonian and general relativistic barotropic tori in Schwarzschild–de Sitter spacetimes
• Equatorial photon motion in the Kerr-Newman spacetimes with a non-zero cosmological constant
• INFLUENCE OF THE RELICT COSMOLOGICAL CONSTANT ON ACCRETION DISCS
• Relativistic thick discs in the Kerr–de Sitter backgrounds

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