Relativistic thick discs in the Kerr–de Sitter backgrounds
From MaRDI portal
Publication:5696074
DOI10.1088/0264-9381/22/17/019zbMath1089.83019OpenAlexW1483334018MaRDI QIDQ5696074
Publication date: 7 October 2005
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0264-9381/22/17/019
Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar dynamics (85A05)
Related Items (9)
Proto-jet configurations in RADs orbiting a Kerr SMBH: symmetries and limiting surfaces ⋮ 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 ⋮ Charged fluids encircling compact objects: force representations and conformal geometries ⋮ PSEUDO-NEWTONIAN GRAVITATIONAL POTENTIAL FOR SCHWARZSCHILD–DE SITTER SPACE–TIMES ⋮ Shadow of the rotating black hole with quintessential energy in the presence of plasma ⋮ Aspects of GRMHD in high-energy astrophysics: geometrically thick disks and tori agglomerates around spinning black holes ⋮ RELATIVISTIC DYNAMICS WITH COSMOLOGICAL CONSTANT: SPINNING TEST PARTICLES AND PERFECT FLUID TORI ⋮ Retrograde polish doughnuts around boson stars
This page was built for publication: Relativistic thick discs in the Kerr–de Sitter backgrounds