Self-similar relativistic discs with pressure

DOI10.1088/0264-9381/6/9/007zbMath0672.76123OpenAlexW2060127955MaRDI QIDQ3826310

José P. S. Lemos

Publication date: 1989

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/0264-9381/6/9/007

zbMATH Keywords

WKB approximationspacetimesinertial framesself-similar relativistic discsself-similar stationary

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

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Exact relativistic magnetized haloes around rotating disks ⋮ Stability of general relativistic static thick disks: the isotropic Schwarzschild thick disk ⋮ Lensing and shadow of a black hole surrounded by a heavy accretion disk ⋮ Exact relativistic models of conformastatic charged dust thick disks ⋮ Planar and axisymmetric walls in general relativity, a comparison ⋮ An infinite family of magnetized Morgan-Morgan relativistic thin disks ⋮ General magnetized Weyl solutions: disks and motion of charged particles ⋮ Exact relativistic models of perfect fluid disks in a magnetic field ⋮ EXACT RELATIVISTIC MODELS OF THIN DISKS AROUND STATIC BLACK HOLES IN A MAGNETIC FIELD ⋮ Models of spherical shells as sources of Majumdar-Papapetrou type spacetimes ⋮ Topological defects with axial symmetry: A disk + a string ⋮ Three-dimensional axisymmetric sources for Majumdar–Papapetrou type spacetimes ⋮ ROTATING RELATIVISTIC THIN DISKS AS SOURCES OF CHARGED AND MAGNETIZED KERR–NUT SPACE–TIMES

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