Two-fluid atmosphere for relativistic stars
From MaRDI portal
Publication:4699921
DOI10.1088/0264-9381/16/4/007zbMath0942.83023arXivgr-qc/9901034OpenAlexW3106098823MaRDI QIDQ4699921
Publication date: 18 November 1999
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/9901034
Einstein's field equationsanalytic solutionsstring fluidSchwarzschild vacuumValidya radiating mettric
String and superstring theories in gravitational theory (83E30) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Related Items
Scale symmetries of spherical string fluids ⋮ Radiating stars with generalised Vaidya atmospheres ⋮ Radiating fluid sphere immersed in an anisotropic atmosphere ⋮ Stability and horizon formation during dissipative collapse ⋮ Wavefronts in a relativistic two-phase turbulent flow ⋮ Non-equilibrium relativistic two-phase flow with heat exchange ⋮ Diffusive and dynamical radiating stars with realistic equations of state ⋮ CHARGED BLACK HOLES IN VAIDYA BACKGROUNDS: HAWKING'S RADIATION ⋮ EXACT NONSPHERICAL RELATIVISTIC STAR ⋮ Conformal symmetries in generalised Vaidya spacetimes ⋮ Radiating black hole solutions in arbitrary dimensions ⋮ Dimension in a radiative stellar atmosphere. ⋮ NONSPHERICAL COLLAPSE OF TWO-FLUID STAR ⋮ Vaidya-Bonnor black hole in monopole-de Sitter space with variable \(\varLambda (u)\) ⋮ Schwarzschild atmospheric processes: A classical path to the quantum ⋮ Energy transport in the Vaidya system
