A shearing non-adiabatic solution of Einstein's equations
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Publication:1299795
DOI10.1023/A:1001515109762zbMath0929.76149OpenAlexW1631556308MaRDI QIDQ1299795
Publication date: 2 February 2000
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1023/a:1001515109762
analytical solutionpressuredensitymassluminosityisotropic fluidcollapsing radiating bodyradial heat flow
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (8)
Imperfect fluid cosmology with heat flow ⋮ RADIATING GRAVITATIONAL COLLAPSE WITH SHEAR VISCOSITY AND BULK VISCOSITY ⋮ Causal thermodynamics of a gravitational collapse model for an anisotropic fluid with dissipative flows ⋮ Some cosmological models with heat and null radiation flow ⋮ RADIATING GRAVITATIONAL COLLAPSE WITH SHEAR REVISITED ⋮ Radiating gravitational collapse with shear viscosity revisited ⋮ Radiating gravitational collapse with an initial inhomogeneous energy density distribution ⋮ RADIATING GRAVITATIONAL COLLAPSE WITH SHEARING MOTION AND BULK VISCOSITY REVISITED
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