Thermodynamics of a model of nonadiabatic spherical gravitational collapse

DOI10.1007/BF00658039zbMath0805.76099OpenAlexW1999864892MaRDI QIDQ1331345

V. Pereyra

Publication date: 21 August 1994

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00658039

zbMATH Keywords

diffusion approximationradiation transportdissipative relativistic fluidsFriedmann-like model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Thermodynamics and heat transfer (80A99) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (4)

Collapsing shear-free perfect fluid spheres with heat flow ⋮ Causal thermodynamics of a gravitational collapse model for an anisotropic fluid with dissipative flows ⋮ Gravitational collapse without a remnant ⋮ The gravitational field of a radiating and contracting spherically-symmetric body with heat flow

Cites Work

• Unnamed Item
• Isotropic solutions of the Einstein-Boltzmann equations
• Energy conditions for an imperfect fluid
• Quantum Cosmology. I
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid
• ‘Newtonian’ Time in General Relativity

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