Relaxation versus collision times in the cosmological radiative era

DOI10.1088/0264-9381/18/9/302zbMath0984.83055arXivgr-qc/0103053OpenAlexW2009696913MaRDI QIDQ2724792

Roberto A. Sussman, Diego Pavón

Publication date: 14 May 2002

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0103053

zbMATH Keywords

viscous fluid sourceLemaître-Tolman-Bondi metriccosmological radiative era

Mathematics Subject Classification ID

Supergravity (83E50) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (3)

Causal heat flow in Bianchi type-V Universe ⋮ Hyperbolic theories of dissipation: Why and when do we need them? ⋮ Adiabatic models of the cosmological radiative era

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