Qualitative Viscous Cosmology
arXiv:gr-qc/9605063 · doi:10.1103/PhysRevD.54.1393
Abstract
The Full (non--truncated) Israel--Stewart theory of bulk viscosity is applied to dissipative FRW spacetimes. Dimensionless variables and dimensionless equations of state are used to write the Einstein--thermodynamic equations as a plane autonomous system and the qualitative behaviour of this system is determined. Entropy production in these models is also discussed.
13 pages, REVTeX, accepted for publication in Physical Review D
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Cited by in corpus (34)
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