Dissipative effects in Bianchi type-III cosmologies

Details Dissipative effects in Bianchi type-III cosmologies Dissipative effects in Bianchi type-III cosmologies

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvd..50.2572r&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 50, Issue 4, 15 August 1994, pp.2572-2580

Mathematics

Logic

27

Einstein-Maxwell Spacetimes, Spacetimes With Fluids, Radiation Or Classical Fields

Scientific paper

Both the truncated and the full version of the causal thermodynamic
theory of nonequilibrium phenomena are used to study the evolution of a
Bianchi type-III cosmological model. The initial anisotropy dies away
rapidly and the de Sitter solutions are stable while the Friedmann ones
are not.

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