Dissipative effects in Bianchi type-III cosmologies

Vittorio Romano, Diego Pavn

Research output: Contribution to journalArticleResearchpeer-review

30 Citations (Scopus)


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. © 1994 The American Physical Society.
Original languageEnglish
Pages (from-to)2572-2580
JournalPhysical Review D
Publication statusPublished - 1 Jan 1994


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