Dissipative effects in Bianchi type-III cosmologies

Vittorio Romano; Diego Pavn

doi:https://doi.org/10.1103/PhysRevD.50.2572

Dissipative effects in Bianchi type-III cosmologies

Vittorio Romano, Diego Pavn

Department of Physics

Research output: Contribution to journal › Article › Research › peer-review

30 Citations (Scopus)

Abstract

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 language	English
Pages (from-to)	2572-2580
Journal	Physical Review D
Volume	50
DOIs	https://doi.org/10.1103/PhysRevD.50.2572
Publication status	Published - 1 Jan 1994

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title = "Dissipative effects in Bianchi type-III cosmologies",

abstract = "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. {\textcopyright} 1994 The American Physical Society.",

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AB - 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.

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DO - https://doi.org/10.1103/PhysRevD.50.2572

M3 - Article

VL - 50

SP - 2572

EP - 2580

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Dissipative effects in Bianchi type-III cosmologies

Abstract

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