Dissipative effects in Bianchi type-III cosmologies

Vittorio Romano; Diego Pavn

doi:10.1103/PhysRevD.50.2572

Dissipative effects in Bianchi type-III cosmologies

Vittorio Romano, Diego Pavn

Departament de Física

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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.

Idioma original	Anglès
Pàgines (de-a)	2572-2580
Revista	Physical Review D
Volum	50
DOIs	https://doi.org/10.1103/PhysRevD.50.2572
Estat de la publicació	Publicada - 1 de gen. 1994

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10.1103/PhysRevD.50.2572

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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.",

author = "Vittorio Romano and Diego Pavn",

year = "1994",

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day = "1",

doi = "10.1103/PhysRevD.50.2572",

language = "English",

volume = "50",

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TY - JOUR

T1 - Dissipative effects in Bianchi type-III cosmologies

AU - Romano, Vittorio

AU - Pavn, Diego

PY - 1994/1/1

Y1 - 1994/1/1

N2 - 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.

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.

U2 - 10.1103/PhysRevD.50.2572

DO - 10.1103/PhysRevD.50.2572

M3 - Article

SN - 0556-2821

VL - 50

SP - 2572

EP - 2580

JO - Physical Review D

JF - Physical Review D

ER -

Dissipative effects in Bianchi type-III cosmologies

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