Causal dissipative Bianchi cosmology

Vittorio Romano; Diego Pavón

doi:10.1103/PhysRevD.47.1396

Causal dissipative Bianchi cosmology

Vittorio Romano, Diego Pavón

Departament de Física

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Resum

With the aid of causal thermodynamics, the Bianchi type-I cosmological model is analyzed under the assumption of plane symmetry. The initial anisotropy gets rapidly extinguished, and for an ample range of values of the parameters describing the cosmic fluid one has inflationary expansion. © 1993 The American Physical Society.

Idioma original	Anglès
Pàgines (de-a)	1396-1403
Revista	Physical Review D
Volum	47
DOIs	https://doi.org/10.1103/PhysRevD.47.1396
Estat de la publicació	Publicada - 1 de gen. 1993

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10.1103/PhysRevD.47.1396

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title = "Causal dissipative Bianchi cosmology",

abstract = "With the aid of causal thermodynamics, the Bianchi type-I cosmological model is analyzed under the assumption of plane symmetry. The initial anisotropy gets rapidly extinguished, and for an ample range of values of the parameters describing the cosmic fluid one has inflationary expansion. {\textcopyright} 1993 The American Physical Society.",

author = "Vittorio Romano and Diego Pav{\'o}n",

year = "1993",

month = jan,

day = "1",

doi = "10.1103/PhysRevD.47.1396",

language = "English",

volume = "47",

pages = "1396--1403",

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T1 - Causal dissipative Bianchi cosmology

AU - Romano, Vittorio

AU - Pavón, Diego

PY - 1993/1/1

Y1 - 1993/1/1

N2 - With the aid of causal thermodynamics, the Bianchi type-I cosmological model is analyzed under the assumption of plane symmetry. The initial anisotropy gets rapidly extinguished, and for an ample range of values of the parameters describing the cosmic fluid one has inflationary expansion. © 1993 The American Physical Society.

AB - With the aid of causal thermodynamics, the Bianchi type-I cosmological model is analyzed under the assumption of plane symmetry. The initial anisotropy gets rapidly extinguished, and for an ample range of values of the parameters describing the cosmic fluid one has inflationary expansion. © 1993 The American Physical Society.

U2 - 10.1103/PhysRevD.47.1396

DO - 10.1103/PhysRevD.47.1396

M3 - Article

SN - 0556-2821

VL - 47

SP - 1396

EP - 1403

JO - Physical Review D

JF - Physical Review D

ER -

Causal dissipative Bianchi cosmology

Resum

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