Relaxation dominated cosmological expansion
The behavior near the singularity of an isotropic, homogeneous cosmological model with a viscous fluid source is investigated. This turns out to be a relaxation dominated regime. Full extended irreversible thermodynamics is used, and a comparison with results of the truncated theory is made. New sin...
Guardado en:
Autores principales: | , |
---|---|
Formato: | JOUR |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03759601_v212_n6_p320_Chimento |
Aporte de: |
id |
todo:paper_03759601_v212_n6_p320_Chimento |
---|---|
record_format |
dspace |
spelling |
todo:paper_03759601_v212_n6_p320_Chimento2023-10-03T15:30:59Z Relaxation dominated cosmological expansion Chimento, L.P. Jakubi, A.S. The behavior near the singularity of an isotropic, homogeneous cosmological model with a viscous fluid source is investigated. This turns out to be a relaxation dominated regime. Full extended irreversible thermodynamics is used, and a comparison with results of the truncated theory is made. New singular behaviors are found and it is shown that a relaxation dominated inflationary epoch may exist for fluids with a small heat capacity. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Jakubi, A.S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03759601_v212_n6_p320_Chimento |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
The behavior near the singularity of an isotropic, homogeneous cosmological model with a viscous fluid source is investigated. This turns out to be a relaxation dominated regime. Full extended irreversible thermodynamics is used, and a comparison with results of the truncated theory is made. New singular behaviors are found and it is shown that a relaxation dominated inflationary epoch may exist for fluids with a small heat capacity. |
format |
JOUR |
author |
Chimento, L.P. Jakubi, A.S. |
spellingShingle |
Chimento, L.P. Jakubi, A.S. Relaxation dominated cosmological expansion |
author_facet |
Chimento, L.P. Jakubi, A.S. |
author_sort |
Chimento, L.P. |
title |
Relaxation dominated cosmological expansion |
title_short |
Relaxation dominated cosmological expansion |
title_full |
Relaxation dominated cosmological expansion |
title_fullStr |
Relaxation dominated cosmological expansion |
title_full_unstemmed |
Relaxation dominated cosmological expansion |
title_sort |
relaxation dominated cosmological expansion |
url |
http://hdl.handle.net/20.500.12110/paper_03759601_v212_n6_p320_Chimento |
work_keys_str_mv |
AT chimentolp relaxationdominatedcosmologicalexpansion AT jakubias relaxationdominatedcosmologicalexpansion |
_version_ |
1782026940138389504 |