Dissipative cosmological solutions
The exact general solution to the Einstein equations in a homogeneous Universe with a full causal viscous fluid source for the bulk viscosity index m = 1/2 is found. We have investigated the asymptotic stability of Friedmann and de Sitter solutions, the former is stable for m ≥ 1/2 and the latter fo...
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1997
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paper:paper_02649381_v14_n7_p1811_Chimento2023-06-08T15:23:20Z Dissipative cosmological solutions Chimento, Luis Pascual Jakubi, Alejandro Silvio The exact general solution to the Einstein equations in a homogeneous Universe with a full causal viscous fluid source for the bulk viscosity index m = 1/2 is found. We have investigated the asymptotic stability of Friedmann and de Sitter solutions, the former is stable for m ≥ 1/2 and the latter for m ≤ 1/2. The comparison with results of the truncated theory is made. For m = 1/2, it was found that families of solutions with extrema no longer remain in the full case and they are replaced by asymptotically Minkowski evolutions. These solutions are monotonic. 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. 1997 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02649381_v14_n7_p1811_Chimento http://hdl.handle.net/20.500.12110/paper_02649381_v14_n7_p1811_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 exact general solution to the Einstein equations in a homogeneous Universe with a full causal viscous fluid source for the bulk viscosity index m = 1/2 is found. We have investigated the asymptotic stability of Friedmann and de Sitter solutions, the former is stable for m ≥ 1/2 and the latter for m ≤ 1/2. The comparison with results of the truncated theory is made. For m = 1/2, it was found that families of solutions with extrema no longer remain in the full case and they are replaced by asymptotically Minkowski evolutions. These solutions are monotonic. |
author |
Chimento, Luis Pascual Jakubi, Alejandro Silvio |
spellingShingle |
Chimento, Luis Pascual Jakubi, Alejandro Silvio Dissipative cosmological solutions |
author_facet |
Chimento, Luis Pascual Jakubi, Alejandro Silvio |
author_sort |
Chimento, Luis Pascual |
title |
Dissipative cosmological solutions |
title_short |
Dissipative cosmological solutions |
title_full |
Dissipative cosmological solutions |
title_fullStr |
Dissipative cosmological solutions |
title_full_unstemmed |
Dissipative cosmological solutions |
title_sort |
dissipative cosmological solutions |
publishDate |
1997 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02649381_v14_n7_p1811_Chimento http://hdl.handle.net/20.500.12110/paper_02649381_v14_n7_p1811_Chimento |
work_keys_str_mv |
AT chimentoluispascual dissipativecosmologicalsolutions AT jakubialejandrosilvio dissipativecosmologicalsolutions |
_version_ |
1768541607834943488 |