Dark energy, dissipation, and the coincidence problem

In a recent paper we showed that a quintessence scalar field plus a dissipative matter fluid can drive late cosmic accelerated expansion and simultaneously solve the coincidence problem. In this Brief Report we extend this result to the cases when the scalar field is replaced either by a Chaplygin g...

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Detalles Bibliográficos
Publicado: 2003
Materias:
article
calculation
cosmos
density
energy
gravity
liquid
model
pressure
thermodynamics
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v67_n8_p_Chimento
http://hdl.handle.net/20.500.12110/paper_15507998_v67_n8_p_Chimento
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_15507998_v67_n8_p_Chimento
record_format dspace
spelling paper:paper_15507998_v67_n8_p_Chimento2023-06-08T16:21:52Z Dark energy, dissipation, and the coincidence problem article calculation cosmos density energy gravity liquid model pressure thermodynamics In a recent paper we showed that a quintessence scalar field plus a dissipative matter fluid can drive late cosmic accelerated expansion and simultaneously solve the coincidence problem. In this Brief Report we extend this result to the cases when the scalar field is replaced either by a Chaplygin gas or a tachyonic fluid. © 2003 The American Physical Society. 2003 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v67_n8_p_Chimento http://hdl.handle.net/20.500.12110/paper_15507998_v67_n8_p_Chimento
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic article
calculation
cosmos
density
energy
gravity
liquid
model
pressure
thermodynamics
spellingShingle article
calculation
cosmos
density
energy
gravity
liquid
model
pressure
thermodynamics
Dark energy, dissipation, and the coincidence problem
topic_facet article
calculation
cosmos
density
energy
gravity
liquid
model
pressure
thermodynamics
description In a recent paper we showed that a quintessence scalar field plus a dissipative matter fluid can drive late cosmic accelerated expansion and simultaneously solve the coincidence problem. In this Brief Report we extend this result to the cases when the scalar field is replaced either by a Chaplygin gas or a tachyonic fluid. © 2003 The American Physical Society.
title Dark energy, dissipation, and the coincidence problem
title_short Dark energy, dissipation, and the coincidence problem
title_full Dark energy, dissipation, and the coincidence problem
title_fullStr Dark energy, dissipation, and the coincidence problem
title_full_unstemmed Dark energy, dissipation, and the coincidence problem
title_sort dark energy, dissipation, and the coincidence problem
publishDate 2003
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v67_n8_p_Chimento
http://hdl.handle.net/20.500.12110/paper_15507998_v67_n8_p_Chimento
_version_ 1768542334372282368

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