Inhomogeneous cosmologies with Q matter and varying Λ

Starting from the inhomogeneous shear-free Nariai metric we show, by solving the Einstein-Klein-Gordon field equations, how a self-interacting scalar field plus a material fluid, a variable cosmological term, and a heat flux can drive the universe to its currently observed state of homogeneous accel...

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Autores principales: Chimento, L.P., Jakubi, A.S., Pavón, D.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_05562821_v60_n10_p1_Chimento
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spelling todo:paper_05562821_v60_n10_p1_Chimento2023-10-03T15:35:37Z Inhomogeneous cosmologies with Q matter and varying Λ Chimento, L.P. Jakubi, A.S. Pavón, D. Starting from the inhomogeneous shear-free Nariai metric we show, by solving the Einstein-Klein-Gordon field equations, how a self-interacting scalar field plus a material fluid, a variable cosmological term, and a heat flux can drive the universe to its currently observed state of homogeneous accelerated expansion. A quintessence scenario where power-law inflation takes place for a string-motivated potential in the late-time dominated field regime is proposed. ©1999 The American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_05562821_v60_n10_p1_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 Starting from the inhomogeneous shear-free Nariai metric we show, by solving the Einstein-Klein-Gordon field equations, how a self-interacting scalar field plus a material fluid, a variable cosmological term, and a heat flux can drive the universe to its currently observed state of homogeneous accelerated expansion. A quintessence scenario where power-law inflation takes place for a string-motivated potential in the late-time dominated field regime is proposed. ©1999 The American Physical Society.
format JOUR
author Chimento, L.P.
Jakubi, A.S.
Pavón, D.
spellingShingle Chimento, L.P.
Jakubi, A.S.
Pavón, D.
Inhomogeneous cosmologies with Q matter and varying Λ
author_facet Chimento, L.P.
Jakubi, A.S.
Pavón, D.
author_sort Chimento, L.P.
title Inhomogeneous cosmologies with Q matter and varying Λ
title_short Inhomogeneous cosmologies with Q matter and varying Λ
title_full Inhomogeneous cosmologies with Q matter and varying Λ
title_fullStr Inhomogeneous cosmologies with Q matter and varying Λ
title_full_unstemmed Inhomogeneous cosmologies with Q matter and varying Λ
title_sort inhomogeneous cosmologies with q matter and varying λ
url http://hdl.handle.net/20.500.12110/paper_05562821_v60_n10_p1_Chimento
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AT pavond inhomogeneouscosmologieswithqmatterandvaryingl
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