Exact scalar field cosmologies in (1+1) dimensions
We report a series of exact cosmological solutions of the gravitational (1+1)-dimensional equations with a classical scalar field and an isotropic perfect fluid source. We consider a Robertson - Walker universe and obtain the scale factor and the field for several physically interesting potentials....
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todo:paper_02649381_v11_n5_p1177_Chimento2023-10-03T15:13:06Z Exact scalar field cosmologies in (1+1) dimensions Chimento, L.P. Cossarini, A.E. We report a series of exact cosmological solutions of the gravitational (1+1)-dimensional equations with a classical scalar field and an isotropic perfect fluid source. We consider a Robertson - Walker universe and obtain the scale factor and the field for several physically interesting potentials. In the case of a non-vanishing positive cosmological constant , we have found asymptotically de Sitter solutions which resemble the (3+1)-dimensional results. When we have to take restrictive conditions on the sign of the potential function in order to obtain exactly solvable models which include exponential inflationary processes. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Cossarini, A.E. 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_02649381_v11_n5_p1177_Chimento |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
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R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
We report a series of exact cosmological solutions of the gravitational (1+1)-dimensional equations with a classical scalar field and an isotropic perfect fluid source. We consider a Robertson - Walker universe and obtain the scale factor and the field for several physically interesting potentials. In the case of a non-vanishing positive cosmological constant , we have found asymptotically de Sitter solutions which resemble the (3+1)-dimensional results. When we have to take restrictive conditions on the sign of the potential function in order to obtain exactly solvable models which include exponential inflationary processes. |
format |
JOUR |
author |
Chimento, L.P. Cossarini, A.E. |
spellingShingle |
Chimento, L.P. Cossarini, A.E. Exact scalar field cosmologies in (1+1) dimensions |
author_facet |
Chimento, L.P. Cossarini, A.E. |
author_sort |
Chimento, L.P. |
title |
Exact scalar field cosmologies in (1+1) dimensions |
title_short |
Exact scalar field cosmologies in (1+1) dimensions |
title_full |
Exact scalar field cosmologies in (1+1) dimensions |
title_fullStr |
Exact scalar field cosmologies in (1+1) dimensions |
title_full_unstemmed |
Exact scalar field cosmologies in (1+1) dimensions |
title_sort |
exact scalar field cosmologies in (1+1) dimensions |
url |
http://hdl.handle.net/20.500.12110/paper_02649381_v11_n5_p1177_Chimento |
work_keys_str_mv |
AT chimentolp exactscalarfieldcosmologiesin11dimensions AT cossariniae exactscalarfieldcosmologiesin11dimensions |
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1807322995333529600 |