Brane cosmology as a dynamical system
We investigate the qualitative dynamical properties of a brane model for the flat isotropic universe with a single matter component represented by a scalar field. We study the flat and quadratic potential. Three classes of behaviors of the scale factor are determined. In particular, in the case of t...
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2004
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v70_n4A_p_Lara http://hdl.handle.net/20.500.12110/paper_05562821_v70_n4A_p_Lara |
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paper:paper_05562821_v70_n4A_p_Lara2023-06-08T15:42:34Z Brane cosmology as a dynamical system article cosmos dynamics mathematical analysis oscillation radiation space We investigate the qualitative dynamical properties of a brane model for the flat isotropic universe with a single matter component represented by a scalar field. We study the flat and quadratic potential. Three classes of behaviors of the scale factor are determined. In particular, in the case of the brane with dark negative radiation, via a fine tuning, the existence of oscillatory solutions is shown, which is not possible in the traditional flat FRW model. © 2004 The American Physical Society. 2004 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v70_n4A_p_Lara http://hdl.handle.net/20.500.12110/paper_05562821_v70_n4A_p_Lara |
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 cosmos dynamics mathematical analysis oscillation radiation space |
spellingShingle |
article cosmos dynamics mathematical analysis oscillation radiation space Brane cosmology as a dynamical system |
topic_facet |
article cosmos dynamics mathematical analysis oscillation radiation space |
description |
We investigate the qualitative dynamical properties of a brane model for the flat isotropic universe with a single matter component represented by a scalar field. We study the flat and quadratic potential. Three classes of behaviors of the scale factor are determined. In particular, in the case of the brane with dark negative radiation, via a fine tuning, the existence of oscillatory solutions is shown, which is not possible in the traditional flat FRW model. © 2004 The American Physical Society. |
title |
Brane cosmology as a dynamical system |
title_short |
Brane cosmology as a dynamical system |
title_full |
Brane cosmology as a dynamical system |
title_fullStr |
Brane cosmology as a dynamical system |
title_full_unstemmed |
Brane cosmology as a dynamical system |
title_sort |
brane cosmology as a dynamical system |
publishDate |
2004 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v70_n4A_p_Lara http://hdl.handle.net/20.500.12110/paper_05562821_v70_n4A_p_Lara |
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1768543185004396544 |