K-essence and extended tachyons in brane-worlds
We study a k-essence field evolving linearly with the cosmic time and the atypical k-essence model on a homogeneous and isotropic flat 3-brane. We show that the k-field is driven by an inverse quadratic polynomial potential. The solutions represent expanding, contracting or bouncing universes with a...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_17426588_v229_n_p_Chimento |
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paperaa:paper_17426588_v229_n_p_Chimento2023-06-12T16:51:01Z K-essence and extended tachyons in brane-worlds J. Phys. Conf. Ser. 2010;229 Chimento, L.P. Richarte, M.G. Cosmology Big Crunch Finite time Homogeneous and isotropic Kinetic functions Low-energy limit Negative energy density Quadratic polynomial Tachyon fields Control equipment We study a k-essence field evolving linearly with the cosmic time and the atypical k-essence model on a homogeneous and isotropic flat 3-brane. We show that the k-field is driven by an inverse quadratic polynomial potential. The solutions represent expanding, contracting or bouncing universes with a finite time span and some of them end in a big crunch or a big rip. Besides, by selecting the extended tachyonic kinetic functions we analyze the high and low energy limits of our model, obtaining the nearly power law solution. We introduce a tachyon field with negative energy density and show that the universe evolves between two singularities. © 2010 IOP Publishing Ltd. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Richarte, M.G. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2010 info:eu-repo/semantics/conferenceObject info:ar-repo/semantics/documento de conferencia info:eu-repo/semantics/publishedVersion application/pdf eng info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17426588_v229_n_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) |
language |
Inglés |
orig_language_str_mv |
eng |
topic |
Cosmology Big Crunch Finite time Homogeneous and isotropic Kinetic functions Low-energy limit Negative energy density Quadratic polynomial Tachyon fields Control equipment |
spellingShingle |
Cosmology Big Crunch Finite time Homogeneous and isotropic Kinetic functions Low-energy limit Negative energy density Quadratic polynomial Tachyon fields Control equipment Chimento, L.P. Richarte, M.G. K-essence and extended tachyons in brane-worlds |
topic_facet |
Cosmology Big Crunch Finite time Homogeneous and isotropic Kinetic functions Low-energy limit Negative energy density Quadratic polynomial Tachyon fields Control equipment |
description |
We study a k-essence field evolving linearly with the cosmic time and the atypical k-essence model on a homogeneous and isotropic flat 3-brane. We show that the k-field is driven by an inverse quadratic polynomial potential. The solutions represent expanding, contracting or bouncing universes with a finite time span and some of them end in a big crunch or a big rip. Besides, by selecting the extended tachyonic kinetic functions we analyze the high and low energy limits of our model, obtaining the nearly power law solution. We introduce a tachyon field with negative energy density and show that the universe evolves between two singularities. © 2010 IOP Publishing Ltd. |
format |
Documento de conferencia Documento de conferencia publishedVersion |
author |
Chimento, L.P. Richarte, M.G. |
author_facet |
Chimento, L.P. Richarte, M.G. |
author_sort |
Chimento, L.P. |
title |
K-essence and extended tachyons in brane-worlds |
title_short |
K-essence and extended tachyons in brane-worlds |
title_full |
K-essence and extended tachyons in brane-worlds |
title_fullStr |
K-essence and extended tachyons in brane-worlds |
title_full_unstemmed |
K-essence and extended tachyons in brane-worlds |
title_sort |
k-essence and extended tachyons in brane-worlds |
publishDate |
2010 |
url |
http://hdl.handle.net/20.500.12110/paper_17426588_v229_n_p_Chimento |
work_keys_str_mv |
AT chimentolp kessenceandextendedtachyonsinbraneworlds AT richartemg kessenceandextendedtachyonsinbraneworlds |
_version_ |
1769810047144034304 |