Crossing the phantom barrier with purely kinetic multiple k-essence
We consider multiple k-essence sources and obtain the conditions their kinetic functions must satisfy so that purely kinetic k-essences lead to models with phantom barrier crossing. After that, we show that polynomial kinetic functions allow the integration of the dynamical equations determining the...
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2006
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03702693_v639_n6_p591_Chimento http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_03702693_v639_n6_p591_Chimento_oai |
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I28-R145-paper_03702693_v639_n6_p591_Chimento_oai2020-10-19 Chimento, L.P. Lazkoz, R. 2006 We consider multiple k-essence sources and obtain the conditions their kinetic functions must satisfy so that purely kinetic k-essences lead to models with phantom barrier crossing. After that, we show that polynomial kinetic functions allow the integration of the dynamical equations determining the geometry and the k-fields. The models thus obtained have accelerated expansion at late cosmic time, representing universes ending at a finite time with a big rip singularity. In addition, these models begin to evolve from an initial singularity, so they have a finite time span. © 2006 Elsevier B.V. All rights reserved. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. application/pdf http://hdl.handle.net/20.500.12110/paper_03702693_v639_n6_p591_Chimento info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar Phys Lett Sect B Nucl Elem Part High-Energy Phys 2006;639(6):591-595 Crossing the phantom barrier with purely kinetic multiple k-essence info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_03702693_v639_n6_p591_Chimento_oai |
institution |
Universidad de Buenos Aires |
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I-28 |
repository_str |
R-145 |
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Repositorio Digital de la Universidad de Buenos Aires (UBA) |
description |
We consider multiple k-essence sources and obtain the conditions their kinetic functions must satisfy so that purely kinetic k-essences lead to models with phantom barrier crossing. After that, we show that polynomial kinetic functions allow the integration of the dynamical equations determining the geometry and the k-fields. The models thus obtained have accelerated expansion at late cosmic time, representing universes ending at a finite time with a big rip singularity. In addition, these models begin to evolve from an initial singularity, so they have a finite time span. © 2006 Elsevier B.V. All rights reserved. |
format |
Artículo Artículo publishedVersion |
author |
Chimento, L.P. Lazkoz, R. |
spellingShingle |
Chimento, L.P. Lazkoz, R. Crossing the phantom barrier with purely kinetic multiple k-essence |
author_facet |
Chimento, L.P. Lazkoz, R. |
author_sort |
Chimento, L.P. |
title |
Crossing the phantom barrier with purely kinetic multiple k-essence |
title_short |
Crossing the phantom barrier with purely kinetic multiple k-essence |
title_full |
Crossing the phantom barrier with purely kinetic multiple k-essence |
title_fullStr |
Crossing the phantom barrier with purely kinetic multiple k-essence |
title_full_unstemmed |
Crossing the phantom barrier with purely kinetic multiple k-essence |
title_sort |
crossing the phantom barrier with purely kinetic multiple k-essence |
publishDate |
2006 |
url |
http://hdl.handle.net/20.500.12110/paper_03702693_v639_n6_p591_Chimento http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_03702693_v639_n6_p591_Chimento_oai |
work_keys_str_mv |
AT chimentolp crossingthephantombarrierwithpurelykineticmultiplekessence AT lazkozr crossingthephantombarrierwithpurelykineticmultiplekessence |
_version_ |
1766026700400885760 |