Dark matter to dark energy transition in k-essence cosmologies
We implement the transition from dark matter to dark energy in k-essence cosmologies for a very large set of kinetic functions F, in a way alternative to recent proposals which use generalized Chaplygin gas and transient models. Here we require that the pressure admits a power-law expansion around s...
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2005
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paper:paper_02177323_v20_n27_p2075_Chimento2023-06-08T15:21:01Z Dark matter to dark energy transition in k-essence cosmologies Chimento, Luis Pascual Forte, Mónica Isabel Dark energy Dark matter k-essence We implement the transition from dark matter to dark energy in k-essence cosmologies for a very large set of kinetic functions F, in a way alternative to recent proposals which use generalized Chaplygin gas and transient models. Here we require that the pressure admits a power-law expansion around some value of the kinetic energy where the pressure vanishes. In addition, for suitable values of the parameters of the model, the speed of sound of the dark matter will be low. We first present the discussion in fairly general terms, and later consider for illustration two examples. © World Scientific Publishing Company. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Forte, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2005 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02177323_v20_n27_p2075_Chimento http://hdl.handle.net/20.500.12110/paper_02177323_v20_n27_p2075_Chimento |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Dark energy Dark matter k-essence |
spellingShingle |
Dark energy Dark matter k-essence Chimento, Luis Pascual Forte, Mónica Isabel Dark matter to dark energy transition in k-essence cosmologies |
topic_facet |
Dark energy Dark matter k-essence |
description |
We implement the transition from dark matter to dark energy in k-essence cosmologies for a very large set of kinetic functions F, in a way alternative to recent proposals which use generalized Chaplygin gas and transient models. Here we require that the pressure admits a power-law expansion around some value of the kinetic energy where the pressure vanishes. In addition, for suitable values of the parameters of the model, the speed of sound of the dark matter will be low. We first present the discussion in fairly general terms, and later consider for illustration two examples. © World Scientific Publishing Company. |
author |
Chimento, Luis Pascual Forte, Mónica Isabel |
author_facet |
Chimento, Luis Pascual Forte, Mónica Isabel |
author_sort |
Chimento, Luis Pascual |
title |
Dark matter to dark energy transition in k-essence cosmologies |
title_short |
Dark matter to dark energy transition in k-essence cosmologies |
title_full |
Dark matter to dark energy transition in k-essence cosmologies |
title_fullStr |
Dark matter to dark energy transition in k-essence cosmologies |
title_full_unstemmed |
Dark matter to dark energy transition in k-essence cosmologies |
title_sort |
dark matter to dark energy transition in k-essence cosmologies |
publishDate |
2005 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02177323_v20_n27_p2075_Chimento http://hdl.handle.net/20.500.12110/paper_02177323_v20_n27_p2075_Chimento |
work_keys_str_mv |
AT chimentoluispascual darkmattertodarkenergytransitioninkessencecosmologies AT fortemonicaisabel darkmattertodarkenergytransitioninkessencecosmologies |
_version_ |
1768546490027868160 |