DBI models for the unification of dark matter and dark energy
We propose a model based on a DBI action for the unification of dark matter and dark energy. This is supported by the results of the study of its background behavior at early and late times, and reinforced by the analysis of the evolution of perturbations. We also perform a Bayesian analysis to set...
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| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0094243X_v1241_n_p776_Chimento |
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todo:paper_0094243X_v1241_n_p776_Chimento2023-10-03T14:56:00Z DBI models for the unification of dark matter and dark energy Chimento, L.P. Lazkoz, R. Sendra, I. cosmological perturbations dark energy dark matter DBI Lagrangians geometrical constraints We propose a model based on a DBI action for the unification of dark matter and dark energy. This is supported by the results of the study of its background behavior at early and late times, and reinforced by the analysis of the evolution of perturbations. We also perform a Bayesian analysis to set observational constraints on the parameters of the model using type Ia SN, CMB shift and BAO data. Finally, to complete the study we investigate its kinematics aspects, such as the effective equation of state parameter, acceleration parameter and transition redshift. Particularizing them for the best fit one appreciates that an effective phantom behavior is preferred. © 2010 American Institute of Physics. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0094243X_v1241_n_p776_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 |
cosmological perturbations dark energy dark matter DBI Lagrangians geometrical constraints |
| spellingShingle |
cosmological perturbations dark energy dark matter DBI Lagrangians geometrical constraints Chimento, L.P. Lazkoz, R. Sendra, I. DBI models for the unification of dark matter and dark energy |
| topic_facet |
cosmological perturbations dark energy dark matter DBI Lagrangians geometrical constraints |
| description |
We propose a model based on a DBI action for the unification of dark matter and dark energy. This is supported by the results of the study of its background behavior at early and late times, and reinforced by the analysis of the evolution of perturbations. We also perform a Bayesian analysis to set observational constraints on the parameters of the model using type Ia SN, CMB shift and BAO data. Finally, to complete the study we investigate its kinematics aspects, such as the effective equation of state parameter, acceleration parameter and transition redshift. Particularizing them for the best fit one appreciates that an effective phantom behavior is preferred. © 2010 American Institute of Physics. |
| format |
CONF |
| author |
Chimento, L.P. Lazkoz, R. Sendra, I. |
| author_facet |
Chimento, L.P. Lazkoz, R. Sendra, I. |
| author_sort |
Chimento, L.P. |
| title |
DBI models for the unification of dark matter and dark energy |
| title_short |
DBI models for the unification of dark matter and dark energy |
| title_full |
DBI models for the unification of dark matter and dark energy |
| title_fullStr |
DBI models for the unification of dark matter and dark energy |
| title_full_unstemmed |
DBI models for the unification of dark matter and dark energy |
| title_sort |
dbi models for the unification of dark matter and dark energy |
| url |
http://hdl.handle.net/20.500.12110/paper_0094243X_v1241_n_p776_Chimento |
| work_keys_str_mv |
AT chimentolp dbimodelsfortheunificationofdarkmatteranddarkenergy AT lazkozr dbimodelsfortheunificationofdarkmatteranddarkenergy AT sendrai dbimodelsfortheunificationofdarkmatteranddarkenergy |
| _version_ |
1782026160846143488 |