Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component
We examine a Friedmann-Robertson-Walker universe filled with interacting dark matter, modified holographic Ricci dark energy (MHRDE), and a decoupled baryonic component. The estimations of the cosmic parameters with Hubble data lead to an age of the universe of 13. 17 Gyr and show that the MHRDE is...
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todo:paper_14346044_v73_n1_p1_Chimento2023-10-03T16:14:51Z Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component Chimento, L.P. Forte, M. Richarte, M.G. We examine a Friedmann-Robertson-Walker universe filled with interacting dark matter, modified holographic Ricci dark energy (MHRDE), and a decoupled baryonic component. The estimations of the cosmic parameters with Hubble data lead to an age of the universe of 13. 17 Gyr and show that the MHRDE is free from the cosmic-age problem at low redshift (0≤z≤2) in contrast to holographic Ricci dark energy (HRDE) case. We constrain the parameters with the Union2 data set and contrast with the Hubble data. We also study the behavior of dark energy at early times by taking into account the severe bounds found at recombination era and/or at big bang nucleosynthesis. The inclusion of a non-interacting baryonic matter forces that the amount of dark energy at zt~O(1) changes abruptly implying that Ωx(z≃1100)=0. 03, so the bounds reported by the forecast of Planck and CMBPol experiments are more favored for the MHRDE model than in the case of HRDE cutoff. For the former model, we also find that at high redshift the fraction of dark energy varies from 0. 006 to 0. 002, then the amount of Ωx at the big bang nucleosynthesis era does not disturb the observed helium abundance in the universe provided that the bound Ωx(z≃1010)<0. 21 is hold. © 2013 Springer-Verlag Berlin Heidelberg and Società Italiana di Fisica. 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. Fil:Richarte, M.G. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_14346044_v73_n1_p1_Chimento |
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Universidad de Buenos Aires |
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I-28 |
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R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| description |
We examine a Friedmann-Robertson-Walker universe filled with interacting dark matter, modified holographic Ricci dark energy (MHRDE), and a decoupled baryonic component. The estimations of the cosmic parameters with Hubble data lead to an age of the universe of 13. 17 Gyr and show that the MHRDE is free from the cosmic-age problem at low redshift (0≤z≤2) in contrast to holographic Ricci dark energy (HRDE) case. We constrain the parameters with the Union2 data set and contrast with the Hubble data. We also study the behavior of dark energy at early times by taking into account the severe bounds found at recombination era and/or at big bang nucleosynthesis. The inclusion of a non-interacting baryonic matter forces that the amount of dark energy at zt~O(1) changes abruptly implying that Ωx(z≃1100)=0. 03, so the bounds reported by the forecast of Planck and CMBPol experiments are more favored for the MHRDE model than in the case of HRDE cutoff. For the former model, we also find that at high redshift the fraction of dark energy varies from 0. 006 to 0. 002, then the amount of Ωx at the big bang nucleosynthesis era does not disturb the observed helium abundance in the universe provided that the bound Ωx(z≃1010)<0. 21 is hold. © 2013 Springer-Verlag Berlin Heidelberg and Società Italiana di Fisica. |
| format |
JOUR |
| author |
Chimento, L.P. Forte, M. Richarte, M.G. |
| spellingShingle |
Chimento, L.P. Forte, M. Richarte, M.G. Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component |
| author_facet |
Chimento, L.P. Forte, M. Richarte, M.G. |
| author_sort |
Chimento, L.P. |
| title |
Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component |
| title_short |
Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component |
| title_full |
Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component |
| title_fullStr |
Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component |
| title_full_unstemmed |
Modified holographic Ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component |
| title_sort |
modified holographic ricci dark energy coupled to interacting dark matter and a non-interacting baryonic component |
| url |
http://hdl.handle.net/20.500.12110/paper_14346044_v73_n1_p1_Chimento |
| work_keys_str_mv |
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1807320476981133312 |