Dark radiation and dark matter coupled to holographic Ricci dark energy
We investigate a universe filled with interacting dark matter, holographic dark energy, and dark radiation for the spatially flat Friedmann-Robertson-Walker (FRW) spacetime. We use a linear interaction to reconstruct all the component energy densities in terms of the scale factor by directly solving...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_14346044_v73_n4_p1_Chimento |
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paperaa:paper_14346044_v73_n4_p1_Chimento2023-06-12T16:50:16Z Dark radiation and dark matter coupled to holographic Ricci dark energy Eur. Phys. J. C 2013;73(4):1-9 Chimento, L.P. Richarte, M.G. We investigate a universe filled with interacting dark matter, holographic dark energy, and dark radiation for the spatially flat Friedmann-Robertson-Walker (FRW) spacetime. We use a linear interaction to reconstruct all the component energy densities in terms of the scale factor by directly solving the balance's equations along with the source equation. We apply the χ 2 method to the observational Hubble data for constraining the cosmic parameters, contrast with the Union 2 sample of supernovae, and analyze the amount of dark energy in the radiation era. It turns out that our model exhibits an excess of dark energy in the recombination era whereas the stringent bound Ωx(z≃1010) < 0.21 at big-bang nucleosynthesis is fulfilled. We find that the interaction provides a physical mechanism for alleviating the triple cosmic coincidence and this leads to Ωm0/Ωx0≃Ωr0/Ωx0≃O(1). © 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:Richarte, M.G. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2013 info:eu-repo/semantics/article info:ar-repo/semantics/artículo 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_14346044_v73_n4_p1_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 |
description |
We investigate a universe filled with interacting dark matter, holographic dark energy, and dark radiation for the spatially flat Friedmann-Robertson-Walker (FRW) spacetime. We use a linear interaction to reconstruct all the component energy densities in terms of the scale factor by directly solving the balance's equations along with the source equation. We apply the χ 2 method to the observational Hubble data for constraining the cosmic parameters, contrast with the Union 2 sample of supernovae, and analyze the amount of dark energy in the radiation era. It turns out that our model exhibits an excess of dark energy in the recombination era whereas the stringent bound Ωx(z≃1010) < 0.21 at big-bang nucleosynthesis is fulfilled. We find that the interaction provides a physical mechanism for alleviating the triple cosmic coincidence and this leads to Ωm0/Ωx0≃Ωr0/Ωx0≃O(1). © 2013 Springer-Verlag Berlin Heidelberg and Società Italiana di Fisica. |
format |
Artículo Artículo publishedVersion |
author |
Chimento, L.P. Richarte, M.G. |
spellingShingle |
Chimento, L.P. Richarte, M.G. Dark radiation and dark matter coupled to holographic Ricci dark energy |
author_facet |
Chimento, L.P. Richarte, M.G. |
author_sort |
Chimento, L.P. |
title |
Dark radiation and dark matter coupled to holographic Ricci dark energy |
title_short |
Dark radiation and dark matter coupled to holographic Ricci dark energy |
title_full |
Dark radiation and dark matter coupled to holographic Ricci dark energy |
title_fullStr |
Dark radiation and dark matter coupled to holographic Ricci dark energy |
title_full_unstemmed |
Dark radiation and dark matter coupled to holographic Ricci dark energy |
title_sort |
dark radiation and dark matter coupled to holographic ricci dark energy |
publishDate |
2013 |
url |
http://hdl.handle.net/20.500.12110/paper_14346044_v73_n4_p1_Chimento |
work_keys_str_mv |
AT chimentolp darkradiationanddarkmattercoupledtoholographicriccidarkenergy AT richartemg darkradiationanddarkmattercoupledtoholographicriccidarkenergy |
_version_ |
1769810138146799616 |