Holographic dark energy linearly interacting with dark matter
We investigate a spatially flat Friedmann-Robertson-Walker (FRW) cosmological model with cold dark matter coupled to a modified holographic Ricci dark energy through a general interaction term linear in the energy densities of dark matter and dark energy, the total energy density and its derivative...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0094243X_v1471_n_p39_Chimento |
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paperaa:paper_0094243X_v1471_n_p39_Chimento2023-06-12T16:46:08Z Holographic dark energy linearly interacting with dark matter AIP Conf. Proc. 2012;1471:39-44 Chimento, L.P. Forte, M.I. Richarte, M.G. We investigate a spatially flat Friedmann-Robertson-Walker (FRW) cosmological model with cold dark matter coupled to a modified holographic Ricci dark energy through a general interaction term linear in the energy densities of dark matter and dark energy, the total energy density and its derivative 1. Using the statistical method of X2-function for the Hubble data, we obtain H0 = 73.6km/sMpc, ωs = -0.842 for the asymptotic equation of state and zacc = 0.89. The estimated values of Ωc0 which fulfill the current observational bounds corresponds to a dark energy density varying in the range 0.25R < ρx < 0.27R. © 2012 American Institute of Physics. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Forte, M.I. 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. 2012 info:eu-repo/semantics/conferenceObject info:ar-repo/semantics/documento de conferencia 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_0094243X_v1471_n_p39_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 spatially flat Friedmann-Robertson-Walker (FRW) cosmological model with cold dark matter coupled to a modified holographic Ricci dark energy through a general interaction term linear in the energy densities of dark matter and dark energy, the total energy density and its derivative 1. Using the statistical method of X2-function for the Hubble data, we obtain H0 = 73.6km/sMpc, ωs = -0.842 for the asymptotic equation of state and zacc = 0.89. The estimated values of Ωc0 which fulfill the current observational bounds corresponds to a dark energy density varying in the range 0.25R < ρx < 0.27R. © 2012 American Institute of Physics. |
format |
Documento de conferencia Documento de conferencia publishedVersion |
author |
Chimento, L.P. Forte, M.I. Richarte, M.G. |
spellingShingle |
Chimento, L.P. Forte, M.I. Richarte, M.G. Holographic dark energy linearly interacting with dark matter |
author_facet |
Chimento, L.P. Forte, M.I. Richarte, M.G. |
author_sort |
Chimento, L.P. |
title |
Holographic dark energy linearly interacting with dark matter |
title_short |
Holographic dark energy linearly interacting with dark matter |
title_full |
Holographic dark energy linearly interacting with dark matter |
title_fullStr |
Holographic dark energy linearly interacting with dark matter |
title_full_unstemmed |
Holographic dark energy linearly interacting with dark matter |
title_sort |
holographic dark energy linearly interacting with dark matter |
publishDate |
2012 |
url |
http://hdl.handle.net/20.500.12110/paper_0094243X_v1471_n_p39_Chimento |
work_keys_str_mv |
AT chimentolp holographicdarkenergylinearlyinteractingwithdarkmatter AT fortemi holographicdarkenergylinearlyinteractingwithdarkmatter AT richartemg holographicdarkenergylinearlyinteractingwithdarkmatter |
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1769810281573122048 |