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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2012
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v1471_n_p39_Chimento http://hdl.handle.net/20.500.12110/paper_0094243X_v1471_n_p39_Chimento |
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paper:paper_0094243X_v1471_n_p39_Chimento2023-06-08T15:09:12Z Holographic dark energy linearly interacting with dark matter Chimento, Luis Pascual Forte, Mónica Isabel Richarte, Martín Gustavo 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 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v1471_n_p39_Chimento 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) |
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. |
author |
Chimento, Luis Pascual Forte, Mónica Isabel Richarte, Martín Gustavo |
spellingShingle |
Chimento, Luis Pascual Forte, Mónica Isabel Richarte, Martín Gustavo Holographic dark energy linearly interacting with dark matter |
author_facet |
Chimento, Luis Pascual Forte, Mónica Isabel Richarte, Martín Gustavo |
author_sort |
Chimento, Luis Pascual |
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 |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v1471_n_p39_Chimento http://hdl.handle.net/20.500.12110/paper_0094243X_v1471_n_p39_Chimento |
work_keys_str_mv |
AT chimentoluispascual holographicdarkenergylinearlyinteractingwithdarkmatter AT fortemonicaisabel holographicdarkenergylinearlyinteractingwithdarkmatter AT richartemartingustavo holographicdarkenergylinearlyinteractingwithdarkmatter |
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