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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Autores principales: Chimento, L.P., Forte, M.I., Richarte, M.G.
Formato: Documento de conferencia publishedVersion
Publicado: 2012
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0094243X_v1471_n_p39_Chimento
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0094243X_v1471_n_p39_Chimento_oai
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spelling I28-R145-paper_0094243X_v1471_n_p39_Chimento_oai2024-08-16 Chimento, L.P. Forte, M.I. Richarte, M.G. 2012 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. application/pdf http://hdl.handle.net/20.500.12110/paper_0094243X_v1471_n_p39_Chimento info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar AIP Conf. Proc. 2012;1471:39-44 Holographic dark energy linearly interacting with dark matter info:eu-repo/semantics/conferenceObject info:ar-repo/semantics/documento de conferencia info:eu-repo/semantics/publishedVersion https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0094243X_v1471_n_p39_Chimento_oai
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-145
collection Repositorio Digital de la Universidad de Buenos Aires (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.
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
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0094243X_v1471_n_p39_Chimento_oai
work_keys_str_mv AT chimentolp holographicdarkenergylinearlyinteractingwithdarkmatter
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