Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation

We analyze a universe filled with interacting dark matter, a scalar field accommodated as dark radiation along with dark energy plus a decoupled radiation term within the framework of the spatially flat Friedmann-Robertson-Walker (FRW) spacetime. We work in a three-dimensional internal space spanned...

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Main Authors: Chimento, L.P., Richarte, M.G.
Format: Article in Journal/Newspaper
Language:unknown
Published: 2013
Subjects:
Online Access:https://hdl.handle.net/20.500.12110/paper_14346044_v73_n7_p1_Chimento
http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_14346044_v73_n7_p1_Chimento_oai
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spelling ftunbuenosairrdi:oai:RDI UBA:artiaex:paper_14346044_v73_n7_p1_Chimento_oai 2023-05-15T18:22:55+02:00 Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation Chimento, L.P. Richarte, M.G. 2013 application/pdf https://hdl.handle.net/20.500.12110/paper_14346044_v73_n7_p1_Chimento http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_14346044_v73_n7_p1_Chimento_oai unknown http://hdl.handle.net/20.500.12110/paper_14346044_v73_n7_p1_Chimento http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_14346044_v73_n7_p1_Chimento_oai info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar CC-BY Eur. Phys. J. C 2013;73(7):1-18 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion 2013 ftunbuenosairrdi https://doi.org/20.500.12110/paper_14346044_v73_n7_p1_Chimento 2020-10-22T00:10:07Z We analyze a universe filled with interacting dark matter, a scalar field accommodated as dark radiation along with dark energy plus a decoupled radiation term within the framework of the spatially flat Friedmann-Robertson-Walker (FRW) spacetime. We work in a three-dimensional internal space spanned by the interaction vector and use a transversal interaction Qt for solving the source equation in order to find all the interacting component energy densities. We asymptotically reconstruct the scalar field and potential from an early radiation era to the late dominate dark energy one, passing through an intermediate epoch dominated by dark matter. We apply the χ2 method to the updated 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 fulfills the severe bound of Ωφ{symbol}(z≃1100)<0.018 at 2σ level, is consistent with the recent analysis that includes cosmic microwave background anisotropy measurements from the Atacama Cosmology Telescope and the South Pole Telescope along with the future constraints achievable by Planck and CMBPol experiments, and satisfies the stringent bound Ωφ{symbol}(z≃1010)<0.04 at 2σ level in the big-bang nucleosynthesis epoch. © 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. Article in Journal/Newspaper South pole Repositorio Digital Institucional - Universidad de Buenos Aires (RDI UBA) Argentina Hubble ENVELOPE(158.317,158.317,-80.867,-80.867) South Pole
institution Open Polar
collection Repositorio Digital Institucional - Universidad de Buenos Aires (RDI UBA)
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language unknown
description We analyze a universe filled with interacting dark matter, a scalar field accommodated as dark radiation along with dark energy plus a decoupled radiation term within the framework of the spatially flat Friedmann-Robertson-Walker (FRW) spacetime. We work in a three-dimensional internal space spanned by the interaction vector and use a transversal interaction Qt for solving the source equation in order to find all the interacting component energy densities. We asymptotically reconstruct the scalar field and potential from an early radiation era to the late dominate dark energy one, passing through an intermediate epoch dominated by dark matter. We apply the χ2 method to the updated 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 fulfills the severe bound of Ωφ{symbol}(z≃1100)<0.018 at 2σ level, is consistent with the recent analysis that includes cosmic microwave background anisotropy measurements from the Atacama Cosmology Telescope and the South Pole Telescope along with the future constraints achievable by Planck and CMBPol experiments, and satisfies the stringent bound Ωφ{symbol}(z≃1010)<0.04 at 2σ level in the big-bang nucleosynthesis epoch. © 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.
format Article in Journal/Newspaper
author Chimento, L.P.
Richarte, M.G.
spellingShingle Chimento, L.P.
Richarte, M.G.
Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
author_facet Chimento, L.P.
Richarte, M.G.
author_sort Chimento, L.P.
title Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
title_short Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
title_full Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
title_fullStr Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
title_full_unstemmed Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
title_sort nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
publishDate 2013
url https://hdl.handle.net/20.500.12110/paper_14346044_v73_n7_p1_Chimento
http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_14346044_v73_n7_p1_Chimento_oai
long_lat ENVELOPE(158.317,158.317,-80.867,-80.867)
geographic Argentina
Hubble
South Pole
geographic_facet Argentina
Hubble
South Pole
genre South pole
genre_facet South pole
op_source Eur. Phys. J. C 2013;73(7):1-18
op_relation http://hdl.handle.net/20.500.12110/paper_14346044_v73_n7_p1_Chimento
http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_14346044_v73_n7_p1_Chimento_oai
op_rights info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/2.5/ar
op_rightsnorm CC-BY
op_doi https://doi.org/20.500.12110/paper_14346044_v73_n7_p1_Chimento
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