Classical supersymmetric matter and cosmology
We show that supersymmetry may play an important role in giving a reasonable explanation of relevant cosmological features. We work in a classical N=1 supergravity scenario showing that supersymmetric matter leads, in the classical limit, to a fluid model acting as the source of the gravitational fi...
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paper:paper_00017701_v23_n6_p683_Domenech2023-06-08T14:21:31Z Classical supersymmetric matter and cosmology Domenech, Graciela Levinas, Marcelo Leonardo Umerez, Norberto Daniel We show that supersymmetry may play an important role in giving a reasonable explanation of relevant cosmological features. We work in a classical N=1 supergravity scenario showing that supersymmetric matter leads, in the classical limit, to a fluid model acting as the source of the gravitational field. The equation of state arises, in a natural way, as a consequence of the field equations. We study conditions for the matter dominated era and the existence of an inflationary solution. Using upper bounds of several red-shift experimental results we are able to give an estimate of the corresponding Hubble constant. © 1991 Plenum Publishing Corporation. Fil:Domenech, G. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Levinas, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Umérez, N. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 1991 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v23_n6_p683_Domenech http://hdl.handle.net/20.500.12110/paper_00017701_v23_n6_p683_Domenech |
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 show that supersymmetry may play an important role in giving a reasonable explanation of relevant cosmological features. We work in a classical N=1 supergravity scenario showing that supersymmetric matter leads, in the classical limit, to a fluid model acting as the source of the gravitational field. The equation of state arises, in a natural way, as a consequence of the field equations. We study conditions for the matter dominated era and the existence of an inflationary solution. Using upper bounds of several red-shift experimental results we are able to give an estimate of the corresponding Hubble constant. © 1991 Plenum Publishing Corporation. |
author |
Domenech, Graciela Levinas, Marcelo Leonardo Umerez, Norberto Daniel |
spellingShingle |
Domenech, Graciela Levinas, Marcelo Leonardo Umerez, Norberto Daniel Classical supersymmetric matter and cosmology |
author_facet |
Domenech, Graciela Levinas, Marcelo Leonardo Umerez, Norberto Daniel |
author_sort |
Domenech, Graciela |
title |
Classical supersymmetric matter and cosmology |
title_short |
Classical supersymmetric matter and cosmology |
title_full |
Classical supersymmetric matter and cosmology |
title_fullStr |
Classical supersymmetric matter and cosmology |
title_full_unstemmed |
Classical supersymmetric matter and cosmology |
title_sort |
classical supersymmetric matter and cosmology |
publishDate |
1991 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v23_n6_p683_Domenech http://hdl.handle.net/20.500.12110/paper_00017701_v23_n6_p683_Domenech |
work_keys_str_mv |
AT domenechgraciela classicalsupersymmetricmatterandcosmology AT levinasmarceloleonardo classicalsupersymmetricmatterandcosmology AT umereznorbertodaniel classicalsupersymmetricmatterandcosmology |
_version_ |
1768543634198626304 |