Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields
Exact solutions to the Einstein Dirac Klein-Gordon equations are found in Bianchi type-I and type-V spacetimes. When the spinor field is massive, the Bianchi type-I universe has singularities of the Zel dovich type, and it may begin anisotropically at a singularity, leading to a dust-filled Friedman...
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1990
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paper:paper_05562821_v42_n4_p1098_Chimento2023-06-08T15:42:09Z Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields Chimento, Luis Pascual Pensa, Fabián Gabriel Exact solutions to the Einstein Dirac Klein-Gordon equations are found in Bianchi type-I and type-V spacetimes. When the spinor field is massive, the Bianchi type-I universe has singularities of the Zel dovich type, and it may begin anisotropically at a singularity, leading to a dust-filled Friedmann stage at late times. For ghost neutrinos we get an axisymmetric Zel dovich universe. These solutions have particle horizons. For the Bianchi type-V model there exist solutions which begin at a singularity, tending to flat spacetime at late times. In this case the neutrinos are not ghost ones. © 1990 The American Physical Society. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Pensa, F.G. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 1990 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v42_n4_p1098_Chimento http://hdl.handle.net/20.500.12110/paper_05562821_v42_n4_p1098_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 |
Exact solutions to the Einstein Dirac Klein-Gordon equations are found in Bianchi type-I and type-V spacetimes. When the spinor field is massive, the Bianchi type-I universe has singularities of the Zel dovich type, and it may begin anisotropically at a singularity, leading to a dust-filled Friedmann stage at late times. For ghost neutrinos we get an axisymmetric Zel dovich universe. These solutions have particle horizons. For the Bianchi type-V model there exist solutions which begin at a singularity, tending to flat spacetime at late times. In this case the neutrinos are not ghost ones. © 1990 The American Physical Society. |
author |
Chimento, Luis Pascual Pensa, Fabián Gabriel |
spellingShingle |
Chimento, Luis Pascual Pensa, Fabián Gabriel Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
author_facet |
Chimento, Luis Pascual Pensa, Fabián Gabriel |
author_sort |
Chimento, Luis Pascual |
title |
Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
title_short |
Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
title_full |
Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
title_fullStr |
Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
title_full_unstemmed |
Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
title_sort |
exact bianchi type-(i,v) solutions of the einstein equations with scalar and spinor fields |
publishDate |
1990 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v42_n4_p1098_Chimento http://hdl.handle.net/20.500.12110/paper_05562821_v42_n4_p1098_Chimento |
work_keys_str_mv |
AT chimentoluispascual exactbianchitypeivsolutionsoftheeinsteinequationswithscalarandspinorfields AT pensafabiangabriel exactbianchitypeivsolutionsoftheeinsteinequationswithscalarandspinorfields |
_version_ |
1768545789054812160 |