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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todo:paper_05562821_v42_n4_p1098_Chimento2023-10-03T15:35:20Z Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields Chimento, L.P. Pensa, F.G. 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_05562821_v42_n4_p1098_Chimento |
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Universidad de Buenos Aires |
institution_str |
I-28 |
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R-134 |
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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. |
format |
JOUR |
author |
Chimento, L.P. Pensa, F.G. |
spellingShingle |
Chimento, L.P. Pensa, F.G. Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
author_facet |
Chimento, L.P. Pensa, F.G. |
author_sort |
Chimento, L.P. |
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 |
url |
http://hdl.handle.net/20.500.12110/paper_05562821_v42_n4_p1098_Chimento |
work_keys_str_mv |
AT chimentolp exactbianchitypeivsolutionsoftheeinsteinequationswithscalarandspinorfields AT pensafg exactbianchitypeivsolutionsoftheeinsteinequationswithscalarandspinorfields |
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1782028868077486080 |