On big rip singularities
Here we discuss big rip singularities occurring in typical phantom models by violation of the weak energy condition. After that, we compare them with future late-time singularities arising in models where the scale factor ends in a constant value and there is no violation of the strong energy condit...
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todo:paper_02177323_v19_n33_p2479_Chimento2023-10-03T15:10:21Z On big rip singularities Chimento, L.P. Lazkoz, R. article density energy kinetics mathematical analysis mathematical model phantom pressure statistical analysis Here we discuss big rip singularities occurring in typical phantom models by violation of the weak energy condition. After that, we compare them with future late-time singularities arising in models where the scale factor ends in a constant value and there is no violation of the strong energy condition. In phantom models the equation of state is well defined along the whole evolution, even at the big rip. However, both the pressure and the energy density of the phantom field diverge. In contrast, in the second kind of model the equation of state is not defined at the big rip because the pressure bursts at a finite value of the energy density. Fil:Chimento, L.P. 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_02177323_v19_n33_p2479_Chimento |
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Universidad de Buenos Aires |
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I-28 |
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R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
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article density energy kinetics mathematical analysis mathematical model phantom pressure statistical analysis |
spellingShingle |
article density energy kinetics mathematical analysis mathematical model phantom pressure statistical analysis Chimento, L.P. Lazkoz, R. On big rip singularities |
topic_facet |
article density energy kinetics mathematical analysis mathematical model phantom pressure statistical analysis |
description |
Here we discuss big rip singularities occurring in typical phantom models by violation of the weak energy condition. After that, we compare them with future late-time singularities arising in models where the scale factor ends in a constant value and there is no violation of the strong energy condition. In phantom models the equation of state is well defined along the whole evolution, even at the big rip. However, both the pressure and the energy density of the phantom field diverge. In contrast, in the second kind of model the equation of state is not defined at the big rip because the pressure bursts at a finite value of the energy density. |
format |
JOUR |
author |
Chimento, L.P. Lazkoz, R. |
author_facet |
Chimento, L.P. Lazkoz, R. |
author_sort |
Chimento, L.P. |
title |
On big rip singularities |
title_short |
On big rip singularities |
title_full |
On big rip singularities |
title_fullStr |
On big rip singularities |
title_full_unstemmed |
On big rip singularities |
title_sort |
on big rip singularities |
url |
http://hdl.handle.net/20.500.12110/paper_02177323_v19_n33_p2479_Chimento |
work_keys_str_mv |
AT chimentolp onbigripsingularities AT lazkozr onbigripsingularities |
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1807320971485380608 |