Crossing the phantom divide without phantom matter
A class of braneworld models can lead to phantom-like acceleration of the late universe, but without the need for any phantom matter. In the simplest models, the universe contains only cold dark matter and a cosmological constant. We generalize these models by introducing a quintessence field. The n...
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| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_14757516_v_n9_p_Chimento |
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todo:paper_14757516_v_n9_p_Chimento2023-10-03T16:18:57Z Crossing the phantom divide without phantom matter Chimento, L.P. Lazkoz, R. Maartens, R. Quiros, I. Cosmological applications of theories with extra dimensions Dark energy theory A class of braneworld models can lead to phantom-like acceleration of the late universe, but without the need for any phantom matter. In the simplest models, the universe contains only cold dark matter and a cosmological constant. We generalize these models by introducing a quintessence field. The new feature in our models is that quintessence leads to a crossing of the phantom divide, w = -1. This is a purely gravitational effect, and there is no phantom instability. Furthermore, the Hubble parameter is always decreasing, and there is no big rip singularity in the future. © IOP Publishing Ltd. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_14757516_v_n9_p_Chimento |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
Cosmological applications of theories with extra dimensions Dark energy theory |
| spellingShingle |
Cosmological applications of theories with extra dimensions Dark energy theory Chimento, L.P. Lazkoz, R. Maartens, R. Quiros, I. Crossing the phantom divide without phantom matter |
| topic_facet |
Cosmological applications of theories with extra dimensions Dark energy theory |
| description |
A class of braneworld models can lead to phantom-like acceleration of the late universe, but without the need for any phantom matter. In the simplest models, the universe contains only cold dark matter and a cosmological constant. We generalize these models by introducing a quintessence field. The new feature in our models is that quintessence leads to a crossing of the phantom divide, w = -1. This is a purely gravitational effect, and there is no phantom instability. Furthermore, the Hubble parameter is always decreasing, and there is no big rip singularity in the future. © IOP Publishing Ltd. |
| format |
JOUR |
| author |
Chimento, L.P. Lazkoz, R. Maartens, R. Quiros, I. |
| author_facet |
Chimento, L.P. Lazkoz, R. Maartens, R. Quiros, I. |
| author_sort |
Chimento, L.P. |
| title |
Crossing the phantom divide without phantom matter |
| title_short |
Crossing the phantom divide without phantom matter |
| title_full |
Crossing the phantom divide without phantom matter |
| title_fullStr |
Crossing the phantom divide without phantom matter |
| title_full_unstemmed |
Crossing the phantom divide without phantom matter |
| title_sort |
crossing the phantom divide without phantom matter |
| url |
http://hdl.handle.net/20.500.12110/paper_14757516_v_n9_p_Chimento |
| work_keys_str_mv |
AT chimentolp crossingthephantomdividewithoutphantommatter AT lazkozr crossingthephantomdividewithoutphantommatter AT maartensr crossingthephantomdividewithoutphantommatter AT quirosi crossingthephantomdividewithoutphantommatter |
| _version_ |
1807322481189453824 |