Interacting quintessence
We demonstrate that a suitable coupling between a quintessence scalar field and a pressureless cold dark matter (CDM) fluid leads to a constant ratio of the energy densities of both components which is compatible with an accelerated expansion of the Universe. © 2001 Elsevier Science B.V. All rights...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03702693_v521_n3-4_p133_Zimdahl |
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todo:paper_03702693_v521_n3-4_p133_Zimdahl2023-10-03T15:28:52Z Interacting quintessence Zimdahl, W. Pavón, D. Chimento, L.P. Accelerated expansion Cosmology Quintessence acceleration article cosmos density energy mathematical analysis molecular interaction We demonstrate that a suitable coupling between a quintessence scalar field and a pressureless cold dark matter (CDM) fluid leads to a constant ratio of the energy densities of both components which is compatible with an accelerated expansion of the Universe. © 2001 Elsevier Science B.V. All rights reserved. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03702693_v521_n3-4_p133_Zimdahl |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Accelerated expansion Cosmology Quintessence acceleration article cosmos density energy mathematical analysis molecular interaction |
spellingShingle |
Accelerated expansion Cosmology Quintessence acceleration article cosmos density energy mathematical analysis molecular interaction Zimdahl, W. Pavón, D. Chimento, L.P. Interacting quintessence |
topic_facet |
Accelerated expansion Cosmology Quintessence acceleration article cosmos density energy mathematical analysis molecular interaction |
description |
We demonstrate that a suitable coupling between a quintessence scalar field and a pressureless cold dark matter (CDM) fluid leads to a constant ratio of the energy densities of both components which is compatible with an accelerated expansion of the Universe. © 2001 Elsevier Science B.V. All rights reserved. |
format |
JOUR |
author |
Zimdahl, W. Pavón, D. Chimento, L.P. |
author_facet |
Zimdahl, W. Pavón, D. Chimento, L.P. |
author_sort |
Zimdahl, W. |
title |
Interacting quintessence |
title_short |
Interacting quintessence |
title_full |
Interacting quintessence |
title_fullStr |
Interacting quintessence |
title_full_unstemmed |
Interacting quintessence |
title_sort |
interacting quintessence |
url |
http://hdl.handle.net/20.500.12110/paper_03702693_v521_n3-4_p133_Zimdahl |
work_keys_str_mv |
AT zimdahlw interactingquintessence AT pavond interactingquintessence AT chimentolp interactingquintessence |
_version_ |
1807320394222272512 |