Interacting Quintessence
| dc.creator | Zimdahl, Winfried | |
| dc.creator | Pavón, Diego | |
| dc.creator | Chimento, Luis P. | |
| dc.date | 2001-05-28 | |
| dc.date | 2001-10-17 | |
| dc.date.accessioned | 2026-07-07T10:51:19Z | |
| dc.date.available | 2026-07-07T10:51:19Z | |
| dc.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. | |
| dc.description | 12 pages, LaTeX; new material on the stability analysis and on the interaction potential added, reference list enlarged and updated; to be published in PLB | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0105479 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0105479 | |
| dc.identifier | Phys.Lett.B521:133-138,2001 | |
| dc.identifier | doi:10.1016/S0370-2693(01)01174-1 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/184779 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Interacting Quintessence | |
| dc.type | text |