| dc.creator | Zimdahl, Winfried | |
| dc.creator | Pavon, Diego | |
| dc.creator | Chimento, Luis Pascual | |
| dc.date.accessioned | 2019-07-05T16:18:37Z | |
| dc.date.accessioned | 2022-10-15T13:20:00Z | |
| dc.date.available | 2019-07-05T16:18:37Z | |
| dc.date.available | 2022-10-15T13:20:00Z | |
| dc.date.created | 2019-07-05T16:18:37Z | |
| dc.date.issued | 2001-11 | |
| dc.identifier | Zimdahl, Winfried; Pavon, Diego; Chimento, Luis Pascual; Interacting quintessence; Elsevier Science; Physics Letters B; 521; 3-4; 11-2001; 133-138 | |
| dc.identifier | 0370-2693 | |
| dc.identifier | http://hdl.handle.net/11336/79239 | |
| dc.identifier | CONICET Digital | |
| dc.identifier | CONICET | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4390687 | |
| dc.description.abstract | 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.language | eng | |
| dc.publisher | Elsevier Science | |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/https://dx.doi.org/10.1016/S0370-2693(01)01174-1 | |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0370269301011741 | |
| dc.rights | https://creativecommons.org/licenses/by/2.5/ar/ | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.subject | ACCELERATED EXPANSION | |
| dc.subject | COSMOLOGY | |
| dc.subject | QUINTESSENCE | |
| dc.title | Interacting quintessence | |
| dc.type | info:eu-repo/semantics/article | |
| dc.type | info:ar-repo/semantics/artículo | |
| dc.type | info:eu-repo/semantics/publishedVersion | |
