Reheating via gravitational particle production in simple models of quintessence or ¿CDM Inflation
| dc.contributor.author | Haro Cases, Jaume |
| dc.contributor.author | Aresté Saló, Llibert |
| dc.contributor.group | Universitat Politècnica de Catalunya. EDP - Equacions en Derivades Parcials i Aplicacions |
| dc.contributor.other | Universitat Politècnica de Catalunya. Departament de Matemàtiques |
| dc.date.accessioned | 2018-01-10T13:09:38Z |
| dc.date.available | 2018-01-10T13:09:38Z |
| dc.date.issued | 2017-11-14 |
| dc.description.abstract | We have tested some simple CDM (the same test is also valid for quintessence) inflation models, imposing that they match with the recent observational data provided by the BICEP and Planck’s team and leading to a reheating temperature, which is obtained via gravitational particle production after inflation, supporting the nucleosynthesis success. |
| dc.description.peerreviewed | Peer Reviewed |
| dc.description.version | Postprint (published version) |
| dc.identifier.citation | Haro, J., Aresté, L. Reheating via gravitational particle production in simple models of quintessence or ¿CDM Inflation. "Galaxies", 14 Novembre 2017, vol. 5, núm. 4. |
| dc.identifier.doi | 10.3390/galaxies5040078 |
| dc.identifier.issn | 2075-4434 |
| dc.identifier.uri | https://hdl.handle.net/2117/112589 |
| dc.language.iso | eng |
| dc.relation.publisherversion | http://www.mdpi.com/2075-4434/5/4/78 |
| dc.rights.access | Open Access |
| dc.rights.licensename | Attribution-NonCommercial-NoDerivs 3.0 Spain |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ |
| dc.subject | Àrees temàtiques de la UPC::Matemàtiques i estadística |
| dc.subject.lcsh | Cosmology |
| dc.subject.lcsh | Particles (Nuclear physics) |
| dc.subject.lemac | Cosmologia |
| dc.subject.lemac | Partícules (Física nuclear) |
| dc.subject.other | gravitational particle production |
| dc.subject.other | inflation |
| dc.subject.other | kination |
| dc.title | Reheating via gravitational particle production in simple models of quintessence or ¿CDM Inflation |
| dc.type | Article |
| dspace.entity.type | Publication |
| local.citation.author | Haro, J.; Aresté, L. |
| local.citation.number | 4 |
| local.citation.publicationName | Galaxies |
| local.citation.volume | 5 |
| local.identifier.drac | 21671085 |
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