Note on the reheating temperature in Starobinsky-type potentials
The relation between the reheating temperature, the number of e-folds and the spectral index is shown for the Starobinsky model and some of its descendants through a very detailed calculation of these three quantities. The conclusion is that for viable temperatures between 1 MeV and 109 GeV the corr...
| Autores: | , |
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 2020 |
| País: | España |
| Institución: | Universitat Politècnica de Catalunya (UPC) |
| Repositorio: | UPCommons. Portal del coneixement obert de la UPC |
| Idioma: | inglés |
| OAI Identifier: | oai:upcommons.upc.edu:2117/341480 |
| Acceso en línea: | https://hdl.handle.net/2117/341480 https://dx.doi.org/10.1007/s10714-020-02770-3 |
| Access Level: | acceso abierto |
| Palabra clave: | Cosmology Gravitational waves Reheating Number of e-folds Starobinsky model Cosmologia Ones gravitacionals Àrees temàtiques de la UPC::Física::Astronomia i astrofísica |
| Sumario: | The relation between the reheating temperature, the number of e-folds and the spectral index is shown for the Starobinsky model and some of its descendants through a very detailed calculation of these three quantities. The conclusion is that for viable temperatures between 1 MeV and 109 GeV the corresponding values of the spectral index enter perfectly in its 2s C.L., which shows the viability of this kind of models |
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