Publicação: Reheating and Baryogenesis
| dc.contributor.author | Năstase, Horaţiu [UNESP] | |
| dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
| dc.date.accessioned | 2020-12-12T02:07:38Z | |
| dc.date.available | 2020-12-12T02:07:38Z | |
| dc.date.issued | 2019-01-01 | |
| dc.description.abstract | In this chapter we will study reheating, which happens just after inflation, and is a way to populate the Universe with thermally distributed particles, which is followed by the standard Radiation Dominated adiabatic cosmology. Thus reheating is a way to transfer the energy of the inflaton to the Standard Model particles and to transition into standard cosmology. We will also say a few things about baryogenesis which happens around the same time. | en |
| dc.description.affiliation | Instituto de Física Teórica UNESP | |
| dc.description.affiliationUnesp | Instituto de Física Teórica UNESP | |
| dc.format.extent | 123-132 | |
| dc.identifier | http://dx.doi.org/10.1007/978-3-030-15077-8_10 | |
| dc.identifier.citation | Fundamental Theories of Physics, v. 197, p. 123-132. | |
| dc.identifier.doi | 10.1007/978-3-030-15077-8_10 | |
| dc.identifier.issn | 2365-6425 | |
| dc.identifier.issn | 0168-1222 | |
| dc.identifier.scopus | 2-s2.0-85085193737 | |
| dc.identifier.uri | http://hdl.handle.net/11449/200477 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Fundamental Theories of Physics | |
| dc.source | Scopus | |
| dc.title | Reheating and Baryogenesis | en |
| dc.type | Capítulo de livro | |
| dspace.entity.type | Publication | |
| unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |