Reheating and Baryogenesis

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2020-12-12T02:07:38Z
dc.date.accessioned2022-12-19T21:04:58Z
dc.date.available2020-12-12T02:07:38Z
dc.date.available2022-12-19T21:04:58Z
dc.date.created2020-12-12T02:07:38Z
dc.date.issued2019-01-01
dc.identifierFundamental Theories of Physics, v. 197, p. 123-132.
dc.identifier2365-6425
dc.identifier0168-1222
dc.identifierhttp://hdl.handle.net/11449/200477
dc.identifier10.1007/978-3-030-15077-8_10
dc.identifier2-s2.0-85085193737
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5381111
dc.description.abstractIn 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.
dc.languageeng
dc.relationFundamental Theories of Physics
dc.sourceScopus
dc.titleReheating and Baryogenesis
dc.typeCapítulos de libros


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