Năstase, Horaţiu [UNESP]2020-12-122020-12-122019-01-01Fundamental Theories of Physics, v. 197, p. 123-132.2365-64250168-1222http://hdl.handle.net/11449/200477In 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.123-132engCapítulo de livro10.1007/978-3-030-15077-8_102-s2.0-85085193737