Can loop quantum cosmology describe an unified and consistent scenario since bounce until the end of inflation?

11 Sept 2018, 14:00
15m
Talk

Speaker

Eunice Valtânia de Jesus Bezerra (Instituto Nacional de Pesquisas Espaciais (INPE))

Description

The inflationary model was introduced by Guth in the 80's as a way of solving the so-called three cosmological problems: flatness of the space-time, the problem of the horizon, and the question of the magnetic monopoles. Since it was proposed, inflation has become much more than a cosmological model. The inflationary period may perhaps give us some clues about the transition from a continuum space-time (as is the universe at the end of the inflationary period) to a space-time still quantized at the beginning of the inflationary period. In this work, we try to establish a possible transition scenario between loop quantum gravity and inflation (as described by a Higgs model). The main characteristics of this possible connection will be discussed in the present work.

Primary authors

Eunice Valtânia de Jesus Bezerra (Instituto Nacional de Pesquisas Espaciais (INPE)) Oswaldo Duarte Miranda (Instituto Nacional de Pesquisas Espaciais (INPE))

Presentation materials