Ref HAL: hal-01203042_v1
DOI: 10.1088/1475-7516/2015/07/002
WoS: WOS:000359259500002
Exporter : BibTex | endNote
36 Citations
Résumé:

We consider the possibility to produce a bouncing universe in the framework of scalar-tensor gravity models in which the scalar field potential may be negative, and even unbounded from below. We find a set of viable solutions with nonzero measure in the space of initial conditions passing a bounce, even in the presence of a radiation component, and approaching a constant gravitational coupling afterwards. Hence we have a model with a minimal modification of gravity in order to produce a bounce in the early universe with gravity tending dynamically to general relativity (GR) after the bounce.