Speaker
Liliana Velasco-Sevilla
(Sogang University)
Description
The advent of using Gravitational Waves (GW) as a powerful method to understand the evolution of our early universe has arrived. In this talk, I will present an example of how the reheating temperature can be constrained only from GW coming from the Standard Model of Particle Physics plasma of the early universe both in Standard Cosmology and in a particular Gauss-Bonnet Scenario. In addition, if information of a particular model for inflation is given, this can constrain further the reheating temperature.
Primary author
Liliana Velasco-Sevilla
(Sogang University)
