Speaker
Jaime Haro Cases
Description
In this talk, I address the gravitational production of dark matter in two distinct scenarios:
first, when reheating is driven by gravitational particle production, and second, when reheating is dominated by the decay of the inflaton field.
I establish a relationship between the reheating temperature and the mass of dark matter, and by leveraging the constraints on reheating,
I demonstrate how to determine the range of viable dark matter mass values. This analysis provides a framework for understanding the
interplay between reheating dynamics and the properties of dark matter in the early universe
