Speaker
Dr
Gabriella Piccinelli
(Universidad Nacional Autónoma de México)
Description
Magnetic fields are ubiquitous in the Universe and their generation mechanism is an open problem in cosmology. Their presence on all scales strengthens the idea of a primordial origin. If this is the case, a magnetic cosmological model has to be built. Here, we discuss the possible effects that primordial magnetic fields can have on a warm inflation scenario, in particular on the inflaton effective potential.
Primary author
Dr
Gabriella Piccinelli
(Universidad Nacional Autónoma de México)
