The Dark Universe after Reheating in String Inflation
High Energy Physics - Theory
2022-12-28 v1 High Energy Physics - Phenomenology
Abstract
We study the production of dark matter and dark radiation after reheating in string inflation models where the Calabi-Yau has a fibred structure and the visible sector lives on D3 branes. We show how the interplay between different physical constraints from inflation, reheating, supersymmetry breaking and dark radiation, leads to distinct predictions for the nature of dark matter.
Cite
@article{arxiv.2208.01017,
title = {The Dark Universe after Reheating in String Inflation},
author = {Michele Cicoli and Kuver Sinha and Robert Wiley Deal},
journal= {arXiv preprint arXiv:2208.01017},
year = {2022}
}
Comments
12 pages, 4 figures