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arXiv · 2210.15653

Freezing-in hadrophilic dark matter at low reheating temperatures

Abstract

If the reheating temperature at the end of inflation is low, of order 10 MeV, then dark matter produced through ultraviolet freeze-in has a large direct detection cross section. We study such a scenario in which dark matter is hadrophilic. This leads to dark matter-nucleon scattering cross sections of interest for near-future experiments for dark matter masses in the range of 100 keV-100 MeV. We explore how these predictions vary if reheating is non-instantaneous.

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Prudhvi N. Bhattiprolu, Gilly Elor, Robert McGehee, Aaron Pierce. 2022-10-27. Freezing-in hadrophilic dark matter at low reheating temperatures. https://doi.org/10.1007/jhep01(2023)128

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