Minimal dark matter freeze-in with low reheating temperatures and implications for direct detection
We investigate the influence of the reheating temperature of the visible sector on the freeze-in dark matter (DM) benchmark model for direct detection experiments, where DM production is mediated by an ultralight dark photon. Here, we consider a new regime for this benchmark: we take the initial temperature of the thermal Standard Model (SM) bath to be below the DM mass. The production rate from the SM bath is drastically reduced due to Boltzmann suppression, necessitating a significant increase in the portal coupling between DM and the SM to match the observed relic DM abundance. This enhancement in coupling strength increases the predicted DM-electron scattering cross section, making freeze-in DM more accessible to current direct detection experiments.
Authors
- Kimberly K. Boddy (ORCID: https://orcid.org/0000-0003-1928-4667)
- Katherine Freese (ORCID: https://orcid.org/0000-0001-9490-020X)
- Gabriele Montefalcone (ORCID: https://orcid.org/0000-0002-6794-9064)
- Barmak Shams Es Haghi (ORCID: https://orcid.org/0000-0001-9563-0299)
Institutions
- Nordic Institute for Theoretical Physics (SE)
- Stockholm University (SE)
- The University of Texas at Austin (US)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2025-03-17
- DOI
- https://doi.org/10.1103/physrevd.111.063537
- Citations
- 15
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 28.05
Funders
- National Science Foundation
- U.S. Department of Energy
- University of Texas at Austin
- Vetenskapsrådet
- High Energy Physics