Lepton collider as a window to reheating via freezing in dark matter detection. Part II
arXiv:2410.18198 · doi:10.1007/JHEP07(2025)157
Abstract
Dark matter (DM) genesis via Ultraviolet (UV) freeze-in embeds the seed of reheating temperature and dynamics in its relic density. Thus, discovery of such a DM candidate can possibly open the window for post-inflationary dynamics. However, there are several challenges in this exercise, as freezing-in DM possesses feeble interaction with the visible sector and therefore very low production cross-section at the collider. We show that mono-photon (and dilepton) signal at the ILC, arising from DM effective operators connected to the SM field strength tensors, can still warrant a signal discovery. We study both the scalar and fermionic DM production during reheating via UV freeze-in, when the inflaton oscillates at the bottom of a general monomial potential. Interestingly, we see, right DM abundance can be achieved only in the case of bosonic reheating scenario, satisfying bounds from big bang nucleosynthesis (BBN). This provides a unique correlation between collider signal and the post-inflationary dynamics of the Universe within single-field inflationary models.
28 pages, 11 figures, 4 tables, and matches the version published in JHEP
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Cited by in corpus (6)
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- Multi-messenger FIMP
- Freeze-in and freeze-out production of Higgs portal Majorana fermionic dark matter during and after reheating
- Seasons of Dark Matter Freeze-In Shaped by the Weather of the Early Universe
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- Photonic Freeze-In