Collider fingerprints of freeze-in dark matter produced during the fast expansion phase of Universe
Anupam Ghosh, Partha Konar, Sudipta Show

TL;DR
This paper investigates a non-standard early universe expansion scenario affecting freeze-in dark matter production, proposing a novel LHC search strategy using jet substructure and machine learning to probe the expanded parameter space.
Contribution
It introduces a new approach to detect freeze-in dark matter produced during rapid expansion phases, utilizing boosted jets and advanced analysis techniques at the LHC.
Findings
Enhanced sensitivity to non-standard cosmology scenarios.
Inclusion of one-loop QCD corrections improves prediction accuracy.
Machine learning techniques effectively discriminate signal from background.
Abstract
We examine a simple dark sector extension where the observed dark matter (DM) abundance arises from a freeze-in process through the decay of heavy vector-like quarks into a scalar dark matter candidate. The detection prospects of such DM are challenging due to the feeble nature of the interactions, but these vector-like quarks can be produced copiously at the LHC, where they decay to Standard Model quarks along with DM. Depending on the decay rate, this scenario is typically probed through long-lived particle or displaced vertex signatures, assuming a radiation-dominated background. An alternative hypothesis suggests that the Universe may have experienced a rapid expansion phase instead of the standard radiation-dominated one during freeze-in. This would significantly alter the dark matter phenomenology, requiring a substantial increase in the interaction rate to match the observed…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · International Science and Diplomacy · Particle physics theoretical and experimental studies
