English

Up-type FCNC in presence of Dark Matter

High Energy Physics - Phenomenology 2026-03-31 v2 High Energy Physics - Experiment

Abstract

Dark Matter (DM) is a known unknown. Apart, current experimental constraints on flavor-changing neutral current (FCNC) processes involving up-type quarks also provide scope to explore physics beyond the Standard Model (SM). In this article, we establish a connection between the flavor sector and the DM sector with minimal extension of the SM. Here a singlet complex scalar field, stable under Z3\mathbb{Z}_3 symmetry, acts as DM and couples to SM up-type quarks through a heavy Dirac vector-like quark (VLQ), which shares the same Z3\mathbb{Z}_3 charge as of the DM. The model thus addresses the observed D0D0ˉD^0-\bar{D^0} mixing, top-FCNC interactions, and D0D^0 meson decays, together with DM relic density, while evading the direct and indirect DM search bounds. The model can be probed at the future high-energy muon collider, through distinctive signatures of VLQ production, where the VLQ decays into DM and SM particles, abiding by the existing bounds.

Keywords

Cite

@article{arxiv.2504.20045,
  title  = {Up-type FCNC in presence of Dark Matter},
  author = {Subhaditya Bhattacharya and Lipika Kolay and Dipankar Pradhan and Abhik Sarkar},
  journal= {arXiv preprint arXiv:2504.20045},
  year   = {2026}
}

Comments

Added new top-FCNC bounds and a section on future predictions