Up-type FCNC in presence of Dark Matter
Up-type FCNC in presence of Dark Matter
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 $\mathbb{Z}_3$ symmetry, acts as DM and couples to SM up-type quarks through a heavy Dirac vector-like quark (VLQ), which shares the same $\mathbb{Z}_3$ charge as of the DM. The model thus addresses the observed $D^0-\bar{D^0}$ mixing, top-FCNC interactions, and $D^0$ 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.
Subhaditya Bhattacharya、Lipika Kolay、Dipankar Pradhan、Abhik Sarkar
物理学
Subhaditya Bhattacharya,Lipika Kolay,Dipankar Pradhan,Abhik Sarkar.Up-type FCNC in presence of Dark Matter[EB/OL].(2025-04-28)[2025-06-23].https://arxiv.org/abs/2504.20045.点此复制
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