English

A Flavour Inspired Model for Dark Matter

High Energy Physics - Phenomenology 2022-06-15 v1 Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena

Abstract

The discrepancies between data on rare bb-hadron decays, controlled by the underlying neutral-current transitions bs+(=e,μ)b\to s\ell^+\ell^- (\ell = e, \mu), and the corresponding Standard Model predictions constitute one of the most intriguing hints for new physics. Leptoquarks are prime candidates to solve these anomalies and, in particular, the scalar leptoquark, S3S_3, triplet under SU(2)LSU(2)_L with hypercharge Y=1/3Y=-1/3, provides a very good fit to data. Here, for the first time, we entertain the possibility that the same scalar leptoquark, responsible for the LFU anomalies, is the portal to a dark sector consisting of two additional vector-like fermions, one of which is a candidate for the cosmological dark matter. We study two scenarios, where the dark matter candidate belongs to an SU(2)LSU(2)_L singlet and triplet respectively, and discuss the theory parameter space in the context of the dark matter candidate's relic density and prospects for direct and indirect dark matter searches. Direct detection rates are highly suppressed, and generically below the neutrino floor. Current observations with, and future prospects for, high-energy gamma-ray telescopes such as HESS and the Cherenkov Telescope Array are much more promising, as they already provide powerful constraints on the models under consideration, and will potentially probe the full parameter space in the future.

Keywords

Cite

@article{arxiv.2206.06768,
  title  = {A Flavour Inspired Model for Dark Matter},
  author = {Claudio Andrea Manzari and Stefano Profumo},
  journal= {arXiv preprint arXiv:2206.06768},
  year   = {2022}
}

Comments

11 pages, 4 figures and 1 table

R2 v1 2026-06-24T11:50:36.945Z