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August 17, 2025Journal of High Energy Physics2 citationsOpen Access

Multicomponent dark matter with collider implications

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LCLaura CoviSDShyamashish DeySKSarif Khan

Key Points

  • Distinctive collider signals may indicate a multicomponent dark matter model, focusing on specific DM interactions.
  • The model yields potential signals in LHC experiments with dark fermions and inert doublets due to Higgs resonance.
  • By extending the standard model via dark gauge symmetry, new particle behaviors may lead to unique detection prospects.
  • Collider experiments and direct detection methods are crucial for fully understanding the dark matter parameter space.

Abstract

A bstract The present work aims to study an extension of the Standard Model (SM) that addresses the prominent SM shortcomings, i.e., can explain the neutrino mass, the dark matter (DM) content, and the matter-antimatter asymmetry of the Universe. The model introduces the possibility of a multicomponent DM scenario leading to distinctive signals at colliders. The SM is extended by a “dark” SU(2) D gauge symmetry and new fermions and scalar doublets, charged only under SU(2) D , that provide candidates for a multicomponent DM. Previously, we have considered in this model the asymmetric DM scenario, while in the present work, we explore the symmetric DM case. We focus on the parameter region where the dark fermion DM annihilates dominantly into the additional dark gauge bosons and the “inert” doublet DM annihilates to SM states via the SM Higgs resonance. This particular choice of doublet mass ensures that the heavier BSM Higgs always has one decay mode open to DM leading to the possibility of detecting such particles at the LHC, in the missing energy plus dijet ("Image missing" + 2 j ) final states. We also discuss the prospects for detecting DM through direct and indirect detection experiments and via Long-Lived-Particle searches. Finally, we show that, as typical of other WIMP models, for low DM mass, signals can be expected in future collider experiments, but for the higher mass range above 500 GeV we have to rely solely on direct detection experiments. Both types of experiments will be essential to fully cover the allowed parameter space.

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Cite This Study

Covi et al. (2025) studied this question.

synapsesocial.com/papers/68a36c210a429f797332fbfehttps://doi.org/10.1007/jhep08(2025)046
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