Fermion-portal dark matter at a high-energy muon collider
In this work, we provide a comprehensive study of fermion-portal dark matter models in the freeze-in regime at a future muon collider. For different possible nonsinglet fermion portals, we calculate the upper bound on the mediator’s mass arising from the relic abundance calculation and discuss the reach of a future muon collider in probing their viable parameter space in prompt and long-lived particle search strategies. In particular, we develop rudimentary search strategies in the prompt region and show that cuts on the invariant dilepton or dijet masses, the missing transverse mass <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msub><a:mi>M</a:mi><a:mrow><a:mi>T</a:mi><a:mn>2</a:mn></a:mrow></a:msub></a:math>, pseudorapidity and energy of leptons or jets, and the opening angle between the lepton or the jet pair can be employed to subtract the Standard Model background. In the long-lived particle regime, we discuss the signals of each model and calculate their event counts. In this region, the lepton-(quark-)portal model signal consists of charged tracks (<c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>R</c:mi></c:math>-hadrons) that either decay in the detector to give rise to a displaced lepton (jet) signature, or are detector stable and give rise to heavy stable charged track signals. As a byproduct, a pipeline is developed for including the nontrivial parton distribution function of a muon component inside a muon beam; it is shown that this leads to nontrivial effects on the kinematic distributions and attainable significances. We also highlight phenomenological features of all models unique to a muon collider and hope our results, for this motivated and broad class of dark matter models, inform the design of a future muon collider detector. We also speculate on suggestions for improving the sensitivity of a muon collider detector to long-lived particle signals in fermion-portal models.
Authors
- Samuel Homiller (ORCID: https://orcid.org/0000-0002-0063-6856)
- Pouya Asadi (ORCID: https://orcid.org/0000-0003-4712-402X)
- Aria Radick (ORCID: https://orcid.org/0000-0002-5398-6884)
- T. Yu (ORCID: https://orcid.org/0000-0003-4708-809X)
Institutions
- Cornell University (US)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2025-09-26
- DOI
- https://doi.org/10.1103/p7p8-wqqb
- Citations
- 1
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 1.87