Muonphilic asymmetric dark matter at a future muon collider
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arXiv
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| Hauptverfasser: | , |
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| Format: | Preprint |
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2025
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| author | Roy, Arnab Volkas, Raymond R. |
| author_facet | Roy, Arnab Volkas, Raymond R. |
| contents | We explore phenomenological constraints on, and future muon collider sensitivities to, the parameter spaces of various muonphilic portals to fermionic asymmetric dark matter (ADM). Both WEFT-level dimension-6 effective operators and two UV models based on gauged $L_μ- L_τ$ are considered. One of the latter features a vector coupling to the dark matter and the other an axial vector coupling. The ADM criterion that at least $99\%$ of the dark matter relic density is asymmetric is also imposed. We identify which of these scenarios are currently allowed by direct detection and collider constraints, and then determine how much more of the parameter space could be probed by 3 and 10 TeV muon colliders with 1 ab$^{-1}$ of data. For the UV models, the constraints from $g-2$ of the muon are included. The future sensitivity curves due to neutron star heating considerations are also depicted. We present results for both the few-GeV dark matter mass regime motivated by ADM approaches to the $Ω_b \simeq Ω_\text{DM}/5$ coincidence problem, and for larger masses in the context of more general ADM. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_23159 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Muonphilic asymmetric dark matter at a future muon collider Roy, Arnab Volkas, Raymond R. High Energy Physics - Phenomenology High Energy Physics - Experiment We explore phenomenological constraints on, and future muon collider sensitivities to, the parameter spaces of various muonphilic portals to fermionic asymmetric dark matter (ADM). Both WEFT-level dimension-6 effective operators and two UV models based on gauged $L_μ- L_τ$ are considered. One of the latter features a vector coupling to the dark matter and the other an axial vector coupling. The ADM criterion that at least $99\%$ of the dark matter relic density is asymmetric is also imposed. We identify which of these scenarios are currently allowed by direct detection and collider constraints, and then determine how much more of the parameter space could be probed by 3 and 10 TeV muon colliders with 1 ab$^{-1}$ of data. For the UV models, the constraints from $g-2$ of the muon are included. The future sensitivity curves due to neutron star heating considerations are also depicted. We present results for both the few-GeV dark matter mass regime motivated by ADM approaches to the $Ω_b \simeq Ω_\text{DM}/5$ coincidence problem, and for larger masses in the context of more general ADM. |
| title | Muonphilic asymmetric dark matter at a future muon collider |
| topic | High Energy Physics - Phenomenology High Energy Physics - Experiment |
| url | https://arxiv.org/abs/2512.23159 |