Unraveling the sensitivity of a future muon collider to dark Z resonances

Authors

  • Nicko Angelo Rabang National Institute of Physics, University of the Philippines Diliman
  • Marvin Flores National Institute of Physics, University of the Philippines Diliman
  • Philip Tanedo Department of Physics and Astronomy, University of California, Riverside

Abstract

We explore the sensitivity of a future muon collider to dark Z decaying to e−e+, μ−μ+, τ−τ+, qq̅, W−W+, and ZH at √s = 3 TeV  (ℒ = 2ab−1) and √s = 10 TeV (ℒ = 10 ab−1) centre-of-mass energies and projected integrated luminosities. We found that without putting explicit cuts on the background, the muon collider is mostly sensitive in the production mode channel where dark Z decays to W−W+ due to longitudinal W± contributions to the signal cross section. This corresponds to the branching ratio where mass mixing dominates over kinetic mixing. Thus, the muon collider can effectively distinguish dark Z from a dark photon.

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Published

2025-06-15

How to Cite

[1]
“Unraveling the sensitivity of a future muon collider to dark Z resonances”, Proc. SPP, vol. 43, no. 1, pp. SPP–2025, Jun. 2025, Accessed: Mar. 31, 2026. [Online]. Available: https://proceedings.spp-online.org/article/view/SPP-2025-2B-02