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

Authors

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

Abstract

We explore the sensitivity of a future muon collider to dark Z decaying to ee+, μμ+, ττ+, qq̅, WW+, 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 WW+ 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.

Issue

Article ID

SPP-2025-2B-02

Section

High Energy and Nuclear Physics

Published

2025-06-15

How to Cite

[1]
NA Rabang, M Flores, and P Tanedo, Unraveling the sensitivity of a future muon collider to dark Z resonances, Proceedings of the Samahang Pisika ng Pilipinas 43, SPP-2025-2B-02 (2025). URL: https://proceedings.spp-online.org/article/view/SPP-2025-2B-02.