Journal
PHYSICAL REVIEW LETTERS
Volume 124, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.124.041802
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Funding
- U.S. Department of Energy [DE-AC02-07CH11359]
- DOE [DE-SC0012012]
- NSF [PHY-1620074]
- Maryland Center for Fundamental Physics
- Florida State University [084011-550-042584]
- National Science Foundation [NSF PHY-1748958]
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Rare kaon decays are excellent probes of light, new weakly coupled particles. If such particles X couple preferentially to muons, they can be produced in K -> mu nu X decays. We evaluate the future sensitivity for this process at NA62 assuming X decays either invisibly or to dimuons. Our main physics target is the parameter space that resolves the (g - 2)(mu) anomaly, where X is a gauged L-mu - L-tau vector or a muonphilic scalar. The same parameter space can also accommodate dark matter freeze-out or reduce the tension between cosmological and local measurements of H-0 if the new force decays to dark matter or neutrinos, respectively. We show that for invisible X decays, a dedicated single muon trigger analysis at NA62 could probe much of the remaining (g - 2)(mu) favored parameter space. Alternatively, if X decays to muons, NA62 can perform a dimuon resonance search in K -> 3 mu nu events and greatly improve existing coverage for this process. Independently of its sensitivity to new particles, we find that NA62 is also sensitive to the standard model predicted rate for K -> 3 mu nu, which has never been measured.
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