Probing Muonphilic Force Carriers and Dark Matter at Kaon Factories

被引:67
作者
Krnjaic, Gordan [1 ]
Marques-Tavares, Gustavo [2 ,3 ]
Redigolo, Diego [4 ,5 ,6 ]
Tobioka, Kohsaku [7 ,8 ]
机构
[1] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA
[2] Univ Maryland, Dept Phys, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA
[3] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94305 USA
[4] Tel Aviv Univ, IL-6997801 Tel Aviv, Israel
[5] Inst Adv Study, Princeton, NJ 08540 USA
[6] Weizmann Inst Sci, IL-7610001 Rehovot, Israel
[7] Florida State Univ, Tallahassee, FL 32306 USA
[8] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan
基金
美国国家科学基金会;
关键词
SEARCH; K+;
D O I
10.1103/PhysRevLett.124.041802
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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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页数:6
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