Ústav technické a experimentální fyziky Institute of Experimental and Applied Physics

Dark matter and B-meson anomalies in a flavor dependent gauge symmetry

NázevTitle
Dark matter and B-meson anomalies in a flavor dependent gauge symmetryDark matter and B-meson anomalies in a flavor dependent gauge symmetry
Druh výsledkuResult type
Článek v časopiseJournal article
AutořiAuthors
P.T.P. Hutauruk, T. Nomura, H. Okada, Y. Orikasa
DOIDOI
10.1103/PhysRevD.99.055041
Časopis / citaceJournal / citation
Physical Review D. 2019, 99(5), 1-8. ISSN 2470-0010.
RokYear
2019
JazykLanguage
eng
WoSWoS
000462913900008
ScopusScopus
2-s2.0-85064394848
RIVRIV
RIV/68407700:21670/19:00338226!RIV20-MSM-21670___
ProjektProject
Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics

AbstraktAbstract

A possibility of explaining the anomalies in the semileptonic B-meson decay B→K*μμ¯ has been explored in the framework of the gauged U(1)μ-τ symmetry. Apart from the muon anomalous magnetic moment and neutrino sector, we formulate the model starting with a valid Lagrangian and consider the constraints from the neutral meson mixings, the bounds on direct detection and the relic density of the bosonic dark matter candidate augmented to collider constraints. We search the parameter space, which accommodate the size of the anomaly of the B→K*μμ¯ decay, to satisfy all experimental constraints. We found the allowed region on the plane of the dark matter and Z′ masses is rather narrow compared to the previous analysis.

A possibility of explaining the anomalies in the semileptonic B-meson decay B→K*μμ¯ has been explored in the framework of the gauged U(1)μ-τ symmetry. Apart from the muon anomalous magnetic moment and neutrino sector, we formulate the model starting with a valid Lagrangian and consider the constraints from the neutral meson mixings, the bounds on direct detection and the relic density of the bosonic dark matter candidate augmented to collider constraints. We search the parameter space, which accommodate the size of the anomaly of the B→K*μμ¯ decay, to satisfy all experimental constraints. We found the allowed region on the plane of the dark matter and Z′ masses is rather narrow compared to the previous analysis.