Abstract

Muonium is a bound state composed of an antimuon and an electron, and it constitutes a hydrogen-like atom. Because of the absence of the hadronic matter in the bound state, the muonium is a useful probe to explore new physics being free from the hadronic uncertainties. The process of the muonium-to-antimuonium transition is considered to be effective to identify fundamental interactions which relate to the lepton flavor and lepton number violation. New experiments are being planned at J-PARC in Japan and CSNS in China, and it is expected to attract more attention in the near future. In this paper, we will study what kind of model can be verified in the next generation of the muonium-to-antimuonium transition search experiments while escaping the limitations from other experiments. Though the transition probability is strongly suppressed by the lepton flavor conservation in the standard model, it can be much larger by the exchanges of neutral and doubly charged bosons, and by box loop diagrams in new physics beyond the standard model. We study the neutrino models with heavy Majorana neutrinos at TeV scale, a type-II seesaw model, left--right models, and models for radiative neutrino masses such as the Zee-Babu model in particular, in addition to other possible models to induce the sizable transition probability, which can be tested in the forthcoming experiments.

Highlights

  • The muonium (Mu∶ μþe−) to antimuonium (Mu∶ μ−eþ) transition is an interesting phenomenological possibility [1,2,3,4]

  • The process of the muonium-toantimuonium transition is considered to be effective to identify fundamental interactions which relate to the lepton flavor and lepton number violation

  • Though the transition probability is strongly suppressed by the lepton flavor conservation in the standard model, it can be much larger by the exchanges of neutral and doubly charged bosons, and by box loop diagrams in new physics beyond the standard model

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Summary

INTRODUCTION

The muonium (Mu∶ μþe−) to antimuonium (Mu∶ μ−eþ) transition is an interesting phenomenological possibility [1,2,3,4]. If the lepton flavor numbers of the new particles are even, the severe experimental constraints can be avoided and an observable size of the Mu-to-Mu transition at near-future experiments can be induced at the tree level. Those circumstances of the new physics contributions from flavor violation are similar to the meson mixings in the models beyond the SM. We classify the new particles and interactions that causes the Mu-to-Mu transition in the models beyond the SM, and make introductory remarks on how a sizable transition to be observed in the near-future experiments can be induced avoiding the constraints such as LFV processes, which we have briefly mentioned above (Sec. III).

MODEL INDEPENDENT DESCRIPTION OF Mu-to-Mu TRANSITION
Operators
Magnetic field dependence
Muonium hyperfine structure
CLASSIFICATION OF THE MEDIATORS
HEAVY MAJORANA NEUTRINOS
UμiUÃei i
XαI XβI
TYPE-II SEESAW MODEL
Δþ ð5:24Þ
LEFT-RIGHT MODEL
Case 1
WL ð6:10Þ
X ð6:14Þ
Case 2
RADIATIVE NEUTRINO MASS
Models with doubly charged scalar
Cocktail model
Charged Higgs contribution
KNT model
AKS model
VIII. NEUTRAL SCALAR EXCHANGE
R-parity violation
Gaugino contribution
Charged Higgsino contribution
DILEPTON GAUGE BOSONS
FLAVORED GAUGE BOSONS
Leptoquark
Vectorlike fermions
Axionlike particle
XIII. CONCLUSION
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