Abstract

We consider a class of models in which the neutrinos acquire Majorana masses through mixing with singlet neutrinos that emerge as composite states of a strongly coupled hidden sector. In this framework, the light neutrinos are partially composite particles that obtain their masses through the inverse seesaw mechanism. We focus on the scenario in which the strong dynamics is approximately conformal in the ultraviolet, and the compositeness scale lies at or below the weak scale. The small parameters in the Lagrangian necessary to realize the observed neutrino masses can naturally arise as a consequence of the scaling dimensions of operators in the conformal field theory. We show that this class of models has interesting implications for a wide variety of experiments, including colliders and beam dumps, searches for lepton flavor violation and neutrinoless double beta decay, and cosmological observations. At colliders and beam dumps, this scenario can give rise to striking signals involving multiple displaced vertices. The exchange of hidden sector states can lead to observable rates for flavor violating processes such as μ → eγ and μ → e conversion. If the compositeness scale lies at or below a hundred MeV, the rate for neutrinoless double beta decay is suppressed by form factors and may be reduced by an order of magnitude or more. The late decays of relic singlet neutrinos can give rise to spectral distortions in the cosmic microwave background that are large enough to be observed in future experiments.

Highlights

  • PWODGT XKQNCVKQP smallness of neutrino masses is explained by the fact they arise from operators of dimension greater than four

  • We consider a class of models in which the neutrinos acquire Majorana masses through mixing with singlet neutrinos that emerge as composite states of a strongly coupled hidden sector

  • We consider a framework in which the neutrinos acquire Majorana masses through mixing with singlet neutrinos that emerge as composite states of a strongly coupled hidden sector, as shown schematically in figure 1

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Summary

An inverse seesaw model from strong dynamics

We describe our framework for neutrino mass generation based on the partial compositeness of neutrinos. For high values of MUV, even if λis of order one in the ultraviolet, the mixing can be sufficiently suppressed so as to result in suitably small masses for the light neutrinos This remains true even if O2Nc is a (slightly) relevant operator, so that overall lepton number is violated by order one in the infrared, as illustrated in Benchmark I in the table. If O2Nc is instead a (slightly) irrelevant operator, overall lepton number can emerge as an accidental symmetry at the compositeness scale, in which case it will play a role in the suppression of neutrino masses This is illustrated in Benchmark II in the table. We will connect the parameter space to specific experimental observations

Colliders
W and Z decays
Current constraints and future reach from HNL searches
Novel signatures
Beam dumps
Muon magnetic moment and lepton flavor violation
Muon magnetic moment
Lepton flavor violation
Neutrinoless double beta decay
Cosmological history
Cosmological bounds on the compositeness scale
Spectral distortions of the CMB from late decays
Astrophysics
Conclusions
A Matrix elements and widths
Full Text
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