Abstract

Secret neutrino interactions can play an essential role in the origin of dark matter. We present an anatomy of production mechanisms for sterile neutrino dark matter, a keV-scale gauge-singlet fermion that mixes with active neutrinos, in the presence of a new vector boson mediating secret interactions among active neutrinos. We identify three regimes of the vector boson's mass and coupling where it makes distinct impact on dark matter production through the dispersion relations and/or scattering rates. We also analyze models with gauged $L_\mu-L_\tau$ and $B-L$ numbers which have a similar dark matter cosmology but different vector boson phenomenology. We derive the parameter space in these models where the observed relic abundance is produced for sterile neutrino dark matter. They serve as well-motivated target for the upcoming experimental searches.

Highlights

  • The nature of dark matter is one of the biggest puzzles of our Universe

  • We present an anatomy of production mechanisms for sterile neutrino dark matter, a keV-scale gauge-singlet fermion that mixes with active neutrinos, in the presence of a new vector boson mediating secret interactions among active neutrinos

  • We explore the impact of a new vector boson with coupling to neutrinos on the production of sterile neutrino dark matter

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Summary

INTRODUCTION

The nature of dark matter is one of the biggest puzzles of our Universe. Many experimental searches for dark matter are ongoing but with no success yet. Alternative proposals include inflaton decays [31], freeze-in via additional particles [32,33], new interactions in the sterile sector [34,35], and gauge extensions of the Standard Model [36,37,38] These mechanisms often make dramatic changes to the ultraviolet side of the story, i.e., the initial conditions of the early Universe. Dark matter relic abundance is set by the product of the two ingredients in this mechanism, active-sterile neutrino mixing and the active neutrino reaction rate While the former is strongly constrained by indirect searches, the.

MOTIVATION FOR SECRET NEUTRINO INTERACTIONS
MODEL WITH A NEUTRINOPHILIC VECTOR BOSON
The anatomy of sterile neutrino dark matter production
Constraint from the Higgs boson invisible decay
Constraint from W boson decay width
Constraint from Z boson invisible width
Constraints from BBN and Supernova 1987A
Mono-neutrino probes at DUNE
On V coupling to other neutrino flavors
A possible UV completion
MN yLH: ð3:27Þ
CONCLUSION
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