Abstract

“Portal” models that connect the Standard Model to a Dark Sector allow for a wide variety of scenarios beyond the simplest WIMP models. Kinetic mixing of gauge fields in particular has allowed a broad range of new ideas. However, the models that evade CMB constraints are often non-generic, with new mass scales and operators to split states and suppress indirect detection signals. Models with a “portalino”, a neutral fermion that marries a linear combination of a standard model neutrino and dark sector fermion and carries a conserved quantum number, can be simpler. This is especially interesting for interacting dark sectors; then the unmarried linear combination which we identify as the standard model neutrino inherits these interactions too, and provides a new, effective interaction between the dark sector and the standard model. These interactions can be simple Z′ type interactions or lepton-flavor changing. Dark matter freezes out into neutrinos, thereby evading CMB constraints, and conventional direct detection signals are largely absent. The model offers different signals, however. The “portalino” mechanism itself predicts small corrections to the standard model neutrino couplings as well as the possibility of discovering the portalino particle in collider experiments. Possible cosmological and astroparticle signatures include monochromatic neutrino signals from annihilation, spectral features in high energy CR neutrinos as well as conventional signals of additional light species and dark matter interactions.

Highlights

  • The kinetic mixing portal, and the neutrino portal

  • Abstract: “Portal” models that connect the Standard Model to a Dark Sector allow for a wide variety of scenarios beyond the simplest WIMP models

  • Models with a “portalino”, a neutral fermion that marries a linear combination of a standard model neutrino and dark sector fermion and carries a conserved quantum number, can be simpler

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Summary

The portalino

The neutrino portal is typically thought of as a relatively benign interaction. It produces a. If the gauge symmetry is broken, just as the standard model neutrino does, ψ can marry the singlet, and the massless eigenstate will inherit its interactions This singlet fermion which conveys these new interactions to the physical neutrino, and the resulting mass eigenstate we refer to as the “portalino.”. Unlike kinetic mixing which requires a U(1) for a renormalizable interaction, here, regardless of how complicated the new sector’s particle content is and what the gauge sector looks like, so long is there is a gauge singlet operator (akin to Lh in the SM) one can develop the interaction in question While this particular scenario is new, it draws from a number of ingredients that have existed in the literature. These last two are closest in content to the scenario described here

A simple model
Multiple portalinos
Non-Abelian models
Dark matter freezeout
Portalino phenomenology and neutrino constraints
Portalino cosmology
Light species
Findings
Discussion
Full Text
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