Sneutrino dark matter in light of PAMELA

TL;DR

This paper explores right-handed sneutrino dark matter within a U(1)_{B-L} extended supersymmetric model, showing it can explain PAMELA and FERMI data and be detected in future experiments.

Contribution

It demonstrates that right-handed sneutrinos in a U(1)_{B-L} model can serve as viable thermal dark matter candidates compatible with recent cosmic ray observations.

Findings

Sneutrino annihilation is enhanced via Higgs sector exchange.

Sneutrino masses of 1-2 TeV fit PAMELA and FERMI data.

Elastic scattering cross section is within reach of future detection experiments.

Abstract

In the U(1)_{B-L} extension of the minimal supersymmetric standard model the right-handed sneutrino is a natural candidate for thermal dark matter. Sneutrino annihilation at the present time can be considerably enhanced due to the exchange of the lightest field in the Higgs sector that breaks U(1)_{B-L}. The annihilation mainly produces taus (or muons) by the virtue of B-L charge assignments. A sneutrino mass of 1-2 TeV provides a good fit to the PAMELA and is compatible with the latest results from the FERMI experiment. In addition, the sneutrino-nucleon elastic scattering cross section is within the reach of the upcoming and future direct detection experiments.