Right-handed sneutrinos as thermal dark matter

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Abstract

We analyse the abundance of right-handed sneutrinos in the supersymmetric FD-term model of hybrid inflation. As well as providing a natural solution to the μ- and gravitino overabundance problems, the model offers the lightest right-handed sneutrino as a candidate for thermal dark matter. The FD-term model predicts a new quartic coupling of purely right-handed sneutrinos to the Higgs doublets that thermalises the sneutrinos and makes them annihilate sufficiently fast to a level compatible with the current cosmic microwave background data. We discuss this scenario and identify favourable regions of the parameter space within mSUGRA. © 2010 IOP Publishing Ltd.

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APA

Deppisch, F., & Pilaftsis, A. (2010). Right-handed sneutrinos as thermal dark matter. In Journal of Physics: Conference Series (Vol. 259). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/259/1/012078

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