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keV Neutrino Model Building

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If you have a question about this talk, please contact Helen Vryonidou.

In this talk, an introduction to keV sterile neutrinos as Dark Matter particles is given. After reviewing the cosmological aspects of (Warm) Dark Matter, I will explain why the topic is interesting for particle physics model building and also point out the differences to ordinary neutrino model building. We will go through a couple of generic models, all of which yield interesting and fundamental connections between the neutrino and the Dark Matter sectors. We finally present some alternative ideas and generalizations.

This talk is part of the HEP phenomenology joint Cavendish-DAMTP seminar series.

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