Speaker
Sushant Yadav 2020504
Description
The Dirac scotogenic model provides an elegant mechanism which generates small Dirac neutrino masses at the one loop level with a single symmetry, the so-called chiral $U(1)_{B-L}$, simultaneously protecting the ``Diracness'' of the neutrinos, the smallness of their mass and the stability of the dark matter candidate. Despite being chiral, this symmetry is also anomaly-free and thus could be gauged. Here we thoroughly explore the phenomenological implications of such a construction in the Dark Matter (DM) sector, charged Lepton Flavor Violation (cLFV) and ElectroWeak (EW) vacuum stability.
Track type | Dark Matter |
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