Neutrino magnetic moment and inert doublet dark matter in a Type-III radiative scenario
arXiv:2306.14801 · doi:10.1103/PhysRevD.108.095048
Abstract
We narrate dark matter, neutrino magnetic moment and mass in a Type-III radiative scenario. The Standard Model is enriched with three vector-like fermion triplets and two inert doublets to provide a suitable platform for the above phenomenological aspects. The inert scalars contribute to total relic density of dark matter in the Universe. Neutrino aspects are realized at one-loop with magnetic moment obtained through charged scalars, while neutrino mass gets contribution from charged and neutral scalars. Taking inert scalars up to TeV and triplet fermion in few hundred TeV range, we obtain a common parameter space, compatible with experimental limits associated with both neutrino and dark matter sectors. Using a specific region for transition magnetic moment ()), we explain the excess recoil events, reported by the XENON1T collaboration. Finally, we demonstrate that the model is able to provide neutrino magnetic moments in a wide range from to , meeting the bounds of various experiments such as Super-K, TEXONO, Borexino and XENONnT.
arXiv comment21 pages, 9 figures, version to appear in PRD
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