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Dipolar dark matter in light of 3.5 keV X-ray Line, Neutrino mass and LUX data

A simple extension of the standard model (SM) providing transient magnetic moments to right-handed neutrinos is presented. In this model, the decay of next-to-lightest right-handed heavy neutrino to the lightest one and a photon (N 2 -> N 1 + gamma) can explain the 3.5 keV X-ray line signal observed by XMM-Newton X-ray observatory. Beside the SM particles and heavy right-handed Majorana neutrinos, the model contains a singly charged scalar (H) and an extra Higgs doublet (Sigma). Within this minimal set of extra fields the sub-eV masses of left-handed neutrinos are also explained. Moreover, we show that the spin-independent DM-nucleon cross-section is compatible with latest LUX data.

preprint2014arXivOpen access
Sudhanwa PatraNirakar SahooNarendra Sahu
hep-phastro-ph.HE
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Sudhanwa PatraNirakar SahooNarendra Sahu

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