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Neutrino Masses and Sterile Neutrino Dark Matter from the PeV Scale

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arxiv 1412.4791 v2 pith:NWIBFA45 submitted 2014-12-15 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords neutrinodarkmatterenergyfreeze-inmassesscalarscale
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We show that active neutrino masses and a keV-GeV mass sterile neutrino dark matter candidate can result from a modified, low energy seesaw mechanism if right-handed neutrinos are charged under a new symmetry broken by a scalar field vacuum expectation value at the PeV scale. The dark matter relic abundance can be obtained through active-sterile oscillation, freeze-in through the decay of the heavy scalar, or freeze-in via non-renormalizable interactions at high temperatures. The low energy effective theory maps onto the widely studied nuMSM framework.

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  1. Cosmic Colliders: High Energy Physics with First-Order Phase Transitions

    hep-ph 2024-12 conditional novelty 2.0 of 10

    Cosmic bubble collisions in runaway first-order phase transitions can, if the runaway regime holds, produce particles with masses far above the transition scale and energies approaching the Planck scale.

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