Warm Dark Matter from keVins
arXiv:1205.0551 · doi:10.1088/1475-7516/2012/08/016
Abstract
We propose a simple model for Warm Dark Matter (WDM) in which two fermions are added to the Standard Model: (quasi-) stable "keVins" (keV inert fermions) which account for WDM and their unstable brothers, the "GeVins" (GeV inert fermions), both of which carry zero electric charge and lepton number, and are (approximately) "inert", in the sense that their only interactions are via suppressed couplings to the Z. We consider scenarios in which stable keVins are thermally produced and their abundance is subsequently diluted by entropy production from the decays of the heavier unstable GeVins. This mechanism could be implemented in a wide variety of models, including E_6 inspired supersymmetric models or models involving sterile neutrinos.
32 pages, 9 figures, 2 tables
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Cited by in corpus (26)
- Sterile Neutrino Dark Matter
- A White Paper on keV Sterile Neutrino Dark Matter
- The Present and Future Status of Heavy Neutral Leptons
- New Production Mechanism for keV Sterile Neutrino Dark Matter by Decays of Frozen-In Scalars
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- Fermionic WIMPs and Vacuum Stability in the Scotogenic Model
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- Dark Radiation or Warm Dark Matter from long lived particle decays in the light of Planck
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- Exotic Higgs decays in the E6 inspired SUSY models
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- Common origin of reactor and sterile neutrino mixing
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