Physical Review Letters · 1999 · 796 citations · 20 references
Natural SciencesAstronomyPhysicsAstrophysicsCosmologyParticle PhysicsDark MatterDark Matter CandidatesFlavor PhysicsNeutrino CosmologyNeutrino PhysicsNucleosynthesisDark Matter PhenomenologyDark Matter ProductionNeutrino AstrophysicsNeutrino Flavor PhysicsSterile Neutrinos In Cosmology
The authors propose a new dark matter candidate: sterile neutrinos with masses between ~100 eV and ~10 keV produced via lepton‑number‑driven resonant MSW conversion of active neutrinos. Production occurs through resonant MSW conversion driven by lepton‑number asymmetries of 10⁻³–10⁻¹ relative to the photon density. The resulting nonthermal, cold spectrum causes the sterile neutrinos to become nonrelativistic early, yielding free‑streaming lengths at or below dwarf‑galaxy scales and thereby avoiding the usual light‑neutrino dark‑matter constraints.
We propose a new and unique dark matter candidate: $\ensuremath{\sim}100$ eV to $\ensuremath{\sim}10$ keV sterile neutrinos produced via lepton-number-driven resonant Mikheyev-Smirnov-Wolfenstein conversion of active neutrinos. The requisite lepton number asymmetries in any of the active neutrino flavors range from ${10}^{\ensuremath{-}3}$ to ${10}^{\ensuremath{-}1}$ of the photon number. The unique feature here is that the adiabaticity condition of the resonance strongly favors the production of lower energy sterile neutrinos. The resulting nonthermal (cold) energy spectrum can cause these sterile neutrinos to revert to nonrelativistic kinematics at an early epoch, so that free-streaming lengths at or below the dwarf galaxy scale are possible. Therefore, the main problem associated with light neutrino dark matter can be circumvented in our model.
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