We propose a new and unique dark matter candidate: similar to 100 eV to similar to 10 keV sterile neutrinos produced via lepton-number-driven resonant Mikheyev-Smimov-Wolfenstein conversion of active neutrinos. The requisite lepton number asymmetries in any of the active neutrino flavors range from 10(-3) to 10(-1) of the photon number. The unique feature here is that the adiabaticity condition of the resonance strongly fat ors 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 fret-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 stir model. [S0031-9007(99)08792-X].
机构:
Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China
Chinese Univ Hong Kong, Inst Theoret Phys, Shatin, Hong Kong, Peoples R ChinaChinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China