Dark Population Transfer Mechanism for Sterile Neutrino Dark Matter

被引:0
|
作者
Fuller, George M. [1 ]
Graf, Lukas [1 ,2 ]
Patwardhan, Amol, V [3 ,4 ]
Spisak, Jacob [1 ,5 ]
机构
[1] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[2] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[3] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
[4] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[5] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany
基金
美国国家科学基金会;
关键词
DWARF GALAXIES; CONSTRAINTS; DISPERSION; VMSM;
D O I
10.1103/PhysRevLett.133.181002
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We present a mechanism for producing a cosmologically significant relic density of one or more sterile neutrinos. This scheme invokes two steps: First, a population of "heavy" sterile neutrinos is created by scattering-induced decoherence of active neutrinos. Second, this population is transferred, via sterile neutrino self-interaction-mediated scatterings and decays, to one or more lighter mass ( 10 keV to 1 GeV) sterile neutrinos that are far more weakly (or not at all) mixed with active species and could constitute dark matter. Dark matter produced this way can evade current electromagnetic and structure- based bounds, but may nevertheless be probed by future observations.
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页数:7
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