Can sterile neutrinos be the dark matter?

被引:297
|
作者
Seljak, Uros
Makarov, Alexey
McDonald, Patrick
Trac, Hy
机构
[1] Int Ctr Theoret Phys, Trieste, Italy
[2] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[3] Univ Zurich, Inst Theoret Phys, CH-8057 Zurich, Switzerland
[4] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
[5] Princeton Univ Observ, Princeton, NJ 08544 USA
关键词
D O I
10.1103/PhysRevLett.97.191303
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We use the Ly-alpha forest power spectrum measured by the Sloan Digital Sky Survey and high-resolution spectroscopy observations in combination with cosmic microwave background and galaxy clustering constraints to place limits on a sterile neutrino as a dark matter candidate in the warm dark matter scenario. Such a neutrino would be created in the early Universe through mixing with an active neutrino and would suppress structure on scales smaller than its free-streaming scale. We ran a series of high-resolution hydrodynamic simulations with varying neutrino masses to describe the effect of a sterile neutrino on the Ly-alpha forest power spectrum. We find that the mass limit is m(s)> 13 keV at 95% C.L. (9 keV at 99.9%), which is above the upper limit allowed by x-ray constraints, excluding this candidate from being all of the dark matter in this model.
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