Seljak Uros, Makarov Alexey, McDonald Patrick, Trac Hy
International Center for Theoretical Physics, Trieste, Italy.
Phys Rev Lett. 2006 Nov 10;97(19):191303. doi: 10.1103/PhysRevLett.97.191303. Epub 2006 Nov 8.
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.
我们结合斯隆数字巡天测量的莱曼α森林功率谱和高分辨率光谱观测数据,以及宇宙微波背景和星系团聚类限制,对作为温暗物质情景中暗物质候选者的惰性中微子进行限制。这样的中微子会在早期宇宙中通过与活性中微子混合而产生,并会抑制小于其自由流尺度的尺度上的结构形成。我们进行了一系列具有不同中微子质量的高分辨率流体动力学模拟,以描述惰性中微子对莱曼α森林功率谱的影响。我们发现,在95%置信水平下,质量限制为m(s)>13 keV(在99.9%置信水平下为9 keV),这高于X射线限制所允许的上限,排除了该候选者作为该模型中所有暗物质的可能性。