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无菌中微子会是暗物质吗?

Can sterile neutrinos be the dark matter?

作者信息

Seljak Uros, Makarov Alexey, McDonald Patrick, Trac Hy

机构信息

International Center for Theoretical Physics, Trieste, Italy.

出版信息

Phys Rev Lett. 2006 Nov 10;97(19):191303. doi: 10.1103/PhysRevLett.97.191303. Epub 2006 Nov 8.

Abstract

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.

摘要

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。

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