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共振暗能量和小尺度结构。

Resonant dark forces and small-scale structure.

机构信息

Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA.

Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA and School of Natural Sciences, Institute for Advanced Study, Princeton, New Jersey 08540, USA.

出版信息

Phys Rev Lett. 2013 Mar 15;110(11):111301. doi: 10.1103/PhysRevLett.110.111301. Epub 2013 Mar 12.

Abstract

A dark force can impact the cosmological history of dark matter (DM), both explaining observed cores in dwarf galaxies and setting the DM relic density through annihilation to dark force bosons. For GeV-TeV DM mass, DM self-scattering in dwarf galaxy halos exhibits quantum mechanical resonances, analogous to a Sommerfeld enhancement for annihilation. We show that a simple model of DM with a dark force can accommodate all astrophysical bounds on self-interactions in halos and explain the observed relic density, through a single coupling constant.

摘要

暗物质(DM)的宇宙历史可能会受到暗力量的影响,这种影响既能解释在矮星系中观测到的核心,又能通过暗物质与暗力量玻色子的湮灭来设定 DM 的残余密度。对于 GeV-TeV 质量的 DM,在矮星系晕中 DM 自散射表现出量子力学共振,类似于湮灭的索末菲增强。我们表明,一个简单的具有暗力量的 DM 模型可以通过单个耦合常数来容纳晕中所有关于自相互作用的天体物理限制,并解释观测到的残余密度。

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