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Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation

机译:哈勃常数和结构形成的浅暗光子和费米离子暗辐射

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摘要

Motivated by the tensions in the Hubble constant H-0 and the structure growth sigma(8) between Planckresults and other low redshift measurements, we discuss some cosmological effects of a dark sector model in which dark matter (DM) interacts with fermionic dark radiation (DR) through a light gauge boson (dark photon). Such kind of models are very generic in particle physics with a dark sector with dark gauge symmetries. The effective number of neutrinos is increased by delta N-eff similar to 0.5 due to light dark photon and fermionic DR, thereby resolving the conflicts in H-0. The elastic scattering between DM and DR induces suppression for DM's density perturbation, but without acoustic oscillations. For weakly-interacting DM around 100GeV, the new gauge coupling should be similar to 10(-4) to have sizable effect on matter power spectrum in order to relax the tension in s8. (C) 2016 The Author(s). Published by Elsevier B.V.
机译:根据哈勃常数H-0的张力以及普朗克结果与其他低红移测量之间的结构增长sigma(8)的张力,我们讨论了暗区模型的一些宇宙学效应,在暗区模型中,暗物质(DM)与铁电暗辐射相互作用( DR)通过一个轻型玻色子(深色光子)。这种类型的模型在粒子物理学中非常普遍,具有带有暗规对称性的暗区。由于光暗光子和铁离子DR,中微子的有效数目增加了δN-eff,接近0.5,从而解决了H-0的冲突。 DM和DR之间的弹性散射可抑制DM的密度扰动,但不会产生声波振荡。对于100GeV附近的弱相互作用DM,新规范的耦合应与10(-4)相似,以对物质功率谱产生相当大的影响,从而缓和s8中的张力。 (C)2016作者。由Elsevier B.V.发布

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