首页> 外文期刊>Bulletin of the American Physical Society >APS -Spring 2017 Joint Meeting of the Texas Section of AAPT, Texas Section of APS, and Zone 13 of the Society of Physics Students - Event - The influence of dark energy on the expansion rate of the universe and its effects on dark matter relic abundance
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APS -Spring 2017 Joint Meeting of the Texas Section of AAPT, Texas Section of APS, and Zone 13 of the Society of Physics Students - Event - The influence of dark energy on the expansion rate of the universe and its effects on dark matter relic abundance

机译:APS-AAPT德克萨斯州分校,APS德克萨斯州分校和物理学会第13区的2017年春季联合会议-事件-暗能量对宇宙膨胀率的影响及其对暗物质遗迹丰度的影响

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The expansion rate of the universe had a strong influence on the origin of the dark matter abundance during the early stagesof the universe’s evolution, mainly prior to big-bang nucleosynthesis. Any departure of the expansion rate of the universe from the standardcosmological model during that time can modify the dark matter abundance. In this talk, I will explore the role played by a scalar field onthe modification of the expansion rate of the universe arising from scalar-tensor theories of gravity coupled both conformally and disformallyto matter, and also, I will show how these variations to the expansion rate would modify the dark matter content of the Universe.
机译:在宇宙演化的早期阶段,主要是在大爆炸核合成之前,宇宙的膨胀率对暗物质丰度的起源有很大的影响。在此期间,宇宙膨胀率与标准宇宙学模型的任何偏离都可以改变暗物质的丰度。在本次演讲中,我将探讨标量场在因标量-张量引力理论共形和非形变耦合于物质而引起的宇宙膨胀率变化中的作用,并且,我还将展示这些变化对膨胀的影响速率会改变宇宙的暗物质含量。

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