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Non-Abelian Dark Forces and the Relic Densities of Dark Glueballs

机译:非阿贝尔黑暗力量和深色胶球的遗物密度

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摘要

Our understanding of the Universe is known to be incomplete and new gaugeforces beyond those of the Standard Model might be crucial to describing itsobserved properties. A minimal and well-motivated possibility is a pureYang-Mills non-Abelian dark gauge force with no direct connection to theStandard Model. We determine here the relic abundances of the glueball boundstates that arise in such theories and investigate their cosmological effects.Glueballs are first formed in a confining phase transition, and their relicdensities are set by a network of annihilation and transfer reactions. Thelightest glueball has no lighter states to annihilate into, and its yield isset mainly by 3 to 2 number-changing processes which persistently releaseenergy into the glueball gas during freeze-out. The abundances of the heavierglueballs are dominated by 2 to 2 transfer reactions, and tend to be muchsmaller than the lightest state. We also investigate potential connectorsbetween the dark force and the Standard Model that allow some or all of thedark glueballs to decay. If the connection is weak, the lightest glueball canbe very long-lived or stable and is a viable dark matter candidate. Forstronger connections, the lightest glueball will decay quickly but otherheavier glueball states can remain stable and contribute to the dark matterdensity.
机译:我们对宇宙的理解是不完整的,并且超出标准模型的新的表压可能对于描述其观察到的特性至关重要。动机极少且动机充分的是纯Yang-Mills非阿贝尔暗规力,与标准模型没有直接关系。我们在这里确定在此类理论中出现的胶球结合态的遗迹丰度,并研究其宇宙学效应。胶球首先在密闭相变中形成,其残余物由an灭和转移反应网络设定。最轻的胶球没有更轻的状态可以消灭,其产量主要由3到2个数字转换过程确定,这些过程会在冻结过程中不断向胶球气体释放能量。重胶球的丰度主要受2到2个转移反应的控制,并且比最轻的状态要小得多。我们还研究了暗力和标准模型之间的潜在连接器,这些连接器允许部分或全部黑暗胶球衰减。如果连接较弱,则最轻的胶球可能寿命很长或很稳定,并且是可行的暗物质候选对象。对于更强的连接,最轻的胶球会迅速衰减,但其他较重的胶球状态则可以保持稳定并有助于暗密度。

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