SU（$N$）暗胶球凝聚体的扩展最小几何形变
The extended minimal geometric deformation of SU($N$) dark glueball condensates
摘要：
扩展的最小几何变形（EMGD）的程序，在全息膜范例，模型恒星的分布所产生的自相互作用的标量胶球暗物质凝聚。这种纯量胶球是超越标准模型的SU（$N$）Yang-Mills隐扇区。然后，在EMGD框架下，导出了SU（$N$）EMGD暗胶球星合并产生的引力波辐射的修正，并研究了它们各自的谱.驱动EMGD的散装外尔流体，然后提出在eLISA和LIGO的增强窗口实验检测。
英文摘要：
The extended minimal geometric deformation (EMGD) procedure, in the holographic membrane paradigm, is employed to model stellar distributions that arise upon self-interacting scalar glueball dark matter condensation. Such scalar glueballs are SU($N$) Yang-Mills hidden sectors beyond the Standard Model. Then, corrections to the gravitational wave radiation, emitted by SU($N$) EMGD dark glueball stars mergers, are derived, and their respective spectra are studied in the EMGD framework, due to a phenomenological brane tension with finite value. The bulk Weyl fluid that drives the EMGD is then proposed to be experimentally detected by enhanced windows at the eLISA and LIGO.
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