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arXiv 2012.11614hep-phastro-ph.HEgr-qchep-lathep-th
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测试暗SU(N)杨-米尔斯理论的禁闭景观:从格点到引力波

Testing the dark SU(N) Yang-Mills theory Confined Landscape: From the Lattice to Gravitational Waves

Wei-Chih Huang, Manuel Reichert, Francesco Sannino, Zhi-Wei Wang

AI总结:

该研究结合格点QCD和有效场论,预测暗SU(N)杨-米尔斯禁闭相变的引力波特征,为未来探测器约束暗区提供方法。

摘要:

我们为未来的引力波探测实验(如大爆炸观测者和DECIGO)铺平道路,以约束由SU(N)杨-米尔斯禁闭理论构成的暗区。我们超越了现有技术水平,通过结合第一性原理格点结果和有效场论方法,推断关于驱动早期宇宙引力波产生的非微扰暗退禁闭相变的关键信息,如相变的阶数、持续时间和能量预算,这些对于确定所产生的引力波信号的强度至关重要。

英文摘要:

We pave the way for future gravitational-wave detection experiments, such as the Big Bang Observer and DECIGO, to constrain dark sectors made of SU(N) Yang-Mills confined theories. We go beyond the state-of-the-art by combining first principle lattice results and effective field theory approaches to infer essential information about the non-perturbative dark deconfinement phase transition driving the generation of gravitational-waves in the early universe, such as the order, duration and energy budget of the phase transition which are essential in establishing the strength of the resulting gravitational-wave signal.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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