论文标题
部分可观测时空混沌系统的无模型预测
Sensitivity to Dark Sector Scales from Gravitational Wave Signatures
论文作者
论文摘要
我们认为由一阶相变产生的引力波信号，具有通用rentalized的幂律形式的通用热效率有效潜在的理论。我们发现重力波信号的频率和振幅可以直接与热有效电位的参数相关。这导致了总体结论。如果深色希格斯的质量小于深色希格斯真空期望值的1％，则在即将到来的所有即将到来和计划的重力波观测站中，重力波信号将无法观察到。
We consider gravitational wave signals produced by a first-order phase transition in a theory with a generic renormalizable thermal effective potential of power law form. We find the frequency and amplitude of the gravitational wave signal can be related in a straightforward manner to the parameters of the thermal effective potential. This leads to a general conclusion; if the mass of the dark Higgs is less than 1% of the dark Higgs vacuum expectation value, then the gravitational wave signal will be unobservable at all upcoming and planned gravitational wave observatories.
