论文标题
解决重力波 - 对撞机逆问题
Addressing the Gravitational Wave - Collider Inverse Problem
论文作者
论文摘要
我们提供了一个路线图,用于分析假设的未来对撞机观测和检测强大的一阶electroweak相变产生的重力波信号之间的相互作用,以超越标准模型(BSM)理论。该路线图的基石是尺寸降低的三维有效场理论以及扰动理论和非扰动晶格模拟的结果的组合。我们第一次将这些最新方法应用于BSM理论的综合参数空间扫描。具体而言,我们使用真实的标量三重态研究了扩展,该延伸部分承认了可能的两步电动对称对称性的热史。 We find that (1) a first order transition during the second step could generate a signal accessible to LISA generation detectors and (2) the gravitational wave signal displays a strong sensitivity to the portal coupling between the new scalar and the Higgs boson, and (3) the ability for future experiments to detect the produced gravitational waves depends decisively on the wall velocity of the bubbles produced during the phase transition.我们说明了新标量特性的直接和间接测量的组合,结合了引力波检测的存在或不存在,可以测试模型并确定模型参数的值。
We provide a roadmap for analyzing the interplay between hypothetical future collider observations and the detection of a gravitational wave signal produced by a strong first order electroweak phase transition in beyond the Standard Model (BSM) theories. A cornerstone of this roadmap is a combination of a dimensionally reduced, three-dimensional effective field theory and results of both perturbation theory and non-perturbative lattice simulations. For the first time we apply these state-of-the-art methods to a comprehensive parameter space scan of a BSM theory. Concretely, we study an extension with the real scalar triplet, which admits a possible two-step electroweak symmetry-breaking thermal history. We find that (1) a first order transition during the second step could generate a signal accessible to LISA generation detectors and (2) the gravitational wave signal displays a strong sensitivity to the portal coupling between the new scalar and the Higgs boson, and (3) the ability for future experiments to detect the produced gravitational waves depends decisively on the wall velocity of the bubbles produced during the phase transition. We illustrate how a combination of direct and indirect measurements of the new scalar properties, in combination with the presence or absence of a gravitational wave detection, could test the model and identify the values of the model parameters.