Higgs physics and cosmology: gravitational waves from the electroweak phase transition

D. Weir
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Abstract

In the Standard Model, the electroweak phase transition is a crossover. In many extensions, including those with additional charged Higgs bosons, the phase transition can be of first order – even strongly so. In such a phase transition, the resulting collisions of bubbles of the new Higgs phase, and the associated interactions of sound waves in the plasma, are substantial sources of gravitational waves. For a phase transition at or around the electroweak scale, these gravitational waves may be detectable by future or planned missions, such as LISA. This can indirectly provide a complementary probe of particle physics beyond the Standard Model. I will review the physics that makes this possible.
希格斯物理学与宇宙学:来自电弱相变的引力波
在标准模型中,电弱相变是一个交叉。在许多扩展中,包括那些带有额外带电希格斯玻色子的扩展,相变可以是一阶的——甚至是强烈的。在这样一个相变中,新希格斯相气泡的碰撞,以及等离子体中声波的相关相互作用,是引力波的重要来源。对于电弱尺度或电弱尺度附近的相变,这些引力波可能会被未来或计划中的任务探测到,比如LISA。这可以间接地为标准模型之外的粒子物理提供补充探测。我将回顾一下使其成为可能的物理原理。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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