| Literature DB >> 29358351 |
Abstract
We review the production of gravitational waves by an electroweak first-order phase transition. The resulting signal is a good candidate for detection at next-generation gravitational wave detectors, such as LISA. Detection of such a source of gravitational waves could yield information about physics beyond the Standard Model that is complementary to that accessible to current and near-future collider experiments. We summarize efforts to simulate and model the phase transition and the resulting production of gravitational waves.This article is part of the Theo Murphy meeting issue 'Higgs cosmology'.Keywords: electroweak symmetry breaking; gravitational waves; phase transitions
Year: 2018 PMID: 29358351 PMCID: PMC5784032 DOI: 10.1098/rsta.2017.0126
Source DB: PubMed Journal: Philos Trans A Math Phys Eng Sci ISSN: 1364-503X Impact factor: 4.226