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arXiv 0709.2091hep-phastro-ph
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nMSSM中引力波的产生

Production of Gravitational Waves in the nMSSM

Stephan J. Huber, Thomas Konstandin

摘要:

在强烈的一阶相变过程中,气泡碰撞和湍流等离子体运动会产生引力波。我们分析了nMSSM中电弱相变的相关特征,确定了产生的引力波信号。此外,我们评论的引力波和重子生成的生产之间的相关性。我们的结论是,该模型中的引力波遗迹密度一般太小,在不久的将来被LISA实验检测。我们还考虑了具有六维希格斯势的“标准模型“的情况,这导致引力波信号略强。

英文摘要:

During a strongly first-order phase transition gravitational waves are produced by bubble collisions and turbulent plasma motion. We analyze the relevant characteristics of the electroweak phase transition in the nMSSM to determine the generated gravitational wave signal. Additionally, we comment on correlations between the production of gravitational waves and baryogenesis. We conclude that the gravitational wave relic density in this model is generically too small to be detected in the near future by the LISA experiment. We also consider the case of a "Standard Model" with dimension-six Higgs potential, which leads to a slightly stronger signal of gravitational waves.

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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