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arXiv 2502.04445hep-phastro-ph.COgr-qc
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希格斯诱导的引力波:非最小耦合、动力学与顶夸克质量的相互作用

Higgs-Induced Gravitational Waves: the Interplay of Non-Minimal Couplings, Kination and Top Quark Mass

Giorgio Laverda, Javier Rubio

AI总结:

本文提出一种最小模型,其中希格斯场在暴胀后再加热宇宙并产生可探测的引力波背景,通过曲率诱导的不稳定性关联暴胀标度、非最小耦合和顶夸克质量,为再加热和标准模型等离子体起源提供新解释。

摘要:

我们探索了一个最小情景,其中唯一的标准模型希格斯场负责在暴胀后对宇宙进行再加热,产生显著的引力波背景,并维持电弱真空的完全经典稳定性。由于希格斯自耦合在高能标下趋向负值,在刚性背景膨胀时期与曲率的非最小相互作用驱使希格斯涨落接近不稳定标度。这种曲率诱导的 tachyonic 不稳定性导致希格斯粒子的大量产生,并伴随随机引力波背景。该信号的特征可直接与暴胀标度、非最小耦合参数和顶夸克汤川耦合相关联。我们区分了三种可能的情景:低顶夸克质量下的绝对稳定性、势真空不稳定性,以及不稳定标度之上存在新物理的绝对稳定性。我们的发现表明,探测到具有暴胀尾部的峰值引力波背景,有可能揭示极高能标下希格斯有效势的特征,同时为再加热阶段和早期宇宙中标准模型等离子体的出现提供最小解释。与文献中的其他研究不同,我们情景中引力波的产生不依赖于标准模型真空的量子不稳定性。

英文摘要:

We explore a minimal scenario where the sole Standard-Model Higgs is responsible for reheating the Universe after inflation, produces a significant background of gravitational waves and maintains the full classical stability of the electroweak vacuum. As the Higgs self-coupling runs toward negative values at high energy scales, a non-minimal interaction with curvature during a stiff background expansion era drives the Higgs fluctuations closer to the instability scale. This curvature-induced tachyonic instability leads to an intense production of Higgs particles, accompanied by a stochastic gravitational-wave background. The characteristic features of such signal can be directly correlated to the inflationary scale, the non-minimal coupling parameter and the top quark Yukawa coupling. We distinguish between three possible scenarios: absolute stability with low top quark masses, potential vacuum instability, and absolute stability with new physics above the instability scale. Our findings suggest that the detection of a peaked background of gravitational waves together with its inflationary tail has the potential to unveil the features of the Higgs effective potential at very high energy scales while providing a minimal explanation for the reheating phase and the emergence of the Standard-Model plasma in the early Universe. Unlike other studies in the literature, the generation of gravitational waves in our scenario does not depend on the quantum instability of the Standard Model vacuum.

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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