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arXiv 2302.08520hep-phhep-th
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非超对称弦理论中的希格斯门户暗物质

Higgs-portal dark matter from non-supersymmetric strings

Esau Cervantes, Omar Perez-Figueroa, Ricardo Perez-Martinez, Saul Ramos-Sanchez

AI总结:

本研究在非超对称heterotic orbifold弦模型中实现希格斯门户暗物质,发现一个样本模型具有一圈稳定的希格斯真空,其中标量可解释暗物质丰度,并对暗物质候选者及重希格斯扇区质量施加了有趣约束。

摘要:

已构建了多类具有标准模型特征的非超对称弦模型,但对其唯象学知之甚少。有趣的是,它们的谱包含标量场,这些标量场与观测粒子的唯一耦合是通过多希格斯扇区实现的。另一方面,具有希格斯门户的自下而上模型仍为暗物质提供了可接受的框架。我们探索了在无超对称的有前景的heterotic orbifold模型中实现此类希格斯门户的可能性。我们发现,一个样本模型包含在一圈水平上稳定的希格斯真空,其中希格斯扇区与粒子物理观测相容,且一个标量可以解释测得的暗物质丰度。在这样的真空中,我们揭示了关于暗物质候选者质量及重希格斯扇区的有趣约束。这些引人注目的结果不仅限于弦模型,因为它们可以嵌入类似动机的自下而上方案中。

英文摘要:

Large classes of non-supersymmetric string models equipped with standard-model features have been constructed, but very little of their phenomenology is known. Interestingly, their spectra exhibit scalar fields whose only couplings to observed particles is through a multi-Higgs sector. On the other hand, bottom-up models with Higgs portals offer still an acceptable framework for dark matter. We explore realizations of such Higgs portals in promising heterotic orbifold models without supersymmetry. We find that a sample model includes Higgs vacua that are stable at one-loop, in which the Higgs sector is compatible with particle-physics observations and a scalar can account for the measured dark matter abundance. In such vacua, interesting constraints on the masses of the dark matter candidate and the heavy Higgs sector are uncovered. These compelling results are not limited to string models, as they can be embedded in similarly motivated bottom-up schemes.

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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