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arXiv 2304.08040hep-thhep-ph
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Kaluza-Klein理论中的自然性与紫外敏感性

Naturalness and UV sensitivity in Kaluza-Klein theories

Carlo Branchina, Vincenzo Branchina, Filippo Contino

AI总结:

本文分析具有紧致额外维和Scherk-Schwarz超对称破缺的Kaluza-Klein理论,指出Higgs质量及单圈有效势存在与时空非平凡拓扑相关的强紫外敏感性,需重新审视该机制。

摘要:

二十多年前出现了一种范式,认为对紫外不敏感的Higgs质量$m_H$以及(更一般地)对紫外不敏感的Higgs有效势$V_{1l}(\phi)$可从具有紧致额外维和Scherk-Schwarz超对称破缺的高维理论中得到。自那时起,这些思想被应用于各种具有唯象意义的模型,包括近期在暗能量问题上的应用。通过对该范式所依据的框架进行透彻分析,我们表明,$m_H$和$V_{1l}(\phi)$存在一个此前被忽视的强紫外敏感性来源,它与这些模型时空的非平凡拓扑密切相关。Scherk-Schwarz机制的通常图像及其物理后果需要被认真重新审视。

英文摘要:

More than twenty years ago a paradigm emerged according to which a UV-insensitive Higgs mass $m_H$ and (more generally) a UV-insensitive Higgs effective potential $V_{1l}(ϕ)$ are obtained from higher-dimensional theories with compact extra dimensions and Scherk-Schwarz supersymmetry breaking. Since then, these ideas have been applied to different models of phenomenological interest, including recent applications to the dark energy problem. A thorough analysis of the framework on which such a paradigm is based allows us to show that a source of strong UV sensitivity for $m_H$ and $V_{1l}(ϕ)$, intimately connected to the non-trivial topology of these models' spacetime, was missed. The usual picture of the Scherk-Schwarz mechanism and its physical consequences need to be seriously reconsidered.

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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