arXivDaily arXiv每日学术速递 周一至周五更新
arXiv周末暂无论文更新,休息一下吧,周末愉快~~
arXiv 2512.25035hep-ph
收藏

大规模中微子-暗物质相互作用:从有效场论到紫外完成

Large Neutrino-Dark Matter Interactions: From Effective Field Theory to Ultraviolet Completions

Oklahoma State University(俄克拉荷马州立大学);Washington University(华盛顿大学);Colorado State University(科罗拉多州立大学)

K. S. Babu, P. S. Bhupal Dev, Anil Thapa

AI总结:

本文提出了一种有效场论框架,用于研究中微子-暗物质相互作用,并构建了多种紫外完成模型,以实现较大的中微子-暗物质耦合,同时满足理论和实验约束。

摘要:

我们开发了一个通用的有效场论(EFT)框架,用于中微子-暗物质(DM)相互作用,并将其应用于系统地寻找所有可能的规范不变紫外(UV)完成,以给定的EFT算符维度。我们的目标是找到简单且完整的紫外完成模型,能够实现可能的中微子-DM相互作用,同时符合所有现有的理论和实验约束。我们首先构建了中微子-DM散射在低能有效理论中的主导非导数算符基,以及其在标准模型EFT(DM-SMEFT)中的规范不变嵌入。然后我们构建了所有可重整化的树级紫外完成模型,利用拓扑学分类,生成相关的DM-SMEFT算符,直到维度8。使用这一框架,我们为不同类型的DM提供了最小的紫外完成模型,这些模型可以产生有效的中微子-DM耦合,比费米耦合大几个数量级,同时满足所有约束,特别是来自中微子质量以及带电轻子部分的约束。这包括在scotogenic中微子质量模型中的伪狄拉克费尔米子DM实现,以及受II型和反见素基中微子质量模型启发的Majorana DM模型。对DM热 relic � � 密度和直接探测前景,以及各种宇宙学和实验室对模型参数空间的约束,也进行了分析。

英文摘要:

We develop a general effective field theory (EFT) framework for neutrino-dark matter (DM) interactions, and apply it to systematically find all possible gauge-invariant ultraviolet (UV) completions at a given EFT operator dimension. Our goal here is to find simple UV-complete models that can realize potentially large neutrino-DM interactions, while being consistent with all existing theoretical and experimental constraints. We first construct the leading non-derivative operator basis for neutrino-DM scattering in a low-energy effective theory with neutrinos and DM (DM-LEFT), together with its gauge-invariant embedding in the Standard Model EFT (DM-SMEFT). We then construct all renormalizable tree-level UV completions that generate the relevant DM-SMEFT operators up to dimension-8 using a topology-based classification. Using this framework, we present minimal UV-complete models for different DM types that can yield effective neutrino-DM couplings up to several orders of magnitude larger than the Fermi coupling, while satisfying all constraints, most notably from neutrino mass and from the charged-lepton sector. This includes a pseudo-Dirac fermion DM realization in the scotogenic neutrino mass model and models of Majorana DM inspired by type-II and inverse seesaw-based neutrino mass models. Phenomenological implications for DM thermal relic abundance and direct detection prospects, as well as various cosmological and laboratory constraints on the model parameter space, are also analyzed.

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。

↑