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arXiv 2209.03371hep-ph
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来自轻子味破缺衰变的轴子暗物质

Axion Dark Matter from Lepton flavor-violating Decays

Paolo Panci, Diego Redigolo, Thomas Schwetz, Robert Ziegler

AI总结:

本研究提出轻子味破缺耦合通过keV级类轴子粒子冻结产生暗物质的机制,该机制具备稳定性强、约束宽松等优势,可由未来X射线望远镜及高强度轻子味破缺实验检验。

摘要:

我们提出了几种简单的情形:在这些情形中,轻子味破缺耦合通过质量在数千电子伏特范围内的类轴子粒子的冻结产生,生成观测到的暗物质丰度。与味对角冻结相比,该机制增强了暗物质的稳定性,放宽了恒星冷却约束,并提升了加速器搜索实验的灵敏度。这些情形可由未来的X射线望远镜检验,且在部分情况下,几乎能被Mu3e和MEG II等高强度实验中针对轻子味破缺的新搜索完全探测。

英文摘要:

We propose simple scenarios where lepton flavor-violating couplings generate the observed dark matter abundance through freeze-in of an axion-like particle with mass in the few keV range. Compared to flavor-diagonal freeze-in, this mechanism enhances dark matter stability, softens stellar cooling constraints and improves the experimental sensitivity of accelerator-based searches. These scenarios can be tested by future X-ray telescopes, and in some cases will be almost entirely probed by new searches for lepton flavor violation at high-intensity experiments such as Mu3e and MEG II.

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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