Kim Younggeun, Jeong Junu, Youn SungWoo, Bae Sungjae, Lee Kiwoong, van Loo Arjan F, Nakamura Yasunobu, Oh Seonjeong, Seong Taehyeon, Uchaikin Sergey, Kim Jihn E, Semertzidis Yannis K
Center for Axion and Precision Physics Research, <a href="https://ror.org/00y0zf565">IBS</a>, Daejeon 34051, Republic of Korea.
Department of Physics, <a href="https://ror.org/05apxxy63">KAIST</a>, Daejeon 34141, Republic of Korea.
Phys Rev Lett. 2024 Aug 2;133(5):051802. doi: 10.1103/PhysRevLett.133.051802.
The axion has emerged as the most attractive solution to two fundamental questions in modern physics related to the charge-parity invariance in strong interactions and the invisible matter component of our Universe. Over the past decade, there have been many theoretical efforts to constrain the axion mass based on various cosmological assumptions. Interestingly, different approaches from independent groups produce good overlap between 20 and 30 μeV. We performed an experimental search to probe the presence of dark matter axions within this particular mass region. The experiment utilized a multicell cavity haloscope embedded in a 12 T magnetic field to seek for microwave signals induced by the axion-photon coupling. The results ruled out the KSVZ axions as dark matter over a mass range between 21.86 and 22.00 μeV at a 90% confidence level. This represents a sensitive experimental search guided by specific theoretical predictions.
轴子已成为现代物理学中两个基本问题最具吸引力的解决方案,这两个问题分别与强相互作用中的电荷宇称不变性以及宇宙中不可见物质成分有关。在过去十年中,基于各种宇宙学假设,人们进行了许多理论研究来限制轴子质量。有趣的是,不同独立团队采用的不同方法在20至30 μeV之间产生了很好的重叠。我们进行了一项实验搜索,以探测在这个特定质量区域内暗物质轴子的存在。该实验利用嵌入12 T磁场中的多单元腔式轴子探测器来寻找由轴子 - 光子耦合诱导的微波信号。结果在90%置信水平下排除了KSVZ轴子在21.86至22.00 μeV质量范围内作为暗物质的可能性。这代表了一次由特定理论预测指导的灵敏实验搜索。