标题： 测试真实WIMPs的CTAO 显示英文标题

标题： Testing Real WIMPs with CTAO

摘要： 我们预测了即将建成的切连科夫望远镜阵列观测站（CTAO）在最小暗物质范式下对全部真实表示的探测能力。我们采用有效场论技术计算当费米子暗物质是任意奇数和真实表示的中性成分时的湮灭截面和光子谱，包括索末菲增强、相关电弱效应的次领头对数重求和以及束缚态的贡献。我们还计算了标量暗物质的相应信号，但不包括束缚态的贡献。结果展示了从$\sim$3 TeV 三重态（或温子），一个$\mathbf{3}$的 SU(2)，到$\sim$300 TeV 十三重态，一个$\mathbf{13}$的 SU(2) 的所有真实表示，该表示处于单位性界限的临界点。利用这些结果，我们预测如果进行 500 小时的银河系中心观测，并假设背景系统误差控制在${\cal O}(1\%)$的水平，那么如果没有信号出现，CTAO 可以排除所有直到$\mathbf{11}$的 SU(2) 表示，即使是在暗物质密度最保守的模型中，无论是在费米子暗物质还是标量暗物质的情况下。假设默认的 CTAO 配置，十三重态将勉强逃过排除，尽管我们概述了 CTAO 可以采取的步骤来测试这种情形。总之，CTAO 似乎准备就绪，可以对真实 WIMPs 是否构成我们宇宙的暗物质做出明确的判断。 显示英文摘要

摘要： We forecast the reach of the upcoming Cherenkov Telescope Array Observatory (CTAO) to the full set of real representations within the paradigm of minimal dark matter. We employ effective field theory techniques to compute the annihilation cross section and photon spectrum that results when fermionic dark matter is the neutral component of an arbitrary odd and real representation of SU(2), including the Sommerfeld enhancement, next-to-leading log resummation of the relevant electroweak effects, and the contribution from bound states. We also compute the corresponding signals for scalar dark matter, with the exception of the bound state contribution. Results are presented for all real representations from the $\sim$3 TeV triplet (or wino), a $\mathbf{3}$ of SU(2), to the $\sim$300 TeV tredecuplet, a $\mathbf{13}$ of SU(2) that is at the threshold of the unitarity bound. Using these results, we forecast that with 500 hrs of Galactic Center observations and assuming background systematics are controlled at the level of ${\cal O}(1\%)$, then should no signal emerge, CTAO could exclude all representations up to the $\mathbf{11}$ of SU(2) in even the most conservative models for the dark-matter density in the inner galaxy, in both the fermionic and scalar dark matter cases. Assuming the default CTAO configuration, the tredecuplet will marginally escape exclusion, although we outline steps that CTAO could take to test even this scenario. In summary, CTAO appears poised to make a definitive statement on whether real WIMPs constitute the dark matter of our universe.