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arXiv 2207.04519astro-ph.HEastro-ph.IMhep-ex
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西太平洋中的一座立方公里级中微子望远镜

A multi-cubic-kilometre neutrino telescope in the western Pacific Ocean

Z. P. Ye, F. Hu, W. Tian, Q. C. Chang, Y. L. Chang, Z. S. Cheng, J. Gao, T. Ge, G. H. Gong, J. Guo, X. X. Guo, X. G. He, J. T. Huang, K. Jiang, P. K. Jiang, Y. … 展开作者

Z. P. Ye, F. Hu, W. Tian, Q. C. Chang, Y. L. Chang, Z. S. Cheng, J. Gao, T. Ge, G. H. Gong, J. Guo, X. X. Guo, X. G. He, J. T. Huang, K. Jiang, P. K. Jiang, Y. P. Jing, H. L. Li, J. L. Li, L. Li, W. L. Li, Z. Li, N. Y. Liao, Q. Lin, F. Liu, J. L. Liu, X. H. Liu, P. Miao, C. Mo, I. Morton-Blake, T. Peng, Z. Y. Sun, J. N. Tang, Z. B. Tang, C. H. Tao, X. L. Tian, M. X. Wang, Y. Wang, Y. Wang, H. D. Wei, Z. Y. Wei, W. H. Wu, S. S. Xian, D. Xiang, D. L. Xu, Q. Xue, J. H. Yang, J. M. Yang, W. B. Yu, C. Zeng, F. Y. D. Zhang, T. Zhang, X. T. Zhang, Y. Y. Zhang, W. Zhi, Y. S. Zhong, M. Zhou, X. H. Zhu, G. J. Zhuang

AI总结:

研究基于南海考察数据设计立方公里级深海中微子望远镜 TRIDENT,预计运行一年即可对 NGC 1068 达到 5σ 探测,显著提升中微子源定位与宇宙线起源研究能力。

摘要:

为了精确定位 IceCube 探测到的弥散天体物理中微子流的来源,并解开存在一个世纪之久的宇宙线起源之谜,需要灵敏度显著提升的下一代中微子望远镜。赤道附近的探测器将提供观测中微子天空的独特视角,与 IceCube 及北半球的其他中微子望远镜形成互补。在此,我们展示了前往西太平洋南海东北部海域一次考察的结果。在深度约 3.5 公里的一处深海平原上发现了条件适宜的中微子望远镜台址。在 3 公里以下深度,测得海流速度、水对切伦科夫光的吸收长度和散射长度分别为 v_c<10 cm/s、λ_abs≈27 m 和 λ_sca≈63 m。基于这些测量结果,我们提出了下一代中微子望远镜 TRopIcal DEep-sea Neutrino Telescope(TRIDENT,热带深海中微子望远镜)的设计和预期性能。凭借先进的光子探测技术和巨大的尺度,TRIDENT 预计在运行 1 年内即可观测到 IceCube 的稳定源候选体 NGC 1068,显著性达到 5σ。这一灵敏度水平将开辟一个新的舞台,用于诊断宇宙线起源并在天文基线尺度上检验基础物理。

英文摘要:

Next-generation neutrino telescopes with significantly improved sensitivity are required to pinpoint the sources of the diffuse astrophysical neutrino flux detected by IceCube and uncover the century-old puzzle of cosmic ray origins. A detector near the equator will provide a unique viewpoint of the neutrino sky, complementing IceCube and other neutrino telescopes in the Northern Hemisphere. Here we present results from an expedition to the north-eastern region of the South China Sea, in the western Pacific Ocean. A favorable neutrino telescope site was found on an abyssal plain at a depth of $\sim$ 3.5km. At depths below 3km, the sea current speed, water absorption and scattering lengths for Cherenkov light, were measured to be $v_{\mathrm{c}}<$10cm/s, $λ_{\mathrm{abs} }\simeq$ 27m and $λ_{\mathrm{sca} }\simeq$ 63m, respectively. Accounting for these measurements, we present the design and expected performance of a next-generation neutrino telescope, TRopIcal DEep-sea Neutrino Telescope (TRIDENT). With its advanced photon-detection technology and large dimensions, TRIDENT expects to observe the IceCube steady source candidate NGC 1068 with 5$σ$ significance within 1 year of operation. This level of sensitivity will open a new arena for diagnosing the origin of cosmic rays and probing fundamental physics over astronomical baselines.

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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