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1980年至2000年间高能中微子和宇宙射线探测器的发展

The Development of Detectors of High Energy Neutrinos and Cosmic Rays between 1980 and 2000

A A Watson

arXiv 2607.25535首次发表:更新:

AI 中文总结

概括了1980年至2000年间高能中微子和宇宙射线探测器的发展情况,提及相关探测器建设困难及发展历程,指出20世纪80年代对天鹅座X-3的观测说法对冰立方和奥格天文台发展有重要作用。

AI 中文摘要

本文讨论了DUMAND、贝加尔湖和冰立方高能中微子探测器的建设,重点阐述了遇到的困难。还介绍了1990年代奥格天文台构想及合作发展过程中克服的难题。对于冰立方和奥格天文台,20世纪80年代关于观测天鹅座X-3的PeV伽马射线的说法在其发展中起到了重要作用。

英文摘要

The construction of the DUMAND, Lake Baikal and IceCube detectors of high-energy neutrinos are discussed, with some emphasis on the difficulties encountered. The decade from 1990 marked the period in which the Auger Observatory was conceived and the Collaboration evolved. Again, the difficulties that were overcome to create the Observatory are described. For both IceCube and the Auger Observatory, claims made in the 1980s for the observation of PeV gamma-rays from Cygnus X-3, played a not-insignificant role in their advance.

Comments12 pages, 5 figures, Based on talk at 4th Symposium on History of Particle Physics, CERN, November 2025

论文原文

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