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高能中微子天文学——实验综述

Neutrino Astronomy at High Energies - An Experimental Review

Christian Spiering

arXiv 2609.26436首次发表:更新:

AI 中文总结

本文综述高能中微子天文学的发展历程,回顾了探测到TeV-PeV地外中微子弥散通量及识别单个源的突破,并展望未来方向。

AI 中文摘要

高能中微子天文学是一个新兴领域,但仍处于起步阶段。大约在十几年前,人们探测到了能量在太电子伏特(TeV)和拍电子伏特(PeV)范围内的地外中微子弥散通量,而识别出首批单个中微子源则是在更晚的时候。经过四十年的努力,实现了促成这一突破的巨型仪器,从而为宇宙打开了一扇新的窗口。本综述描述了通往当前成就的道路,回顾了该领域的实际现状,并展望了未来的发展。

英文摘要

Neutrino astronomy at high energies is an emerging field but still in a state of infancy. It is barely a dozen years ago that a diffuse flux of extraterrestrial neutrinos with energies in the TeV and PeV ranges was detected and even fewer that first individual sources could be identified. A new window to the universe has been opened after four decades of efforts to realize the gigantic instruments that made that breakthrough possible. This review describes the road towards the present, reviews the actual status of the field and sketches future developments.

Journal refUNIVERSE 2026, 12/9

DOI:10.3390/universe12090273

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