银河闪耀着高能中微子的光芒

IF 44.8 1区 物理与天体物理 Q1 PHYSICS, APPLIED
M. Bustamante
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引用次数: 0

摘要

银河系中能量最大的天体物理源——能够产生高能宇宙射线的宇宙加速器——一个多世纪以来一直没有被发现。到目前为止,天体物理学家寻找这些源主要是通过在银河系中搜寻它们预计会发射的伽马射线。2023年,冰立方中微子天文台发现了来自银河系的高能中微子,开启了银河系宇宙射线产生和相互作用的证据流。2023年,冰立方中微子天文台发现了来自银河系的高能中微子,这是了解高能宇宙射线起源的重要线索。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

The Milky Way shines in high-energy neutrinos

The Milky Way shines in high-energy neutrinos

The Milky Way shines in high-energy neutrinos
The most energetic astrophysical sources in the Milky Way, cosmic accelerators capable of producing high-energy cosmic rays, have resisted discovery for over a century. Up to now, astrophysicists sought these sources mainly by scouring the Galaxy for the gamma rays they are expected to emit. In 2023, the IceCube Neutrino Observatory discovered high-energy neutrinos from the Milky Way, inaugurating a tell-tale stream of evidence of cosmic-ray production and interaction in the Galaxy. In 2023, the IceCube Neutrino Observatory discovered high-energy neutrinos from the Milky Way, an important clue towards understanding the origin of high-energy cosmic rays.
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来源期刊
CiteScore
47.80
自引率
0.50%
发文量
122
期刊介绍: Nature Reviews Physics is an online-only reviews journal, part of the Nature Reviews portfolio of journals. It publishes high-quality technical reference, review, and commentary articles in all areas of fundamental and applied physics. The journal offers a range of content types, including Reviews, Perspectives, Roadmaps, Technical Reviews, Expert Recommendations, Comments, Editorials, Research Highlights, Features, and News & Views, which cover significant advances in the field and topical issues. Nature Reviews Physics is published monthly from January 2019 and does not have external, academic editors. Instead, all editorial decisions are made by a dedicated team of full-time professional editors.
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