论文标题
识别高能中微子的银河系来源
Identifying Galactic Sources of High-Energy Neutrinos
论文作者
论文摘要
高能中微子呈现宇宙射线加速器的最终签名。在宇宙射线光谱中，导致宇宙射线加速到膝盖的银河系来源将为高能宇宙中微子通量提供保证的，尽管是亚域的贡献。在这篇综述中，我们讨论了从银河系中非常高的能量伽马射线排放来源鉴定高能中微子的前景。我们介绍了从这些来源寻找类似点状和扩展发射的状态，并描述了这些研究的结果如何表明中微子望远镜正在关闭识别高能中微子的银河系来源。
High-energy neutrinos present the ultimate signature for a cosmic ray accelerator. Galactic sources responsible for acceleration of cosmic ray up to the knee in cosmic ray spectrum will provide a guaranteed, albeit subdominant, contribution to the high-energy cosmic neutrino flux. In this review, we discuss the the prospects for identification of high-energy neutrinos from sources of the very high energy gamma ray emission in the Milky Way. We present the status of the search for point-like and extended emission from these sources, and describe how the results of these studies indicate that neutrino telescopes are closing in on identifying Galactic sources of high-energy neutrinos.
