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来自近邻活动星系 NGC 1068 的中微子发射证据。

Evidence for neutrino emission from the nearby active galaxy NGC 1068.

出版信息

Science. 2022 Nov 4;378(6619):538-543. doi: 10.1126/science.abg3395. Epub 2022 Nov 3.

Abstract

A supermassive black hole, obscured by cosmic dust, powers the nearby active galaxy NGC 1068. Neutrinos, which rarely interact with matter, could provide information on the galaxy's active core. We searched for neutrino emission from astrophysical objects using data recorded with the IceCube neutrino detector between 2011 and 2020. The positions of 110 known gamma-ray sources were individually searched for neutrino detections above atmospheric and cosmic backgrounds. We found that NGC 1068 has an excess of [Formula: see text] neutrinos at tera-electron volt energies, with a global significance of 4.2σ, which we interpret as associated with the active galaxy. The flux of high-energy neutrinos that we measured from NGC 1068 is more than an order of magnitude higher than the upper limit on emissions of tera-electron volt gamma rays from this source.

摘要

一个被宇宙尘埃遮挡的超大质量黑洞为附近的活动星系 NGC 1068 提供能量。中微子很少与物质相互作用,因此它们可以提供有关星系活动核心的信息。我们使用 IceCube 中微子探测器在 2011 年至 2020 年间记录的数据,搜索来自天体物理物体的中微子发射。逐个搜索 110 个已知伽马射线源的位置,以探测大气和宇宙背景之上的中微子探测。我们发现 NGC 1068 在太电子伏特能量下有 [Formula: see text] 个中微子过量,整体显著性为 4.2σ,我们将其解释为与活动星系有关。我们从 NGC 1068 测量到的高能中微子通量比该源太电子伏特伽马射线发射的上限高出一个数量级以上。

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