潮汐破坏事件和高能中微子

R. Stein
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引用次数: 3

摘要

潮汐破坏事件(TDEs)发生在恒星靠近超大质量黑洞时,长期以来一直被预测会发射宇宙射线和中微子。最近,作为兹威基瞬态设施(ZTF)中微子后续计划的一部分,TDE AT2109dsg在空间和时间上与高能中微子IC191001A重合,提供了第一个直接观测证据,支持这些物体是多信使源。在这些程序中,我将把我们的ZTF中微子后续计划的最新结果置于TDE和中微子天文学发展的更广泛背景下。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Tidal Disruption Events and High-energy Neutrinos
Tidal Disruption Events (TDEs) occur when stars pass close to supermassive black holes, and have long been predicted to emit cosmic rays and neutrinos. Recently the TDE AT2109dsg was identified in spatial and temporal coincidence with high-energy neutrino IC191001A as part of the Zwicky Transient Facility (ZTF) neutrino follow-up program, providing the first direct observational evidence supporting these objects as multi-messenger sources. In these proceedings, I will place the recent results of our ZTF neutrino follow-up program into the broader context of developments in TDE and neutrino astronomy.
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