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首页> 外文期刊>The Astrophysical Journal. Letters >SEARCH FOR NEUTRINOS IN SUPER-KAMIOKANDE ASSOCIATED WITH GRAVITATIONAL-WAVE EVENTS GW150914 AND GW151226
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SEARCH FOR NEUTRINOS IN SUPER-KAMIOKANDE ASSOCIATED WITH GRAVITATIONAL-WAVE EVENTS GW150914 AND GW151226

机译:与重力波事件GW150914和GW151226相关的超级神冈中的中子的搜寻

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摘要

We report the results from a search in Super-Kamiokande for neutrino signals coincident with the first detected gravitational-wave events, GW150914 and GW151226, as well as LVT151012, using a neutrino energy range from 3.5 MeV to 100. PeV. We searched for coincident neutrino events within a time window of. +/- 500 s around the gravitational-wave detection time. Four neutrino candidates are found for GW150914, and no candidates are found for GW151226. The remaining neutrino candidates are consistent with the expected background events. We calculated the 90% confidence level upper limits on the combined neutrino fluence for both gravitational-wave events, which depends on event energy and topologies. Considering the upward-going muon data set (1.6 GeV-100 PeV), the neutrino fluence limit for each gravitational-wave event is 14-37 (19-50) cm(-2) for muon neutrinos (muon antineutrinos), depending on the zenith angle of the event. In the other data sets, the combined fluence limits for both gravitational-wave events range from 2.4 x 10(4) to 7.0 x 10(9) cm(-2).
机译:我们报告了在Super-Kamiokande中搜索中微子信号的结果,该中微子信号与第一个检测到的重力波事件GW150914和GW151226以及LVT151012一致,所使用的中微子能量范围为3.5 MeV至100. PeV。我们在的时间窗口内搜索了同时发生的中微子事件。引力波检测时间大约+/- 500 s。找到了GW150914的四个中微子候选物,而未找到GW151226的中子候选物。剩余的中微子候选者与预期的背景事件一致。我们针对两种引力波事件计算了组合中微子注量的90%置信水平上限,这取决于事件能量和拓扑。考虑到向上的μon数据集(1.6 GeV-100 PeV),对于μ中子(μon反中微子),每个引力波事件的中微子注量极限为14-37(19-50)cm(-2),具体取决于事件的天顶角。在其他数据集中,两个重力波事件的总能量密度范围为2.4 x 10(4)到7.0 x 10(9)cm(-2)。

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