标题： M101中的SN 2023ixf的低能和高能中微子 显示英文标题

标题： Low and High Energy Neutrinos from SN 2023ixf in M101

摘要： 位于M101中的超新星（SN）2023ixf是过去十年观测到的最近的一次超新星爆炸。因此，它是研究喷流在驱动超新星抛射物中的作用的一个合适的试验平台。为了这个目的，我们探讨了高能中微子可能在喷流与超新星爆炸产生的强烈辐射场相互作用期间产生，并最终被IceCube中微子望远镜观测到的可能性。这种中微子的未被探测到显著限制了产生喷流的恒星坍缩的比例和/或中微子产生的理论模型。最后，我们调查了使用超级和超长基线Kamiokande实验检测来自SN 2023ixf的低能中微子的可能性，在这两种情况下都获得了亚阈值估计。 显示英文摘要

摘要： Supernova (SN) 2023ixf in M101 is the closest SN explosion observed in the last decade. Therefore it is a suitable test bed to study the role of jets in powering the SN ejecta. With this aim, we explored the idea that high-energy neutrinos could be produced during the interaction between the jets and the intense radiation field produced in the SN explosion and eventually be observed by the IceCube neutrino telescope. The lack of detection of such neutrinos has significantly constrained both the fraction of stellar collapses that produce jets and/or the theoretical models for neutrino production. Finally, we investigated the possibility of detecting low-energy neutrinos from SN 2023ixf with the Super- and Hyper-Kamiokande experiments, obtaining in both cases sub-threshold estimates.