论文标题
超新星物质的穆斯化
Muonization of supernova matter
论文作者
论文摘要
本文调查了穆恩对核心 - 循环超新星的影响，尤其关注早期的中微子排放。虽然在中子恒星的背景下，人们已经充分理解了兆人的存在，直到Bollig等人最近的研究。 [物理。莱特牧师。 119，242702（2017）]穆斯在核心折叠超新星中的作用被忽略了 - 电子和中微子是唯一考虑的卵子。在他们的研究中，Bollig等人。解散了若恩和tau中微子和抗肿瘤，其中包括各种Muonic弱反应，所有这些反应都紧随其后。只有这样，才有可能在恒星核心弹跳前不久量化MUON的外观以及如何修改后中微子发射后中微子的发射
The present article investigates the impact of muons on core-collapse supernovae, with particular focus on the early muon neutrino emission. While the presence of muons is well understood in the context of neutron stars, until the recent study by Bollig et al. [Phys. Rev. Lett. 119, 242702 (2017)] the role of muons in core-collapse supernovae had been neglected--electrons and neutrinos were the only leptons considered. In their study, Bollig et al. disentangled the muon and tau neutrinos and antineutrinos and included a variety of muonic weak reactions, all of which the present paper follows closely. Only then does it becomes possible to quantify the appearance of muons shortly before stellar core bounce and how the post-bounce prompt neutrino emission is modified
