论文标题
tau中微子的EAS光学Cherenkov特征，用于空间和轨道检测器
EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors
论文作者
论文摘要
对瞬态天体物理源的多理智观察有可能表征最高能量加速器和宇宙中最极端的环境。中微子的检测，尤其是由中微子振荡从其来源到地球产生的tau中微子，使用光学Cherenkov检测器在10 PEV上方的中微子能量可用于向上移动的广泛的空气淋浴（EAS）。这些EA是由地球相互作用的tau中微子产生的，导致tau lept子随后在大气中腐烂。我们将中微子的检测敏感性比较了通用短期和长期短暂的短暂性中微子源和敏感性与超级压力气球（EUSO-SPBB2）气球 - 生气 - 启用气球的跨性别宇宙太空观测的弥漫性中微子通量的敏感性，并提出了对极端多人跨型体形的传教士（POEEMSIS）的探测。
Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe. Detection of neutrinos, in particular tau neutrinos generated by neutrino oscillations in transit from their sources to Earth, is possible for neutrino energies above 10 PeV using optical Cherenkov detectors imaging upward-moving extensive air showers (EAS). These EAS are produced from Earth interacting tau neutrinos leading to tau leptons that subsequently decay in the atmosphere. We compare neutrino detection sensitivities for generic short- and long-burst transient neutrino sources and sensitivities to the diffuse neutrino flux for the second generation Extreme Universe Space Observatory on a Super Pressure Balloon (EUSO-SPB2) balloon-borne mission and the proposed space-based Probe of Extreme Multi-Messenger Astrophysics (POEMMA) mission.
