Department of Physics and Astronomy, University of Hawaii, Manoa, Hawaii 96822, USA.
Department of Physics, Center for Cosmology and AstroParticle Physics, Ohio State University, Columbus, Ohio 43210, USA.
Phys Rev Lett. 2018 Oct 19;121(16):161102. doi: 10.1103/PhysRevLett.121.161102.
We report on an upward traveling, radio-detected cosmic-ray-like impulsive event with characteristics closely matching an extensive air shower. This event, observed in the third flight of the Antarctic Impulsive Transient Antenna (ANITA), a NASA-sponsored long-duration balloon payload, is consistent with a similar event reported in a previous flight. These events could be produced by the atmospheric decay of an upward-propagating τ lepton produced by a ν_{τ} interaction, although their relatively steep arrival angles create tension with the standard model neutrino cross section. Each of the two events have a posteriori background estimates of ≲10^{-2} events. If these are generated by τ-lepton decay, then either the charged-current ν_{τ} cross section is suppressed at EeV energies, or the events arise at moments when the peak flux of a transient neutrino source was much larger than the typical expected cosmogenic background neutrinos.
我们报告了一个向上传播的、无线电探测到的类宇宙射线的脉冲事件,其特征与广延空气簇射非常匹配。这个事件是在 NASA 资助的长时气球有效载荷南极脉冲瞬变天线(ANITA)的第三次飞行中观测到的,与之前一次飞行中报告的类似事件一致。这些事件可能是由一个向上传播的 τ 中微子通过 ντ 相互作用产生的,其在大气中的衰减导致了与标准模型中微子横截面的紧张关系,尽管它们相对陡峭的到达角。这两个事件中的每一个都有 ≲10^{-2}的事后背景估计。如果这些事件是由 τ 中微子衰变产生的,那么要么是在 EeV 能区,带电电流 ντ 横截面被抑制,要么是在瞬态中微子源的峰值通量远远大于典型的预期宇宙成因背景中微子时,事件才会产生。