2018/03/14 by P. W. Gorham, P. W. Gorham, B. Rotter +104 · 1 voice · 138 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #COSMIC cancer database #Cosmic ray #Dark Matter and Cosmic Phenomena #Event (particle physics) #Nuclear physics #Physics #Solar and Space Plasma Dynamics #astro-ph.HE
paper · pdf · doi:10.1103/physrevlett.121.161102
published in Physical Review Letters 121(16), 161102 (American Physical Society) · 5 pages, 4 figures. Supplemental material available from corresponding author by request
arxiv created 2018/03/14 · arxiv published 2018/03/14 · openalex publication_date 2018/10/18 · arxiv updated 2018/10/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
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 ντ 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 ντ 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.