Observation of an Unusual Upward-Going Cosmic-Ray-like Event in the Third Flight of ANITA

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...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physical review letters 2018-10, Vol.121 (16), p.161102-161102, Article 161102
Hauptverfasser: Gorham, P W, Rotter, B, Allison, P, Banerjee, O, Batten, L, Beatty, J J, Bechtol, K, Belov, K, Besson, D Z, Binns, W R, Bugaev, V, Cao, P, Chen, C C, Chen, C H, Chen, P, Clem, J M, Connolly, A, Cremonesi, L, Dailey, B, Deaconu, C, Dowkontt, P F, Fox, B D, Gordon, J W H, Hast, C, Hill, B, Hughes, K, Huang, J J, Hupe, R, Israel, M H, Javaid, A, Lam, J, Liewer, K M, Lin, S Y, Liu, T C, Ludwig, A, Macchiarulo, L, Matsuno, S, Miki, C, Mulrey, K, Nam, J, Naudet, C J, Nichol, R J, Novikov, A, Oberla, E, Olmedo, M, Prechelt, R, Prohira, S, Rauch, B F, Roberts, J M, Romero-Wolf, A, Russell, J W, Saltzberg, D, Seckel, D, Schoorlemmer, H, Shiao, J, Stafford, S, Stockham, J, Stockham, M, Strutt, B, Varner, G S, Vieregg, A G, Wang, S H, Wissel, S A
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung: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.
ISSN:0031-9007
1079-7114
DOI:10.1103/PhysRevLett.121.161102