Abstract
Delayed extensive air showers with N e > 5 × 106 are detected. The detection of such events indicates the existence of new processes for energies above 1016 eV.
Similar content being viewed by others
References
J. Linsley and L. Scarsi, Phys. Rev. 128, 2384 (1962).
O. V. Vedeneev, Yu. A. Nechin, Yu. A. Fomin, and G. B. Khristiansen, Vopr. At. Nauki Tekh., Ser.: Tekh. Fiz. Éksp., No. 3 (29), 47 (1986).
V. P. Antonova, A. P. Chubenko, S. V. Kryukov, et al., J. Phys. G 28, 251 (2002).
A. D. Erlykin, The talk at 20th European Cosmic Ray Symposium, ECRS 2006 (Lisbon, 2006).
M. Yoshida, Y. Toyoda, and T. Maeda, J. Phys. Soc. Jpn. 53, 1983 (1984).
G. B. Khristiansen et al., in Proceedings of XXI Interaction Cosmic Ray Conference (Adelaide, Australia, 1990), Vol. 9, p. 150.
Author information
Authors and Affiliations
Additional information
Original Russian Text © V.I. Yakovlev, M.I. Vil’danova, N.G. Vil’danov, 2007, published in Pis’ma v Zhurnal Éksperimental’noĭ i Teoreticheskoĭ Fiziki, 2007, Vol. 85, No. 2, pp. 111–113.
Rights and permissions
About this article
Cite this article
Yakovlev, V.I., Vil’danova, M.I. & Vil’danov, N.G. Detection and investigation of delayed extensive air showers with N e > 5 × 106 . Jetp Lett. 85, 101–103 (2007). https://doi.org/10.1134/S0021364007020014
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1134/S0021364007020014