Deficit of Ultrahigh Energy Extensive Air Showers

Simple item page
dc.creatorMikhailov, A. A.
dc.creatorEfremov, N. N.
dc.creatorMakarov, I. T.
dc.creatorNikolayeva, G. V.
dc.creatorStruchkov, G. G.
dc.date2004-05-31
dc.date.accessioned2026-07-07T02:13:21Z
dc.date.available2026-07-07T02:13:21Z
dc.descriptionArrival directions of extensive air showers by using world data are considered. It is shown that distributions of showers in zenith angle at E>10^{19}eV and E>4.10^{19}eV differ from each other. On this basis the conclusions are made: the estimation of the energy of inclined showers at E>4.10^{19}eV at Yakutsk and AGASA arrays is incorrect; the cosmic ray spectrum is not break up and most likely continued up to E=10^{20}eV and higher. It is found that ultrahigh energy cosmic rays are, probably, superheavy nuclei.
dc.description4 pages, 4 figures. The paper will be published in Proc. 28-th Russian conf. on cosm. rays, Moscow, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0405613
dc.identifierhttp://arxiv.org/abs/astro-ph/0405613
dc.identifierProc. 28-th RCRC, Moscow, 2004, 1411.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7785
dc.subjectAstrophysics
dc.titleDeficit of Ultrahigh Energy Extensive Air Showers
dc.typetext

Files

Collections

arXiv