Testing chemical composition of highest energy comic rays

0456433 - FZÚ 2016 RIV SG eng C - Konferenční příspěvek (zahraniční konf.)
Nosek, D. - Vícha, Jakub - Nosková, J. - Ebr, Jan
Testing chemical composition of highest energy comic rays.
Proceedings of the 33rd International Cosmic Rays Conference. Singapore: International Union of Pure and Applied Physics (IUPAP), 2013, s. 0472. ISBN 978-85-89064-29-3.
[The 33rd International Cosmic Ray Conference (ICRC2013). Rio de Janeiro (BR), 20.7..02.0-09.07.2013]
Grant CEP: GA MŠMT(CZ) LG13007
Institucionální podpora: RVO:68378271
Klíčová slova: ultra-high energy cosmic rays * chemical composition
Kód oboru RIV: BF - Elementární částice a fyzika vys. energií
http://www.cbpf.br/~icrc2013/proc_icrc2013.html

We study basic characteristics of distributions of the depths of shower maximum in air showers caused by cosmic rays with the highest energies. The consistency between their average values and widths, and their energy dependences are discussed within a simple phenomenological model of shower development independently of assumptions about detailed features of high–energy interactions. It is shown that reliable information on primary species can be derived within a partition method. We present examples demonstrating implications for the changes in mass composition of primary cosmic rays./n
Trvalý link: http://hdl.handle.net/11104/0256964