EPJ Web of Conferences
Volume 52, 2013ISVHECRI 2012 – XVII International Symposium on Very High Energy Cosmic Ray Interactions
|Number of page(s)||3|
|Section||Hadronic Interaction Models|
|Published online||10 June 2013|
An empirical model to describe rapidity density and transverse momentum distributions
1 Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, 277-8582, Japan
2 Instituto de Fisica Gleb Wataghin, Universidade Estadual de Campinas, Campinas, 13083-970, Brasil
3 Faculty of Science and Engineering, Kinki University, Higashi-Osaka, 577-8502, Japan
The distribution of rapidity density and transverse momentum is formulated empirically and analytically. It describes the data quite well over the wide energy range of √s = 22.4 – 7000 GeV.
© Owned by the authors, published by EDP Sciences, 2013
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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