Nuclear interactions and primary cosmic-ray component around 1015 eV viewed through the cluster analysis of -ray families

M. Amenomori, E. Konishi, H. Nanjo, K. Mizutani, K. Kasahara, Shoji Torii, T. Yuda, T. Shirai, N. Tateyama, T. Taira, I. Mito, M. Shibata, H. Sugimoto, K. Taira, N. Hotta

研究成果: Article

18 引用 (Scopus)

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An analysis of the -ray families (E100 TeV) obtained with the Mt. Fuji emulsion chambers was made focusing attention on the cluster structure of families, and the validity of scaling in the fragmentation region in the 1015-eV region was examined by comparing the results with those of artificial families. We deduced that (i) scaling in the fragmentation region (Feynman x>0.1) is not broken appreciably, at least below 1015 eV, (ii) scaling in the central region (x<<0.1) seems to be broken largely at E>1015 eV; multiplicity increases proportionally to E14 or even stronger (say, E13), (iii) the iron component in the primary cosmic rays rapidly increases and occupies 60-70% of the total flux at 1015 eV and that of the protons decreases to f 10%, and (iv) the average transverse momentum of produced pions in the fragmentation region stays within 400 MeV/c.

元の言語English
ページ(範囲)2807-2819
ページ数13
ジャーナルPhysical Review D
25
発行部数11
DOI
出版物ステータスPublished - 1982
外部発表Yes

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

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  • これを引用

    Amenomori, M., Konishi, E., Nanjo, H., Mizutani, K., Kasahara, K., Torii, S., Yuda, T., Shirai, T., Tateyama, N., Taira, T., Mito, I., Shibata, M., Sugimoto, H., Taira, K., & Hotta, N. (1982). Nuclear interactions and primary cosmic-ray component around 1015 eV viewed through the cluster analysis of -ray families. Physical Review D, 25(11), 2807-2819. https://doi.org/10.1103/PhysRevD.25.2807