Hadronic interactions and primary-cosmic-ray composition at energies around1015–1016eV derived from the analysis of high-energy gamma families-Reference-Cited by-同舟云学术

Hadronic interactions and primary-cosmic-ray composition at energies around1015–1016eV derived from the analysis of high-energy gamma families

Published:1988-09-01 Issue:5 Volume:38 Page:1404-1416
ISSN:0556-2821
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Ren J. R.,Huo A. X.,Lu S. L.,Su S.,Wang C. R.,Chang N. J.,Cao P. Y.,Li J. Y.,Zou B. T.,Wang S. Z.,Bai G. Z.,Liu Z. H.,Li G. J.,Geng Q. X.,He R. D.,Zhou W. D.,Amenomori M.,Nanjo H.,Hotta N.,Ohta I.,Mizutani K.,Kasahara K.,Yuda T.,Shirai T.,Tateyama N.,Torii S.,Shibata M.,Sugimoto H.,Taira K.

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.38.1404/fulltext

Reference25 articles.

1. Hadronic interactions at energies around103TeV inferred from the large-scale emulsion-chamber experiment at Mt. Fuji

2. Nuclear interactions and primary cosmic-ray component around1015eV viewed through the cluster analysis ofγ-ray families

3. Particle multiplicities in interactions at √s=540 GeV

4. Scaling of pseudorapidity distributions at c.m. energies up to 0.9 TeV

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