Study of primary cosmic ray composition from gamma ray families in air shower cores

被引：0
|
作者：
Honda, K
Kawasumi, N
Tsushima, I
Hashimoto, K
Nishida, T
Matano, T
Inoue, N
Ohsawa, A
Tamada, M
Ohmori, N
Martinic, N
Ticona, R
Gironda, N
Osco, F
Aguirre, C
机构：
[1] FUKUI UNIV TECHNOL,DEPT APPL PHYS & CHEM,FUKUI 910,JAPAN
[2] SAITAMA UNIV,FAC SCI,URAWA,SAITAMA 388,JAPAN
[3] UNIV TOKYO,INST COSM RAY RES,TANASHI,TOKYO 188,JAPAN
[4] KINKI UNIV,FAC SCI & TECHNOL,HIGASHIOSAKA,OSAKA 577,JAPAN
[5] KOCHI UNIV,FAC SCI,KOCHI 780,JAPAN
[6] UNIV MAYOR SAN ANDRES,INST INVEST FIS,LA PAZ,BOLIVIA
来源：
NUCLEAR PHYSICS B | 1997年
关键词：
D O I：
暂无
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
We have observed high energy gamma families and associated air showers simultaneously at Mt. Chacaltaya. Monte Carlo simulations were calculated for the present experimental setup. From comparisons with both results, mechanism of gamma family production, change of interaction model, study of the chemical composition are discussed.
引用
收藏
页码：191 / 193
页数：3
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