ORIGIN OF GALACTIC COSMIC-RAYS

被引：42

作者：

BIERMANN, PL ^{[1
]}

GAISSER, TK ^{[1
]}

STANEV, T ^{[1
]}

机构：

[1] UNIV DELAWARE,BARTOL RES INST,NEWARK,DE 19716

来源：

PHYSICAL REVIEW D | 1995年 / 51卷 / 07期

关键词：

D O I：

10.1103/PhysRevD.51.3450

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Motivated by recent measurements of the major components of the cosmic radiation around 10 TeV/nucleon and above, we discuss the phenomenology of a model in which there are two distinct kinds of cosmic ray accelerators in the galaxy. A comparison of the spectra of hydrogen and helium up to 100 TeV per nucleon suggests that these two elements do not have the same spectrum of magnetic rigidity over this entire region and that these two dominant elements therefore receive contributions from different sources. © 1995 The American Physical Society.

引用

页码：3450 / 3454

页数：5

共 28 条

[1] ASAKIMORI K, 1994, COSMIC RAY C, V2, P25
[2] BIERMANN PL, 1993, ASTRON ASTROPHYS, V271, P649
[3] BIERMANN PL, 1993, ASTRON ASTROPHYS, V277, P691
[4] BIERMANN PL, 1993, ASTRON ASTROPHYS, V275, P659
[5] BIERMANN PL, 1994, COSMIC RAY C, V2
[6] DWYER J, 1994, COSMIC RAY C, V1, P587
[7] OBSERVATION OF HEAVY COSMIC-RAY PRIMARIES OVER THE WIDE ENERGY-RANGE FROM SIMILAR-TO 100 GEV/PARTICLE TO SIMILAR-TO 100 TEV/PARTICLE - IS THE CELEBRATED KNEE ACTUALLY SO PROMINENT
ICHIMURA, M
KOGAWA, M
KURAMATA, S
MITO, H
MURABAYASHI, T
NANJO, H
NAKAMURA, T
OHBA, K
OHUCHI, T
OZAWA, T
YAMADA, Y
MATSUTANI, H
WATANABE, Z
KAMIOKA, E
KIRII, K
KITAZAWA, M
KOBAYASHI, T
MIHASHI, A
SHIBATA, T
SHIBUTA, K
SUGIMOTO, H
NAKAZAWA, K
[J]. PHYSICAL REVIEW D, 1993, 48 (05): : 1949 - 1975
[8] IVANENKO IP, 1993, COSMIC RAY C, V2, P25
[9] QUASIDIRECT OBSERVATIONS OF COSMIC-RAY PRIMARIES IN THE ENERGY REGION 10(12)-10(14)EV
KAWAMURA, Y
MATSUTANI, H
NANJYO, H
TERAOKA, K
TODA, K
ICHIMURA, M
KIRII, K
KOBAYASHI, T
NIIHORI, Y
SHIBATA, T
SHIBUTA, K
YOSHIZUMI, Y
[J]. PHYSICAL REVIEW D, 1989, 40 (03): : 729 - 753
[10] LUND N, 1989, AIP C P, V183, P111

← 1 2 3 →