ESTIMATION OF GALACTIC NEUTRON-FLUX IN ULTRAHIGH-ENERGY COSMIC-RAYS

被引：1

作者：

MIKHAILOV, AA

机构：

[1] Inst. of Cosmophysical Res. and Aeronomy, Yakutak

来源：

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS | 1994年 / 20卷 / 05期

关键词：

D O I：

10.1088/0954-3899/20/5/016

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

On the basis of an analysis of 17 403 showers with energies above 10(18) eV, recorded by the Yakutsk array between 1974 and 1991, the upper limit of neutrons from the Galaxy is estimated. The neutral particles are searched for in the direction of known gamma sources and pulsars.

引用

页码：841 / 844

页数：4

共 7 条

[1] BEREZINSKY VS, 1987, 20TH P INT COSM RAY, V2, P54
[2] CAPDEVIELLE JN, 1990, P INT S ASTROPHYSICA, P246
[3] COSMIC-RAYS OF THE HIGHEST ENERGIES .3. THE NATURE OF THE CANDIDATE DISCRETE SOURCES
CHI, X
SZABELSKI, J
VAHIA, MN
WDOWCZYK, J
WOLFENDALE, AW
[J]. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 1992, 18 (03) : 567 - 577
[4] EFIMOV NN, 1983, 18TH P INT COSM RAY, V2, P149
[5] EGOROV TA, 1991, 22ND P INT COSM RAY, V2, P121
[6] HAYASHIDA N, 1991, 22ND P INT COSM RAY, V2, P117
[7] JONES LW, 1988, 5TH P INT S VER HIGH, P358

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