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Chinese Academy of Sciences Institutional Repositories Grid
Statistic model for galactic cosmic rays

文献类型:期刊论文

作者Xu, CX; Dai, HY
刊名High energy physics & nuclear physics-english edition
出版日期1997
卷号21期号:2页码:25-32
关键词Primary cosmic rays Cosmic ray composition Cosmic ray spectra Cosmic ray propagation
ISSN号0899-9996
通讯作者Xu, cx()
英文摘要This paper supposes that all cosmic ray (cr) particles of energy below 3 x 10(18)ev mainly originate and accelerate in an individual explosion of the supernova (sn) in the galaxy; with the use of an isotropic diffusion propagation model, the non-steady state density distribution of iron nuclei is investigated. considering the effect of extragalactic crs and the variety of the galactic cr nuclei, the statistic model of galactic crs with a reasonable distribution of the galactic sns in space and time can account for the spectrum of crs in the energy range of 10(12) - 10(20)ev quite well.
WOS关键词HIGH-ENERGIES ; ORIGIN
WOS研究方向Physics
WOS类目Physics, Nuclear ; Physics, Particles & Fields
语种英语
WOS记录号WOS:000080844300004
出版者ALLERTON PRESS INC
URI标识http://www.irgrid.ac.cn/handle/1471x/2176254
专题高能物理研究所
通讯作者Xu, CX
作者单位Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China
推荐引用方式
GB/T 7714
Xu, CX,Dai, HY. Statistic model for galactic cosmic rays[J]. High energy physics & nuclear physics-english edition,1997,21(2):25-32.
APA Xu, CX,&Dai, HY.(1997).Statistic model for galactic cosmic rays.High energy physics & nuclear physics-english edition,21(2),25-32.
MLA Xu, CX,et al."Statistic model for galactic cosmic rays".High energy physics & nuclear physics-english edition 21.2(1997):25-32.

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来源:高能物理研究所

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