A Statistic Model for Galactic Cosmic Rays

Xu Chunxian; Dai Hongyue

Chinese Physics C> 1997, Vol. 21> Issue(6) : 486-493

A Statistic Model for Galactic Cosmic Rays

Xu Chunxian ^, ,
Dai Hongyue

Institute of High Energy Physics,The Chinese Academy of Sciences,Beijing 1000392 Department of Physics,University of Utah, Salt Lake City, UT84112 U.S.A

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Abstract：
Supposed that all of cosmic ray particles of energy below 3×10¹⁸eV are mainly originated and accelerated in an individual explosion of the galactic supernovae(SNs).By using an isotropic diffusion propagation model,non-steady state density of the iron nucleus is investigated.Considering the effect of extra-galactic cosmic rays and the variety of the galactic cosmic ray nuclei,the statistic model of galactic cosmic rays with a reasonable distribution of the SNs in space and time can account for the spectrum of cosmic ray in the energy range of 10¹²—10²⁰eV quitewell.

References

[1]

K.Asakimori et al.,22nd ICRC,2（1991）57.[2]D.J.Bird et al.,Ap.J.,424（1994）494[3]T.K.Gaisser et al.,Phys.Rev.,D47（1993）1919.[4]D.Muller et al.,Ap.J.,374.（1991）356.[5]S.P.Swordy et al,Ap.J,403（1993）658.[6]G.Cunning et al.,Ap.J,236（1980）L71[7]J.Buckley et al.,Ap.J.,429（1994）736.[8]I.L,Rasussen.B.Peters,Nature,258（1975）412.[9]J.Wdowczyk,A.W.Wolfendale,Nature,281（1979）356.[10]L.OC.Drury23rd ICRC,Invited,Rapporteur Highlight Papers（1993）307.[11]J.Ormes,P.Freier,Ap,J.222（1978）471.[12]Chunxian Xu,19th ICRC,2（1985）314.[13]A.M.hillas,M.ouldridge,Nature,253（1975）609.[14]D.J.Bird et al,23rd ICRC,2（1993）51.[15]V.L.Ginzburg.v.s.Ptuskin,Rev.of Mod.Phys.,48（1976）161.[16]A.Lukasiak et al.Ap.J.,430（1994）L69.[17]R.Battiston et al,CERN/EP:No.111.1982.[18]A.Z.Dolginov,M.E.Katz,Physics Reports,239（1994）285.[19]W.R.Webber et al,Ap.J,429（1994）764[20]J.Buckley et al.Ap.J,429（1994）736.[21]J.F.Ormes.18th.ICRC,2（1983）187.[22]Chunxian Xu.Chinese Journal of Space Science,5（1985）123.[23]J.L.Puget.F.W.Stecker,Ap.J,191（1974）323.[24]F.W.Stecker,Phys.Rev.Lett.,35（1975）188.[25]J.R Jokipii,G.E. Morfill,Ap.J., 290(1985)L1.[26]P.L.Biermann,23rd ICRC,Invited,Rapporteur Highlight Papers (1993)45.

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[15]	JIANG Yin-Lin , YUAN Yu-Kui , LI Yan-Guo , CHEN Duan-Bao , ZHENG Rong-Ting , SONG Jian-Ning . RESEARCH FOR THE POSSIBILITY ON DETECTING COSMIC RAY PARTICLES BY ACOUSTIC WAY. Chinese Physics C, 1986, 10(1): 9-14.
[16]	LU Chang-Guo , LU Wei-Da , ZHOU Yue-Hua , ZHANG Yu , GU Wei-Xin . TESTING RESULTS ON THE PROTOTYPE OF SHOWER COUNTER WITH COSMIC RAYS. Chinese Physics C, 1985, 9(4): 397-404.
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[18]	ZHANG HE-QI . PROPAGATION OF COSMIC RAY ELECTRONS IN THE GALAXY. Chinese Physics C, 1981, 5(4): 477-483.
[19]	Kuang Hao-huai , Hu Wen-jun , Zhou Yin-zao , Tan You-HENG , Shen Chang-quan , Jang Yin-lin , Zhu Qing-qi , Qin Ke-yu , Li Yan-guo , Wang Li-an . IDENTIFICATION OF THE HORIZONTAL COSIMC RAY PENETRATING PARTICLES. Chinese Physics C, 1980, 4(4): 413-416.
[20]	CHANG KONG-LIANG . PROPAGATION EFFECTS OF SOLAR COSMIC RAYS. Chinese Physics C, 1978, 2(5): 385-393.

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Xu Chunxian and Dai Hongyue. A Statistic Model for Galactic Cosmic Rays[J]. Chinese Physics C, 1997, 21(6): 486-493.

Xu Chunxian and Dai Hongyue. A Statistic Model for Galactic Cosmic Rays[J]. Chinese Physics C, 1997, 21(6): 486-493. shu

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Received: 1900-01-01
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通讯作者: 陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

A Statistic Model for Galactic Cosmic Rays

Corresponding author: Xu Chunxian,

Institute of High Energy Physics,The Chinese Academy of Sciences,Beijing 1000392 Department of Physics,University of Utah, Salt Lake City, UT84112 U.S.A

Received Date: 1900-01-01

Accepted Date: 1900-01-01

Available Online: 1997-06-05

Abstract: Supposed that all of cosmic ray particles of energy below 3×10¹⁸eV are mainly originated and accelerated in an individual explosion of the galactic supernovae(SNs).By using an isotropic diffusion propagation model,non-steady state density of the iron nucleus is investigated.Considering the effect of extra-galactic cosmic rays and the variety of the galactic cosmic ray nuclei,the statistic model of galactic cosmic rays with a reasonable distribution of the SNs in space and time can account for the spectrum of cosmic ray in the energy range of 10¹²—10²⁰eV quitewell.

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A Statistic Model for Galactic Cosmic Rays

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