HIGH ENERGY PRIMARY ELECTRON SPECTRUM AND DIFFUSION X-RAY SOURCE

Xu CHUN-XLAN; ZHANG HE-QI

Chinese Physics C> 1981, Vol. 5> Issue(4) : 484-488

HIGH ENERGY PRIMARY ELECTRON SPECTRUM AND DIFFUSION X-RAY SOURCE

Abstract
HTML
Reference
Related

PDF

Abstract：
Non-steady state electron spectrum in interstellar medium is investigated by using the model of isotropic diffusion of primary cosmic electrons originated from explosion of supernovae. The diffusion coefficient was determined semi-experientially according to particles resonant scattering on the turbulent by dromagnetic wave. Comparing the solution of the diffusion equation with the electron spectrum which was measured near the earth, we derived the index Γ of the electron spectrum to be Γ～2. Assuming that the electron inverse Compton scattering on 2.7°K background field forms diffusion X-ray sources, we deduce the energy-state function, and then obtain the X-ray spectrum near the earth. The index Γ～2 decided above can also explain the X-ray spectrum index of Nebuler.

References

[1]

Dietrich Miiller et al., 16th Int. Gosmic Ray Conf., Vol. 12, p. 102[2] T. Taira. et al., 16th Int. Cosmic Ray Conf., Vol. 1, p. 478.[3] J. Nishimura et al., 16th Int. Cosmic Ray Coraf., Vol. 1, p. 488.[4] P. Meyer, "Origin of Coemie Raye", p. 233-266; D. Reided Publiehing Company, Dorect- Holland.[5] Gratton, Astrophys. and Space Sci., 16(1972), S1.[5] F. W. Btecker, "Origin of Cosmic Rays," p. 267-335; D. Reided Publishing Company.Dordrecht-Holland.[7] 张和棋,天文学报,(1981),[8] 张和棋,高能物理与核物理,5(1981),477,[9] J. L. Osborne, "Origin of Cosmic Rays,',p. 203-219.[10] G. F. Carpenter et al., Nature, Jan. 15, 1976, p. 99.[11] W. R. Webber et al., 16th Int. Cksmic Ray Conf., Vol. 1, p. 495.[12] Wentzel,Astrophys. J., 152(1968), 987[13] Kulerud and Pearce, Astrophys. J,156(1969), 446

[1]	XIONG Yong-Qian , QIN Bin , FENG Guang-Yao , TAN Ping , TIAN Jia-Shen , CHEN Ping , YANG Jun , YU Tiao-Qin , PEI Yuan-Ji , FAN Ming-Wu . Preliminary Design of Compact FEL Terahertz Radiation Source. Chinese Physics C, 2008, 32(S1): 301-303.
[2]	WANG Si-Guang , ZHOU Shu-Hua , YE Yun-Xiu , YE Zhen-Yu , MAO Ya-Jun . Research on Depolarization of Transversely Polarized Gas Target Induced by High Energy e-Beam. Chinese Physics C, 2006, 30(9): 892-895.
[3]	SHI Jiang-Jun , LIU Jun , LIU Jin , LI Bi-Yong . Beam Parameter Requrements for Radiography. Chinese Physics C, 2006, 30(S1): 31-33.
[4]	PEI Guo-Xi , SUN Yao-Lin , LIU Jin-Tong , CHI Yun-Long , LIU Yu-Cheng , LIU Nian-Zong . BEPCⅡ Positron Source. Chinese Physics C, 2006, 30(1): 66-70.
[5]	LIU Jin-Tong , GEN Zhe-Qiao , SUN Xian-Jing , SUN Yao-Lin , PEI Guo-Xi . Development of the BEPCⅡ Positron Source Flux Concentrator. Chinese Physics C, 2005, 29(4): 404-407.
[6]	KONG Wei , XI Chuan-Ying , YE Bang-Jiao , WENG Hui-Min , ZHOU Xian-Yi , HAN Rong-Dian . Two-Detector Doppler Broadening of Annihilation Radiation in Metals. Chinese Physics C, 2004, 28(11): 1234-1237.
[7]	SU Run , LIU Feng-Qin , QIAN Hai-Jie . Study of Electronic Structure of Ultrathin Co Films Epitaxially Grown on Cu (111) by Angle-Resolved Photoemission Spectroscopy. Chinese Physics C, 2003, 27(2): 178-182.
[8]	XING Xiu-Wen , ZHONG Wei-Li , LIU Lian-Shou . A Monte Carlo Study of the Fractal Property inside Jets Produced in High Energy e⁺e^－ Collisions. Chinese Physics C, 2003, 27(2): 95-98.
[9]	LIN Xiao-Yan , LIU Lian-Shou . Scale for the Production of Jets in High Energy e⁺e^－ Collisions. Chinese Physics C, 2003, 27(1): 7-11.
[10]	LIU Jun , GENG Qing-Xi , YANG Hong-Tao , LIU Chang-Qin , ZHANG Pin , GAO Xiao-Yu , JING Cai-Liu , ZHA Min , JING Gui-Ru , ZHU Qing-Qi , Cheung T , Ng L . Study of EAS Local Muon Density Spectrum and the Knee in the Energy Spectrum of Primary Cosmic Rays. Chinese Physics C, 2003, 27(2): 109-112.
[11]	ZHANG Yong-Hui , CHEN Hong-Bin , KANG Qiang , CAO Shao-Yun , CHANG An-Bi . Development of Repetition Frequency Electron-Beam Generator Technology. Chinese Physics C, 2002, 26(8): 876-881.
[12]	GOU Wei-Ping , PEI Guo-Xi . Design of BEPCⅡ Positron Source. Chinese Physics C, 2002, 26(3): 279-285.
[13]	ZHU Zhi-Yong , JIN Yun-Fan , LIU Chang-Long , SUN You-Mei , WANG Yan-Bin , HOU Ming-Dong , CHEN Xiao-Xi , WANG Zhi-Guang , ZHANG Chong-Hong , LIU Jie , LI Bao-Quan . Electronic Energy Loss Effects in Polystyrene Irradiated with High Energy Argon Ions. Chinese Physics C, 2001, 25(1): 74-78.
[14]	Geng Rongli , Song Jinhu , Yu Jin . Studies on a Laser Driven Photoemissive High-Brightness Electron Source and Novel Photocathodes. Chinese Physics C, 1997, 21(1): 67-74.
[15]	REN Jing-Ru , LU Sui-Ling , SU Shi , HUO An-Xiang , WANG Cheng-Rui , HE Mao , CAO Pei-Yuan , LI Jin-Yu , WANG Shi-Zhi , LI Guang-Ju , BAI Guang-Zhi , LIU Zhong-He , MU Jun , . Identification of Primary Cosmic Ray Particles Producing Big Gamma-Families in Emulsion Chambers. Chinese Physics C, 1992, 16(3): 193-196.
[16]	LIU Yi-Ming , HUO Lei , JIANG Yu-Zhen , WANG Shan . Source Density Distribution and Intensity Interferometry in High-Energy Heavy-Ion Collisions. Chinese Physics C, 1991, 15(2): 123-130.
[17]	SHI Ya-Fei , ZHUANG Peng-Fei , LIU Lian-Shou . PAPIDITY DISTRIBUTIONS IN HIGH-ENERGY NUCLEUS-NUCLEUS COLLISIONS AND MULTISOURCE MODEL. Chinese Physics C, 1990, 14(1): 56-63.
[18]	PEI Guo-Xi , XIE Jia-Lin , ZHOU Shu , SUN Song-Lan . OPTIMIZATION OF BEPC POSITRON SOURCE. Chinese Physics C, 1990, 14(2): 110-117.
[19]	ZHANG Tian-Bao , TANG Xiao-Wei , WANG Yun-Yu , LI Yao-Qing , YIU Ke , WANG Shao-Jie . MEASUREMENT OF THE WHOLE GAMMA-RAY ENERGY SPECTRUM IN o-Ps 3 GAMMA-DECAY. Chinese Physics C, 1984, 8(4): 385-391.
[20]	CHEN YING-XUAN , REN GUO-XIAO , WU MEI , HE CHANG-XIAO , SHEN PEI-RUO , LI YIAN-GUO , XIAO QIAN-YI , WANG JUN , CHEN DUAN-BAO , ZHENG RONG-TING . THE EAS ELECTRON DENSITY SPECTRUM. Chinese Physics C, 1981, 5(1): 1-4.

Access

Get Citation

Xu CHUN-XLAN and ZHANG HE-QI. HIGH ENERGY PRIMARY ELECTRON SPECTRUM AND DIFFUSION X-RAY SOURCE[J]. Chinese Physics C, 1981, 5(4): 484-488.

Xu CHUN-XLAN and ZHANG HE-QI. HIGH ENERGY PRIMARY ELECTRON SPECTRUM AND DIFFUSION X-RAY SOURCE[J]. Chinese Physics C, 1981, 5(4): 484-488. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 1980-07-18
Revised: 1900-01-01

Article Metric

Article Views(1924)
PDF Downloads(282)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

HIGH ENERGY PRIMARY ELECTRON SPECTRUM AND DIFFUSION X-RAY SOURCE

Received Date: 1980-07-18

Accepted Date: 1900-01-01

Available Online: 1981-08-05

Abstract: Non-steady state electron spectrum in interstellar medium is investigated by using the model of isotropic diffusion of primary cosmic electrons originated from explosion of supernovae. The diffusion coefficient was determined semi-experientially according to particles resonant scattering on the turbulent by dromagnetic wave. Comparing the solution of the diffusion equation with the electron spectrum which was measured near the earth, we derived the index Γ of the electron spectrum to be Γ～2. Assuming that the electron inverse Compton scattering on 2.7°K background field forms diffusion X-ray sources, we deduce the energy-state function, and then obtain the X-ray spectrum near the earth. The index Γ～2 decided above can also explain the X-ray spectrum index of Nebuler.

HTML

Reference (1)

HIGH ENERGY PRIMARY ELECTRON SPECTRUM AND DIFFUSION X-RAY SOURCE

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

HIGH ENERGY PRIMARY ELECTRON SPECTRUM AND DIFFUSION X-RAY SOURCE

HTML

目录