CALCULATION OF THE SECONDARY ANTIPROTON FLUX IN COSMIC SPACE

QIN Ke-Yu

近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。

本刊再次郑重声明：

（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137

（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。

（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。

《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 1983, Vol. 7> Issue(2) : 257-261

CALCULATION OF THE SECONDARY ANTIPROTON FLUX IN COSMIC SPACE

QIN Ke-Yu ^,

Institute of High Energy Physics, Academia Sinica

Abstract
HTML
Reference
Related

PDF

Abstract：
Using recent experimental results, we calculate the antiproton flux which is produced by the collisions of cosmic rays with the interstellar matter. This calculated result is compared with the experimental result of Golden et al. It is shown that it is quite possible that primary antiproton exists in cosmic space.

References

[1]

T. K. Gaisser and R. H. Maurer, Phys. Rev. Lett., 30 (1973), 1264[2] S. R. Ganguli and B. V. Sreekantan, J. Phys. A, 9 (1976), 311.[3] G. D. Badhwar et al., Astrophys. Space Sci., 37 (1975), 283.[4] J. A. Lezniak and W. R. Webber, Astrophys. J., 223 (1978), 676[5] R. L. Golden et al., Phys. Rev. Lett., 43 (1979), 1196[6] M. Antinucci et al., Lett. Nuovo Cimento, 6 (1973), 121.[7] A, M. Hillas, Phys. Reports. 20C (1975), 59.[8] A. R. Das and A. K. De, J. Phys. G., 5 (1979), 445.[9] A. A. VPatsoil, 第十四届国际宇宙线会议文集, 12(1975), 4019,[10] D. D. Krasihlikov,第十四届国际宇宙线会议文集, 12 (1975), 4347.

[1]	YAN Mu-Lin . X(1835) as Proton-Antiproton Bound State in Skyrme Model. Chinese Physics C, 2006, 30(11): 1141-1150.
[2]	WANG Rui-Guang , YU Zhong-Qiang , DING Lin-Kai , MA Yu-Qian , ZHU Qing-Qi . Estimation of the Flux Upper Limit for a Solar Energetic Proton Beam. Chinese Physics C, 2004, 28(10): 1017-1020.
[3]	GU An-Jia , ZHAO Kui , DING Yuan-Tao , ZHANG Bao-Cheng , QUAN Sheng-Wen , CHEN Jia-Er . Beam 2-D Phase-Space Measurement with CT and Cerenkov Radiation “Double Imaging Method”. Chinese Physics C, 2003, 27(5): 455-459.
[4]	OUYANG Hua-Fu . Effects of the Space Charge Forces and the Beam Halo in an AVF Cyclotron with Intense Beam Currents. Chinese Physics C, 2001, 25(6): 561-570.
[5]	Li Yangguo . Antiproton-Nucleus Charge Exchange Reaction in Mirror Nuclei. Chinese Physics C, 1997, 21(6): 554-561.
[6]	Li Yangguo , Zhang Yushun . Low-Energy Antiproton-Nucleus Scattering and Glauber Theory. Chinese Physics C, 1995, 19(4): 348-353.
[7]	Li Yangguo . Antiproton-Nucleus Inelastic Scattering at Intermediate Energies. Chinese Physics C, 1994, 18(2): 186-192.
[8]	Jia Huanyu , Cao Zhen , Zhang Huimin . The Study of Meteorological Effects on TeV Cosmic Ray Flux. Chinese Physics C, 1994, 18(9): 788-793.
[9]	LI Yang-Guo . The Spin Effect of Antiproton-Nucleus Inelastic Collison. Chinese Physics C, 1992, 16(2): 137-144.
[10]	SONG Zhong-Heng , WANG Xiao-Min . Calculation of Space Charge Field for Annulus and Disc Bunch of Charged Particles. Chinese Physics C, 1991, 15(1): 7-12.
[11]	LI Yang-Guo . SPIN OBSERVABLE IN ANTIPROTON-NUCLEUS ELASTIC SCATTERINGS. Chinese Physics C, 1989, 13(6): 539-543.
[12]	LI Yang-Guo . ANTIPROTON-NUCLEUS INELASTIC COLLISION. Chinese Physics C, 1989, 13(5): 433-439.
[13]	LUO Zi-Hua , WANG Shu-Hong . BEAM MATCHING CALCULATIONS IN TRANSVERSE MOTION FOR THE 10MeV BEIJING PROTON LINAC. Chinese Physics C, 1985, 9(2): 191-199.
[14]	ZHU Qing-Qi , WU Shi-Pei . SIMULATION CALCULATION FOR DETECTION EFFICIENCY IN THE MEASUREMENT OF COSMIC RAY HADRON SPECTRA. Chinese Physics C, 1985, 9(3): 263-267.
[15]	QIN KE-YU . THE VERTICAL INTENSITY OF THE ANTIPROT ON AT THE ATOMOSPHERIC DEPTH x=700g/cm². Chinese Physics C, 1981, 5(4): 472-476.
[16]	Wei Kai-yu , Lin Zhen-hua . A COMPUTATIONAL METHOD FOR THE DESIGN ENERGY HIGH INTENSITY BEAM TRANSPORT SYSTEMS. Chinese Physics C, 1980, 4(5): 555-562.
[17]	Yu Qing-chang . THEORY OF NONLINEAR SPACE-CHARGE EFFECTS OF LOW ENERGY INTENSE CHARGED PARTICLE BEAMS. Chinese Physics C, 1980, 4(5): 579-587.
[18]	Ding Lin-kai , Zhu Qing-qi . MONTE-CARLO SIMULATION OF COSMIC RAY ANTIPROTON INTENSITY. Chinese Physics C, 1980, 4(6): 735-740.
[19]	XU CHUN-XIAN , HUO AN-XIANG , YUAN YN-KUI , GU YI-DONG , LI TI-PEI , SHEN PEI-RO , JIA GUEI-BIN , XIAO QIAN-YI , ZHANG CHENG-MO , CHEN DUAN-BAO . THE NEGATIVE-POSITIVE RATIO OF CHARGED COSMIC RAY HADRONS AT THE 3220 m ABOVE SEA-LEVEL. Chinese Physics C, 1978, 2(5): 423-427.
[20]	YUAN YU-KUI , HUO AN-XIANG , ZHANG CHANG-CHUN , QIN KE-YU , ZHU AI-MIN , ZHANG REN-QING , GUO KE-ZUN , YANG CHANG-TOU , LI QIN-LIAN , FAN SHI-HE . PRELIMINARY MEASUREMENT OF THE ANTIPROTON COMPONENT IN COSMIC RAYS AT A 3220m ALTITUDE. Chinese Physics C, 1978, 2(5): 478-480.

Access

Get Citation

QIN Ke-Yu. CALCULATION OF THE SECONDARY ANTIPROTON FLUX IN COSMIC SPACE[J]. Chinese Physics C, 1983, 7(2): 257-261.

QIN Ke-Yu. CALCULATION OF THE SECONDARY ANTIPROTON FLUX IN COSMIC SPACE[J]. Chinese Physics C, 1983, 7(2): 257-261. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 1900-01-01
Revised: 1900-01-01

Article Metric

Article Views(2268)
PDF Downloads(500)
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, [email protected]

1.
沈阳化工大学材料科学与工程学院沈阳 110142

CALCULATION OF THE SECONDARY ANTIPROTON FLUX IN COSMIC SPACE

QIN Ke-Yu ^,

Corresponding author: QIN Ke-Yu,

Institute of High Energy Physics, Academia Sinica

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1983-04-05

Abstract: Using recent experimental results, we calculate the antiproton flux which is produced by the collisions of cosmic rays with the interstellar matter. This calculated result is compared with the experimental result of Golden et al. It is shown that it is quite possible that primary antiproton exists in cosmic space.