Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays

FAN Xiao-Ling; ZHANG Chun-Sheng

Chinese Physics C> 1992, Vol. 16> Issue(4) : 289-296

Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays

FAN Xiao-Ling ^, ,
ZHANG Chun-Sheng

Institute of High Energy Physics,Academia Sinica,Beijing 100039

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Abstract：
Under the assumption of mixed primary cosmic ray composition and using a hadron-hadron interaction parametrization model to describe hadron-hadron nuclear interaction,the behavior of superhigh energy cosmic ray particles in the atmosphere is simulated,and the simulated results compared with experimental data of Mt.emulsion chamber in details.The influences from the mean transverse momentum value of secondary particles in fragmentation region on simulated results are discussed also in details.

References

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范晓岭，张春生，高能物理与核物理，16(1992),[2] China-Japan Collaboration, Proceedings of International Symposium on Cosmic Ray Superhigh Interactions,Beijing, (1986) 3-24.[3] M. Haguenauer et al., 21th ICRC, Austrilia, Vol. 8 (1990), 209.[4] N, L. Grigorov et al., 12th ICRC, Vol. 5 (1971), 1746.[5] M. Nagano, J. Phys., G10 (1984), 1295.[6] M. Simon et al., Ap. J., Vol. 239 (1980), 712.[7] M. G. Ryan et al., Phys, Rev, Lett., Vol. 28 (1972), 985.[8] T, H. Burnett et al., Phys. Rev. Lett., Vol. 51 (1983), I010. 19th ICRC, Vol. 2 (1985), 48.[9] J. M. Grunsfeld et al., Ap. J., Vol. 327 (1988), 31.[10] 丁林澄等，高能物理与核物理，7(1983)，129,[11] J. R, Ren et al., Phys. Rev., D38 (1988), 1404.[12] J. E. Elias et al., Phys. Rev., D22 (1980), 13.[13] F. Fumuro et al., Nucl. Phys., B152 (1979), 376.[14] L. K. Ding et al., Proceedings of International Symposium on Cosmic Ray Superhigh Interactions, Beijing,(1986) 3-49[15] Q. Q. Zhu et al., Proceedings of International Symposium on Cosmic Ray Superhigh Interactions, Beijing,(1986) 7-1.[16] A.M.Dunaevsky et al., 18th ICRC, Vol. 5 (1983), 449

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FAN Xiao-Ling and ZHANG Chun-Sheng. Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays[J]. Chinese Physics C, 1992, 16(4): 289-296.

FAN Xiao-Ling and ZHANG Chun-Sheng. Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays[J]. Chinese Physics C, 1992, 16(4): 289-296. shu

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

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沈阳化工大学材料科学与工程学院沈阳 110142

Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays

FAN Xiao-Ling ^,
ZHANG Chun-Sheng

Corresponding author: FAN Xiao-Ling,

Institute of High Energy Physics,Academia Sinica,Beijing 100039

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1992-04-05

Abstract: Under the assumption of mixed primary cosmic ray composition and using a hadron-hadron interaction parametrization model to describe hadron-hadron nuclear interaction,the behavior of superhigh energy cosmic ray particles in the atmosphere is simulated,and the simulated results compared with experimental data of Mt.emulsion chamber in details.The influences from the mean transverse momentum value of secondary particles in fragmentation region on simulated results are discussed also in details.