Propagation of Cosmic-Ray Nuclei with Reacceleration

ZHANG Li; ZHANG Ming; MU Jun; YU Chuan-Zan

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《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 1992, Vol. 16> Issue(5) : 392-397

Propagation of Cosmic-Ray Nuclei with Reacceleration

Deparment of Physics,Yunnan University,Kunming 650091

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Abstract：
Introducing effective energy change tate of galactic cosmic ray (GCR) during interstellar propagation,we obtain a general method of solving the propagation equation of GCR nuclei-modified slab weighted method.In the leaky box model,we give comparisons of calculated ratios of secondary and primary nuclei and primary energy spectra with observed results.

References

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Letaw, J. R., et al., Astrophys. J. Suppl., 56(1984), 369.[2] Cesarsky, C. J., 20th ICRC Rapporteur Talk，8(1987), 87.[3] Berezinsky, V. S., 21th ICRC Rapporteur Talk，11(1990), 115[4] Letaw, J. R., et al., Astrophy, J, Suppl，51(1983), 271.[5] Webber, W, R., et al., Phys. Rev. C, 41(1990), 533.[6] Drury, LOC, Prog. Phys., 46(1983), 973.[7] Simpson, J. A., Ann. Rev. Nucl. Part, Sci., 33(1983), 323,[8] Heinbach, U. and Simon, M., 21th ICRC, 3(1990), 361.[9] Wiedenbeck, M. E., 21th ICRC, 11(1990), 57.[10] Simon, M., et al., Astrophys. J., 300(1986), 32.[11] Tang, K. K., 21th ICRC, 3(1990), 373.[12] Schlickeiser, R., Astrophys. J., 336(1989), 243.[13] 张力，喻传赞，天体物理学报，11(1991)，111,[14] Giler, M., et al., Astron. Astrophys., 217(1989), 311.

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ZHANG Li, ZHANG Ming, MU Jun and YU Chuan-Zan. Propagation of Cosmic-Ray Nuclei with Reacceleration[J]. Chinese Physics C, 1992, 16(5): 392-397.

ZHANG Li, ZHANG Ming, MU Jun and YU Chuan-Zan. Propagation of Cosmic-Ray Nuclei with Reacceleration[J]. Chinese Physics C, 1992, 16(5): 392-397. shu

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

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1.
沈阳化工大学材料科学与工程学院沈阳 110142

Propagation of Cosmic-Ray Nuclei with Reacceleration

Corresponding author: ZHANG Li,

Deparment of Physics,Yunnan University,Kunming 650091

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

Abstract: Introducing effective energy change tate of galactic cosmic ray (GCR) during interstellar propagation,we obtain a general method of solving the propagation equation of GCR nuclei-modified slab weighted method.In the leaky box model,we give comparisons of calculated ratios of secondary and primary nuclei and primary energy spectra with observed results.