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New measurement of the elemental fragmentation cross sections of 218 MeV/nucleon 28 Si on a carbon target

Authors :
Li, Guang-Shuai
Su, Jun
Sun, Bao-Hua
Terashima, Satoru
Zhao, Jian-Wei
Xu, Xiao- Dong
Zhang, Ji-Chao
Guo, Ge
He, Liu-Chun
Lin, Wei-Ping
Lin, Wen-Jian
Liu, Chuan-Ye
Lu, Chen-Gui
Mei, Bo
Sun, Zhi-Yu
Tanihata, Isao
Wang, Meng
Wang, Feng
Wang, Shi-Tao
Wei, Xiu-Lin
Wang, Jing
Xu, Jun-Yao
Liu, Jin-Rong
Zhang, Mei-Xue
Zheng, Yong
Zhu, Li-Hua
Zhang, Xue-Heng
Source :
Phys. Rev. C 107, 024609 (2023)
Publication Year :
2023

Abstract

Elemental fragmentation cross sections (EFCSs) of stable and unstable nuclides have been investigated with various projectile-target combinations at a wide range of incident energies. These data are critical to constrain and develop the theoretical reaction models and to study the propagation of galactic cosmic rays (GCR). In this work, we present a new EFCS measurement for $^{28}$Si on carbon at 218~MeV/nucleon performed at the Heavy Ion Research Facility (HIRFL-CSR) complex in Lanzhou. The impact of the target thickness has been well corrected to derive an accurate EFCS. Our present results with charge changes $\Delta Z$ = 1-6 are compared to the previous measurements and to the predictions from the models modified EPAX2, EPAX3, FRACS, ABRABLA07, NUCFRG2, and IQMD coupled with GEMINI (IQMD+GEMINI). All the models fail to describe the odd-even staggering strength in the elemental distribution, with the exception of the IQMD+GEMINI model, which can reproduce the EFCSs with an accuracy of better than 3.5\% for $\Delta Z\leq5$. The IQMD+GEMINI analysis shows that the odd-even staggering in EFCSs occurs in the sequential statistical decay stage rather than in the initial dynamical collision stage. This offers a reasonable approach to understand the underlying mechanism of fragmentation reactions.<br />Comment: 13 pages, 8 figures

Subjects

Subjects :
Nuclear Experiment

Details

Database :
arXiv
Journal :
Phys. Rev. C 107, 024609 (2023)
Publication Type :
Report
Accession number :
edsarx.2302.09349
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevC.107.024609