| Issue |
EPJ Web of Conferences
Volume 109, 2016
The 13th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG2015)
|
|
|---|---|---|
| Article Number | 04002 | |
| Number of page(s) | 7 | |
| Section | Experimental Nuclear Physics for Astrophysics | |
| DOI | https://doi.org/10.1051/epjconf/201610904002 | |
| Published online | 12 February 2016 | |
https://doi.org/10.1051/epjconf/201610904002
Optical potential parameters from 12C + Zr elastic scattering
1 China Institute of Atomic Energy, P.O. Box 275(10), Beijing, 102413, China
2 Shenzhen University, Shenzhen, 518060, China
a e-mail: ganlin2007@hotmail.com
b e-mail: zhli@ciae.ac.cn
Published online: 12 February 2016
The angular distributions of 12C + 90,92,94,96Zr elastic scattering were measured with the Q3D magnetic spectrometer at the HI-13 tandem accelerator, Beijing. The real part of optical potential were extracted by analysing these angular distributions. The analysis enable us to avoid the influence of Coulomb effect and to observe the dependence of optical potential on the nuclear properties. With the deduced potential parameters, the experimental elastic scattering angular distributions can be reproduced very well. Formulas to infer global heavy-ion potential parameters were obtained then by analyzing the extracted optical potential parameters. The formulas can be used widely in heavy-ion nuclear reactions.
© Owned by the authors, published by EDP Sciences, 2016
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