Elastic α-scattering on proton rich nuclei at astrophysically relevant energies

被引：0

作者：

Fulop, Zs. ^{[1
]}

Galaviz, D. ^{[2
]}

Gyurky, Gy. ^{[1
]}

Kiss, G. G. ^{[1
]}

Mate, Z. ^{[1
]}

Mohr, P. ^{[2
]}

Rauscher, T. ^{[3
]}

Somorjai, E.

Zilges, A. ^{[2
]}

机构：

[1] ATOMKI, POB 51, D-64289 Darmstadt, Germany

[2] Tech Univ Darmstadt, Darmstadt 64289, Germany

[3] Univ Basel, Basel CH4056, Switzerland

来源：

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES | 2006年 / 847卷

关键词：

astrophysical p-process; elastic scattering; optical potential;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In order to improve the reliability of statistical model calculations in the region of heavy proton rich nuclei several elastic alpha scattering experiments have been carried out at low bombarding energies on various even-even and semi-magic nuclei. The extracted local optical potential parameters can be compared with the predictions of global alpha potentials. A study on Sn-112,Sn-124(alpha,alpha)Sn-112,Sn-124 has been made to test the global alpha potentials at both the proton and neutron rich sides of an isotopic chain. The present work describes the experimental challenges of high precision scattering experiments at low energy.

引用

页码：351 / +

页数：3

共 24 条

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