ASTROPHYSICAL S-FACTOR OF THE p9Be→ 10Bγ RADIATIVE CAPTURE

被引：6

作者：

Dubovichenko, S. B. ^{[1
,2
]}

机构：

[1] Natl Space Agcy Kazakhstan Republ, VG Fesenkov Astrophys Inst, Natl Ctr Space Res & Technol, Alma Ata, Kazakhstan

[2] Natl Nucl Ctr Kazakhstan Republ, Inst Nucl Phys, Alma Ata, Kazakhstan

来源：

RUSSIAN PHYSICS JOURNAL | 2011年 / 54卷 / 07期

关键词：

nuclear physics; low astrophysical energies; elastic scattering; p(9)Be system; potential description; astrophysical S-factors; LIGHT-NUCLEI; ENERGY-LEVELS;

D O I：

10.1007/s11182-011-9688-y

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The S-factor of the p(9)Be -> B-10 gamma radiative capture is considered at astrophysical energies in the potential cluster model where orbital states are classified by the Young schemes.

引用

页码：814 / 821

页数：8

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