Contribution of the M1 process to the astrophysical S-factor of the p 2H radiative capture

被引：19

作者：

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

机构：

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

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

来源：

RUSSIAN PHYSICS JOURNAL | 2011年 / 54卷 / 02期

关键词：

cluster model; photonuclear processes; thermonuclear reactions; low energy; light atomic nuclei; astrophysical S-factors; PHASE-SHIFT ANALYSIS; LIGHT-NUCLEI; COUPLING-CONSTANTS; SCATTERING; MODEL;

D O I：

10.1007/s11182-011-9593-4

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The experimental data on the astrophysical S-factor of the p H-2 radiative capture are well described for energies from 1 keV to 10 MeV using the potential cluster model and the Young schemes of orbital cluster state classification with allowance for the E1 and M1 transitions.

引用

页码：157 / 164

页数：8

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