Astrophysical S factors of radiative 3He4He, 3H4He, and 2H4He capture

被引：22

作者：

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

机构：

[1] Natl Acad Sci Republ Kazakstan, Fesenkov Astrophys Inst, Alma Ata 480068, Kazakhstan

来源：

PHYSICS OF ATOMIC NUCLEI | 2010年 / 73卷 / 09期

关键词：

PHASE-SHIFT ANALYSIS; SUPERMULTIPLET POTENTIAL MODEL; THERMONUCLEAR REACTION-RATES; ALPHA-ELASTIC-SCATTERING; LIGHT-NUCLEI; FORBIDDEN STATES; VERTEX CONSTANT; CLUSTER MODEL; CROSS-SECTION; COUPLING-CONSTANTS;

D O I：

10.1134/S1063778810090073

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The possibility of describing the astrophysical S factors for radiative (HeHe)-He-3-He-4 capture at energies of up to 15 keV and radiative (HHe)-H-3-He-4 and (HHe)-H-2-He-4 capture at energies of up 5 keV is considered on the basis of the potential cluster model involving forbidden states.

引用

页码：1526 / 1538

页数：13

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