S factor of the 3H(3H,2n)4He and 3He(3He,2p)4He reactions using a three-cluster exit channel -: art. no. 064604

被引：12

作者：

Vasilevsky, V ^{[1
]}

Nesterov, AV

Arickx, F

Broeckhove, J

机构：

[1] Bogolyubov Inst Theoret Phys, Kiev, Ukraine

[2] Univ Antwerp, RUCA, Dept Math & Comp Sci, B-2020 Antwerp, Belgium

来源：

PHYSICAL REVIEW C | 2001年 / 63卷 / 06期

关键词：

D O I：

10.1103/PhysRevC.63.064604

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 reactions H-3(H-3,2n)He-4 and He-3(He-3,2p)He-4 are investigated within a fully microscopic cluster model featuring a three-cluster exit channel. A hyperspherical harmonics basis is used to describe the three-cluster continuum. The resulting astrophysical S factor of both reactions is in good agreement with experimental data. Analysis of the low-energy scattering parameters reveals no evidence for a hidden resonance state that would increase the cross section of the reactions, and would help to resolve the solar neutrino problem.

引用

页数：8

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