DIRECT PROJECTILE BREAK-UP AND ITS RELATION TO THE ASTROPHYSICALLY RELEVANT FUSION REACTIONS

被引：16

作者：

BERTULANI, CA ^{[1
]}

HUSSEIN, MS ^{[1
]}

机构：

[1] UNIV SAO PAULO,INST FIS,BR-01498 SAO PAULO,BRAZIL

来源：

NUCLEAR PHYSICS A | 1991年 / 524卷 / 02期

基金：

巴西圣保罗研究基金会;

关键词：

D O I：

10.1016/0375-9474(91)90028-5

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 break-up into two pieces of weakly bound nuclei passing by the Coulomb field of a large-Z nucleus can provide useful information on the inverse fusion reactions which are important for the elemental formation in the stars. However, the nuclear interaction complicates considerably the extraction of such information. We make a study of the contributions of the Coulomb and nuclear interaction to the process, showing when the Coulomb break-up prevails and how a reliable separation of multipolarities can be done.

引用

收藏

页码：306 / 320

页数：15

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