Deep sub-barrier fusion reactions of the light nuclei 12C and 16O

被引：5

作者：

Misicu, S. ^{[1
]}

Carstoiu, F. ^{[1
]}

机构：

[1] NIPNE HH, Dept Theoret Phys, Bucharest 077125, Romania

来源：

NUCLEAR PHYSICS A | 2010年 / 834卷 / 1-4期

关键词：

D O I：

10.1016/j.nuclphysa.2009.12.033

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：

Fusion reactions relevant for the carbon and oxygen burning cycles in highly evolved stars are investigated in a standard approach to fusion. We employ the double folding method to evaluate the ion-ion interactions with Gogny-D1 and M3Y-Paris n - n effective forces. The cross-section evaluation do not indicate a possible hindrance even at the lowest energies under the barrier. Reaction rates at temperatures relevant for the stellar processes are estimated and compared to the traditional and modern extrapolation formulas.

引用

页码：180C / 182C

页数：3

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