Study of the 15N(p,γ)16O reaction at the LUNA accelerator with a gas target setup

被引：0

作者：

Caciolli, Antonio ^{[1
]}

机构：

[1] Univ Padua, Padua, Italy

来源：

FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS | 2010年 / 1213卷

关键词：

N-15(p; gamma)O-16; CNO cycle; Direct measurement; Underground accelerator; PROTON CAPTURE; CROSS-SECTION; N-14(P; N-15;

D O I：

10.1063/1.3362571

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The N-15(p,gamma)O-16 reaction links the CN cycle to the NO cycle allowing for the production of the oxygen and fluorine isotopes during the hydrogen burning in novae and AGB stars. This reaction has been intensively studied by the LUNA collaboration. In this contribution the experiment performed using a BGO detector and a windowless gas target setup is described. The measurement of the astrophysical S-factor has been done in the center of mass energy range from 90 keV to 230 keV. The cross section is found to be a factor two lower than previously believed.

引用

页码：192 / 194

页数：3

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