Introduction to experimental nuclear astrophysics

被引:1
作者
Formicola, A. [1 ]
Imbriani, G. [2 ,3 ]
机构
[1] INFN, Lab Nazl Gran Sasso, Via Acitelli 22, I-67100 Laquila, Italy
[2] Univ Napoli Federico II, Dipartimento Fis E Pancini, Naples, Italy
[3] INFN, Naples, Italy
关键词
TOTAL CROSS-SECTION; S-FACTOR; N-14(P; GAMMA)O-15;
D O I
10.1140/epjp/i2019-12497-1
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
.The present contribution aims to present some general features of the experimental approaches in Nuclear Astrophysics. After a general introduction on light elements nucleosynthesis and on how to determine the reaction rates in a stellar environment, we will focus our attention on underground experiments aimed to directly measure nuclear cross sections of astrophysics interest. We will discuss the N-14(p,)O-15 and C-12 + C-12 reactions, underlying the advantages in approaching these measurements in a deep underground laboratory, as the Laboratori Nazionali del Gran Sasso.
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页数:13
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