Underground Nuclear Astrophysics: Present and future of the LUNA experiment

被引：0

作者：

Gustavino, Carlo ^{[1
]}

机构：

[1] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

来源：

7TH ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS (RICAP18) | 2019年 / 209卷

关键词：

1ST MEASUREMENT; CROSS-SECTION; S-FACTOR; N-14(P; GAMMA)O-15;

D O I：

10.1051/epjconf/201920901043

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The evolution of celestial bodies is regulated by gravitation and thermonuclear reaction rates, while the Big Bang nucleosynthesis is the result of nuclear processes in a rapidly expanding Universe. The LUNA Collaboration has shown that, by exploiting the ultra low background achievable deep underground, it is possible to study the relevant nuclear processes down to the nucleosynthesis energy inside stars and during the first minutes of Universe. In this paper the main results of LUNA are overviewed, as well as the scientific program the forthcoming 3.5 MV underground accelerator.

引用

页数：4

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