Nuclear Astrophysics with the Trojan Horse Method

被引：3

作者：

Tumino, A. ^{[1
,2
]}

Spitaleri, C. ^{[2
,3
]}

Lamia, L. ^{[3
]}

Pizzone, R. G. ^{[2
]}

Cherubini, S. ^{[2
,3
]}

Gulino, M. ^{[1
,2
]}

La Cognata, M. ^{[2
]}

Puglia, S. M. R. ^{[2
,3
]}

Rapisarda, G. G. ^{[2
,3
]}

Romano, S. ^{[2
,3
]}

Sergi, M. L. ^{[2
,3
]}

Sparta, R. ^{[2
,3
]}

机构：

[1] Univ Enna Kore, Fac Ingn & Architettura, Enna, Italy

[2] Ist Nazl Fis Nucl, Lab Nazl Sud, I-95129 Catania, Italy

[3] Univ Catania, Dipartimento Fis & Astron, Catania, Italy

来源：

NUCLEAR PHYSICS IN ASTROPHYSICS VI (NPA6) | 2016年 / 665卷

关键词：

CROSS-SECTION; LOW-ENERGY; LI-7(P; ALPHA)ALPHA; LI-6(P;

D O I：

10.1088/1742-6596/665/1/012009

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Trojan Horse Method (THM) represents the indirect path to determine the bare nucleus astrophysical S(E) factor for reactions between charged particles at astrophysical energies. This is done by measuring the quasi free cross section of a suitable three body process. The basic features of the THM will be presented together with some applications to demonstrate its practical use.

引用

页数：8

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