Resonance strength measurement at astrophysical energies: The 17O(p,α)14N reaction studied via THM

被引：0
|
作者：
Sergi, M. L. [1 ]
Spitaleri, C. [1 ,2 ]
La Cognata, M. [1 ]
Lamia, L. [2 ]
Pizzone, R. G. [1 ]
Rapisarda, G. G. [2 ,3 ]
Mukhamedzhanov, A. [3 ]
Irgaziev, B. [4 ]
Tang, X. D. [5 ]
Wischer, M. [5 ]
Mrazek, J.
Kroha, V.
机构：
[1] INFN Lab Naz Sud, Catania, Italy
[2] Univ Catania, Dipartimento Fis & Astron, Catania, Italy
[3] Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA
[4] GIK Inst Engn Sci & Technol, Topi, Pakistan
[5] ASCR, Inst Nucl Phys, Rez, Czech Republic
来源：
12TH INTERNATIONAL CONFERENCE ON NUCLEUS-NUCLEUS COLLISIONS 2015 | 2016年 / 117卷
关键词：
D O I：
10.1051/epjconf/201611709016
中图分类号：
TL [原子能技术]; O571 [原子核物理学];
学科分类号：
0827 ; 082701 ;
摘要：
In recent years, the Trojan Horse Method (THM) has been used to investigate the low-energy cross sections of proton-induced reactions on O-17 nuclei, overcoming extrapolation procedures and enhancement effects due to electron screening. We will report on the indirect study of the O-17(p,alpha)N-14 reaction via the Trojan Horse Method by applying the approach developed for extracting the resonance strength of narrow resonance in the ultralow energy region. The mean value of the strengths obtained in the two measurements was calculated and compared with the direct data available in literature.
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页数：4
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