ANC experiments for nuclear astrophysics

被引：0

作者：

D'Agata, G. ^{[1
]}

Burjan, V. ^{[1
]}

Mrazek, J. ^{[1
]}

Glagolev, V ^{[1
]}

Kilic, A. I. ^{[1
]}

Kroha, V. ^{[1
]}

La Cognata, M. ^{[2
]}

Lamia, L. ^{[2
,3
]}

Palmerini, S. ^{[4
,5
]}

Piskor, S. ^{[1
]}

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

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

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

Sivacek, I. ^{[1
]}

Spitaleri, C. ^{[2
]}

Sparta, R. ^{[2
]}

Tumino, A. ^{[2
,6
]}

机构：

[1] Czech Acad Sci, Nucl Phys Inst, Rez 25068, Czech Republic

[2] INFN Lab Nazl Sud, Via Santa Sofia 62, I-95123 Catania, Italy

[3] Univ Catania, Dipartimento Fis & Astron, Via S Sofia 64, I-95123 Catania, Italy

[4] Univ Perugia, Dipartimento Fis & Geol, Via A Pascoli S-N, I-06123 Perugia, Italy

[5] INFN Sez Perugia, Via A Pascoli S-N, I-06123 Perugia, Italy

[6] Kore Univ, Fac Ingn Architettura, Viale Olimpiadi 1, I-94100 Enna, Italy

来源：

10TH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS, 2019 | 2020年 / 227卷

关键词：

S-FACTOR; NORMALIZATION;

D O I：

10.1051/epjconf/202022701003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Among the indirect methods to determine nuclear cross-section present in literature, the so-called Asymptotic Normalization Coefficient (ANC) has proven to be useful in retrieving the direct part of a radiative capture cross-section in reactions of interest for astrophysics. In this work, the method will be presented, and some results obtained in collaboration between NPI CAS and INFN-LNS will be presented.

引用

页数：6

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