ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case

G. D’Agata; A. I. Kilic; V. Burjan; J. Mrázek; V. Glagolev; V. Kroha; A. Cassisa; G. L. Guardo; M. La Cognata; L. Lamia; S. Palmerini; R. G. Pizzone; G. G. Rapisarda; S. Romano; M. L. Sergi; R. Spartà; C. Spitaleri; A. Tumino

doi:10.1051/epjconf/202327902002

All issues

Volume 279 (2023)

EPJ Web Conf., 279 (2023) 02002

Abstract

Open Access

Issue		EPJ Web Conf. Volume 279, 2023 Nuclear Physics in Astrophysics – X (NPA-X 2022)


Article Number		02002
Number of page(s)		6
Section		Galactic Chemical Evolution / Presolar Radioactivities
DOI		https://doi.org/10.1051/epjconf/202327902002
Published online		22 March 2023

EPJ Web of Conferences 279, 02002 (2023)
https://doi.org/10.1051/epjconf/202327902002

ANC experiments for nuclear astrophysics: The ²⁶Si(p, γ)²⁷P case

G. D’Agata¹^,2^,3^*, A. I. Kilic³, V. Burjan³, J. Mrázek³, V. Glagolev³, V. Kroha³, A. Cassisa³, G. L. Guardo¹, M. La Cognata¹, L. Lamia¹^,2^,4, S. Palmerini⁵^,6, R. G. Pizzone¹, G. G. Rapisarda¹^,2, S. Romano¹^,2^,4, M. L. Sergi¹^,2, R. Spartà¹, C. Spitaleri¹^,2 and A. Tumino²^,7

¹ INFN Laboratori Nazionali del Sud, Via Santa Sofia 62, 95123, Catania, Italy
² Dipartimento di Fisica e Astronomia, Università degli Studi di Catania, Via S. Sofia, 64, 95123, Catania, Italy
³ Nuclear Physics Institute of the Czech Academy of Sciences, 250 68 Rˇ ež, Czech Republic
⁴ Centro Siciliano di Fisica Nucleare e Struttura della Materia (CSFNSM), Catania 77843, Italy
⁵ Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, via A. Pascoli s/n, 06123, Perugia, Italy
⁶ INFN-sezione di Perugia, via A. Pascoli s/n, 06123, Perugia, Italy
⁷ Facoltà di Ingegneria ed Architettura, Kore University, Viale delle Olimpiadi, 1, I-94100 Enna, Italy

^* e-mail: giuseppe.dagata@dfa.unict.it

Published online: 22 March 2023

Abstract

The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the ²⁶Si(p, γ)²⁷P reaction, studied via the ANC in its extension for mirror nuclei will be discussed.

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