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Determination of alpha spectroscopic factors for unbound 17O states

De Séréville, Nicolas; Meyer, Anne; Hammache, Faïrouz; Laird, Alison M.; Pignatari, Marco

Authors

Nicolas De Séréville

Anne Meyer

Faïrouz Hammache

Alison M. Laird

Marco Pignatari



Contributors

M. La Cognata
Editor

M. Lattuada
Editor

S. Palmerini
Editor

R.G. Pizzone
Editor

C. Spitaleri
Editor

Abstract

© The Authors, published by EDP Sciences, 2017. It has been recently suggested that hydrogen ingestion into the helium shell of massive stars could lead to high 13 C and 15 N excesses when the blast of a core collapse supernova (ccSN) passes through its helium shell. This prediction questions the origin of extremely high 13 C and 15 N abundances observed in rare presolar SiC grains which is usually attributed to classical novae. In this context the 13 N(α,p) 16 O reaction plays an important role since it is in competition with 13 N β + -decay to 13 C. As a first step to the determination of the 13 N(α,p) 16 O reaction rate, we present a study aiming at the determination of alpha spectroscopic factors of 17 O states which are the analog ones to those in 17 F, the compound nucleus of the 13 N(α,p) 16 O reaction.

Citation

De Séréville, N., Meyer, A., Hammache, F., Laird, A. M., & Pignatari, M. (2017). Determination of alpha spectroscopic factors for unbound 17O states. EPJ Web of Conferences, 165, 01022. https://doi.org/10.1051/epjconf/201716501022

Journal Article Type Article
Acceptance Date Dec 30, 2017
Online Publication Date Dec 30, 2017
Publication Date Dec 30, 2017
Deposit Date Jun 28, 2018
Publicly Available Date Jul 3, 2018
Journal EPJ Web of Conferences
Print ISSN 2100-014X
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 165
Article Number 01022
Pages 01022
ISBN 9782759890309
DOI https://doi.org/10.1051/epjconf/201716501022
Public URL https://hull-repository.worktribe.com/output/745948
Publisher URL https://www.epj-conferences.org/articles/epjconf/abs/2017/34/epjconf_npa82017_01022/epjconf_npa82017_01022.html
Contract Date Jun 28, 2018

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Copyright Statement
© The Authors, published by EDP Sciences, 2017.

This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).






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