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Astrophysical rate of the 11C+p reaction from the Coulomb break-up of a 12N radioactive beam

✍ Scribed by A. Lefebvre; P. Aguer; J. Kiener; G. Bogaert; A. Coc; F. de Oliveira; J.P. Thibaud; D. Disdier; L. Kraus; I. Linck; S. Fortier; J.A. Scarpaci; C. Stephan; L. Tassan-Got; Ph. Eudes; F. Guilbault; Th. Reposeur; C. Grunberg; P. Roussel-Chomaz; F. Attallah


Book ID
107984113
Publisher
Elsevier Science
Year
1995
Tongue
English
Weight
975 KB
Volume
592
Category
Article
ISSN
0375-9474

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The 19Ne(p,Ξ³)20Na astrophysical reaction
✍ G. Vancraeynest; C.R. Bain; F. Binon; R. Coszach; T. Davinson; P. Decrock; Th. D πŸ“‚ Article πŸ“… 1997 πŸ› Elsevier Science 🌐 English βš– 503 KB

The 19Ne(p,y)\*% a as well as the '9Ne(d,n)2%a reaction have been studied in inverse kinematics using '"Ne radioactive beams. Upper and lower limits for the '9Ne(p,y)20Na astrophysical reaction rate have been deduced, for the first time on the basis of direct experimental data. It is concluded that