Loading…

Study of the [sup 13]N([ital d],[ital n])[sup 14]O reaction cross section and its astrophysical implications for the [sup 13]N proton capture reaction

The total cross section for the [sup 13]N([ital d],[ital n])[sup 14]O[sub g.s.] reaction has been measured with [sup 13]N radioactive beams at laboratory energies of 8.2, 12.0, 16.2, and 28.5 MeV. A spectroscopic factor of 0.9 is obtained from a distorted-wave Born approximation analysis of this tra...

Full description

Saved in:
Bibliographic Details
Published in:Physical review. C, Nuclear physics Nuclear physics, 1993-10, Vol.48:4
Main Authors: Decrock, P., Gaelens, M., Huyse, M., Reusen, G., Vancraeynest, G., Van Duppen, P., Wauters, J., Delbar, T., Galster, W., Leleux, P., Licot, I., Lienard, E., Lipnik, P., Michotte, C., Vervier, J., Oberhummer, H.
Format: Article
Language:English
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:The total cross section for the [sup 13]N([ital d],[ital n])[sup 14]O[sub g.s.] reaction has been measured with [sup 13]N radioactive beams at laboratory energies of 8.2, 12.0, 16.2, and 28.5 MeV. A spectroscopic factor of 0.9 is obtained from a distorted-wave Born approximation analysis of this transfer reaction. The astrophysical [ital S] factor for the [sup 13]N([ital p],[gamma])[sup 14]O reaction is calculated using the experimentally known resonance parameters for the resonant contribution and the direct-capture model with the experimental spectroscopic factor for the nonresonant contribution.
ISSN:0556-2813
1089-490X
DOI:10.1103/PhysRevC.48.2057