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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...
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Published in: | Physical review. C, Nuclear physics Nuclear physics, 1993-10, Vol.48:4 |
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Main Authors: | , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
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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. |
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ISSN: | 0556-2813 1089-490X |
DOI: | 10.1103/PhysRevC.48.2057 |