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Neutron-Spectroscopic Factors for Low-Lying 16N Levels...

Publication Type
Conference Paper
Journal Name
PoS - Proceedings of Science
Publication Date
Volume
N/A
Conference Name
Nuclei in the Cosmos X
Conference Location
Mackinac Island, Michigan, United States of America
Conference Date
-

The magnitude of the 15N(n,gamma )16N reaction rate in asymptotic giant branch stars depends directly on the neutron spectroscopic factors of low-lying 16N levels. A new study of the 15N(d, p)16N reaction is reported populating the ground and first three excited states in 16N. The preliminary spectroscopic factors are near unity as expected from shell model calculations, resolving a longstanding discrepancy with previous experiments. The data and analysis are presented.