Publication Date:
2018-01-04
Description:
Author(s): L. Wagner, S. Akhmadaliev, M. Anders, D. Bemmerer, A. Caciolli, St. Gohl, M. Grieger, A. Junghans, M. Marta, F. Munnik, T. P. Reinhardt, S. Reinicke, M. Röder, K. Schmidt, R. Schwengner, M. Serfling, M. P. Takács, T. Szücs, A. Vomiero, A. Wagner, and K. Zuber The N 14 ( p , γ ) O 15 reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning and thus determines its rate. The precise knowledge of its rate is required to correctly model hydrogen burning in asymptotic giant branch stars. In addition, it is a necessary ingredient for a possible... [Phys. Rev. C 97, 015801] Published Wed Jan 03, 2018
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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