3 years ago

Astrophysical $S$ factor of the $^{14}\mathrm{N}(p,γ)^{15}\mathrm{O}$ reaction at 0.4–1.3 MeV

Astrophysical $S$ factor of the $^{14}\mathrm{N}(p,γ)^{15}\mathrm{O}$ reaction at 0.4–1.3 MeV
D. Bemmerer, A. Wagner, M. P. Takács, T. Szücs, R. Schwengner, K. Zuber, A. Vomiero, F. Munnik, L. Wagner, M. Röder, M. Serfling, S. Reinicke, A. Caciolli, K. Schmidt, T. P. Reinhardt, S. Akhmadaliev, M. Grieger, St. Gohl, M. Marta, A. Junghans, M. Anders
The $^{14}\mathrm{N}(p,γ)\phantom{\rule{0.16em}{0ex}}^{15}\mathrm{O}$ 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...

Publisher URL: http://link.aps.org/doi/10.1103/PhysRevC.97.015801

DOI: 10.1103/PhysRevC.97.015801

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