Phys.Rev. C 83, 045804 (2011)

M.Marta, A.Formicola, D.Bemmerer, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, A.Lemut, B.Limata, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero, for the LUNA Collaboration

The ¹⁴N( p, γ )¹⁵O reaction studied with a composite germanium detector

NUCLEAR REACTIONS ¹⁴N(p, γ), E=359, 380, 399 keV; measured Eγ, Iγ, σ. ¹⁵O; deduced levels, J, π, branching ratios for four major resonances, corresponding astrophysical S factors. R-matrix analysis for capture to ground state. Relevance to (CNO) cycle of hydrogen burning.

doi: 10.1103/PhysRevC.83.045804