Phys.Rev. C 87, 015803 (2013)

B.Guo, J.Su, Z.H.Li, Y.B.Wang, S.Q.Yan, Y.J.Li, N.C.Shu, Y.L.Han, X.X.Bai, Y.S.Chen, W.P.Liu, H.Yamaguchi, D.N.Binh, T.Hashimoto, S.Hayakawa, D.Kahl, S.Kubono, J.J.He, J.Hu, S.W.Xu, N.Iwasa, N.Kume, Z.H.Li

Determination of the astrophysical ¹²N(p, γ)¹³O reaction rate from the ²H(¹²N, ¹³O)n reaction and its astrophysical implications

NUCLEAR REACTIONS ²H(¹²N, ¹³O)¹n, E=59 MeV; measured reaction products, energy loss, time-of-flight, differential σ(θ); deduced ANC, astrophysical S factors. ¹²N(p, γ)¹³O, at T₉=0.3-3.0; deduced stellar reaction rate. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.87.015803