Phys.Rev. C 89, 012801 (2014)

B.Guo, Z.H.Li, Y.J.Li, J.Su, D.Y.Pang, S.Q.Yan, Z.D.Wu, E.T.Li, X.X.Bai, X.C.Du, Q.W.Fan, L.Gan, J.J.He, S.J.Jin, L.Jing, L.Li, Z.C.Li, G.Lian, J.C.Liu, Y.P.Shen, Y.B.Wang, X.Q.Yu, S.Zeng, L.Y.Zhang, W.J.Zhang, W.P.Liu

Spectroscopic factors for low-lying ¹⁶N levels and the astrophysical ¹⁵N(n, γ)¹⁶N

NUCLEAR REACTIONS ¹⁵N(⁷Li, ⁶Li)¹⁶N, E=44 MeV; measured ⁶Li spectrum, σ(θ) using Q3D magnetic spectrograph at CIAE's HI-13 tandem accelerator facility. ¹⁶N; deduced levels, J, π, configurations, spectroscopic factors for ground and first three excited states. DWBA analysis. Comparison with shell model calculations. ¹⁵N(n, γ)¹⁶N, at T=0.01-3 GK; deduced astrophysical reaction rates. Comparison with previous experimental and theoretical results.

doi: 10.1103/PhysRevC.89.012801