Phys.Rev. C 106, 025807 (2022)

X.Y.Li, B.Guo, Z.H.Li, Y.J.Li, J.Su, D.Y.Pang, J.J.He, S.Q.Yan, Q.W.Fan, J.C.Liu, L.Gan, Z.Y.Han, E.T.Li, G.Lian, Y.P.Shen, Y.B.Wang, S.Zeng, W.P.Liu

Astrophysical ¹⁵N(n, γ)¹⁶N reaction rate from precision measurement of the ¹⁵N(d, p)¹⁶N angular distributions

NUCLEAR REACTIONS ¹⁵N(d, p), (d, d), E=15 MeV; measured particle spectra, 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 and ADWA analysis. ¹⁵N(n, γ), T=0.01-10 GK; deduced astrophysical reaction rates; calculated σ(E). Comparison with previous experimental results, and with OXBASH shell-model predictions.

doi: 10.1103/PhysRevC.106.025807