NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = W.Xin Found 2 matches. 2023XI03 Chin.Phys.C 47, 034107 (2023) Impact of the new 12C+12C reaction rate on presupernova nucleosynthesis NUCLEAR REACTIONS 12C(12C, p), (12C, n), (12C, α), E<0.5 MeV; calculated a series of stellar evolution models with the near solar abundance from the zero-age main-sequence through presupernova stages for initial masses of 20 to 40 solar masses; deduced the impact of reaction rates.
doi: 10.1088/1674-1137/aca1ff
2020ZH02 Phys.Lett. B 801, 135170 (2020), Corrigendum Phys.Lett. B 803, 135278 (2020) N.T.Zhang, X.Y.Wang, D.Tudor, B.Bucher, I.Burducea, H.Chen, Z.J.Chen, D.Chesneanu, A.I.Chilug, L.R.Gasques, D.G.Ghita, C.Gomoiu, K.Hagino, S.Kubono, Y.J.Li, C.J.Lin, W.P.Lin, R.Margineanu, A.Pantelica, I.C.Stefanescu, M.Straticiuc, X.D.Tang, L.Trache, A.S.Umar, W.Y.Xin, S.W.Xu, Y.Xu Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies NUCLEAR REACTIONS 12C(13C, p)24Na, E=4.640-10.995 MeV; measured reaction products, Eγ, Iγ; deduced σ, branching ratio, S-factor.
doi: 10.1016/j.physletb.2019.135170
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