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NSR database version of April 27, 2024.

Search: Author = O.S.Khwairakpam

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2020MO18      Phys.Rev. C 101, 044608 (2020)

G.Montagnoli, A.M.Stefanini, C.L.Jiang, G.Colucci, S.Bottoni, D.Brugnara, P.Colovic, L.Corradi, E.Fioretto, F.Galtarossa, A.Goasduff, O.S.Khwairakpam, M.Heine, G.Jaworski, M.Mazzocco, T.Mijatovic, M.Siciliano, F.Scarlassara, S.Szilner, T.Van Patten, I.Zanon

Fusion of ¹²C + ²⁴Mg far below the barrier: Evidence for the hindrance effect

NUCLEAR REACTIONS ¹²C(²⁴Mg, X), E=26-52 MeV; measured evaporation residues (ERs), fusion σ(E) using E-ΔE and time-of-flight telescope for detection of ERs at LNL-Legnaro; deduced S factor, influence of inelastic channels on fusion, hindrance effect with energy threshold. Comparison with coupled channels calculations using the CCFULL code and Woods Saxon (WS) internuclear potential, and with systematics of energy threshold of hindrance for other medium-light systems: ¹²C+¹²C, ¹²C+¹⁶O, ¹⁶O+¹⁶O, ¹²C+³⁰Si, ²⁴Mg+³⁰Si, ²⁸Si+³⁰Si, ¹⁶O+⁷⁶Ge, and ²⁷Al+⁴⁵Sc. Discussed astrophysical significance of reactions in the carbon and oxygen burning stages of heavy stars.

doi: 10.1103/PhysRevC.101.044608
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD8028.