12C(20Ne, 16O)16O α-transfer reaction and astrophysical S-factors at 300keV

Ashok Kumar Mondal, C. Basu,S. Adhikari, C. Bhattacharya,T. K. Rana,S. Kundu,S. Manna,R. Pandey,P. Roy,A. Sen, J. K. Meena, A. K. Saha, J. K. Sahoo,Dipali Basak,Tanmay Bar,Haridas Pai,A. Bisoi, A. K. Mitra,Piyasi Biswas

International Journal of Modern Physics E(2021)

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摘要
The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O reaction has been used for the first time to determine ANC of [Formula: see text]O levels. The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O [Formula: see text]-transfer angular distributions are measured at [Formula: see text][Formula: see text]MeV and used to determine the ANC of the ground, 6.05[Formula: see text]MeV ([Formula: see text]), 6.13[Formula: see text]MeV ([Formula: see text]), 6.92[Formula: see text]MeV ([Formula: see text]) and 7.12[Formula: see text]MeV ([Formula: see text]) states of [Formula: see text]O. The ANC values are [Formula: see text] [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text] and [Formula: see text] [Formula: see text]. Astrophysical S-factors at 300[Formula: see text]keV are extracted [Formula: see text]) keV b and [Formula: see text] keV b[Formula: see text] using these ANC values by R-matrix theory.
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