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Description of the 17F(p,gamma)18Ne radiative capture reaction in the continuum shell model

R. Chatterjee·J. Okolowicz·M. Ploszajczak
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Abstract

The shell model embedded in the continuum is applied to calculate the astrophysical S-factor and the reaction rate for the radiative proton capture reaction 17F(p,gamma)18Ne. The dominant contribution to the cross-section at very low energies is due to M1 transitions J_i^pi = 2^+ --> J_f^pi = 2_1^+ whose magnitude is controlled by a weakly bound 2_2^+ state at the excitation energy E_x = 3.62 MeV.

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R. Chatterjee, J. Okolowicz, M. Ploszajczak. 2005-09-12. Description of the 17F(p,gamma)18Ne radiative capture reaction in the continuum shell model. https://doi.org/10.1016/j.nuclphysa.2005.10.002

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