From Coulomb excitation cross sections to non-resonant astrophysical rates in three-body systems: Ne case
arXiv:1804.02674 · doi:10.1103/PhysRevC.98.034608
Abstract
Coulomb and nuclear dissociation of Ne on light and heavy targets are studied theoretically. The dipole E1 strength function is determined in a broad energy range including energies of astrophysical interest. Dependence of the strength function on different parameters of the Ne ground state structure and continuum dynamics is analyzed in a three-body model. The discovered dependence plays an important role for studies of the strength functions for the three-body E1 dissociation and radiative capture. The constraints on the configuration mixing in Ne and on -wave interaction in the O+ channel are imposed based on experimental data for Ne Coulomb dissociation on heavy target.
arXiv comment12 pages, 13 figures
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- Three-body vs. dineutron approach to two-neutron radiative capture in He
- Asymptotic normalization coefficient method for two-proton radiative capture