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Dependence of fusion on isospin dynamics

Kyle GodbeyDepartment of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235, USAA. S. UmarDepartment of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235, USAC. SimenelDepartment of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, Canberra ACT 2601, Australia
2017en
ABI

Аннотация

We introduce a new microscopic approach to calculate the dependence of fusion barriers and cross sections on isospin dynamics. The method is based on the time-dependent Hartree--Fock theory and the isoscalar and isovector properties of the energy density functional (EDF). The contribution to the fusion barriers originating from the isoscalar and isovector parts of the EDF is calculated. It is shown that, for nonsymmetric systems, the isovector dynamics influence the subbarrier fusion cross sections. For most systems this results in an enhancement of the subbarrier cross sections, while for others we observe differing degrees of hindrance. We use this approach to provide an explanation of recently measured fusion cross sections which show a enhancement at low ${E}_{\mathrm{c}.\mathrm{m}.}$ energies for the system $^{40}\mathrm{Ca}+^{132}\mathrm{Sn}$ as compared with the more neutron-rich system $^{48}\mathrm{Ca}+^{132}\mathrm{Sn}$ and discuss the dependence of subbarrier fusion cross sections on transfer.

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