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Mapping the proton drip-line up to A=70

W. E. Ormand
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Abstract

Coulomb energy differences between mirror nuclei with $A \le 70$ are calculated within the framework of the nuclear shell model using an effective Coulomb plus isovector and isotensor interaction. Absolute binding energies for proton-rich nuclei are predicted by adding the calculated Coulomb shifts to experimentally measured binding energies for the neutron-rich mirror. The location of the proton drip-line is investigated, as well as candidates for the exotic decay mode known as di-proton emission. Taking into account the lifetimes of competing decay modes and limits imposed by experimental setups, it is concluded that the best candidates for the observation of correlated di-proton emission are $^{45}$Fe, $^{48}$Ni, and $^{63}$Se.

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W. E. Ormand. 1997-01-02. Mapping the proton drip-line up to A=70. https://doi.org/10.1103/physrevc.55.2407

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