Mapping the proton drip-line up to A=70
| dc.creator | Ormand, W. E. | |
| dc.date | 1997-01-02 | |
| dc.date.accessioned | 2026-07-07T11:11:02Z | |
| dc.date.available | 2026-07-07T11:11:02Z | |
| dc.description | 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. | |
| dc.description | 30 pages, 3 postscript figures, uses RevTex | |
| dc.identifier | https://arxiv.org/abs/nucl-th/9701002 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/9701002 | |
| dc.identifier | Phys.Rev.C55:2407-2417,1997 | |
| dc.identifier | doi:10.1103/PhysRevC.55.2407 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/190962 | |
| dc.subject | Nuclear Theory | |
| dc.title | Mapping the proton drip-line up to A=70 | |
| dc.type | text |