Nuclear Shell Effects near the r-Process Path at N=82 in the Relativistic Hartree-Bogoliubov Theory

dc.creatorSharma, M. M.
dc.creatorFarhan, A. R.
dc.date2000-06-21
dc.date.accessioned2026-07-07T05:38:07Z
dc.date.available2026-07-07T05:38:07Z
dc.descriptionEvolution of the shell structure of nuclei near the neutron drip line is investigated in the Relativistic Hartree-Bogoliubov (RHB) theory. By introducing the vector self-coupling of $ω$ meson in the RHB theory, we reproduce successfully the experimental data on the shell effects about the waiting-point nucleus $^{80}$Zn. With this basis, it is shown that the shell effects at N=82 in the inaccessible region of the r-process path remain strong. In contrast, a quenching exhibited by the HFB+SkP approach is shown to be incompatible with the available data. Consequently, the neutrino-driven mechanism of the nucleosynthesis is supported.
dc.description5 page revtex, 3 ps figures, submitted tp Phys. Rev. Lett
dc.identifierhttps://arxiv.org/abs/nucl-th/0006046
dc.identifierhttp://arxiv.org/abs/nucl-th/0006046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/81506
dc.subjectNuclear Theory
dc.titleNuclear Shell Effects near the r-Process Path at N=82 in the Relativistic Hartree-Bogoliubov Theory
dc.typetext

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