Charge density of light exotic nuclei and $ρNN$ tensor coupling

dc.creatorJiang, W. Z.
dc.creatorZhao, Y. L.
dc.date2006-02-16
dc.date.accessioned2026-07-07T11:28:21Z
dc.date.available2026-07-07T11:28:21Z
dc.descriptionWe use a relativistic mean field model to study the charge density distributions of exotic oxygen isotopes. Nonlinear isoscalar-isovector terms which are not constrained by the present data are considered and the $ρNN$ tensor coupling that does not affect the symmetry energy in the mean field model is included. Strong correlations between the neutron radius of $^{208}$Pb and the charge radius of $^{12,13,23,24}$O are found. The $ρNN$ tensor coupling explicitly enhances the radius correlations between $^{23,24}$O and $^{208}$Pb. This enhancement is due to the neutron occupation of the orbital $2s_{1/2}$. The charge radius is sensitive to the change of the density dependence of the symmetry energy as the isotope goes towards the proton drip line.
dc.description13 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0602049
dc.identifierhttp://arxiv.org/abs/nucl-th/0602049
dc.identifierPhys.Lett.B617:33,2005
dc.identifierdoi:10.1016/j.physletb.2005.04.055
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196415
dc.subjectNuclear Theory
dc.subjectNuclear Experiment
dc.titleCharge density of light exotic nuclei and $ρNN$ tensor coupling
dc.typetext

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