Why is Tin so soft?

dc.creatorPiekarewicz, J.
dc.date2007-05-10
dc.date.accessioned2026-07-07T10:35:50Z
dc.date.available2026-07-07T10:35:50Z
dc.descriptionThe distribution of isoscalar monopole strength in the neutron-even 112-124Sn-isotopes has been computed using a relativistic random-phase-approximation approach. The accurately-calibrated model used here (``FSUGold'') has been successful in reproducing both ground-state observables as well as collective excitations - including the giant monopole resonance (GMR) in 90Zr, 144Sm, and 208Pb. Yet this same model significantly overestimates the GMR energies in the Sn isotopes. It is argued that the question of ``Why is Tin so soft?'' becomes an important challenge to the field and one that should be answered without sacrificing the success already achieved by several theoretical models.
dc.description5 pages, 3 figures to be submitted to PRC
dc.identifierhttps://arxiv.org/abs/0705.1491
dc.identifierhttp://arxiv.org/abs/0705.1491
dc.identifierPhys.Rev.C76:031301,2007
dc.identifierdoi:10.1103/PhysRevC.76.031301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179856
dc.subjectNuclear Theory
dc.subjectNuclear Experiment
dc.titleWhy is Tin so soft?
dc.typetext

Files

Collections