Evolution of Nuclear Spectra with Nuclear Forces

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dc.creatorWiringa, R. B.
dc.creatorPieper, Steven C.
dc.date2002-07-16
dc.date.accessioned2026-07-07T11:32:39Z
dc.date.available2026-07-07T11:32:39Z
dc.descriptionWe first define a series of NN interaction models ranging from very simple to fully realistic. We then present Green's function Monte Carlo calculations of light nuclei to show how nuclear spectra evolve as the nuclear forces are made increasingly sophisticated. We find that the absence of stable five- and eight-body nuclei depends crucially on the spin, isospin, and tensor components of the nuclear force.
dc.description5 pages, 2 figures, submitted to Phys. Rev. Lett
dc.identifierhttps://arxiv.org/abs/nucl-th/0207050
dc.identifierhttp://arxiv.org/abs/nucl-th/0207050
dc.identifierPhys.Rev.Lett.89:182501,2002
dc.identifierdoi:10.1103/PhysRevLett.89.182501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/197669
dc.subjectNuclear Theory
dc.titleEvolution of Nuclear Spectra with Nuclear Forces
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