dc.contributorUniversidade Federal Fluminense (UFF)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniv Coimbra
dc.date.accessioned2014-05-20T15:30:07Z
dc.date.accessioned2022-10-05T16:57:28Z
dc.date.available2014-05-20T15:30:07Z
dc.date.available2022-10-05T16:57:28Z
dc.date.created2014-05-20T15:30:07Z
dc.date.issued2004-08-01
dc.identifierInternational Journal of Modern Physics D. Singapore: World Scientific Publ Co Pte Ltd, v. 13, n. 7, p. 1447-1451, 2004.
dc.identifier0218-2718
dc.identifierhttp://hdl.handle.net/11449/39568
dc.identifier10.1142/S0218271804005675
dc.identifierWOS:000224485500042
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3910653
dc.description.abstractWe show that relativistic mean fields theories with scalar S, and vector V, quadratic radial potentials can generate a harmonic oscillator with exact pseudospin symmetry and positive energy bound states when S = -V. The eigenenergies are quite different from those of the non-relativistic harmonic oscillator. We also discuss a mechanism for perturbatively breaking this, symmetry by introducing a tensor potential. Our results shed light into the intrinsic relativistic nature of the pseudospin symmetry, which might be important in high density systems such as neutron stars.
dc.languageeng
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relationInternational Journal of Modern Physics D
dc.relation2.171
dc.relation1,079
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectpseudospin symmetry
dc.subjectharmonic oscillator
dc.subjecttensor potential
dc.titlePerturbative breaking of the pseudospin symmetry in the relativistic harmonic oscillator
dc.typeArtigo


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