| dc.contributor | Universidade Federal Fluminense (UFF) | |
| dc.contributor | Universidade Estadual Paulista (Unesp) | |
| dc.contributor | Univ Coimbra | |
| dc.date.accessioned | 2014-05-20T15:30:07Z | |
| dc.date.accessioned | 2022-10-05T16:57:28Z | |
| dc.date.available | 2014-05-20T15:30:07Z | |
| dc.date.available | 2022-10-05T16:57:28Z | |
| dc.date.created | 2014-05-20T15:30:07Z | |
| dc.date.issued | 2004-08-01 | |
| dc.identifier | International Journal of Modern Physics D. Singapore: World Scientific Publ Co Pte Ltd, v. 13, n. 7, p. 1447-1451, 2004. | |
| dc.identifier | 0218-2718 | |
| dc.identifier | http://hdl.handle.net/11449/39568 | |
| dc.identifier | 10.1142/S0218271804005675 | |
| dc.identifier | WOS:000224485500042 | |
| dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/3910653 | |
| dc.description.abstract | We 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.language | eng | |
| dc.publisher | World Scientific Publ Co Pte Ltd | |
| dc.relation | International Journal of Modern Physics D | |
| dc.relation | 2.171 | |
| dc.relation | 1,079 | |
| dc.rights | Acesso restrito | |
| dc.source | Web of Science | |
| dc.subject | pseudospin symmetry | |
| dc.subject | harmonic oscillator | |
| dc.subject | tensor potential | |
| dc.title | Perturbative breaking of the pseudospin symmetry in the relativistic harmonic oscillator | |
| dc.type | Artigo | |