Perturbative breaking of the pseudospin symmetry in the relativistic harmonic oscillator
arXiv:nucl-th/0410096 · doi:10.1142/S0218271804005675
Abstract
We show that relativistic mean fields theories with scalar, , and vector, , quadratic radial potentials can generate a harmonic oscillator with exact pseudospin symmetry {\it and positive energy bound states} when . 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.
arXiv comment5 pages, 4 figures, uses World Scientific style file. Contribution presented at the International Workshop on Astronomy and Relativistic Astrophysics, Olinda, PE, Brazil, October 12-16, 2003. Published by World Scientific in International Journal of Modern Physics D
References in corpus (1)
Cited by in corpus (10)
- Tensor coupling and pseudospin symmetry in nuclei
- Relating pseudospin and spin symmetries through charge conjugation and chiral transformations: the case of the relativistic harmonic oscillator
- Relativistic and nonrelativistic bound states of the isotonic oscillator by Nikiforov-Uvarov method
- Exact Solution of Dirac Equation with Charged Harmonic Oscillator in Electric Field: Bound States
- Green's function method for the spin and pseudospin symmetries in the single-particle resonant states
- Bounded solutions of neutral fermions with a screened Coulomb potential
- Conservation and breaking of pseudospin symmetry
- Confinement of spinless particles by Coulomb potentials in two-dimensional space-time
- Uniform descriptions of pseudospin symmetries in bound and resonant states
- Unsuitable use of spin and pseudospin symmetries with a pseudoscalar Cornell potential