Approximative analytical solutions of the Dirac equation in Schwarzschild spacetime
arXiv:gr-qc/0701119 · doi:10.1142/S0217732307024437
Abstract
Approximative analytic solutions of the Dirac equation in the geometry of Schwarzschild black holes are derived obtaining information about the discrete energy levels and the asymptotic behavior of the energy eigenspinors.
8 pages
References in corpus (7)
- Fermion scattering by a Schwarzschild black hole
- Late-time behavior of massive Dirac fields in a Schwarzschild background
- Dirac Quasinormal modes of Schwarzschild black hole
- High overtones of Dirac perturbations of a Schwarzschild black hole
- The Dirac particle on de Sitter background
- The Dirac particle on central backgrounds and the anti-de Sitter oscillator
- The normalized energy eigenspinors of the Dirac field on anti-de Sitter spacetime
Cited by in corpus (10)
- Partial wave analysis of the Dirac fermions scattered from Schwarzschild black holes
- Fermion production in a magnetic field in a de Sitter Universe
- Greybody Radiation of scalar and Dirac perturbations of NUT Black Holes
- Partial wave analysis of the Dirac fermions scattered from Reissner - Nordstr\" om charged black holes
- Scattering of massless fermions by Schwarzschild and Reissner-Nordström black holes
- New modes for massive Dirac field in higher dimensional Black Holes
- Scattering of Dirac fermions by spherical massive bodies
- Fermion scattering by a class of Bardeen black holes
- Quasibound states of the Dirac field in Schwarzschild and Reissner-Nordström black hole backgrounds
- Scattering of quantum fields by a MOG Black Hole