Decay of Dirac Massive Hair in the Background of Spherical Black Hole
arXiv:0805.0665 · doi:10.1103/PhysRevD.77.124007
Abstract
The intermediate and late-time behaviour of massive Dirac hair in the static spherically symmetric black hole spacetime was studied. It was revealed that the intermediate asymptotic pattern of decay of massive Dirac spinor hair is dependent on the mass of the field under consideration as well as the multiple number of the wave mode. The long-lived oscillatory tail observed at timelike infinity in the considered background decays slowly as t^{-5/6}.
8 pages, 5 figures, RevTex, to be published in Phys.Rev.D15
References in corpus (5)
- Split fermion quasi-normal modes
- Late-time evolution of charged massive Dirac fields in the Kerr-Newman background
- Influence of Lorentz violation on Dirac quasinormal modes in the Schwarzschild black hole spacetime
- Fermion excitations of a tense brane black hole
- Decay of massive scalar hair in the background of a dilaton gravity black hole