Decay of Dirac Massive Hair in the Background of Spherical Black Hole

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 (8)

• Late time tails of the massive vector field in a black hole background
• Classification of Static Charged Black Holes in Higher Dimensions
• Split fermion quasi-normal modes
• Late-time evolution of charged massive Dirac fields in the Kerr-Newman background
• Decay of massive hair on brane black hole
• 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

Cited by in corpus (10)

• Kerr-Newman black holes with stationary charged scalar clouds
• Echoes of novel black-bounce spacetimes
• Gravitational ringing and superradiant instabilities of the Kerr-like black holes in a dark matter halo
• Radiation processes in the vicinity of non-Schwarzschild and non-Kerr black holes
• Fermionic greybody factors of two and five-dimensional dilatonic black holes
• Late-time evolution of Dirac field around Schwarzschild-quintessence black hole
• Fermionic greybody factors in Schwarzschild acoustic black holes
• Evolution of Massive Scalar Fields in the Spacetime of a Tense Brane Black Hole
• Greybody Factors of Massive Charged Fermionic Fields in a Charged Two-Dimensional Dilatonic Black Hole
• Massive spin-2 and spin-1/2 no hair theorems for stationary axisymmetric black holes