The Decay of Dirac Hair around a Dilaton Black Hole
arXiv:0801.3130 · doi:10.1103/PhysRevD.77.044034
Abstract
The intermediate and late-time behaviour of a massive Dirac field in the background of static spherically symmetric black hole solutions is investigated. The intermediate asymptotic behaviour of a massive Dirac field depends on the mass parameter as well as the wave number of the mode, while the late time behaviour has a power law decay rate independent of both.
RevTex, 8 pages, to be published in Phys.Rev.D15
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- Evolution of Massive Scalar Fields in the Spacetime of a Tense Brane Black Hole