Phys. Rev. D 72, 027501 (2005) [4 pages]Late-time evolution of charged massive Dirac fields in the Reissner-Nordströmblack-hole backgroundReceived 31 August 2004; published 5 July 2005 The late-time evolution of the charged massive Dirac fields in the background of a Reissner-Norström (RN) black hole is studied. It is found that the intermediate late-time behavior is dominated by an inverse power-law decaying tail without any oscillation in which the dumping exponent depends not only on the multiple number of the wave mode but also on the field parameters. It is also found that, at very late times, the oscillatory tail has the decay rate of t-5/6 and the oscillation of the tail has the period 2π/μ which is modulated by two types of long-term phase shifts. © 2005 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevD.72.027501
DOI:
10.1103/PhysRevD.72.027501
PACS:
04.70.Bw, 03.65.Pm, 04.30.Nk, 97.60.Lf
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