Resonant Behaviors of Massive Scalar Fields in Black Hole Spacetimes

Details Resonant Behaviors of Massive Scalar Fields in Black Hole Spacetimes Resonant Behaviors of Massive Scalar Fields in Black Hole Spacetimes

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002bhap.conf...89k&link_type=abstract

BLACK HOLE ASTROPHYSICS 2002 . Proceedings of the Sixth APCTP Winter School . Held 9-12 January 2002 in Pohang, Korea. Edited by

Astronomy and Astrophysics

Astrophysics

Scientific paper

We investigate dominant late-time tail behaviors of massive scalar fields in black-hole spacetimes. It is shown that the oscillatory tail of the scalar fields has the decay rate of t-5/6 at asymptotically late times. The physical mechanism by which the asymptotic t-5/6 tail is generated and the relation between the field mass and the time scale when the tail begins to dominate, are discussed in terms of resonance backscattering due to spacetime curvature. We also discuss the universality of the decay law of t-5/6.

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