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Phys. Rev. D 79, 064022 (2009) [9 pages]

Scattering of massless scalar waves by Reissner-Nordström black holes

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Luís C. B. Crispino*
Faculdade de Física, Universidade Federal do Pará, 66075-110, Belém, PA, Brazil

Sam R. Dolan
School of Mathematical Sciences, University College Dublin, Belfield, Dublin 4, Ireland

Ednilton S. Oliveira
Instituto de Física, Universidade de São Paulo, CP 66318, 05315-970, São Paulo, SP, Brazil

Received 9 January 2009; published 20 March 2009

We present a study of scattering of massless planar scalar waves by a charged nonrotating black hole. Partial wave methods are applied to compute scattering and absorption cross sections, for a range of incident wavelengths. We compare our numerical results with semiclassical approximations from a geodesic analysis, and find excellent agreement. The glory in the backward direction is studied, and its properties are shown to be related to the properties of the photon orbit. The effects of the black hole charge upon scattering and absorption are examined in detail. As the charge of the black hole is increased, we find that the absorption cross section decreases, and the angular width of the interference fringes of the scattering cross section at large angles increases. In particular, the glory spot in the backward direction becomes wider. We interpret these effects under the light of our geodesic analysis.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.79.064022
DOI:
10.1103/PhysRevD.79.064022
PACS:
04.40.−b, 04.70.−s, 11.80.−m

*crispino@ufpa.br

sam.dolan@ucd.ie

ednilton@fma.if.usp.br