Scattering of massless scalar waves by Reissner-Nordstrom black holes

被引:99
作者
Crispino, Luis C. B. [1 ]
Dolan, Sam R. [2 ]
Oliveira, Ednilton S. [3 ]
机构
[1] Fed Univ Para, Fac Fis, BR-66075110 Belem, PA, Brazil
[2] Univ Coll Dublin, Sch Math Sci, Dublin 4, Ireland
[3] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
来源
PHYSICAL REVIEW D | 2009年 / 79卷 / 06期
关键词
ABSORPTION CROSS-SECTIONS; EMISSION-SPECTRA; UNIVERSALITY; PARTICLE;
D O I
10.1103/PhysRevD.79.064022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
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页数:9
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