Resonance and absorption spectra of the Schwarzschild black hole for massive scalar perturbations: A complex angular momentum analysis

被引:41
作者
Decanini, Yves [1 ,2 ]
Folacci, Antoine [1 ,2 ,3 ,4 ,5 ,6 ]
Raffaelli, Bernard [1 ,2 ]
机构
[1] CNRS, UMR 6134, SPE, Equipe Phys Theor, F-20250 Corte, France
[2] Univ Corse, Fac Sci, F-20250 Corte, France
[3] CNRS, Ctr Phys Theor, UMR 6207, F-13288 Marseille, France
[4] Univ Aix Marseille 1, F-13288 Marseille, France
[5] Univ Aix Marseille 2, F-13288 Marseille, France
[6] Univ Sud Toulon Var, CNRS Luminy Case 907, F-13288 Marseille, France
来源
PHYSICAL REVIEW D | 2011年 / 84卷 / 08期
关键词
QUASI-NORMAL MODES; EMISSION-SPECTRA; CROSS-SECTIONS; BOUND-STATES; WKB APPROACH; QUANTUM; SCATTERING; FIELD; WAVES; DECAY;
D O I
10.1103/PhysRevD.84.084035
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We reexamine some aspects of scattering by a Schwarzschild black hole in the framework of complex angular momentum techniques. More precisely, we consider, for massive scalar perturbations, the high-energy behavior of the resonance spectrum and of the absorption cross section by emphasizing analytically the role of the mass. This is achieved (i) by deriving asymptotic expansions for the Regge poles of the S-matrix and then for the associated weakly damped quasinormal frequencies and (ii) by taking into account the analytic structure of the greybody factors which allows us to extract by resummation the physical information encoded in the absorption cross section.
引用
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页数:14
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