Scattering from compact objects: Regge poles and the complex angular momentum method

被引:10
|
作者
El Hadj, Mohamed Ould [1 ,2 ,3 ]
Stratton, Tom [3 ]
Dolan, Sam R. [3 ]
机构
[1] CNRS, Equipe Phys Theor, SPE, UMR 6134, BP 52, F-20250 Corte, France
[2] Univ Corse, Fac Sci, BP 52, F-20250 Corte, France
[3] Univ Sheffield, Consortium Fundamental Phys, Sch Math & Stat, Hicks Bldg,Hounsfield Rd, Sheffield S3 7RH, S Yorkshire, England
基金
欧盟地平线“2020”; 英国工程与自然科学研究理事会; 英国科学技术设施理事会;
关键词
SCHWARZSCHILD BLACK-HOLE; MASSLESS SCALAR WAVES; QUASI-NORMAL MODES; NONRADIAL OSCILLATIONS; GRAVITATIONAL-RADIATION; PULSATION; STARS;
D O I
10.1103/PhysRevD.101.104035
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We calculate the Regge poles of the scattering matrix for a gravitating compact body, for scalar fields and for gravitational waves in the axial sector. For a neutron-starlike body, the spectrum exhibits two distinct branches of poles, labeled surface waves and broad resonances; for ultracompact objects, the spectrum also includes a finite number of narrow resonances. We show, via a WKB analysis, that the discontinuity of the effective potential at the body's surface determines the imaginary component of the broad-resonance poles. Next, we examine the role of Regge poles in the time-independent scattering of monochromatic planar waves. We apply complex angular momentum techniques to re-sum the partial wave series for the scattering amplitude, expressing it as a residue series evaluated at poles in the first quadrant, accompanied by a background integral. We compute the scattering cross section at several frequencies, and show precise agreement with the partial-wave calculations. Finally, we show that compact bodies naturally give rise to orbiting, glory, and rainbow-scattering interference effects.
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页数:18
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