Gravitational wave scattering

Details Gravitational wave scattering Gravitational wave scattering

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980phrvd..22.2331h&link_type=abstract

Physical Review D (Particles and Fields), Volume 22, Issue 10, 15 November 1980, pp.2331-2348

Physics

Optics

15

Scientific paper

We consider scattering of gravitational radiation incident axially on Kerr black holes. A Jeffreys-Wentzel-Kramers-Brillouin formulation applied to a combination of the Teukolsky-Press and Chandrasekhar-Detweiler formalisms allows the integration for relatively large frequencies |Mω|. Many interesting structures arise in the resultant cross sections. These include glories, dips in the cross section "due to" geometrical-optics orbits near the capture orbits, preferential polarization of the scattered wave, and very strong backward scattering when the conditions for superradiance hold.

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