Electromagnetic wave tails on curved spacetime and their observational implications

Details Electromagnetic wave tails on curved spacetime and their observational implications Electromagnetic wave tails on curved spacetime and their observational implications

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000phrvd..62d1501m&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 62, Issue 4, 15 August 2000, id.041501

Physics

3

Classical General Relativity, Relativity And Gravitation

Scientific paper

We calculate the tail term of the electromagnetic potential of a pulsed source in arbitrary bounded motion in a weak gravitational field using a higher-order Green's function approach and demonstrate that generally the received radiation tail arrives after a time delay which represents geometrical backscattering by the central gravitational source. We apply the results to a compact binary system and conclude that under certain conditions the tail energy can be a noticeable fraction of the direct pulse energy.

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