NASA NTRS · 19730039544
Vector and tensor radiation from Schwarzschild relativistic circular geodesics.
Abstract
A technique developed by Regge and Wheeler (1957) is applied in the Schwarzschild background geometry to treat the radiation emitted by a test particle moving at a speed close to the local speed of light in the vicinity of a black hole. An analytic expression is obtained for the gravitational and electromagnetic radiation spectrum of a particle traveling in a highly relativistic orbit around a Schwarzschild blac hole.
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Breuer, R. A., Ruffini, R., Tiomno, J., Vishveshwara, C. V.. 1973-02-15. Vector and tensor radiation from Schwarzschild relativistic circular geodesics.. https://ntrs.nasa.gov/citations/19730039544
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