Synchrotron scalar radiation from a source in ultrarelativistic circular orbits around a Schwarzschild black hole

Details Synchrotron scalar radiation from a source in ultrarelativistic circular orbits around a Schwarzschild black hole Synchrotron scalar radiation from a source in ultrarelativistic circular orbits around a Schwarzschild black hole

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phrvd..77d7503c&link_type=abstract

Physical Review D, vol. 77, Issue 4, id. 047503

Physics

2

Quantum Field Theory In Curved Spacetime, Quantum Aspects Of Black Holes, Evaporation, Thermodynamics, Radiation By Moving Charges

Scientific paper

Using the framework of quantum field theory in curved spacetime, I analyze the synchrotron scalar radiation emitted by a source orbiting a Schwarzschild black hole in both stable and unstable circular orbits. The comparison between the emitted power in Schwarzschild spacetime and the one obtained in Minkowski spacetime assuming Newtonian gravitation is performed. The amount of the emitted radiation which is absorbed by the black hole is also computed.

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