Synchrotron radiation in a curved space-time

Details Synchrotron radiation in a curved space-time Synchrotron radiation in a curved space-time

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983fiz....26...37s&link_type=abstract

Fizika, vol. 26, Jan. 1983, p. 37-42. In Russian.

Astronomy and Astrophysics

Astronomy

Particle Motion, Relativistic Particles, Space-Time Functions, Synchrotron Radiation, Astronomical Coordinates, Maxwell Equation, Particle Emission, Quantum Theory, Spectral Energy Distribution

Scientific paper

The method of local coordinates is used to examine synchrotron radiation from ultrarelativistic particles moving in a magnetic field in a curved space-time. General invariant formulas are obtained for the radiation spectrum in the classical and quantum cases. It is shown that the relative value of quantum corrections to the radiation spectrum increases as the particle moves close to the event horizon in the Kerr metric. The limiting transition to the regime of geodesic synchrotron radiation is considered.

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