Observational Appearance of Magnetic Field Reconnections in Single Black Hole Accretion Flow

Details Observational Appearance of Magnetic Field Reconnections in Single Black Hole Accretion Flow Observational Appearance of Magnetic Field Reconnections in Single Black Hole Accretion Flow

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002bhap.conf..227b&link_type=abstract

BLACK HOLE ASTROPHYSICS 2002 . Proceedings of the Sixth APCTP Winter School . Held 9-12 January 2002 in Pohang, Korea. Edited by

Astronomy and Astrophysics

Astrophysics

Scientific paper

Observational appearance of magnetic field reconnections of spherically-symmetric accretion of magnetized plasma onto a black hole is studied. Spectral and temporal properties of accelerated particles emission are discussed. Total efficiency of such mechanism of gravitational energy-to-radiation conversion is shown to be comparable to efficiency of quasithermal background flow emission. Possible applications of this process to search for single stellar mass black holes are discussed.

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