Gamma-rays from rotating black holes

Details Gamma-rays from rotating black holes Gamma-rays from rotating black holes

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...280..848p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 280, May 15, 1984, p. 848-852.

Astronomy and Astrophysics

Astronomy

3

Black Holes (Astronomy), Gamma Ray Spectra, Stellar Mass Accretion, Stellar Temperature, Bremsstrahlung, Gas Density, Integral Equations, Interstellar Gas, Kerr Effects, Pion Beams, Schwarzschild Metric

Scientific paper

The gamma-ray luminosity due to the decay of pions produced during spherical accretion onto rotating black holes has been calculated. The model consists of a Kerr black hole of arbitrary angular momentum surrounded by interstellar gas consisting of completely ionized hydrogen atoms. There is an 80 percent increase in flux as we go from Schwarzschild to the extreme Kerr case.

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