Accretion processes in magnetically and tidally perturbed Schwarzschild black holes

Details Accretion processes in magnetically and tidally perturbed Schwarzschild black holes Accretion processes in magnetically and tidally perturbed Schwarzschild black holes

2011-06-04

arxiv.org/abs/1106.0799v1

Phys.Rev.D84:024018,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

to be published in Phys. Rev. D, 13 pages, 7 figures, 1 table

Scientific paper

10.1103/PhysRevD.84.024018

We study the accretion process in the region of the Preston-Poisson space-time describing a Schwarzschild black hole perturbed by asymptotically uniform magnetic field and axisymmetric tidal structures. We find that the accretion disk shrinks and the marginally stable orbit shifts towards the black hole with the perturbation. The radiation intensity of the accretion disk increases, while the radius where radiation is maximal remains unchanged. The spectrum is blue-shifted. Finally, the conversion efficiency of accreting mass into radiation is decreased by both the magnetic and the tidal perturbations.

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