Slim disks around Kerr black holes revisited

Abstract

We investigate stationary slim accretion disks around Kerr black holes. We construct a new numerical method based on the relaxation technique. We systematically cover the whole parameter space relevant to stellar mass X-ray binaries. We also notice some non-monotonic features in the disk structure, overlooked in previous studies.

arXiv comment12 pages, 11 figures. The relativistic slim accretion disk solutions have been published online at http://users.camk.edu.pl/as/slimdisk. An appendix containing the manual for the data available online has been added to the previous version of the paper

References in corpus (13)

• Advection-Dominated Accretion: A Self-Similar Solution
• Advection-Dominated Accretion: Underfed Black Holes and Neutron Stars
• Thermal Equilibria of Accretion Disks
• Advection-Dominated Accretion and the Black Hole Event Horizon
• Estimating the Spin of Stellar-Mass Black Holes via Spectral Fitting of the X-ray Continuum
• Relativistic Accretion Disk Models of High State Black Hole X-ray Binary Spectra
• Advection Dominated Accretion Flows in the Kerr Metric: I. Basic Equations
• Advection Dominated Accretion Flows Around Kerr Black Holes
• Super-Eddington accretion rates in Narrow Line Seyfert 1 galaxies
• Super-Eddington accretion disc around a Kerr black hole
• Black hole spin in GRS 1915+105
• Accretion disc outbursts: a new version of an old model
• Super-Eddington black hole accretion: Polish doughnuts and slim disks

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