Numerical Simulations of Black Hole Accretion Flows

Details Numerical Simulations of Black Hole Accretion Flows Numerical Simulations of Black Hole Accretion Flows

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprc12005f&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present results of three-dimensional fully general relativistic numerical simulations of accretion flows around black holes. We evolve the flows in a fixed Kerr metric with a range of angular momenta, from non-rotating (Schwarzschild) to maximally rotating. We consider different initial flow geometries including spherical inflow, axisymmetric disks, and non-symmetric (tilted) disks. We discuss some astrophysical implications of our results.

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