Statistics – Computation
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...277..296h&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 277, Feb. 1, 1984, p. 296-311. Research supported by the U.S. Department of
Statistics
Computation
158
Astronomical Models, Black Holes (Astronomy), Hydrodynamics, Stellar Mass Accretion, Computational Fluid Dynamics, Hydrodynamic Equations, Relativity, Shock Waves, Transonic Flow
Scientific paper
The authors have developed a 2D axisymmetric, general relativistic code to study inviscid hydrodynamic accretion flows in a fixed Kerr black hole gravitational field. In this first of several papers documenting the methods and results, they describe and discuss the hydrodynamic equations in the form used in the code. Certain analytic solutions for shock tubes and special accretion flows are derived; these solutions will form the basis for code testing and calibration.
Hawley John F.
Smarr Larry
Wilson Richard J.
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