Statistics – Computation
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.8113r&link_type=abstract
American Astronomical Society Meeting 203, #81.13; Bulletin of the American Astronomical Society, Vol. 35, p.1333
Statistics
Computation
Scientific paper
We present our computational results for the formation of relativistic jets using a three-dimensional general relativistic MHD simulation method. Our goal is to study the dynamics of an accretion disk with a magnetic field, and the associated formation of relativistic jets in the environment around a black hole. We present and compare our 2-D and 3-D simulation results, which demonstrate the initial stages of jet formation.
This project was funded in part by the National Research Council, Research Associateship program.
Nishikawa Ken-Ichi
Richardson Georgia A.
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