3-D GRMHD Simulations of Generating Jets

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dc.creatorNishikawa, K. -I.
dc.creatorKoide, S.
dc.creatorShibata, K.
dc.creatorKudoh, T.
dc.creatorSol, H.
dc.date2002-08-05
dc.date.accessioned2026-07-07T02:04:35Z
dc.date.available2026-07-07T02:04:35Z
dc.descriptionWe have performed a first fully 3-D GRMHD simulation with Schwarzschild black hole with a free falling corona. The initial simulation results show that a jet is created as in the previous simulations using the axisymmetric geometry with the mirror symmetry at the equator. However, the time to generate the jet is longer than in the 2-D axisymmetric simulations. We expect that due to the additional freedom in the azimuthal dimension without axisymmetry with respect to the z axis and reflection symmetry with respect to the equatorial plane, the dynamics of jet formation can be modified. Further simulations are required for the study of instabilities along the azimuthal direction such as accretion-eject instability
dc.description4 pages, 1 fig (color), Proc. 4th Microquasar Workshop, 2002; Proceedings of the 4th Microquasar Workshop, 2002, eds. Durouchoux, Fuchs & Rodriguez, published by the Center for Space Physics: Kolkata
dc.identifierhttps://arxiv.org/abs/astro-ph/0208092
dc.identifierhttp://arxiv.org/abs/astro-ph/0208092
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4811
dc.subjectAstrophysics
dc.title3-D GRMHD Simulations of Generating Jets
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