3-D General Relativistic MHD 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.date2002-02-21
dc.date.accessioned2026-07-07T02:02:53Z
dc.date.available2026-07-07T02:02:53Z
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 previous axisymmetric simulations. However, the time to generate the jet is longer than in the 2-D simulations. We expect that due to the additional azimuthal dimension the dynamics of jet formation can be modified.
dc.description4 pages Proc. Oxford Radio Galaxy Workshop ed. R. Laing & K. Blundell (San Francisco: PASP) in press (revised)
dc.identifierhttps://arxiv.org/abs/astro-ph/0202396
dc.identifierhttp://arxiv.org/abs/astro-ph/0202396
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4197
dc.subjectAstrophysics
dc.title3-D General Relativistic MHD Simulations of Generating Jets
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