3-D GRMHD and GRPIC Simulations of Disk-Jet Coupling and Emission

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dc.creatorNishikawa, K. -I.
dc.creatorMizuno, Y.
dc.creatorWatson, M.
dc.creatorHardee, P.
dc.creatorFuerst, S.
dc.creatorWu, K.
dc.creatorFishman, G. J.
dc.date2006-12-12
dc.date.accessioned2026-07-07T07:31:08Z
dc.date.available2026-07-07T07:31:08Z
dc.descriptionWe investigate jet formation in black-hole systems using 3-D General Relativistic Particle-In-Cell (GRPIC) and 3-D GRMHD simulations. GRPIC simulations, which allow charge separations in a collisionless plasma, do not need to invoke the frozen condition as in GRMHD simulations. 3-D GRPIC simulations show that jets are launched from Kerr black holes as in 3-D GRMHD simulations, but jet formation in the two cases may not be identical. Comparative study of black hole systems with GRPIC and GRMHD simulations with the inclusion of radiate transfer will further clarify the mechanisms that drive the evolution of disk-jet systems.
dc.description3 pages, 1 figure, Proceedings of the Eleventh Marcel Grossmann Meeting on General Relativity, edited by H. Kleinert, R.T. Jantzen and R. Ruffini, World Scientific, Singapore, 2007
dc.identifierhttps://arxiv.org/abs/astro-ph/0612328
dc.identifierhttp://arxiv.org/abs/astro-ph/0612328
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118643
dc.subjectAstrophysics
dc.title3-D GRMHD and GRPIC Simulations of Disk-Jet Coupling and Emission
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