Computational Relativistic Fluids and Jet Formation

Details Computational Relativistic Fluids and Jet Formation Computational Relativistic Fluids and Jet Formation

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..286r&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 286-289 (2004).

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Magnetohydrodynamics And Plasmas, Relativity And Gravitation

Scientific paper

We present our methodology for numerically solving the fluid equations in general relativistic environments with magnetic fields. Our motivation for the development of such a method is to study the environment around a rotating black hole, specifically the dynamics of the accretion disk and the associated formation of relativistic jets. We present our three-dimensional results confirming previous two-dimensional simulations, which demonstrate the initial stages of jet formation. Without injecting matter, the generated jet evolves into a wind. Consequently, a state change of the jet and accretion disk system is observed.

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