We present a systematic numerical study of the propagation of astrophysical magnetized relativistic jets, in the context of resistive relativistic magnetohydrodynamics (RRMHD) simulations. Simulations are obtained with the PLUTO code. We investigated different values and models for the plasma resistivity coefficient, assessing their impact on the level of turbulence, the formation of current sheets and reconnection plasmoid, and the electromagnetic energy content.
Resistive Relativistic Simulations of Astrophysical Jets / Del Zanna L.; Bugli M.; Mignone A.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - ELETTRONICO. - 461:(2024), pp. 0-0. ( 8th High Energy Phenomena in Relativistic Outflows, HEPRO 2023 Institut d'Astrophysique de Paris and Observatoire de Paris, fra 2023).
Resistive Relativistic Simulations of Astrophysical Jets
Del Zanna L.;
2024
Abstract
We present a systematic numerical study of the propagation of astrophysical magnetized relativistic jets, in the context of resistive relativistic magnetohydrodynamics (RRMHD) simulations. Simulations are obtained with the PLUTO code. We investigated different values and models for the plasma resistivity coefficient, assessing their impact on the level of turbulence, the formation of current sheets and reconnection plasmoid, and the electromagnetic energy content.
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