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 MHD simulations of astrophysical jets
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Pre-published on:
June 18, 2024
Published on:
July 30, 2024
Abstract
DOI: https://doi.org/10.22323/1.461.0073
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.