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Modeling Poynting flux vs. kinetic-energy dominated jets

We present 3D-MHD AMR simulations of Poynting flux dominated (PFD) jets formed by injection of magnetic energy. We compare their evolution with a hydrodynamic jet which is formed by injecting kinetic energy with the same energy flux than the PFD jets. We predict characteristic emission distributions for each of these jets. Current-driven perturbations in PFD jets are amplified by both cooling and rotation for the regimes studied: Shocks and thermal pressure support are weakened by cooling, making the jets more susceptible to kinking. Rotation amplifies the toroidal magnetic field which also exacerbates the kink instability.

preprint2011arXivOpen access
Martín Huarte-EspinosaAdam FrankEric G. Blackman
physics.plasm-phastro-ph.SR
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Martín Huarte-EspinosaAdam FrankEric G. Blackman

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