Abstract
highly relativistic acceleration of magnetically driven jets, withinthe framework of ideal MHD for cold, stationary, and axisymmetricoutflows,closed-form expression for the transition from a magneticallydominated flow to a kinetic-energy-dominated one,equipartition between magnetic and kinetic energies is realized ata cylindrical radius of the order of RL E/c2,the transverse width of jet after the initial accelerationis of order gamma x 2RL, (with Lorentz factor gamma and light cylinderradius RL)
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CITATION STYLE
Tomimatsu, A., & Takahashi, M. (2003). Relativistic Acceleration of Magnetically Driven Jets. The Astrophysical Journal, 592(1), 321–331. https://doi.org/10.1086/375579
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