Transmission Line Analogy for Relativistic Poynting-Flux Jets
R.V.E. Lovelace, P.P. Kronberg

TL;DR
This paper models relativistic Poynting-flux jets as transmission lines, predicting wave propagation, dissipation, and particle acceleration mechanisms that explain observed jet features and high-energy phenomena.
Contribution
It introduces a transmission line analogy for Poynting-flux jets, deriving impedance and telegrapher's equations to describe jet perturbations and energy dissipation.
Findings
Localized disturbances cause dissipation and enhanced synchrotron radiation.
Reflected waves can lead to magnetic breakdown and particle acceleration.
Particles can reach Lorentz factors up to 10^7 in the jet.
Abstract
Radio emission, polarization, and Faraday rotation maps of the radio jet of the galaxy 3C 303 have shown that one knot of this jet carries a {\it galactic}-scale electric current and that it is magnetically dominated. We develop the theory of magnetically dominated or Poynting-flux jets by making an analogy of a Poynting jet with a transmission line or waveguide carrying a net current and having a potential drop across it (from the jet's axis to its radius) and a definite impedance which we derive. Time-dependent but not necessarily small perturbations of a Poynting-flux jet are described by the "telegrapher's equations." These predict the propagation speed of disturbances and the effective wave impedance for forward and backward propagating wave components. A localized disturbance of a Poynting jet gives rise to localized dissipation in the jet which may explain the enhanced…
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