Determining the composition of radio plasma via circular polarization: the prospects of the Cygnus A hot spots
Torsten A. En{\ss}lin, Sebastian Hutschenreuter, Gopal-Krishna

TL;DR
This paper explores using circular polarization measurements of radio emission from Cygnus A's hot spots to determine whether the plasma is electron-positron or electron-proton, addressing a longstanding question about jet composition.
Contribution
It proposes a novel observational method to distinguish plasma composition in AGN jets through sensitive CP measurements of radio hot spots.
Findings
Circular polarization is zero for electron-positron plasma.
Electron-proton plasma should exhibit measurable fractional CP.
Measurement of CP at the level of 10^{-3} is challenging but feasible.
Abstract
The composition of the relativistic plasma produced in active galactic nuclei and ejected via powerful jets into the interstellar/intergalactic medium is still a major unsettled issue. It might be a positron-electron plasma in case the plasma was created by pair production in the intense photon fields near accreting super-massive black holes. Alternatively, it might be an electron-proton plasma in case magnetic fields lift and accelerate the thermal gas of accretion discs into relativistic jets as the recent detection of -rays from blazars indicates. Despite various attempts to unambiguously establish the composition of the relativistic jets, this remains a major unknown. Here, we propose a way to settle the question via sensitive measurements of circular polarization (CP) in the radio emission of the hot spots of bright radio galaxies like Cygnus A. The CP of synchrotron…
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