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arXiv · 2411.01640

Intergalactic magnetism in a gamma-ray beam as a model of Porphyrion

A. Neronov·F. Vazza·A. Brandenburg·C. Caprini
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Abstract

We estimate the magnetic field in the jets of the recently discovered 7 Mpc long Porphyrion system. We use non-detection of the system in gamma-rays to derive a lower bound on the co-moving magnetic field strength at the level of ~10 nG. This value is consistent with recent estimates of magnetic fields in the filaments of the Large Scale Structure. We discuss the possibility that, instead of being the extreme case of a radio jet formation scenario, Porphyrion actually traces a very-high-energy gamma-ray beam emitted by an active galactic nucleus. In such a model, jets do not need to spread into the voids of the Large Scale Structure to appear straight on a very large distance range, and several anomalies of the standard radio jet scenarios can be solved at once.

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A. Neronov, F. Vazza, A. Brandenburg, C. Caprini. 2024-11-03. Intergalactic magnetism in a gamma-ray beam as a model of Porphyrion. https://doi.org/10.1051/0004-6361%2F202453099

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