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

TL;DR

This paper estimates the intergalactic magnetic field in the Porphyrion system using gamma-ray non-detection, suggesting it may be a gamma-ray beam from an active galactic nucleus rather than a traditional radio jet.

Contribution

It introduces a novel interpretation of Porphyrion as a gamma-ray beam, providing magnetic field estimates consistent with large-scale structure observations.

Findings

Magnetic field in Porphyrion estimated at ~10 nG.

Porphyrion may be a gamma-ray beam, not a radio jet.

Model explains jet straightness without spreading.

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.