Photon-axion mixing within the jets of Active Galactic Nuclei and prospects for detection

TL;DR

This paper investigates how photon-axion-like particle mixing within AGN jets affects gamma-ray spectra and assesses the Cherenkov Telescope Array's potential to detect these effects, which could reveal new physics beyond the Standard Model.

Contribution

It models photon-ALP mixing within AGN jets and evaluates CTA's ability to detect signatures, highlighting the importance of considering jet mixing effects for future observations.

Findings

Photon-ALP mixing can significantly alter observed AGN spectra.

CTA has promising prospects to detect photon-ALP mixing signatures.

PKS 2155-304 is identified as the best target for such observations.

Abstract

Very high energy gamma-ray observations of distant active galactic nuclei (AGN) generally result in higher fluxes and harder spectra than expected, resulting in some tension with the level of the extragalactic background light (EBL). If hypothetical axions or axion-like particles (ALPs) were to exist, this tension could be relieved since the oscillation of photons to ALPs would mitigate the effects of EBL absorption and lead to softer inferred intrinsic AGN spectra. In this paper we consider the effect of photon-ALP mixing on observed spectra, including the photon-ALP mixing that would occur within AGN jets. We then simulate observations of three AGN with the Cherenkov Telescope Array (CTA), a next generation gamma-ray telescope, to determine its prospects for detecting the signatures of photon-ALP mixing on the spectra. We conclude that prospects for CTA detecting these signatures or else setting limits on the ALP parameter space are quite promising. We find that prospects are improved if photon-ALP mixing within the jet is properly considered and that the best target for observations is PKS 2155-304.