Searching for photon-ALPs mixing effects in AGN gamma-ray energy spectra

Abstract

High energy gamma-rays propagating in external magnetic fields may convert into axion-like particles (ALPs). In this case, the observed gamma-ray spectra are modified by the resulting energy-dependent conversion probability. In this study, we use the energy spectra of 20 extra-galactic gamma-ray sources recorded during 10 years of \textit{Fermi}-LAT observations. We define a test statistics based upon the likelihood ratio to test the hypothesis for a spectral model without vs. a model with photon-ALPs coupling. The conversion probability is calculated for fixed values of the mass and two-photon coupling of the pseudo-scalar particle while the external magnetic field is characterized by the additional free parameters length scale $s$ and average field strength $B$. As a consistency check and in order to extend the analysis to include very high energy gamma-ray data, another test statistics is defined with the ${\chi }^2$ method. We find for 18 of the 20 sources a favorable fit, particularly for Markarian~421 and NGC~1275 a significant improvement, with the hypothesis of photon-ALPs coupling in likelihood analysis. The test statistics of the sources are combined and the significance has been estimated $5.3\sigma$ (test statistics summed in local maxima of all sources) and $6.0\sigma$ (global maxima). The significance is estimated from dedicated simulations under the null hypotheses. The locally best-fitting values of $B$ and $s$ fall into the range that is expected for large scale magnetic fields present in relevant astrophysical environments.

40pages, 45figures

References in corpus (10)

• The Milky Way as a Kiloparsec-Scale Axionscope
• Detecting Axion-Like Particles With Gamma Ray Telescopes
• Magnetic Fields in the Center of the Perseus Cluster
• Axion-Like Particles, Cosmic Magnetic Fields and Gamma-Ray Astrophysics
• Discovery of Magnetic Fields Along Stacked Cosmic Filaments as Revealed by Radio and X-Ray Emission
• Photons to axion-like particles conversion in Active Galactic Nuclei
• Magnetic field strength in cosmic web filaments
• Sensitivity of the Cherenkov Telescope Array to the detection of axion-like particles at high gamma-ray opacities
• Detection of magnetic fields in the circumgalactic medium of nearby galaxies using Faraday rotation
• New constraints on the magnetic field in filaments of the cosmic web

Cited by in corpus (2)

• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters