Detection of distant AGN by MAGIC: the transparency of the Universe to high-energy photons
Marco Roncadelli (1), Alessandro De Angelis (2), Oriana Mansutti (3), ((1) INFN, Sezione di Pavia, Italy, (2) Dipartimento di Fisica, Universita', di Udine, and INAF, INFN, Sezioni di Trieste, Italy, (3) Dipartimento di, Fisica, Universita' di Udine, and INFN, Sezione di Trieste

TL;DR
This paper explains how photon oscillations into axion-like particles in extragalactic magnetic fields can account for the universe's unexpected transparency to high-energy gamma rays, supported by recent blazar observations.
Contribution
It introduces a novel explanation involving axion-like particles for the universe's transparency to gamma rays, reconciling observations with standard blazar emission models.
Findings
Detection of blazar 3C279 supports increased universe transparency.
Photon-axion oscillations can explain gamma-ray spectra.
Predictions testable by current and upcoming gamma-ray detectors.
Abstract
The recent detection of blazar 3C279 by MAGIC has confirmed previous indications by H.E.S.S. that the Universe is more transparent to very-high-energy gamma rays than previously thought. We show that this fact can be reconciled with standard blazar emission models provided photon oscillations into a veri light Axion-Like Particle occur in extragalactic magnetic fields. A quantitative estimate of this effect explains the observed spectrum of 3C279. Our prediction can be tested in the near future by the satellite-borne GLAST detector as well as by the ground-based Imaging Atmospheric Cherenkov Telescpoes H.E.S.S., MAGIC, CANGAROO III, VERITAS and by the Extensive Air Shower arrays ARGO-YBJ and MILAGRO.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Computational Physics and Python Applications
