2006/04/30 by A. Neronov, D. V. Semikoz · 5 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Radioactive Decay and Measurement Techniques #astro-ph
paper · pdf · doi:10.1134/s0021364007100013
published as JETPLett.85:473-477,2007 · 4 pages, 2 figures
arxiv created 2007/05/07 · openalex publication_date 2007/07/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
A method is proposed for measuring extragalactic magnetic fields in observations of TeV γ rays from distant sources. Multi-TeV γ rays from these sources interact with the infrared photon background producing secondary electrons and positrons, which can be just slightly deflected by extragalactic magnetic fields before they emit secondary γ rays via inverse Compton scattering of cosmic microwave background photons. Secondary γ rays emitted toward an observer on the Earth can be detected as an extended emission around an initially point source. The energy dependent angular profile of the extended emission is related to the strength of the extragalactic magnetic field along the line of sight. Small magnetic fields B ≤ 10 −12 G in the voids of the large scale structure can be measured in this way.