{ "id": "2306.00960", "version": "v1", "published": "2023-06-01T17:55:08.000Z", "updated": "2023-06-01T17:55:08.000Z", "title": "Hard X-ray emission from blazars associated with high-energy neutrinos", "authors": [ "A. V. Plavin", "R. A. Burenin", "Y. Y. Kovalev", "A. A. Lutovinov", "A. A. Starobinsky", "S. V. Troitsky", "E. I. Zakharov" ], "comment": "9 pages, 8 figures, 2 tables; submitted to MNRAS", "categories": [ "astro-ph.HE", "astro-ph.GA" ], "abstract": "Bright blazars were found to be prominent neutrino sources, and a number of IceCube events were associated with them. Evaluating high-energy photon emission of such blazars is crucial for better understanding of the processes and regions where neutrinos are produced. Here, we focus on hard X-ray emission observed by the SRG/ART-XC telescope, by the Swift/BAT imager, and by the INTEGRAL/IBIS telescope. Their energy range ~10 keV and above is well-suited for probing photons that potentially participate in neutrino production by interacting with ultrarelativistic protons. We find that neutrino-associated blazars tend to demonstrate remarkably strong X-ray emission compared to other VLBI blazars in the sky, chance coincidence probability is p=0.5%. Both neutrinos and hard X-rays are found to come from blazars at cosmological distances z ~ 1, and are boosted by relativistic beaming that makes it possible to detect them on Earth. Our results suggest that neutrinos are produced within compact blazar jets, with target X-ray photons emitted from accelerated jet regions.", "revisions": [ { "version": "v1", "updated": "2023-06-01T17:55:08.000Z" } ], "analyses": { "keywords": [ "hard x-ray emission", "high-energy neutrinos", "demonstrate remarkably strong x-ray emission", "target x-ray photons", "prominent neutrino sources" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }