Active Galactic Nuclei as High-Energy Neutrino Sources

[1511.01590] Active Galactic Nuclei as High-Energy Neutrino Sources Skip to main content Search Submit Donate Log in Astrophysics > High Energy Astrophysical Phenomena arXiv:1511.01590 (astro-ph) [Submitted on 5 Nov 2015 ( v1 ), last revised 6 Jul 2016 (this version, v2)] Title: Active Galactic Nuclei as High-Energy Neutrino Sources Authors: Kohta Murase View PDF HTML (experimental) Abstract: Active galactic nuclei (AGN) are believed to be promising candidates of extragalactic cosmic-ray accelerators and sources, and associated high-energy neutrino and hadronic gamma-ray emission has been studied for many years. We review models of high-energy neutrino production in AGN and discuss their implications for the latest IceCube observation of the diffuse neutrino intensity. Comments: 16 pages, 4 figures, invited review article to appear in "Neutrino Astronomy - Current status, future prospects", Eds. T. Gaisser & A. Karle (World Scientific). Some comments included in v2 Subjects: High Energy Astrophysical Phenomena (astro-ph.HE) ; High Energy Physics - Phenomenology (hep-ph) Cite as: arXiv:1511.01590 [astro-ph.HE] (or arXiv:1511.01590v2 [astro-ph.HE] for this version) https://doi.org/10.48550/arXiv.1511.01590 Focus to learn more arXiv-issued DOI via DataCite Journal reference: Neutrino Astronomy, pp.15-31 (2017) Related DOI : https://doi.org/10.1142/9789814759410_0002 Focus to learn more DOI(s) linking to related resources Submission history From: Kohta Murase [ view email ] [v1] Thu, 5 Nov 2015 03:08:34 UTC (1,159 KB) [v2] Wed, 6 Jul 2016 12:58:47 UTC (1,161 KB) Full-text links: Access Paper: View PDF HTML (experimental) TeX Source view license Current browse context: astro-ph.HE < prev | next > new | recent | 2015-11 Change to browse by: astro-ph hep-ph References & Citations INSPIRE HEP SciX Google Scholar Semantic Scholar export BibTeX citation Bookmark Bibliographic Tools Bibliographic and Citation Tools Bibliographic Explorer Toggle Bibliographic Explorer ( What is the Explorer? ) Connected Papers Toggle Connected Papers ( What is Connected Papers? ) Litmaps Toggle Litmaps ( What is Litmaps? ) scite.ai Toggle scite Smart Citations ( What are Smart Citations? ) Code, Data, Media Code, Data and Media Associated with this Article alphaXiv Toggle alphaXiv ( What is alphaXiv? ) Links to Code Toggle CatalyzeX Code Finder for Papers ( What is CatalyzeX? ) DagsHub Toggle DagsHub ( What is DagsHub? ) GotitPub Toggle Gotit.pub ( What is GotitPub? ) Huggingface Toggle Hugging Face ( What is Huggingface? ) ScienceCast Toggle ScienceCast ( What is ScienceCast? ) Demos Demos Replicate Toggle Replicate ( What is Replicate? ) Spaces Toggle Hugging Face Spaces ( What is Spaces? ) Spaces Toggle TXYZ.AI ( What is TXYZ.AI? ) Related Papers Recommenders and Search Tools Link to Influence Flower Influence Flower ( What are Influence Flowers? ) Core recommender toggle CORE Recommender ( What is CORE? ) IArxiv recommender toggle IArxiv Recommender ( What is IArxiv? ) Author Venue Institution Topic About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs . Which authors of this paper are endorsers? | Disable MathJax ( What is MathJax? ) We gratefully acknowledge support from our major funders , member institutions , and all contributors. About · Help · Contact · Subscribe · Copyright · Privacy · Accessibility · Operational Status (opens in new tab)

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