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On the High-Energy Neutrino Emission from Active Galactic Nuclei

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Institute of Physics, University of Szeged, Dóm tér 9, H-6720 Szeged, Hungary
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Max Planck Institute for Radioastronomy, Auf dem Hügel 69, D-53121 Bonn, Germany
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Department of Physics, Karlsruhe Institute for Technology, P.O. Box 3640, D-76021 Karlsruhe, Germany
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Department of Physics & Astronomy, University of Alabama, Tuscaloosa, AL 35487-0324, USA
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Department of Physics & Astronomy, University of Bonn, Regina-Pacis-Weg 3, 53113 Bonn, Germany
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Author to whom correspondence should be addressed.
This paper is an extended version of our paper published in BGL 17: 10th Bolyai-Gauss-Lobachevsky Conference on Non-Euclidean Geometry and its Applications, 20–26 August 2017, Gyöngyös, Hungary
Universe 2018, 4(2), 24; https://doi.org/10.3390/universe4020024
Received: 14 November 2017 / Revised: 17 January 2018 / Accepted: 17 January 2018 / Published: 1 February 2018
We review observational aspects of the active galactic nuclei and their jets in connection with the detection of high-energy neutrinos by the Antarctic IceCube Neutrino Observatory. We propose that a reoriented jet generated by the spin-flipping supermassive black hole in a binary merger is likely the source of such high-energy neutrinos. Hence they encode important information on the afterlife of coalescing supermassive black hole binaries. As the gravitational radiation emanating from them will be monitored by the future LISA space mission, high-energy neutrino detections could be considered a contributor to multi-messenger astronomy. View Full-Text
Keywords: supermassive black holes; gravitational waves; high-energy neutrino emission; active galactic nuclei; relativistic jets supermassive black holes; gravitational waves; high-energy neutrino emission; active galactic nuclei; relativistic jets
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MDPI and ACS Style

Kun, E.; Biermann, P.L.; Britzen, S.; Gergely, L.Á. On the High-Energy Neutrino Emission from Active Galactic Nuclei. Universe 2018, 4, 24.

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