The Search for High Energy Neutrino Emission from X-ray Bright Seyfert Galaxies with IceCube
Authors/Creators
- 1. Technische Universität München
- 2. IceCube Collaboration
Contributors
- 1. Technische Universität München
- 2. IceCube Collaboration
- 3. University of Nevada, Las Vegas
- 4. Queen's University
-
5.
Michigan State University
Description
Parallel Talk presented at the XX International Workshop on Neutrino Telescopes - Venice 23-27 October 2023
Abstract:
IceCube recently observed neutrino emission from the nearby active Seyfert galaxy NGC 1068 in the TeV energy range. This finding suggests that active galactic nuclei (AGN) could be a source type contributing to the diffuse high-energy astrophysical neutrino flux. The dense environments near the supermassive black holes and the acceleration of cosmic rays in the coronae offer suitable conditions for producing high-energy neutrinos. Such environments can be examined by disk-corona models. In this search, we use disk-corona models to predict the neutrino emission flux from the Seyfert galaxies based on their observed keV X-rays luminosity. In this contribution, we report the results of searches for neutrino emission from X-ray bright Seyfert galaxies using 10 years of IceCube data.
Files
neutel_20231025_seyferts_v2.pdf
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Additional details
Related works
- References
- Publication: 10.1126/science.abg3395 (DOI)
- Publication: arXiv:1904.04226v2 (arXiv)
- Publication: arXiv:2102.04475v2 (arXiv)
- Publication: arXiv:2211.09972v2 (arXiv)