Abstract
High-energy neutrinos present the ultimate signature for a cosmic ray accelerator. Galactic sources responsible for acceleration of cosmic ray up to the knee in cosmic ray spectrum will provide a guaranteed, albeit subdominant, contribution to the high-energy cosmic neutrino flux. In this review, we discuss the the prospects for identification of high-energy neutrinos from sources of the very high energy gamma ray emission in the Milky Way. We present the status of the search for point-like and extended emission from these sources, and describe how the results of these studies indicate that neutrino telescopes are closing in on identifying Galactic sources of high-energy neutrinos.
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Notes
Deep Underwater Muon And Neutrino Detector Project.
Antarctic Muon And Neutrino Detector Array.
For a comprehensive history of neutrino astronomy and development of neutrino detectors see Spiering (2012).
High Energy Stereoscopic System.
Very Energetic Radiation Imaging Telescope Array System.
Major Atmospheric Gamma-Ray Imaging Cherenkov.
High Altitude Water Cherenkov.
tevcat.uchicago.edu.
Energetic Gamma Ray Experiment Telescope.
High-Energy-Gamma-Ray Astronomy.
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Acknowledgements
The author would like to thank Francis Halzen, Kohta Murase, and Ibrahim Safa for useful comments and discussions. The author also acknowledges the IGC Postdoctoral Award.
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Kheirandish, A. Identifying Galactic sources of high-energy neutrinos. Astrophys Space Sci 365, 108 (2020). https://doi.org/10.1007/s10509-020-03816-3
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DOI: https://doi.org/10.1007/s10509-020-03816-3