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Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - NU - Neutrino
Searching for High-Energy Neutrino Emission from TeV Pulsar Wind Nebulae
Q. Liu,* A. Kheirandish
*corresponding author
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Pre-published on: 2019 July 22
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Pulsar wind nebulae (PWNe) are main gamma-ray emitters in the Galactic plane. Although the leptonic scenario is able to explain most PWNe emission well, a hadronic contribution cannot be excluded. High-energy emission raises the possibility that gamma-rays are hadronically produced which inevitably leads to the production of neutrinos. We report a stacking analysis to search for neutrino emission from 35 PWNe that are very-high-energy gamma-ray emitters and the results using 9.5 years of all-sky IceCube data. In the absence of any significant correlation, we set upper limits on the total neutrino emission from those PWNe and constraints on the hadronic component.
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