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| Journal Article | PUBDB-2025-05687 |
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2025
EDP Sciences
Les Ulis
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Please use a persistent id in citations: doi:10.1051/0004-6361/202452143 doi:10.3204/PUBDB-2025-05687
Report No.: arXiv:2409.04165
Abstract: The origin of the astrophysical neutrino flux discovered by IceCube remains largely unknown. Several individual neutrino source candidates were observed. Among them is the gamma-ray flaring blazar TXS 0506+056. A similar coincidence of a high-energy neutrino and a gamma-ray flare was found in blazar PKS 0735+178. By modeling the spectral energy distributions of PKS 0735+178, we expect to investigate the physical conditions for neutrino production during different stages of the source activity. We analyze the multi-wavelength data during the selected periods of time. Using numerical simulations of radiation processes in the source, we study the parameter space of one-zone leptonic and leptohadronic models and find the best-fit solutions that explain the observed photon fluxes. We show the impact of model parameter degeneracy on the prediction of the neutrino spectra. We show that the available mutli-wavelength data are not sufficient to predict the neutrino spectrum unambiguously. Still, under the condition of maximal neutrino flux, we propose a scenario in which 0.2 neutrino events are produced during the 50 days flare.
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Preprint
Multi-epoch leptohadronic modeling of neutrino source candidate blazar PKS 0735+178
[10.3204/PUBDB-2026-00219]
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