Journal Article PUBDB-2025-05687

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Multi-epoch leptohadronic modeling of neutrino source candidate blazar PKS 0735+178

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2025
EDP Sciences Les Ulis

Astronomy and astrophysics 695, A266 () [10.1051/0004-6361/202452143]
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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.

Classification:

Note: A&A 695, A266 (2025). Accepted for publication in A&A

Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
  2. DFG project G:(GEPRIS)445052434 - SFB 1491: Das Wechselspiel der kosmischen Materie - von der Quelle bis zum Signal (445052434) (445052434)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2025
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 Record created 2025-12-17, last modified 2026-01-13


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