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High-Energy Neutrino Fluxes from Hard-TeV BL Lacs

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arxiv 2303.13025 v1 pith:G2UQSTF2 submitted 2023-03-23 astro-ph.HE

classification astro-ph.HE
keywords fluxeshadroniclacsneutrinoblazarsexplainextremeflux
verification ladder T0 review T1 audit T2 compute T3 formal
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Blazars have been pointed out as promising high-energy (HE) neutrinos sources, although the mechanism is still under debate. The blazars with a hard-TeV spectrum, which leptonic models can hardly explain, can be successfully interpreted in the hadronic scenarios. Recently, Aguilar et al. proposed a lepto-hadronic two-zone model to explain the multi-wavelength observations of the six best-known extreme BL Lacs and showed that the hadronic component could mainly interpret very-high-energy (VHE) emission. In this work, we apply this hadronic model to describe the VHE gamma-ray fluxes of 14 extreme BL Lacs and estimate the respective HE neutrino flux from charge-pion decay products. Finally, we compare our result with the diffuse flux observed by the IceCube telescope, showing that the neutrino fluxes from these objects are negligible.

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  1. Blazars Jets and prospects for TeV-PeV neutrinos & gamma-rays through cosmic-ray interactions

    astro-ph.HE 2025-01 conditional novelty 4.0 of 10

    A single-zone model with added proton-proton collisions suggests W Comae and 1ES 1959+650 need hadronic emission, and CTAO sensitivity forecasts show all four BL Lacs are detectable.

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