来自硬tev BL lac的高能中微子通量

IF 10.2 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
E. Aguilar-Ruiz, N. Fraija, A. Galván-Gámez
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引用次数: 3

摘要

Blazars被认为是有前景的高能中微子源,尽管其机制仍在争论中。具有硬TeV谱的blazars,轻子模型很难解释,可以在强子场景中成功解释。最近,Aguilar等人提出了一个轻子强子双区模型来解释六个最著名的极端BL Lacs的多波长观测,并表明强子分量主要可以解释甚高能(VHE)发射。在这项工作中,我们应用这个强子模型来描述14个极端BL Lacs的VHE伽马射线通量,并根据电荷-π衰变产物估计相应的HE中微子通量。最后,我们将我们的结果与冰立方望远镜观测到的扩散通量进行了比较,表明这些物体的中微子通量可以忽略不计。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
High-energy neutrino fluxes from hard-TeV BL Lacs

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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来源期刊
Journal of High Energy Astrophysics
Journal of High Energy Astrophysics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
9.70
自引率
5.30%
发文量
38
审稿时长
65 days
期刊介绍: The journal welcomes manuscripts on theoretical models, simulations, and observations of highly energetic astrophysical objects both in our Galaxy and beyond. Among those, black holes at all scales, neutron stars, pulsars and their nebula, binaries, novae and supernovae, their remnants, active galaxies, and clusters are just a few examples. The journal will consider research across the whole electromagnetic spectrum, as well as research using various messengers, such as gravitational waves or neutrinos. Effects of high-energy phenomena on cosmology and star-formation, results from dedicated surveys expanding the knowledge of extreme environments, and astrophysical implications of dark matter are also welcomed topics.
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