Home > Publications database > Unified thermal model for photohadronic neutrino production in astrophysical sources |
Journal Article | PUBDB-2021-01548 |
; ; ;
2021
IOP
London
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Please use a persistent id in citations: doi:10.1088/1475-7516/2021/07/028 doi:10.3204/PUBDB-2021-01548
Report No.: DESY-21-045; arXiv:2103.16577
Abstract: High-energy astrophysical neutrino fluxes are, for many applications, modeled as simple power laws as a function of energy. While this is reasonable in the case of neutrino production in hadronuclear $pp$ sources, it typically does not capture the behavior in photohadronic $p\gamma$ sources: in that case, the neutrino spectrum depends on the properties of the target photons the cosmic rays collide with and on possible magnetic-field effects on the secondary pions and muons. We show that the neutrino production from known photohadronic sources can be reproduced by a thermal (black-body) target-photon spectrum if one suitably adjusts the temperature, thanks to multi-pion production processes. This allows discussing neutrino production from most known $p\gamma$ sources, such as gamma-ray bursts, active galactic nuclei and tidal disruption events, in terms of a few parameters. We apply this thermal model to study the sensitivity of different classes of neutrino telescopes to photohadronic sources: we classify the model parameter space according to which experiment is most suitable for detection of a specific source class and demonstrate that different experiment classes, such as dense arrays, conventional neutrino telescopes, or radio-detection experiments, cover different parts of the parameter space. Since the model can also reproduce the flavor and neutrino-antineutrino composition, we study the impact on the track-to-shower ratio and the Glashow resonance.
Keyword(s): neutrino: production ; neutrino: detector ; model: thermal ; neutrino: spectrum ; neutrino: flux ; photon: cosmic radiation ; photon hadron ; magnetic field: effect ; gamma ray: burst ; neutrino antineutrino ; temperature ; sensitivity ; black body ; capture ; flavor ; muon ; AGN
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