TY - JOUR
T1 - High-energy neutrino flux from individual blazar flares
AU - Oikonomou, Foteini
AU - Murase, Kohta
AU - Padovani, Paolo
AU - Resconi, Elisa
AU - Mészáros, Peter
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
PY - 2021/7/2
Y1 - 2021/7/2
N2 - Motivated by the recently reported evidence of an association between a high-energy neutrino and a γ-ray flare from the blazar TXS 0506+056, we calculate the expected high-energy neutrino signal from past, individual flares, from twelve blazars, selected in declinations favourable for detection with IceCube. To keep the number of free parameters to a minimum, we mainly focus on BL Lac objects and assume the synchrotron self-Compton mechanism produces the bulk of the high-energy emission. We consider a broad range of the allowed parameter space for the efficiency of proton acceleration, the proton content of BL Lac jets, and the presence of external photon fields. To model the expected neutrino fluence we use simultaneous multi-wavelength observations. We find that in the absence of external photon fields and with jet proton luminosity normalised to match the observed production rate of ultra-high-energy cosmic rays, individual flaring sources produce a modest neutrino flux in IceCube, NνIC,10yrvµ,>100 TeV,> 10−3 muon neutrinos with energy exceeding 100 TeV, stacking ten years of flare periods selected in the > 800 MeV Fermi energy range, from each source. Under optimistic assumptions about the jet proton luminosity and in the presence of external photon fields, we find that the two most powerful sources in our sample, AO 0235+164, and OJ 287, would produce, in total, NICx10,10yrvµ,all flaes,> 100 TeV ≈ 3 muon neutrinos during Fermi flaring periods, in future neutrino detectors with total instrumented volume ∼ ten times larger than IceCube, or otherwise, constrain the proton luminosity of blazar jets.
AB - Motivated by the recently reported evidence of an association between a high-energy neutrino and a γ-ray flare from the blazar TXS 0506+056, we calculate the expected high-energy neutrino signal from past, individual flares, from twelve blazars, selected in declinations favourable for detection with IceCube. To keep the number of free parameters to a minimum, we mainly focus on BL Lac objects and assume the synchrotron self-Compton mechanism produces the bulk of the high-energy emission. We consider a broad range of the allowed parameter space for the efficiency of proton acceleration, the proton content of BL Lac jets, and the presence of external photon fields. To model the expected neutrino fluence we use simultaneous multi-wavelength observations. We find that in the absence of external photon fields and with jet proton luminosity normalised to match the observed production rate of ultra-high-energy cosmic rays, individual flaring sources produce a modest neutrino flux in IceCube, NνIC,10yrvµ,>100 TeV,> 10−3 muon neutrinos with energy exceeding 100 TeV, stacking ten years of flare periods selected in the > 800 MeV Fermi energy range, from each source. Under optimistic assumptions about the jet proton luminosity and in the presence of external photon fields, we find that the two most powerful sources in our sample, AO 0235+164, and OJ 287, would produce, in total, NICx10,10yrvµ,all flaes,> 100 TeV ≈ 3 muon neutrinos during Fermi flaring periods, in future neutrino detectors with total instrumented volume ∼ ten times larger than IceCube, or otherwise, constrain the proton luminosity of blazar jets.
UR - http://www.scopus.com/inward/record.url?scp=85127492687&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85127492687
SN - 1824-8039
VL - 358
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 971
T2 - 36th International Cosmic Ray Conference, ICRC 2019
Y2 - 24 July 2019 through 1 August 2019
ER -