Dissecting the broadband emission from γ-ray blazar PKS 0735+178 in search of neutrinos
arXiv:2301.06565 · doi:10.1093/mnras/stad3804
Abstract
The origin of the diffuse flux of TeV-PeV astrophysical neutrinos is still unknown. The -ray blazar PKS 0735+178, located outside the 90\% localization region at 2.2 deg from the best-fit IC-211208A event, was found to be flaring across all wavebands. In addition to leptonic synchrotron (SYN) and synchrotron self-Compton (SSC) emission, we invoke photohadronic () interactions inside the jet to model the spectral energy distribution (SED) and neutrino emission. We analyze the 100 days -ray and X-ray data and 10 days around the neutrino event is chosen to generate the broadband SED. The temporal light curve indicates that the source was in a high state in optical, UV, -ray, and X-ray frequencies during the neutrino detection epoch. In the one-zone lepto-hadronic model, the SSC photons do not provide enough seed photons for interactions to explain the neutrino event. However, including an external photon field yields a neutrino event rate of 0.12 in 100 days, for the IceCube detector, using physically motivated values of the magnetic field, an external photon field peaking at optical wavelength, and other jet parameters. The radiation from secondary electrons at X-ray energies severely constrains the neutrino flux to a lower value than found in previous studies. Moreover, the flux of high-energy -rays at GeV energies from the decay of neutral pions is subdominant at the high-energy peak of the SED, suggesting a higher correlation of neutrinos flux with X-ray flux is plausible.
9 pages, 5 figures, 1 table, accepted in mnras
References in corpus (10)
- The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux
- TXS 0506+056, the first cosmic neutrino source, is not a BL Lac
- Swift and infra-red observations of the blazar 3C~454.3 during the giant X-ray flare of May 2005
- Bethe-Heitler emission in BL Lacs: filling the gap between X-rays and -rays
- A multi-messenger study of the blazar PKS 0735+178: a new major neutrino source candidate
- X-ray spectra, light-curves and SEDs of blazars frequently observed by Swift
- The BH mass of nearby QSOs: a comparison of the bulge luminosity and virial methods
- Search for Astrophysical Neutrinos from 1FLE Blazars with IceCube
- Cosmogenic gamma-ray and neutrino fluxes from blazars associated with IceCube events
- Implications of multiwavelength spectrum on cosmic-ray acceleration in blazar TXS 0506+056
Cited by in corpus (8)
- The origin of high-energy astrophysical neutrinos: new results and prospects
- Multi-epoch leptohadronic modeling of neutrino source candidate blazar PKS 0735+178
- Insights from leptohadronic modelling of the brightest blazar flare
- Cosmic Clues from Amaterasu: Blazar-Driven Ultrahigh-Energy Cosmic Rays?
- On the origin of multifrequency temporal and spectral variability in Ton 599
- The dynamics of the parsec-scale jet in the neutrino blazar PKS 0735+178
- Rapid jet ejection from PKS 0215+015 coincident with a high-energy neutrino event
- Testing Weak Equivalence Principle with IceCube Event and Blazar