Cosmogenic gamma-ray and neutrino fluxes from blazars associated with IceCube events
arXiv:2108.12120 · doi:10.1051/0004-6361/202142123
Abstract
Blazars constitute the vast majority of extragalactic -ray sources. They can also contribute a sizable fraction of the diffuse astrophysical neutrinos detected by IceCube. In the past few years, the real-time alert system of IceCube has led to multiwavelength follow-up of very high-energy neutrino events of plausible astrophysical origin. Spatial and temporal coincidences of these neutrino events with the high-activity state of -ray blazars can provide a unique opportunity to decipher cosmic-ray interactions in the relativistic jets. Assuming that blazars accelerate cosmic rays up to ultrahigh energies ( eV), we calculate the "guaranteed" contribution to the line-of-sight cosmogenic -ray and neutrino fluxes from four blazars associated with IceCube neutrino events. Detection of these fluxes by upcoming -ray imaging telescopes like CTA and/or by planned neutrino detectors like IceCube-Gen2 may lead to the first direct signature(s) of ultrahigh-energy cosmic-ray (UHECR) sources. We find that detection of the cosmogenic neutrino fluxes from the blazars TXS~0506+056, PKS~1502+106 and GB6~J1040+0617 would require UHECR luminosity times the inferred neutrino luminosity from the associated IceCube events. Blazars TXS~0506+056, 3HSP~J095507.9+355101 and GB6~J1040+0617 can be detected by CTA if the UHECR luminosity is times the neutrino luminosity inferred from the associated IceCube events. Given their relatively low redshifts and hence total energetics, TXS~0506+056 and 3HSP~J095507.9+355101 should be the prime targets for upcoming large neutrino and -ray telescopes.
5 pages, 3 figures, Accepted for publication in Astronomy & Astrophysics
References in corpus (10)
- The major upgrade of the MAGIC telescopes, Part II: A performance study using observations of the Crab Nebula
- Ultra High Energy Cosmic Rays from Black Hole Jets of Radio Galaxies
- AGN jets as the origin of UHECRs and perspectives for the detection of astrophysical source neutrinos at EeV energies
- Multi-wavelength and neutrino emission from blazar PKS 1502+106
- 3HSP J095507.9+355101: a flaring extreme blazar coincident in space and time with IceCube-200107A
- Acceleration of Ultra-High Energy Cosmic Rays in the Colliding Shells of Blazars and GRBs: Constraints from the Fermi Gamma ray Space Telescope
- Comprehensive Multimessenger Modeling of the Extreme Blazar 3HSP J095507.9+355101 and Predictions for IceCube
- Synchrotron pair halo and echo emission from blazars in the cosmic web: application to extreme TeV blazars
- PeV-EeV neutrinos from gamma-ray blazars due to ultrahigh-energy cosmic-ray propagation
- The Cherenkov Telescope Array: layout, design and performance
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- First Search for High-Energy Neutrino Emission from Galaxy Mergers
- Blazars Jets and prospects for TeV-PeV neutrinos & gamma-rays through cosmic-ray interactions
- Hadronic origin of gamma rays and neutrinos from blazars: Multi-messenger implications and observational constraints
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