Neutrinos in IceCube from AGN's
arXiv:1410.8124 · doi:10.1134/S106377611503022X
Abstract
Recently IceCube collaboration has reported first evidence for the astrophysical neutrinos. Observation corresponds to the total astrophysical neutrino flux of the order of in a PeV energy range. Active Galactic Nuclei (AGN) are natural candidate sources for such neutrinos. To model the neutrino creation in AGNs we study photopion production processes on the radiation field of the Shakura-Sunyaev accretion disks in the black hole vicinity. We show that this model can explain detected neutrino flux and avoids, at the same time, existing constraints from the gamma-ray and cosmic ray observations.
6 pages, 5 figures, version accepted for publication in JETP (minor text corrections, few references added)
References in corpus (8)
- Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data
- The Spectrum of the Isotropic Diffuse Gamma-Ray Emission Derived From First-Year Fermi Large Area Telescope Data
- Diffuse Neutrino Intensity from the Inner Jets of Active Galactic Nuclei: Impacts of External Photon Fields and the Blazar Sequence
- Cosmic Neutrino Pevatrons: A Brand New Pathway to Astronomy, Astrophysics, and Particle Physics
- Searches for Point-like and extended neutrino sources close to the Galactic Centre using the ANTARES neutrino Telescope
- High energy radiation from Centaurus A
- Explaining the Spectra of Cosmic Ray Groups above the Knee by Escape from the Galaxy
- Towards a model of population of astrophysical sources of ultra-high-energy cosmic rays
Cited by in corpus (53)
- IceCube-Gen2: The Window to the Extreme Universe
- Hidden Cosmic-Ray Accelerators as an Origin of TeV-PeV Cosmic Neutrinos
- Constraining High-Energy Cosmic Neutrino Sources: Implications and Prospects
- Hidden Cores of Active Galactic Nuclei as the Origin of Medium-Energy Neutrinos: Critical Tests with the MeV Gamma-Ray Connection
- Observational evidence for the origin of high-energy neutrinos in parsec-scale nuclei of radio-bright active galaxies
- Evidence against star-forming galaxies as the dominant source of IceCube neutrinos
- On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity
- Opening a New Window onto the Universe with IceCube
- High-Energy Neutrinos from Magnetized Coronae of Active Galactic Nuclei and Prospects for Identification of Seyfert Galaxies and Quasars in Neutrino Telescopes
- Directional association of TeV to PeV astrophysical neutrinos with radio blazars
- Spectral analysis of the high-energy IceCube neutrinos
- Hidden Hearts of Neutrino Active Galaxies
- Evidence for the Galactic contribution to the IceCube astrophysical neutrino flux
- On high-energy particles in accretion disk coronae of supermassive black holes: implications for MeV gamma rays and high-energy neutrinos from AGN cores
- A Possible Two-component Flux for the High Energy Neutrino Events at IceCube
- Decaying Leptophilic Dark Matter at IceCube
- Analysis of the 4-year IceCube high-energy starting events
- New constraints on the origin of medium-energy neutrinos observed by IceCube
- Interpreting IceCube 6-year HESE data as an evidence for hundred TeV decaying Dark Matter
- Pairwise sums in colourings of the reals
- IceCube Events from Heavy DM decays through the Right-handed Neutrino Portal
- A minimal model for extragalactic cosmic rays and neutrinos
- Multi-component Fermionic Dark Matter and IceCube PeV scale Neutrinos in Left-Right Model with Gauge Unification
- R-parity Violating Supersymmetric Explanation of the Anomalous Events at ANITA
- A search for neutrino emission from cores of Active Galactic Nuclei
- Multi-messenger tests of cosmic-ray acceleration in radiatively inefficient accretion flows
- Constraints on the models of the origin of high-energy astrophysical neutrinos
- Very high energy neutrino emission from the core of low luminosity AGNs triggered by magnetic reconnection acceleration
- Massive Argon Space Telescope (MAST): a concept of heavy time projection chamber for gamma-ray astronomy in the 100 MeV --- 1 TeV energy range
- Probing decaying heavy dark matter with the 4-year IceCube HESE data
- Dark Matter interpretation of low energy IceCube MESE excess
- Boosted Dark Matter and its implications for the features in IceCube HESE data
- Strong constraint on hadronic models of blazar activity from Fermi and IceCube stacking analysis
- Estimating the contribution of Galactic sources to the diffuse neutrino flux
- NGC 1068 constraints on neutrino-dark matter scattering
- High-energy emitting BL Lacs and high-energy neutrinos - Prospects for the direct association with IceCube and KM3NeT
- Neutrino, -ray and cosmic ray fluxes from the core of the closest radio galaxies
- Neutrino telescopes and high-energy cosmic neutrinos
- Gamma-ray and Neutrino Signals from Accretion Disk Coronae of Active Galactic Nuclei
- PeV scale Supersymmetry breaking and the IceCube neutrino flux
- Quantum witness and invasiveness of cosmic neutrino measurements
- Neutrino production in blazar radio cores
- Probing neutrino production in blazars by millimeter VLBI
- Mass and Life Time of Heavy Dark Matter Decaying into IceCube PeV Neutrinos
- Beyond first light: Global monitoring for high-energy neutrino astronomy
- Energy-dependent flavor ratios, cascade/track spectrum tension and high-energy neutrinos from magnetospheres of supermassive black holes
- On the possible contributions of two nearby blazars to the NGC 4151 neutrino hotspot
- IceCube PeV Neutrinos and Leptophilic Dark Matter
- Efficiency of Centrifugal Mechanism in Producing PeV Neutrinos From Active Galactic Nuclei
- General constraints on sources of high-energy cosmic rays from the interaction losses
- Neutrino and Cosmic-Ray Emission and Cumulative Background from Radiatively Inefficient Accretion Flows in Low-Luminosity Active Galactic Nuclei
- Estimation of Baryon Asymmetry from Dark Matter Decaying into IceCube Neutrinos
- Revisiting Disk Winds in Active Galactic Nuclei as an Origin of Cosmic Gamma-ray and Neutrino Backgrounds