REVIEW 23 cited by
Multi-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
Individual astrophysical sources previously detected in neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of high-energy cosmic neutrinos remain unidentified. On 22 September 2017 we detected a high-energy neutrino, IceCube-170922A, with an energy of approximately 290 TeV. Its arrival direction was consistent with the location of a known gamma-ray blazar TXS 0506+056, observed to be in a flaring state. An extensive multi-wavelength campaign followed, ranging from radio frequencies to gamma-rays. These observations characterize the variability and energetics of the blazar and include the first detection of TXS 0506+056 in very-high-energy gamma-rays. This observation of a neutrino in spatial coincidence with a gamma-ray emitting blazar during an active phase suggests that blazars may be a source of high-energy neutrinos.
Forward citations
Cited by 23 Pith papers
-
Probing Neutrino Flavor Composition with the Glashow Resonance at Tau Air-Shower Neutrino Telescopes
Tau air-shower telescopes can potentially measure the PeV \bar{\nu}_e/(\nu_\tau+\bar{\nu}_\tau) ratio via the Glashow resonance, but standalone sensitivity only clearly separates \bar{\nu}_e-rich sources from standard...
-
Time-Dependent Leptohadronic Modeling of Markarian 421
Time-dependent leptohadronic fits show hadronic secondary emission can explain Mrk 421's 2013 hard X-ray excess at sub-Eddington jet power, but cannot explain the 2016 excess without super-Eddington power or the 2017 ...
-
Leading-order gravitational time delay of massive particles by a moving Schwarzschild lens
A unified 1PM formula gives the gravitational time delay of relativistic massive and massless particles by a radially moving Schwarzschild lens, matching known light and static limits.
-
The Highest-Energy Neutrino Event Constrains Dark Matter-Neutrino Interactions
KM3-230213A limits dark matter-neutrino scattering to below about 1e-22 cm^2/GeV at 220 PeV, but most simple dark matter models are excluded by unitarity above MeV masses.
-
The Extreme Universe Observatory on a Super-Pressure Balloon II: Mission, Payload, and Flight
A short balloon flight commissioned a fluorescence and a Cherenkov telescope at 33 km altitude and returned about 10 candidate cosmic-ray extensive air shower events from Cherenkov light.
-
Bayesian Deep-stacking for High-energy Neutrino Searches
A hierarchical Bayesian stacking framework improves sensitivity for detecting faint high-energy neutrino source populations when per-source flux predictions are uncertain.
-
Did IceCube discover Dark Matter around Blazars?
Sub-GeV dark matter scattering off protons in blazar jets can produce the IceCube neutrino from TXS 0506+056 while evading current dark matter constraints.
-
Strong field gravitational lensing of particles by a black-bounce-Schwarzschild black hole
For a black-bounce-Schwarzschild black hole, the paper derives the strong-deflection lensing observables for massive particles and quantifies how they differ from photon lensing.
-
Neutrino-Induced Polarization Rotation in Active Galactic Nuclei Plasmas
Neutrino-induced polarization rotation in AGN plasmas is computed and found to produce a frequency scaling distinct from Faraday rotation, but with angles far below current polarimetric sensitivity.
-
Cosmic-ray boosted inelastic dark matter from neutrino-emitting active galactic nuclei
A cosmic-ray boosted, inelastic dark matter flux from two neutrino-emitting AGNs gives new Super-K and XENONnT limits that reach part of the thermal freeze-out target for sub-GeV dark matter.
-
A Cost Effective Optimization of the hybrid-DOM Design for TRIDENT
Simulations show the 19-PMT, 4-inch hDOM for TRIDENT can match or exceed the 31-PMT, 3-inch design on neutrino efficiency and reconstruction, provided the 4-inch PMTs achieve comparable quantum efficiency and timing.
-
$\nu$SpaceSim: An end-to-end simulation package to model the sensitivity of UHECR experiments to upward-moving extensive air showers sourced by cosmic neutrinos interacting in the Earth
νSpaceSim is an end-to-end Monte Carlo package that simulates tau-neutrino earth-skimming events, from underground interaction through lepton propagation and decay to optical and radio signals at a user-defined detector.
-
Phenomenology of Neutrino-Dark Matter Interaction in DSNB and AGN
Upper limits on the scalar-dark-matter neutrino coupling are derived from DSNB attenuation projected for DUNE/Hyper-K and from IceCube data on NGC 1068 and TXS 0506+056, assuming DM spikes around AGN black holes.
-
Probing Dark Matter and Phantom Field Effects on Neutrino Oscillations around Black Holes
For neutrinos deflected by a black hole embedded in phantom-field dark matter, the oscillation phase gains a logarithmic dark matter correction, while radially moving neutrinos see no net gravity effect.
-
Epicyclic oscillations and accretion disk around a special Buchdahl-inspired spacetime
The Buchdahl-inspired metric shifts the ISCO inward for positive k tilde and produces QPO and disk profiles that the authors fit to microquasar data, claiming 0.03<k<0.19.
-
Prospects for Time-Domain and Multi-Messenger Science with eXTP
A mission white paper forecasting the time-domain and multi-messenger science of the future X-ray observatory eXTP, with detection rates and model-discrimination estimates.
-
Constraints on Neutrino Secret Interactions from Multi-messenger Neutrinos Scattering on C$\nu$B
Astrophysical neutrinos traveling through the cosmic neutrino background set new, generally stronger upper bounds on secret neutrino self-interactions, especially for a vector mediator at low mass.
-
Blazar Boosted ALP and vector portal Dark matter confronting light mediator searches
Blazar-boosted dark matter scattering in Super-Kamiokande can exclude previously unconstrained parameter space for ALP- and vector-mediated sub-MeV dark matter, beating BaBar, NA64, beam dump, and stellar cooling limi...
-
Blazars Jets and prospects for TeV-PeV neutrinos & gamma-rays through cosmic-ray interactions
A single-zone model with added proton-proton collisions suggests W Comae and 1ES 1959+650 need hadronic emission, and CTAO sensitivity forecasts show all four BL Lacs are detectable.
-
Active Galactic Nuclei as high-energy neutrino sources
Review summarizing correlations between astrophysical neutrinos and gamma-ray/radio AGN, specific source associations, proposed production mechanisms, and future prospects.
-
Supermassive black holes and their surroundings: MeV signatures
A review of open questions in supermassive black hole physics that argues the MeV gamma-ray band is the critical missing observational window.
-
Neutrinos from explosive transients at the dawn of multi-messenger astronomy
This review summarizes the state of neutrino emission from supernovae and neutron-star mergers, covering thermal and high-energy signals, flavor conversion, and multi-messenger detection strategies.
-
Transforming Antarctic Ice into a Cherenkov Neutrino Detector
IceCube built a cubic-kilometer Cherenkov detector in Antarctic ice and discovered a diffuse flux of cosmic neutrinos, identified the first neutrino sources, and observed the Galactic plane in neutrinos.
Discussion (0). Continue with ORCID to comment.