Astrophysical Sources of High Energy Neutrinos in the IceCube Era
arXiv:1708.03577 · doi:10.1146/annurev-nucl-101916-123304
Abstract
High energy neutrino astrophysics has come of age with the discovery by IceCube of neutrinos in the TeV to PeV energy range attributable to extragalactic sources at cosmological distances. At such energies, astrophysical neutrinos must have their origin in cosmic ray interactions, providing information about the sources of high energy cosmic rays, as well as leading to the co-production of high energy gamma-rays. The intimate link with these latter two independently observed types of radiation provides important tools in the search for identifying and understanding the nature of their astrophysical sources. These neutrinons can provide important constraints about the cosmic ray acceleration process, and since they travel essentially unimpeded they can probe our Universe out to the farthest cosmological distances.
26 pages, 8 figures; accepted in Annual Review of Nuclear and Particle Science; to appear in vol. 67 (2017)
References in corpus (22)
- The Internal-Collision-Induced Magnetic Reconnection and Turbulence (ICMART) Model of Gamma-Ray Bursts
- The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV
- Compressible Turbulence in Galaxy Clusters: Physics and Stochastic Particle Re-acceleration
- Atmospheric and Astrophysical Neutrinos above 1 TeV Interacting in IceCube
- Star-forming galaxies as the origin of diffuse high-energy backgrounds: Gamma-ray and neutrino connections, and implications for starburst history
- Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube
- Search for Prompt Neutrino Emission from Gamma-Ray Bursts with IceCube
- A unified picture for low-luminosity and long gamma-ray bursts based on the extended progenitor of llgrb 060218/SN 2006aj
- Revealing the Supernova--Gamma-Ray Burst Connection with TeV Neutrinos
- High-energy Cosmic Rays and Neutrinos from Semi-relativistic Hypernovae
- Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf
- Neutrino Spectra from Low and High Luminosity Populations of Gamma Ray Bursts
- High-energy neutrinos from radio galaxies
- High-energy gamma-ray and neutrino backgrounds from clusters of galaxies and radio constraints
- Relativistic Photon Mediated Shocks
- Extragalactic star-forming galaxies with hypernovae and supernovae as high-energy neutrino and gamma-ray sources: the case of the 10 TeV neutrino data
- The diffuse gamma-ray flux associated with sub-PeV/PeV neutrinos from starburst galaxies
- High-energy neutrinos from reverse shocks in choked and successful relativistic jets
- Galaxy Mergers as a Source of Cosmic Rays, Neutrinos, and Gamma Rays
- Gamma Ray Bursts
- A redshift - observation-time relation for gamma-ray bursts: evidence of a distinct sub-luminous population
- Collisionless Shocks and TeV Neutrinos before Supernova Shock Breakout from an Optically Thick Wind
Cited by in corpus (32)
- The IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data
- Beginning a journey across the universe: the discovery of extragalactic neutrino factories
- Constraints on the models of the origin of high-energy astrophysical neutrinos
- Common envelope jets supernovae with a black hole companion as possible high energy neutrino sources
- A ring accelerator? Unusual jet dynamics in the IceCube candidate PKS 1502+106
- Neutrino signal dependence on gamma-ray burst emission mechanism
- Is the high-energy neutrino event IceCube-200530A associated with a hydrogen-rich superluminous supernova?
- Search for directional associations between Baikal Gigaton Volume Detector neutrino-induced cascades and high-energy astrophysical sources
- High-energy neutrinos from X-rays flares of blazars frequently observed by the Swift X-Ray Telescope
- State-of-the-Art Collapsar Jet Simulations Imply Undetectable Subphotospheric Neutrinos
- Optically Informed Searches of High-Energy Neutrinos from Interaction-Powered Supernovae
- Neutrino flares of radio blazars observed from TeV to PeV
- On the energy of the protons producing the very high-energy astrophysical neutrinos
- Spin light of neutrino in astrophysical environments
- First-principle calculation of birefringence effects for in-ice radio detection of neutrinos
- POEMMA (Probe of Extreme Multi-Messenger Astrophysics) design
- Flare Duty Cycle of Gamma-Ray Blazars and Implications for High-Energy Neutrino Emission
- Neutrino Emission from Luminous Fast Blue Optical Transients
- Multi-messenger detection prospects of gamma-ray burst afterglows with optical jumps
- Neutrino production in blazar radio cores
- Hard X-ray emission from blazars associated with high-energy neutrinos
- Contribution of Secondary Neutrinos from Line-of-sight Cosmic Ray Interactions to the IceCube Diffuse Astrophysical Flux
- Medium-band observation of the neutrino emitting blazar, TXS 0506+056
- On the radiation energy density in the jet of high-energy emitting BL Lac objects and its impact on their multi-messenger role
- A test of spatial coincidence between CHIME FRBs and IceCube TeV energy neutrinos
- Time-integrated constraint on neutrino flux of CHIME fast radio burst sources with 10-year IceCube point-source data
- VERITAS and multiwavelength observations of the Blazar B3 2247+381 in response to an IceCube neutrino alert
- Neutrino emission from FRB-emitting magnetars
- Multi-Messenger Astrophysics with THESEUS in the 2030s
- On the relation between the astrophysical neutrino fluxes and the cosmic ray fluxes
- An isotropic full-sky sample of optically selected blazars
- KamLAND's search for correlated low-energy electron antineutrinos with astrophysical neutrinos from IceCube