Energy-dependent extension of the Crab Nebula as a diagnostic of ultrahigh-energy hadronic emission
astro-ph.HE
Submitted: 2026-08-26
Updated: 2026-08-26
Comments: 5 pages, 3 figures. Published in Physical Review D
Journal ref: Phys. Rev. D 114, 043066 (2026)
DOI: 10.1103/dnsv-plc9
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Gamma-ray flares from the Crab Nebula
- Discovery of Powerful Gamma-Ray Flares from the Crab Nebula
- Peta-electron volt gamma-ray emission from the Crab Nebula
- Modeling the broadest spectral band of the Crab nebula and constraining the ions acceleration efficiency
- PeV emission of the Crab Nebula: constraints on the proton content in pulsar wind and implications
- Ultrahigh-energy Gamma-Ray Radiation from the Crab Pulsar Wind Nebula
- All-sky search for time-integrated neutrino emission from astrophysical sources with 7 years of IceCube data
- Time-integrated Neutrino Source Searches with 10 years of IceCube Data
- IceCube Search for High-Energy Neutrino Emission from TeV Pulsar Wind Nebulae
- All-sky neutrino point-source search with IceCube combined track and cascade data
- Observation of high-energy neutrinos from the Galactic plane
- Letter of Intent for KM3NeT 2.0
- Multi-band Emission up to PeV Energy from the Crab Nebula in a Spatially Dependent Lepto-hadronic Model
- Hadronic emission from the environment of the Crab Pulsar Wind Nebula by re-accelerated particles
- Phenomenological modelling of the Crab Nebula's broad band energy spectrum and its apparent extension
- Spectrum and extension of the inverse-Compton emission of the Crab Nebula from a combined Fermi-LAT and H.E.S.S. analysis
- Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated Waves
- Particle acceleration in relativistic collisionless shocks: Fermi process at last?
- Particle Acceleration in Relativistic Magnetized Collisionless Electron-Ion Shocks
- Acceleration of Particles at the Termination Shock of a Relativistic Striped Wind
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