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The interstellar environment of our galaxyObservations and implications of the ultrahigh-energy cosmic raysInterpretation of neutrino flux limits from neutrino telescopes on the Hillas plotUltrahigh energy cosmic raysHigh-energy cosmic rays and neutrinos from semirelativistic hypernovaeImplications of a possible clustering of highest-energy cosmic rays.On the acceleration of ultra-high-energy cosmic rays.Constraint on electromagnetic acceleration of highest energy cosmic rays.Cosmic ray electrons and positrons from supernova explosions of massive stars.Influence of the universal microwave background radiation on the extragalactic cosmic-ray spectrum.ULTRAHIGH ENERGY COSMIC RAYS: THE STATE OF THE ART BEFORE THE AUGER OBSERVATORYNonthermal processes and neutrino emission from the black hole GRO J0422+32 in a bursting stateUltra-high-energy cosmic ray acceleration in engine-driven relativistic supernovaeLimit on the ultrahigh-energy neutrino flux from lunar observations with the Parkes radio telescopeCosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic fieldNeutrino diagnostics of ultrahigh energy cosmic ray protonsIntergalactic propagation of ultrahigh energy cosmic ray nuclei: An analytic approachPredictions for the cosmogenic neutrino flux in light of new data from the Pierre Auger ObservatoryUNDERSTANDING THE VERY-HIGH-ENERGY EMISSION FROM MICROQUASARSDetecting Axionlike Particles with Gamma Ray TelescopesConstraints on the multi-TeV particle population in the Coma galaxy cluster with HESS observationsUltrahigh energy nuclei propagation in a structured, magnetized universeStudy of the ultrahigh-energy primary-cosmic-ray composition with the MACRO experimentInterpretation of ultra-high energy multi-messenger dataUltrahigh energy cosmic rays in a structured and magnetized universeTesting the correlation of ultrahigh energy cosmic rays with high redshift sourcesProbing grand unified theories with cosmic-ray, gamma-ray, and neutrino astrophysicsMaximum likelihood analysis of clusters of ultrahigh energy cosmic raysHelium photodisintegration and nucleosynthesis: Implications for topological defects, high energy cosmic rays, and massive black holesMonopole annihilation and highest energy cosmic raysConstraints on the ultrahigh-energy photon flux using inclined showers from the Haverah Park arrayNew Constraints from Haverah Park Data on the Photon and Iron Fluxes of Ultrahigh-Energy Cosmic RaysGamma-ray astronomy above 50 TeV with muon-poor showersObscured flat spectrum radio active galactic nuclei as sources of high-energy neutrinosANTARES constrains a blazar origin of two IceCube PeV neutrino eventsHigh-energy cosmic ray nuclei from tidal disruption events: Origin, survival, and implicationsNeutrinos from Cosmic Accelerators including Magnetic Field and Flavor EffectsConstraints on direct acceleration of UHECRs in astrophysical sourcesTowards a model of population of astrophysical sources of ultrahigh-energy cosmic raysCoincidence of a high-fluence blazar outburst with a PeV-energy neutrino event
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description
im September 1984 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 1984
@uk
name
The Origin of Ultra-High-Energy Cosmic Rays
@en
The Origin of Ultra-High-Energy Cosmic Rays
@nl
type
label
The Origin of Ultra-High-Energy Cosmic Rays
@en
The Origin of Ultra-High-Energy Cosmic Rays
@nl
prefLabel
The Origin of Ultra-High-Energy Cosmic Rays
@en
The Origin of Ultra-High-Energy Cosmic Rays
@nl
P1476
The Origin of Ultra-High-Energy Cosmic Rays
@en
P2093
A. M. Hillas
P304
P356
10.1146/ANNUREV.AA.22.090184.002233
P407
P577
1984-09-01T00:00:00Z