Giovanni Morlino
Articles 23
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Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-dominated Shells
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Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout
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Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
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Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory
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An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources
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Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
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Large-scale Cosmic-Ray Anisotropies above 4 EeV Measured by the Pierre Auger Observatory
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Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
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Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946
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Balmer Filaments in Tycho’s Supernova Remnant: An Interplay between Cosmic-ray and Broad-neutral Precursors
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The microphysics of collisionless shock waves.
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Cosmic ray acceleration and Balmer emission from RCW 86 (G315.4 – 2.3)
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Broad Balmer line emission and cosmic ray acceleration efficiency in supernova remnant shocks
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Collisionless shocks in a partially ionized medium. III. Efficient cosmic ray acceleration
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Cosmic ray acceleration and Balmer emission from SNR 0509-67.5
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Collisionless shocks in a partially ionized medium. I. Neutral return flux and its effects on acceleration of test particles
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Collisionless shocks in a partially ionized medium. II. Balmer emission
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Spatial structure of X-ray filaments in SN 1006
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Gamma rays and neutrinos from SNR RX J1713.7–3946
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Gamma-ray emission from SNR RX J1713.7−3946 and the origin of galactic cosmic rays
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Cosmic-ray electron injection from the ionization of nuclei
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On Particle Acceleration around Shocks. III. Shock Waves Moving at Arbitrary Speed. The Case of Large‐Scale Magnetic Field and Anisotropic Scattering
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On Particle Acceleration around Shocks. IV. Particle Spectrum as a Function of the Equation of State of the Shocked Plasma
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