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Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
A Aab, P Abreu, M Aglietta… - … of Cosmology and …, 2019 - iopscience.iop.org
Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the
Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all …
Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all …
Newly born pulsars as sources of ultrahigh energy cosmic rays
Newly born pulsars offer favorable sites for the injection of heavy nuclei, and for their further
acceleration to ultrahigh energies. Once accelerated in the pulsar wind, nuclei have to …
acceleration to ultrahigh energies. Once accelerated in the pulsar wind, nuclei have to …
Ultrahigh-energy cosmic-ray nuclei from black hole jets: Recycling galactic cosmic rays through shear acceleration
We perform Monte Carlo simulations of transrelativistic shear acceleration dedicated to a jet-
cocoon system of active galactic nuclei. A certain fraction of galactic cosmic rays in a halo is …
cocoon system of active galactic nuclei. A certain fraction of galactic cosmic rays in a halo is …
On ultra-high energy cosmic ray acceleration at the termination shock of young pulsar winds
M Lemoine, K Kotera, J Pétri - Journal of Cosmology and …, 2015 - iopscience.iop.org
Pulsar wind nebulae (PWNe) are outstanding accelerators in Nature, in the sense that they
accelerate electrons up to the radiation reaction limit. Motivated by this observation, this …
accelerate electrons up to the radiation reaction limit. Motivated by this observation, this …
Case for Centaurus A as the main source of ultrahigh-energy cosmic rays
We discuss the possibility that a dominant fraction of the cosmic rays above the ankle (ie,
above 5 EeV) is due to a single nearby source, considering in particular the radio galaxy …
above 5 EeV) is due to a single nearby source, considering in particular the radio galaxy …
Implications of a PeV neutrino spectral cut-off in gamma-ray burst models
The recent discovery of extragalactic PeV neutrinos opens a new window to the exploration
of cosmic ray accelerators. The observed PeV neutrino flux is close to the Waxman–Bahcall …
of cosmic ray accelerators. The observed PeV neutrino flux is close to the Waxman–Bahcall …
Isotropy constraints on powerful sources of ultrahigh-energy cosmic rays at 1019 eV
ISOTROPY CONSTRAINTS ON POWERFUL SOURCES OF ULTRAHIGH-ENERGY
COSMIC RAYS AT 1019 eV - IOPscience Skip to content IOP Science home Accessibility …
COSMIC RAYS AT 1019 eV - IOPscience Skip to content IOP Science home Accessibility …
[PDF][PDF] Absolute energy calibration of the Pierre Auger Observatory using radio emission of extensive air showers
JC Glaser - 2017 - inspirehep.net
Cosmic rays are the most energetic particles observed in the universe. With energies of
more than 1020 eV p «16 Joulesq concentrated in a single particle, their energy is seven …
more than 1020 eV p «16 Joulesq concentrated in a single particle, their energy is seven …
Ultra-high energy cosmic rays and neutrinos from gamma-ray bursts, hypernovae and galactic shocks
I review gamma-ray burst models (GRBs) and observations, and discuss the possible
production of ultra-high energy cosmic rays and neutrinos in both the standard internal …
production of ultra-high energy cosmic rays and neutrinos in both the standard internal …
Cosmic rays from the ankle to the cutoff
KH Kampert, P Tinyakov - Comptes …, 2014 - comptes-rendus.academie-sciences …
Les récentes avancées des mesures et de l'interprétation des rayons cosmiques, depuis la
caractéristique spectrale appelé «cheville» jusqu'aux plus hautes énergies, sont brièvement …
caractéristique spectrale appelé «cheville» jusqu'aux plus hautes énergies, sont brièvement …