Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

IFM Albuquerque, JA Castillo, H Asorey… - … 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 …
被引用次数：153 相关文章

[引用][C] Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

A Aab, IFM Albuquerque, F Catalani… - Journal of Cosmology …, 2019 - repositorio.usp.br
USP affiliated authors: ALBUQUERQUE, IVONE FREIRE DA MOTA E-IF; SOUZA FILHO,
LUIZ VITOR DE-IFSC; CATALANI, FERNANDO-EEL; SANTOS, EDIVALDO MOURA-IF; …

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, I Albuquerque, JM Albury… - JCAP, 2019 - inria.hal.science
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 …

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, IFM Albuquerque… - 2019 - datosdeinvestigacion.conicet.gov.ar
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 …

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, IFM Albuquerque… - 2019 - openaccess.inaf.it
Neutrinos with energies above 10 17 eV are detectable with the Surface Detector Array of
the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all …

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, IFM Albuquerque… - Journal of Cosmology …, 2019 - osti.gov
Currently, neutrinos with energies above $10^{17} $ eV are detectable with the Surface
Detector Array of the Pierre Auger Observatory. Here, the identification is efficiently …

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, IFM Albuquerque… - 2019 - hekyll.services.adelaide.edu.au
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 …
[PDF] ru.nl

[PDF][PDF] Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

A Aab, F Canfora, SJ de Jong, GD Mauro, H Falcke… - 2019 - repository.ubn.ru.nl
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 …

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, S Andringa, P Assis… - Journal of Cosmology …, 2019 - inis.iaea.org
[en] Neutrinos with energies above 10 17 eV are detectable with the Surface Detector Array
of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all …

[引用][C] 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, IFM Albuquerque… - Journal of Cosmology …, 2019 - cir.nii.ac.jp