Quantum gravity phenomenology at the dawn of the multi-messenger era—A review
A Addazi, J Alvarez-Muniz, RA Batista… - Progress in Particle and …, 2022 - Elsevier
The exploration of the universe has recently entered a new era thanks to the multi-
messenger paradigm, characterized by a continuous increase in the quantity and quality of …
messenger paradigm, characterized by a continuous increase in the quantity and quality of …
Open questions in cosmic-ray research at ultrahigh energies
We review open questions and prospects for progress in ultrahigh-energy cosmic ray
(UHECR) research, based on a series of discussions that took place during the “The High …
(UHECR) research, based on a series of discussions that took place during the “The High …
IceCube-Gen2: the window to the extreme Universe
MG Aartsen, R Abbasi, M Ackermann… - Journal of Physics G …, 2021 - iopscience.iop.org
The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a
wealth of information about the Universe. However, at PeV (10 15 eV) energies and above …
wealth of information about the Universe. However, at PeV (10 15 eV) energies and above …
Observation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 1018 eV
Pierre Auger Collaboration, A Aab, P Abreu, M Aglietta… - Science, 2017 - science.org
Cosmic rays are atomic nuclei arriving from outer space that reach the highest energies
observed in nature. Clues to their origin come from studying the distribution of their arrival …
observed in nature. Clues to their origin come from studying the distribution of their arrival …
Measurement of the cosmic-ray energy spectrum above using the Pierre Auger Observatory
A Aab, P Abreu, M Aglietta, JM Albury, I Allekotte… - Physical Review D, 2020 - APS
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5× 10
18 eV based on 215,030 events recorded with zenith angles below 60°. A key feature of the …
18 eV based on 215,030 events recorded with zenith angles below 60°. A key feature of the …
Ultra high energy cosmic rays The intersection of the Cosmic and Energy Frontiers
The present white paper is submitted as part of the “Snowmass” process to help inform the
long-term plans of the United States Department of Energy and the National Science …
long-term plans of the United States Department of Energy and the National Science …
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above
A Aab, P Abreu, M Aglietta, EJ Ahn, I Al Samarai… - Physical Review D, 2014 - APS
We report a study of the distributions of the depth of maximum, X max, of extensive air-
shower profiles with energies above 1 0 17.8 eV as observed with the fluorescence …
shower profiles with energies above 1 0 17.8 eV as observed with the fluorescence …
[HTML][HTML] The large hadron–electron collider at the HL-LHC
P Agostini, H Aksakal, S Alekhin… - Journal of Physics G …, 2021 - iopscience.iop.org
Abstract The Large Hadron–Electron Collider (LHeC) is designed to move the field of deep
inelastic scattering (DIS) to the energy and intensity frontier of particle physics. Exploiting …
inelastic scattering (DIS) to the energy and intensity frontier of particle physics. Exploiting …
CRPropa 3—a public astrophysical simulation framework for propagating extraterrestrial ultra-high energy particles
We present the simulation framework CRPropa version 3 designed for efficient development
of astrophysical predictions for ultra-high energy particles. Users can assemble modules of …
of astrophysical predictions for ultra-high energy particles. Users can assemble modules of …
Features of the Energy Spectrum of Cosmic Rays above Using the Pierre Auger Observatory
A Aab, P Abreu, M Aglietta, JM Albury, I Allekotte… - Physical review …, 2020 - APS
We report a measurement of the energy spectrum of cosmic rays above 2.5× 10 18 eV
based on 215 030 events. New results are presented: at about 1.3× 10 19 eV, the spectral …
based on 215 030 events. New results are presented: at about 1.3× 10 19 eV, the spectral …