[HTML][HTML] The present and future of QCD

P Achenbach, D Adhikari, A Afanasev, F Afzal… - Nuclear Physics A, 2024 - Elsevier
Abstract This White Paper presents an overview of the current status and future perspective
of QCD research, based on the community inputs and scientific conclusions from the 2022 …

Where Did the Amaterasu Particle Come From?

M Unger, GR Farrar - The Astrophysical Journal Letters, 2024 - iopscience.iop.org
Abstract The Telescope Array Collaboration recently reported the detection of a cosmic-ray
particle," Amaterasu," with an extremely high energy of 2.4× 10 20 eV. Here we investigate …

Nonlinear aspects of stochastic particle acceleration

M Lemoine, K Murase, F Rieger - Physical Review D, 2024 - APS
In turbulent magnetized plasmas, charged particles can be accelerated to high energies
through their interactions with the turbulent motions. As they do so, they draw energy from …

Constraints on UHECR sources and extragalactic magnetic fields from directional anisotropies

T Bister, GR Farrar - The Astrophysical Journal, 2024 - iopscience.iop.org
A dipole anisotropy in ultra–high-energy cosmic ray (UHECR) arrival directions, of
extragalactic origin, is now firmly established at energies E> 8 EeV. Furthermore, the …

Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at …

AA Halim, P Abreu, M Aglietta, I Allekotte… - … of cosmology and …, 2024 - iopscience.iop.org
The combined fit of the measured energy spectrum and shower maximum depth
distributions of ultra-high-energy cosmic rays is known to constrain the parameters of …

A nearby source of ultra-high energy cosmic rays

MY Kuznetsov - Journal of Cosmology and Astroparticle Physics, 2024 - iopscience.iop.org
Abstract Recently the Telescope Array collaboration reported an observation of cosmic ray
event with very high energy 244 EeV (2.44× 10 20 eV). Importantly, the event is hard to …

A relook at the GZK neutrino-photon connection: impact of extra-galactic radio background & UHECR properties

S Chakraborty, P Mehta, P Sarmah - Journal of Cosmology and …, 2024 - iopscience.iop.org
Ultra-high energy cosmic rays (UHECRs) beyond the Greisen-Zatsepin-Kuzmin (GZK) cut-off
provide us with a unique opportunity to understand the universe at extreme energies …

Galactic origin of ultrahigh energy cosmic rays

VN Zirakashvili, VS Ptuskin, SI Rogovaya - Physical Review D, 2024 - APS
It is shown that the acceleration of particles by a powerful relativistic jet associated with the
activity of a supermassive black hole in the Galactic Center several million years ago may …

Impact of the Magnetic Horizon on the Interpretation of the Pierre Auger Observatory Spectrum and Composition Data

AA Halim, P Abreu, M Aglietta, I Allekotte… - arXiv preprint arXiv …, 2024 - arxiv.org
The flux of ultra-high energy cosmic rays reaching Earth above the ankle energy (5 EeV) can
be described as a mixture of nuclei injected by extragalactic sources with very hard spectra …

Constraints on the proton fraction of cosmic rays at the highest energies and the consequences for cosmogenic neutrinos and photons

D Ehlert, A van Vliet, F Oikonomou… - Journal of Cosmology …, 2024 - iopscience.iop.org
Over the last decade, observations have shown that the mean mass of ultra-high-energy
cosmic rays (UHECRs) increases progressively toward the highest energies. However, the …