[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 …

Testing hadronic and photohadronic interactions as responsible for ultrahigh energy cosmic rays and neutrino fluxes from starburst galaxies

A Condorelli, D Boncioli, E Peretti, S Petrera - Physical Review D, 2023 - APS
We test the hypothesis of starburst galaxies as sources of ultrahigh energy cosmic rays and
high energy neutrinos. The computation of interactions of ultrahigh energy cosmic rays in the …

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 …

Impact of Galaxy Clusters on the Propagation of Ultrahigh-energy Cosmic Rays

A Condorelli, J Biteau, R Adam - The Astrophysical Journal, 2023 - iopscience.iop.org
Galaxy clusters are the largest objects in the Universe kept together by gravity. Most of their
baryonic content is made of a magnetized diffuse plasma. We investigate the impact of such …

Joint measurement of the ultra-high-energy neutrino spectrum and cross section

VB Valera, M Bustamante, O Mena - arXiv preprint arXiv:2308.07709, 2023 - arxiv.org
Soon, a new generation of neutrino telescopes, presently under planning, will target the
discovery of ultra-high-energy (UHE) neutrinos of cosmic origin, with energies higher than …

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 …

The role of supernovae inside AGN jets in UHECR acceleration

V Bosch-Ramon - Astronomy & Astrophysics, 2023 - aanda.org
Context. Jets of active galactic nuclei are potential accelerators of ultra high-energy cosmic
rays. Supernovae can occur inside these jets and contribute to cosmic ray acceleration …