[HTML][HTML] The forward physics facility at the high-luminosity LHC

JL Feng, F Kling, MH Reno, J Rojo… - Journal of Physics G …, 2023 - iopscience.iop.org
High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large
number of particles along the beam collision axis, outside of the acceptance of existing LHC …

[HTML][HTML] High-energy and ultra-high-energy neutrinos: A Snowmass white paper

M Ackermann, M Bustamante, L Lu, N Otte… - Journal of high energy …, 2022 - Elsevier
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …

[HTML][HTML] Active galactic nuclei as potential sources of ultra-high energy cosmic rays

FM Rieger - Universe, 2022 - mdpi.com
Active Galactic Nuclei (AGNs) and their relativistic jets belong to the most promising class of
ultra-high-energy cosmic ray (UHECR) accelerators. This compact review summarises basic …

[HTML][HTML] Blazars at Very High Energies: Emission Modelling

H Sol, A Zech - Galaxies, 2022 - mdpi.com
Blazars are very broadband cosmic sources with spectra spanning over twenty orders of
magnitude in frequency, down to the 100 MHz regime in the radio range, up to VHE at …

Dark dimension, the swampland, and the origin of cosmic rays beyond the Greisen-Zatsepin-Kuzmin barrier

LA Anchordoqui - Physical Review D, 2022 - APS
Very recently, it was pointed out that when basic ideas of the swampland program are
combined with the cosmological hierarchy problem (ie, the smallness of the dark energy in …

Demonstrating agreement between radio and fluorescence measurements of the depth of maximum of extensive air showers at the Pierre Auger Observatory

A Abdul Halim, P Abreu, M Aglietta, I Allekotte… - Physical review …, 2024 - APS
We show, for the first time, radio measurements of the depth of shower maximum (X max) of
air showers induced by cosmic rays that are compared to measurements of the established …

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 …

Overview and first results of EUSO-SPB2

J Eser, AV Olinto, L Wiencke - arXiv preprint arXiv:2308.15693, 2023 - arxiv.org
Observing ultra-high energy cosmic rays (UHECR) and very high energy (VHE) neutrinos
from space is a promising way to measure their extremely low fluxes by significantly …

Ultra high energy cosmic rays from tidal disruption events

T Piran, P Beniamini - Journal of Cosmology and Astroparticle …, 2023 - iopscience.iop.org
The tidal disruption event AT2018hyz, was a regular optically detected one with no special
prompt features. However, almost three years after the disruption it suddenly displayed a fast …

Design and initial performance of the prototype for the BEACON instrument for detection of ultrahigh energy particles

D Southall, C Deaconu, V Decoene, E Oberla… - Nuclear Instruments and …, 2023 - Elsevier
Abstract The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a planned
neutrino telescope designed to detect radio emission from upgoing air showers generated …