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 …

Triggering Higgs vacuum decay

A Strumia - Journal of High Energy Physics, 2023 - Springer
A bstract The Standard Model Higgs potential seems unstable at field values h> h top~ 10
10 GeV. Vacuum decay can be triggered by N~ 4π/λ~ 1000 overlapped Higgs bosons with …

[PDF][PDF] CRPropa 3.2: a framework for high-energy astroparticle propagation

R Alves Batista, JB Tjus, J Dörner, A Dundovic… - 2022 - repository.ubn.ru.nl
In the last decade, a wealth of observations of energetic astrophysical phenomena were
delivered with unprecedented precision. At ultra-high energies, the Pierre Auger and the …

Ultra-High-Energy Cosmic Rays: Scientific Motivation

K Fang - Large Area Networked Detectors for Particle …, 2023 - World Scientific
Ultra-high-energy (E> 1018 electron volts) cosmic rays (UHECRs) are the highest energy
particles ever detected by human beings. Decades of measurements have revealed that …

CRPropa 3.2: a framework for high-energy astroparticle propagation

RA Batista, JB Tjus, J Dörner, A Dundovic… - arXiv preprint arXiv …, 2021 - arxiv.org
The landscape of high-and ultra-high-energy astrophysics has changed in the last decade,
in large part owing to the inflow of high-quality data collected by present cosmic-ray, gamma …

Constraints on the population of ultra-high energy cosmic ray sources inferred from the data of the Pierre Auger Observatory

S Marafico - 2022 - theses.hal.science
This thesis focuses on ultra-high energy cosmic rays (UHECRs). The origin of these atomic
nuclei, discovered over a century ago and accelerated to hundreds of EeV, remains a …

[引用][C] Snowmass2021-Letter of Interest Establishing ultra-high-energy cosmic rays as a cutting-edge courier of the multi-messenger program

L Anchordoqui, T Bister, J Biteau, L Caccianiga