activity
20242026
collaborators

14 papers

physics.space-ph2026

Energetic particle-mediated interplanetary shocks observed by Solar Orbiter

D. Trotta, D. Lario, B. Reville +10

Context: In collisionless shocks, energetic particles can carry sufficient pressure to modify the upstream plasma and the shock structure itself, a regime often invoked in theories…

astro-ph.SR2026

Multi-Dimensional MHD simulations of young Core-Collapse Supernova Remnants

C. J. K. Larkin, J. Mackey, B. Reville +3

Supernova remnants (SNRs) play a central role in shaping the interstellar medium. Core-Collapse Supernova (CCSN) progenitors are massive stars, which produce a dense circumstellar…

astro-ph.HE2026

The diffuse gamma-ray sky of a Milky Way analogue: Local diversity and global constraints

Karin Kjellgren, Philipp Girichidis, Maria Werhahn +8

Diffuse gamma-ray emission is a key tracer of cosmic rays (CRs) in galaxies, encoding information about their transport, energetics, and interactions with the interstellar medium.…

astro-ph.HE2026

How interacting winds shape the mechanical feedback of massive star clusters over millions of years

Thibault Vieu, Lucia Härer, Brian Reville

In recent years, massive star cluster environments have proved to be bright sources of very-high energy gamma-rays, in particular young clusters which are powered by the winds inte…

physics.plasm-ph2026

Measurement of ion acceleration and diffusion in a laser-driven magnetized plasma

J. T. Y. Chu, J. W. D. Halliday, C. Heaton +25

Here we present results from an experiment performed at the GSI Helmholtz Centre for Heavy Ion Research. A mono-energetic beam of chromium ions with initial energies of

astro-ph.HE2025

Spectral curvature and breaks from Fermi acceleration at oblique shocks

Asma Shirin T, Brian Reville, Nils W. Schween +2

A major attraction of diffusive shock acceleration is the prediction of power-law spectra for energetic particle distributions. However, this property is not fundamental to the the…