activity
20242026
collaborators

12 papers

physics.space-ph2026

High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields

Daniela Maci, Rony Keppens, Fabio Bacchini

The understanding and modeling of high-energy particles transport in turbulent magnetic fields is an important open question in space- and astrophysics. The multiscale, nonlinear n…

astro-ph.SR2026

Nonthermal electron acceleration in turbulent post-flare coronal loops

Clarissa Mora, Fabio Bacchini, Rony Keppens

The generation of nonthermal electrons during solar flares plays a critical role in energy transport from the corona to the chromosphere, producing regions of observed intense X-ra…

physics.space-ph2026

Comparing Simulated and Observed Particle Energy Distributions through Magnetic Reconnection in Earth's Magnetotail

Nadja Reisinger, Fabio Bacchini

Magnetic reconnection is an explosive process that accelerates particles to high energies in Earth's magnetosphere, offering a unique natural laboratory to study this phenomenon. T…

astro-ph.IM2025

EuroHPC SPACE CoE: Redesigning Scalable Parallel Astrophysical Codes for Exascale

Nitin Shukla, Alessandro Romeo, Caterina Caravita +36

High Performance Computing (HPC) based simulations are crucial in Astrophysics and Cosmology (A&C), helping scientists investigate and understand complex astrophysical phenomena. T…

cs.DC2025

Towards Exascale Computing for Astrophysical Simulation Leveraging the Leonardo EuroHPC System

Nitin Shukla, Alessandro Romeo, Caterina Caravita +16

Developing and redesigning astrophysical, cosmological, and space plasma numerical codes for existing and next-generation accelerators is critical for enabling large-scale simulati…

physics.plasm-ph2025

Driven Collisionless Reconnection of Force-free Flux Tubes: From Onset to Coalescence

Camille Granier, Daniel Groselj, Luca Comisso +1

We investigate the onset of driven collisionless reconnection and plasmoid formation in a magnetically dominated pair plasma, using 2D Particle-in-Cell simulations. Two force-free…