collaborators

10 papers

astro-ph.IM2026

A fast spectral-multigrid Poisson solver in non-Cartesian geometries

Ankush Mandal, Oliver Gressel, Udo Ziegler +1

Accurate and efficient computation of self-gravity is essential in astrophysical fluid dynamics, particularly in spherical and cylindrical geometries where large radial dynamic ran…

cs.DC2026

On the Limits of Performance Portability in Directive-Based GPU Programming

Alessandro Romeo, Nitin Shukla, Stefano Truzzi +2

The transition of scientific applications to GPU-accelerated exascale systems is constrained by trade-offs between performance, portability, and productivity. This work evaluates t…

astro-ph.HE2026

The PLUTO Code on GPUs: Offloading Lagrangian Particle Methods

Alessio Suriano, Stefano Truzzi, Agnese Costa +5

The Lagrangian Particles (LP) module of the PLUTO code offers a powerful simulation tool to predict the non-thermal emission produced by shock accelerated particles in large-scale…

astro-ph.HE2026

2D or not 2D? Exploring 3D relativistic magnetic reconnection dynamics with highly accurate numerical simulations

Vittoria Berta, Matteo Bugli, Andrea Mignone +3

Fast reconnection in magnetically dominated plasmas is widely invoked in models of dissipation in pulsar winds, gamma-ray flares in the Crab nebula, and to explain the radio nanosh…

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…

physics.plasm-ph2025

The PLUTO Code on GPUs: A First Look at Eulerian MHD Methods

Marco Rossazza, Andrea Mignone, Matteo Bugli +7

We present preliminary performance results of gPLUTO, the new GPU-optimized implementation of the PLUTO code for computational plasma astrophysics. Like its predecessor, gPLUTO emp…