collaborators

6 papers

astro-ph.HE2026

Entity -- Hardware-agnostic Particle-in-Cell Code for Plasma Astrophysics. III: Higher-order shape functions & generalized field stencils

Ludwig M. Böss, Arno Vanthieghem, Hayk Hakobyan +2

Modern particle-in-cell (PIC) codes have become an integral tool in plasma astrophysics. As most plasma phenomena grow from initially small instabilities, it is important to ensure…

astro-ph.HE2026

Superluminal Wave Activation at Relativistic Magnetized Shocks

Jens F. Mahlmann, Logan Eskildsen, Arno Vanthieghem +2

Fast radio bursts (FRBs) are extremely energetic radio transients, some are generated in magnetar magnetospheres and winds. Despite a growing number of observations, their emission…

astro-ph.HE2025

Entity -- Hardware-agnostic Particle-in-Cell Code for Plasma Astrophysics. I: Curvilinear Special Relativistic Module

Hayk Hakobyan, Ludwig M. Böss, Yangyang Cai +8

Entity is a new-generation, fully open-source particle-in-cell (PIC) code developed to overcome key limitations in astrophysical plasma modeling, particularly the extreme separatio…

astro-ph.HE2025

Generation of Large-scale Magnetic Fields Upstream of Gamma-Ray Burst Afterglow Shocks

Ryan Golant, Arno Vanthieghem, Daniel Groselj +1

The origins of the magnetic fields that power gamma-ray burst (GRB) afterglow emission are not fully understood. One possible channel for generating these fields involves the pre-c…

astro-ph.HE2025

Relativistically Magnetized Collisionless Shocks in Pair Plasma: I. Solitons, Chaos, and Thermalization

Arno Vanthieghem, Amir Levinson

In this paper, the first in a series, we present a new theoretical model for the global structure and dissipation of relativistically magnetized collisionless shock waves. Quite re…

astro-ph.HE2025

Fast radio bursts as precursor radio emission from monster shocks

Arno Vanthieghem, Amir Levinson

It has been proposed recently that the breaking of MHD waves in the inner magnetosphere of strongly magnetized neutron stars can power different types of high-energy transients. Mo…