activity
20162026
most citedMagnetic field amplification by the Weibel instability at planetary and astrophysical high-Mach-number shocks

50 citations · 410 across the 26 of their papers we have counts for

collaborators

27 papers

physics.plasm-ph2026

PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium

Karol Fulat, Eloise Moore, Mahmoud Alawashra +4

Collisionless shocks are common in astrophysical systems and stand as sites of particle acceleration. While particles at perpendicular shocks may not return to the upstream region,…

astro-ph.HE2025★ 2 cited

Radiative signatures of electron-ion shocks in BL Lac type objects

A. Arbet-Engels, A. Bohdan, F. Rieger +2

Shocks are promising sites of particle acceleration in extragalactic jets. In electron-ion shocks, electrons can be heated up to large Lorentz factors, making them an attractive sc…

astro-ph.HE2025★ 3 cited

Hillas meets Eddington: The case for blazars as ultra-high-energy neutrino sources

Xavier Rodrigues, Frank Rieger, Artem Bohdan +1

Blazars are promising high-energy neutrino source candidates. However, leptohadronic models face challenges in describing neutrino emission within a viable energy budget, and their…

astro-ph.HE2025

Neural Networks for the Analysis of Traced Particles in Kinetic Plasma Simulations

Gabriel Torralba Paz, Artem Bohdan, Jacek Niemiec

Cosmic-ray acceleration processes in astrophysical plasmas are often investigated with fully-kinetic or hybrid kinetic numerical simulations, which enable us to describe a detailed…

physics.space-ph2024

Electrostatic Waves and Electron Holes in Simulations of Low-Mach Quasi-Perpendicular Shocks

Artem Bohdan, Aaron Tran, Lorenzo Sironi +1

Collisionless low Mach number shocks are abundant in astrophysical and space plasma environments, exhibiting complex wave activity and wave-particle interactions. In this paper, we…

astro-ph.HE2024

Diffusive shock acceleration in relativistic, oblique shocks

Allard Jan van Marle, Artem Bohdan, Anabella Araudo +2

Cosmic rays are charged particles that are accelerated to relativistic speeds by astrophysical shocks. Numerical models have been successful in confirming the acceleration process…