collaborators

5 papers

physics.plasm-ph2025

Grid instability growth rates for explicit, electrostatic momentum- and energy-conserving particle-in-cell algorithms

Luke C Adams, Gregory R Werner, John R Cary

When the Debye length is not resolved in a simulation using the most common particle-in-cell (PIC) algorithm, the plasma will unphysically heat until the Debye length becomes resol…

physics.plasm-ph2025

Suppressing grid instability and noise in particle-in-cell simulation by smoothing

Gregory R. Werner, Luke C. Adams, John R. Cary

Smoothing short-wavelength charge density variations can stabilize explicit electrostatic particle-in-cell (PIC) plasma simulations against grid heating and cold beam instabilities…

astro-ph.HE2025

First-principles measurement of ion and electron energization in collisionless accretion flow

Evgeny A. Gorbunov, Fabio Bacchini, Vladimir Zhdankin +3

We present the largest 3D Particle-in-Cell shearing-box simulations of turbulence driven by the magnetorotational instability, for the first time employing the realistic proton-to-…

astro-ph.HE2025

Energy Diffusion and Advection Coefficients in Kinetic Simulations of Relativistic Plasma Turbulence

Kai W. Wong, Vladimir Zhdankin, Dmitri A. Uzdensky +2

Turbulent, relativistic nonthermal plasmas are ubiquitous in high-energy astrophysical systems, as inferred from broadband nonthermal emission spectra. The underlying turbulent non…

astro-ph.HE2025

Dissipation and particle acceleration in astrophysical jets with velocity and magnetic shear: Interaction of Kelvin-Helmholtz and Drift-Kink Instabilities

Tsun Hin Navin Tsung, Gregory R. Werner, Dmitri A. Uzdensky +1

We present 2D particle-in-cell simulations of a magnetized, collisionless, relativistic pair plasma subjected to combined velocity and magnetic-field shear, a scenario typical for…