collaborators

9 papers

astro-ph.HE2026

Synchrotron-Regulated Relativistic Magnetohydrodynamic Turbulence: Emission, Polarization, and Faraday Rotation

Xiaochen Sun, Luca Comisso, Luca Comisso Lorenzo Sironi +3

Relativistic magnetized plasmas in many high-energy astrophysical systems are both turbulent and strongly radiative, yet their nonlinear dynamics and radiative outcomes remain poor…

astro-ph.HE2026

Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability

Matthew Goodbred, Anatoly Spitkovsky

The diocotron instability is a non-axisymmetric plasma instability that should occur generically in the differentially rotating equatorial plane of pulsar magnetospheres. We presen…

astro-ph.HE2026

Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring

Jasmine Parsons, Anatoly Spitkovsky, Alexander Philippov +1

We present the first 3D global kinetic simulations of the interacting magnetospheres of pre-merger binary neutron stars. The stars, whose magnetic moments are anti-aligned, twist t…

astro-ph.HE2026

The role of three-dimensional effects on ion injection and acceleration in perpendicular shocks

Luca Orusa, Damiano Caprioli, Lorenzo Sironi +1

Understanding the conditions that enable particle acceleration at non-relativistic collisionless shocks is essential to unveil the origin of cosmic rays. We employ 2D and 3D hybrid…

astro-ph.HE2026

Synchrotron-cooled plasma distribution in the outer magnetosphere of a neutron star

Mikhail V. Medvedev, Anatoly Spitkovsky, Alexander Philippov

The guiding center formalism is employed to analyze the motion of a charged relativistic particle in an inhomogeneous magnetic field, subject to magnetic mirroring and energy loss…

astro-ph.HE2025

Particle Acceleration in Magnetized Shear-Driven Turbulence

Mingxuan Liu, Mateusz Ruszkowski, Ellen Zweibel +5

Shear flows, ubiquitous in space and astrophysical plasmas, can accelerate particles through turbulence excited by the Kelvin-Helmholtz instability. We present the first numerical…