activity
20242026
collaborators

6 papers

physics.space-ph2026

Transport of electrons in tangled magnetic fields

Daniel Verscharen, Natasha Jeffrey, Anton Artemyev +6

Cosmic magnetic fields are typically inhomogeneous and often highly tangled due to large-scale plasma flows, turbulence, and instabilities. If the variations in the magnetic field…

astro-ph.HE2025

Cosmic-ray transport in inhomogeneous media

Robert J. Ewart, Patrick Reichherzer, Shuzhe Ren +6

A theory of cosmic-ray transport in multi-phase diffusive media is developed, with the specific application to cases in which the cosmic-ray diffusion coefficient has large spatial…

astro-ph.HE2025

Self-Similar Cosmic-Ray Transport in High-Resolution Magnetohydrodynamic Turbulence

Philipp Kempski, Drummond B. Fielding, Eliot Quataert +5

We study the propagation of cosmic rays (CRs) through a simulation of magnetohydrodynamic (MHD) turbulence at unprecedented resolution of . We drive turbulence that is…

astro-ph.HE2025

Efficient micromirror confinement of sub-TeV cosmic rays in galaxy clusters

Patrick Reichherzer, Archie F. A. Bott, Robert J. Ewart +4

Cosmic rays (CRs) play a pivotal role in shaping the thermal and dynamical properties of astrophysical environments, such as galaxies and galaxy clusters. Recent observations sugge…

astro-ph.HE2024

A Unified Model of Cosmic Ray Propagation and Radio Extreme Scattering Events from Intermittent Interstellar Structures

Philipp Kempski, Dongzi Li, Drummond B. Fielding +5

Intermittent magnetic structures are a plausible candidate for explaining cosmic-ray (CR) diffusion rates derived from observed CR energy spectra. Independently, studies of extreme…

astro-ph.HE2024

Collisionless conduction in a high-beta plasma: a collision operator for whistler turbulence

Evan L. Yerger, Matthew W. Kunz, Archie F. A. Bott +1

The regulation of electron heat transport in high-beta, weakly collisional, magnetized plasma is investigated. A temperature gradient oriented along a mean magnetic field can induc…