activity
20232026
most citedCosmic-ray transport in inhomogeneous media

5 citations · 6 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2026

Suppression of spiral density waves in collisionless accretion flows

Stephen Majeski, Matthew W. Kunz, Jason Dexter

Spiral density waves are ubiquitous phenomena in differentially rotating flows. They are non-modal, non-axisymmetric perturbations that, due to shear in the background flow, posses…

astro-ph.SR2026

White Dwarf Natal Kicks as Velocity-Space Random Walks. I. Fokker-Planck Theory

Stephen Majeski, Dang Pham, Taeho Ryu +2

White dwarfs are the most common end state of stellar evolution, including that of our own Sun, making their formation critical to completing a more comprehensive understanding of…

astro-ph.SR2026

White Dwarf Natal Kicks as Velocity-Space Random Walks. II. Binary Stellar Evolution and Observational Kick Constraints

Dang Pham, Stephen Majeski, Taeho Ryu +2

Wide binaries containing white dwarfs (WDs) provide a pathway to exploring post-main-sequence (MS) natal kicks associated with asymmetric mass loss. In this work, we develop a bina…

astro-ph.GA2026

Reduced Effective Viscosity from Anisotropic Transport and Plasma Instabilities in the Sloshing Cores of Galaxy Clusters

John A. ZuHone, Stephen Majeski, Annie Heinrich +3

The G magnetic field in the intracluster medium (ICM) introduces a pressure anisotropy with respect to the magnetic field's direction that manifests as an anisotropic visco…

astro-ph.HE2025★ 5 cited

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.HE2024★ 1 cited

Self-organization in collisionless, high- turbulence

S. Majeski, M. W. Kunz, J. Squire

The MHD equations, as a collisional fluid model that remains in local thermodynamic equilibrium (LTE), have long been used to describe turbulence in myriad space and astrophysical…

astro-ph.HE2023

On hydromagnetic wave interactions in collisionless, high- plasmas

Stephen Majeski, Matthew W. Kunz

We describe the interaction of parallel-propagating Alfvén waves with ion-acoustic waves and other Alfvén waves, in magnetized, high- collisionless plasmas. This is accomplished…

astro-ph.HE2023

Microphysically modified magnetosonic modes in collisionless, high- plasmas

Stephen Majeski, Matthew W. Kunz, Jonathan Squire

With the support of hybrid-kinetic simulations and analytic theory, we describe the nonlinear behaviour of long-wavelength non-propagating (NP) modes and fast magnetosonic waves in…