activity
20182026
most citedNonlinear Evolution of Instabilities Between Dust and Sound Waves

22 citations · 65 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2026

RAMSES-GPU: Cell-by-Cell Adaptive Mesh Refinement with Magneto-Hydrodynamics and Self-Gravity on Graphics Processing Units

Romain Teyssier, Eric Moseley, Robert V. Caddy +9

We present the implementation and optimization of the cosmological simulation code RAMSES on Graphics Processing Units (GPUs) using CUDA Fortran. This accelerated version ports the…

astro-ph.GA2026

Itô tracers: continuous-trajectory Lagrangian particles for Eulerian hydrodynamics

Eric R. Moseley, R. Teyssier, Tom Abel

Lagrangian tracer particles have long been used to track the history of individual gas parcels in hydrodynamical codes. Particles advected by the cell-centered velocity carry no re…

astro-ph.GA2026

Nonlinear Saturation of the Acoustic Resonant Drag Instability

Ben Y. Israeli, Jonathan Squire, Eric Moseley +1

Resonant drag instabilities (RDIs) are a novel type of dust/fluid instability relevant to a diverse range of astrophysical environments. They are driven by a resonant interaction b…

astro-ph.GA2025

Cosmic ray and plasma coupling for isothermal supersonic turbulence in the magnetized interstellar medium

Matt L. Sampson, James R. Beattie, Romain Teyssier +5

Cosmic rays (CRs) are an integral part of the non-thermal pressure budget in the interstellar medium (ISM) and are the leading-order ionization mechanism in cold molecular clouds.…

astro-ph.GA2024★ 3 cited

Dust dynamics in RAMSES -- II. Equilibrium drift velocity distributions of charged dust grains

Eric R. Moseley, Romain Teyssier

We investigate the gas-grain relative drift velocity distributions of charged astrophysical dust grains in MHD turbulence. We do this using a range of MHD-PIC simulations spanning…

astro-ph.GA2022★ 19 cited

Dust dynamics in RAMSES -- I. Methods and turbulent acceleration

Eric R. Moseley, Romain Teyssier, B. T. Draine

Supernova ejecta and stellar winds are believed to produce interstellar dust grains with relatively large sizes. Smaller grains can be produced via the shattering of large grains t…

astro-ph.GA2020★ 21 cited

Turbulent dissipation, CH abundance, H line luminosities, and polarization in the cold neutral medium

Eric R. Moseley, B. T. Draine, Kengo Tomida +1

In the cold neutral medium, high out-of-equilibrium temperatures are created by intermittent dissipation processes, including shocks, viscous heating, and ambipolar diffusion. The…

astro-ph.GA2018★ 22 cited

Nonlinear Evolution of Instabilities Between Dust and Sound Waves

Eric R. Moseley, Jonathan Squire, Philip F. Hopkins

We study the non-linear evolution of the acoustic 'Resonant Drag Instability' (RDI) using numerical simulations. The acoustic RDI is excited in a dust-gas mixture when dust grains…