activity
20192026
most citedCosmic ray transport in large-amplitude turbulence with small-scale field reversals

60 citations · 270 across the 15 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

9 papers · 1 filter

astro-ph.HE2025

Intermittency in Collisionless Large-Amplitude Turbulence

Ryan Golant, Luca Comisso, Philipp Kempski +1

Large-amplitude turbulence -- characterized by a fluctuating magnetic field component, , that is stronger than the mean component, -- is generically intermittent, populat…

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.HE2024★ 2 cited

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.HE2023★ 17 cited

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.HE2023★ 1 cited

Galactic Cosmic-ray Scattering due to Intermittent Structures

Iryna S. Butsky, Philip F. Hopkins, Philipp Kempski +3

Cosmic rays (CRs) with energies TeV comprise a significant component of the interstellar medium (ISM). Major uncertainties in CR behavior on observable scales (much larger th…

astro-ph.HE2023★ 60 cited

Cosmic ray transport in large-amplitude turbulence with small-scale field reversals

Philipp Kempski, Drummond B. Fielding, Eliot Quataert +4

The nature of cosmic ray (CR) transport in the Milky Way remains elusive. The predictions of current micro-physical CR transport models in magneto-hydrodynamic (MHD) turbulence are…

astro-ph.HE2021★ 54 cited

Reconciling cosmic-ray transport theory with phenomenological models motivated by Milky-Way data

Philipp Kempski, Eliot Quataert

Phenomenological models of cosmic-ray (CR) transport in the Milky Way (MW) can reproduce a wide range of observations assuming that CRs scatter off of magnetic-field fluctuations w…

astro-ph.HE2020★ 28 cited

The impact of astrophysical dust grains on the confinement of cosmic rays

Jonathan Squire, Philip F Hopkins, Eliot Quataert +1

We argue that charged dust grains could significantly impact the confinement and transport of galactic cosmic rays. For sub-GeV to ~1000GeV cosmic rays, small-scale parallel Alfvén…

astro-ph.HE2019★ 25 cited

Shearing-box simulations of MRI-driven turbulence in weakly collisional accretion discs

Philipp Kempski, Eliot Quataert, Jonathan Squire +1

We present a systematic shearing-box investigation of MRI-driven turbulence in a weakly collisional plasma by including the effects of an anisotropic pressure stress, i.e. anisotro…