collaborators

12 papers

physics.flu-dyn2026

Transition to dilatation-dominated isothermal compressible turbulence

Shadab Alam, Christoph Federrath, Jörg Schumacher

The kinetic energy dissipation rate is of central importance for small-scale statistics in turbulent flows. Here, we report a transition to the dilatation-dominated regime of three…

astro-ph.GA2026

The statistics and structure of dissipation in subsonic and supersonic turbulence

Edward Troccoli, Christoph Federrath

Turbulence plays a critical role in the atmosphere, oceans, engineering, and astrophysics. The dissipation (heating) induced by turbulent flows is particularly important for the th…

astro-ph.GA2025

ACES: The Magnetic Field in Large Filaments in the Galactic Center

Dylan M. Paré, Zi-Xuan Feng, Yue Hu +33

The Galactic Center (GC) is an extreme region of the Milky Way that is host to a complex set of thermal and non-thermal structures. In particular, the GC contains high-density gas…

physics.flu-dyn2025

Mitigating numerical dissipation in simulations of subsonic turbulent flows

James Watt, Christoph Federrath, Claudius Birke +1

Magnetohydrodynamic (MHD) simulations of subsonic (Mach number~) turbulence are crucial to our understanding of several processes including oceanic and atmospheric flows, the a…

physics.flu-dyn2025

Conservation of magnetic-helicity fluctuations due to spatial decorrelation of fluxes in decaying MHD turbulence

Justin Kin Jun Hew, David N. Hosking, Christoph Federrath +2

Hosking & Schekochihin (2021, Phys. Rev. X 11, 041005) have proposed that statistically isotropic decaying MHD turbulence without net magnetic helicity conserves the mean square fl…

physics.flu-dyn2025

Statistical properties of compressible isothermal turbulence from sub- to supersonic conditions

F. Thiesset, C. Federrath

This paper investigates the statistical properties of isothermal turbulence in both the subsonic and supersonic regimes. The focus is on the influence of the Mach number () and…