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astro-ph.GA2025

Collisionless relaxation to equilibrium distributions in cold dark matter halos: origin of the Navarro-Frenk-White profile

Uddipan Banik, Amitava Bhattacharjee

Collisionless self-gravitating systems such as cold dark matter halos are known to harbor universal density profiles despite the intricate non-linear physics of hierarchical struct…

astro-ph.SR2025

Universal power-law distribution functions in an electromagnetic kinetic plasma: implications for the inverted temperature profile in the solar corona

Uddipan Banik, Amitava Bhattacharjee

We develop a self-consistent quasilinear theory for the relaxation of electromagnetic kinetic plasmas, and demonstrate that the mean distribution functions of both electrons and io…

astro-ph.GA2025

Taking control of compressible modes: bulk viscosity and the turbulent dynamo

James R. Beattie, Christoph Federrath, Neco Kriel +2

Many polyatomic astrophysical plasmas are compressible and out of chemical and thermal equilibrium, introducing a bulk viscosity into the plasma via the internal degrees of freedom…

astro-ph.GA2025

A self-consistent quasilinear theory for collisionless relaxation to universal quasi-steady state attractors in cold dark matter halos

Uddipan Banik, Amitava Bhattacharjee

Collisionless self-gravitating systems, e.g., cold dark matter halos, harbor universal density profiles despite the intricate non-linear physics of hierarchical structure formation…

astro-ph.GA2025

The spectrum of magnetized turbulence in the interstellar medium

James R. Beattie, Christoph Federrath, Ralf S. Klessen +2

The interstellar medium (ISM) of our Galaxy is magnetized, compressible and turbulent, influencing many key ISM properties, like star formation, cosmic ray transport, and metal and…

astro-ph.SR2025

Density fluctuation-Mach number scaling in compressible, high plasma beta turbulence: in-situ space observations and high-Reynolds number simulations

Riddhi Bandyopadhyay, James R. Beattie, Amitava Bhattacharjee

Understanding the nature of compressible fluctuations in a broad range of turbulent plasmas, from the intracluster medium to the solar wind, has been an active field of research in…