activity
20182026
collaborators

6 papers

physics.plasm-ph2026

Collisionless whistler heat-flux instability in ultra-high- plasmas

Rhisiart Davies, Prakriti Pal Choudhury, Archie F. A. Bott

Kinetic instabilities, notably the whistler heat-flux instability (WHFI), are known to suppress thermal transport significantly in the moderate- to high- plasmas relevant to man…

astro-ph.GA2026

Latent thermal instability

Prakriti Pal Choudhury, Archie F. A. Bott

Multiscale temperature fluctuations are abundant in the intracluster medium (ICM) outside of galaxy cluster cores (). Their origin is often attributed to turbul…

physics.plasm-ph2025

Modeling transport in weakly collisional plasmas using thermodynamic forcing

Prakriti Pal Choudhury, Archie F. A. Bott

How momentum, energy, and magnetic fields are transported in the presence of macroscopic gradients is a fundamental question in plasma physics. Answering this question is especiall…

astro-ph.GA2024

Cold fronts in galaxy clusters I: A case for the large-scale global eigen modes in unmagnetized and weakly magnetized cluster core

Prakriti Pal Choudhury, Christopher S. Reynolds

Galaxy clusters show large-scale azimuthal X-ray surface brightness fluctuations known as cold fronts. Cold fronts are argued to originate due to sloshing driven by sub-halo passag…

astro-ph.GA2020

Shatter or not: role of temperature and metallicity in the evolution of thermal instability

Hitesh Kishore Das, Prakriti Pal Choudhury, Prateek Sharma

We test how metallicity variation (a background gradient and fluctuations) affects the physics of local thermal instability using analytical calculations and idealized, high-resolu…

astro-ph.GA2018

A 1-dimensional hydrodynamic model for accretion, cooling and heating of gas in dark matter halos from to

Prakriti Pal Choudhury, Guinevere Kauffmann, Prateek Sharma

We study an idealized 1D model for the evolution of hot gas in dark matter halos for redshifts . We introduce a numerical setup incorporating cosmological accretion of gas…