activity
20242026
collaborators

17 papers

physics.plasm-ph2026

Divergence Without Transition in Adiabatic Theory: Exact Cancellation in Reflectionless Potentials

Amitava Bhattacharjee

Adiabatic invariants play a central role in plasma physics, from magnetic moment and bounce action to wave action in slowly varying media. Their perturbative constructions are ofte…

physics.plasm-ph2026

Local relaxation and scale-dependent alignment in compressible, magnetized turbulence

James R. Beattie, Amitava Bhattacharjee

Driven net- and no-net-flux MHD turbulence simulations up to reveal sign-mixed velocity-magnetic, velocity-vorticity, and magnetic-current aligned patches below the en…

physics.plasm-ph2026

Optical analogy for stellarators: Ridges as caustics and coils as singularities

Wrick Sengupta, Stefan Buller, Rogerio Jorge +7

A common feature of most numerically optimized stellarator geometries is the presence of sharp ridges on outer flux surfaces, irrespective of the rotational transform. Despite thei…

physics.plasm-ph2026

Topological Arrest of Ballooning Modes in Non-Axisymmetric Plasmas

Amitava Bhattacharjee

Why do non-axisymmetric stellarators avoid ballooning crashes that afflict tokamaks? Three-dimensional geometry induces Anderson localization of ballooning modes, converting a glob…

physics.plasm-ph2026

Anderson Localization of Ion-Temperature-Gradient Modes and Ion Temperature Clamping in Aperiodic Stellarators

Amitava Bhattacharjee

Ion temperature clamping -- the saturation of the ion temperature regardless of heating power -- is observed across stellarator experiments. We propose a minimal model based on And…

astro-ph.HE2026

Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations

Uddipan Banik, Amitava Bhattacharjee, James M. Stone

Long-period cyclic reversals of the large-scale magnetic field are a prominent feature of the dynamo associated with the magnetorotational instability (MRI) in accretion disks, but…