activity
20022026
most citedOn the nature of the radial orbit instability in spherically symmetric collisionless stellar systems

27 citations · 93 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2026

A radial basis of massless potential-density pairs

E. V. Polyachenko, I. G. Shukhman

In the matrix method for linear perturbations of spherical stellar systems, the perturbed potential and density are expanded over a set of potential-density pairs. For radial pertu…

astro-ph.GA2026

Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems

E. V. Polyachenko, I. G. Shukhman

The Kalnajs matrix method is a widely used framework for studying the global linear stability and possible Landau damping of collisionless stellar systems. However, for radial pert…

astro-ph.GA2026

A generalized linear matrix method for normal modes in collisionless stellar disks

Evgeny V. Polyachenko, Ilia G. Shukhman

We generalize the linear matrix method for computing normal modes in collisionless stellar disks to distribution functions with sharp edges at zero angular momentum (). The ge…

physics.flu-dyn2026

Landau damping of disturbances in nearly inviscid inflectional shear flows

Evgeny V. Polyachenko, Ilia G. Shukhman, Michael Karp

We investigate the structure of damped two-dimensional perturbations in unstable plane-parallel shear flows with an inflection point. In inviscid flows within the stable wavenumber…

physics.plasm-ph2025

Eigenvalues and Eigenfunctions of Landau Damping Oscillations in Very Weakly Collisional Plasma

Evgeny V. Polyachenko, Ilia G. Shukhman

Landau-damped oscillations in collisionless plasmas, described by van Kampen and Case, are quasi-modes, representing a continuous superposition of singular eigenfunctions, not true…

astro-ph.GA2025★ 1 cited

Dynamics of stellar systems with collisions: eigenvalues and eigenfunctions in nearly collisionless limit

Evgeny V. Polyachenko, Ilia G. Shukhman

We examine the decay of perturbations in an infinite homogeneous self-gravitating model with a Maxwellian distribution function (DF) when weak collisions are present. In collisionl…