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Bibliographic Details
Main Author: Tacu, Mikael
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2504.10382
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author Tacu, Mikael
author_facet Tacu, Mikael
contents We derive analytic dispersion relations for cold, orbitally constrained systems governed by the Vlasov equation. For magnetized plasmas, we obtain the first explicit relation for two-dimensional anisotropic BGK modes with finite magnetic field, showing that only a finite number of angular modes can become unstable and identifying a magnetic-field threshold for stabilization. In the gravitational case, we establish a bound on the growth rate of core perturbations, set by the potential's curvature. These results clarify how orbital constraints shape the spectrum and growth of kinetic instabilities in cold, collisionless media.
format Preprint
id arxiv_https___arxiv_org_abs_2504_10382
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Why Cold BGK Modes Are So Cool: Dispersion Relations from Orbit-Constrained Distribution Functions
Tacu, Mikael
Plasma Physics
Astrophysics of Galaxies
We derive analytic dispersion relations for cold, orbitally constrained systems governed by the Vlasov equation. For magnetized plasmas, we obtain the first explicit relation for two-dimensional anisotropic BGK modes with finite magnetic field, showing that only a finite number of angular modes can become unstable and identifying a magnetic-field threshold for stabilization. In the gravitational case, we establish a bound on the growth rate of core perturbations, set by the potential's curvature. These results clarify how orbital constraints shape the spectrum and growth of kinetic instabilities in cold, collisionless media.
title Why Cold BGK Modes Are So Cool: Dispersion Relations from Orbit-Constrained Distribution Functions
topic Plasma Physics
Astrophysics of Galaxies
url https://arxiv.org/abs/2504.10382