Dust coupling parameter of radio-frequency-discharge complex plasma under microgravity conditions
D. I. Zhukhovitskii, V. N. Naumkin, A. I. Khusnulgatin, V. I., Molotkov, and A. M. Lipaev

TL;DR
This study investigates particle oscillations in a dust crystal formed in a microgravity plasma, revealing high isotropy, significant kinetic overheating, and a low coupling parameter that explains phase transitions.
Contribution
It introduces a novel method to determine the dust particle coupling parameter using oscillation data and provides a theoretical interpretation of large oscillation amplitudes under microgravity.
Findings
Coupling parameter is around 100, much lower than expected from gas temperature.
Particles exhibit significant kinetic overheating under stationary conditions.
Theoretical estimates match experimental oscillation data.
Abstract
Oscillation of particles in a dust crystal formed in a low-pressure radio-frequency gas discharge under microgravity conditions is studied. Analysis of experimental data obtained in our previous study shows that the oscillations are highly isotropic and nearly homogeneous in the bulk of a dust crystal; oscillations of the neighboring particles are significantly correlated. We demonstrate that the standard deviation of the particle radius-vector along with the local particle number density fully define the coupling parameter of the particle subsystem. The latter proves to be of the order of 100, which is two orders of magnitude lower than the coupling parameter estimated for the Brownian diffusion of particles with the gas temperature. This means significant kinetic overheating of particles under stationary conditions. A theoretical interpretation of the large amplitude of oscillation…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
