Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session TP11: Poster Session VII: Basic Plasma Physics: Pure Electron Plasma, Strongly Coupled Plasmas, Self-Organization, Elementary Processes, Dusty Plasmas, Sheaths, Shocks, and Sources; Mini-conference on Nonlinear Waves and Processes in Space Plasmas - Posters; MHD and Stability, Transients (2), Runaway Electrons; NSTX-U; Spherical Tokamaks; Analytical and Computational Techniques; Diagnostics (9:30am-12:30pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.TP11.21
Abstract: TP11.00021 : Transitions between reciprocal and non-reciprocal interactions in complex plasmas*
Presenter:
Lori Scott
(Auburn University)
Authors:
Lori Scott
(Auburn University)
Edward E Thomas
(Auburn University)
Uwe Konopka
(Auburn University)
Jeremiah D Williams
(Wittenberg University)
Mikhail Y Pustylnik
(Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR))
Hubertus Thomas
(Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR))
Complex plasmas are composed of electrons, ions, neutrals, and micron-sized, charged particles (dust). Under microgravity conditions, the dust particles can fill the plasma volume, which enables the study of small-scale inter-dust forces. In this work, we seek to determine how the thermodynamic properties of a complex plasma evolve when the inter-particle potential is modified from a non-reciprocal to a reciprocal structure. In the Plasma Kristall-4 (PK-4) microgravity laboratory on the International Space Station (ISS), particles are injected into a dc glow discharge plasma and flow along an axial electric field. Upon the application of a periodic oscillation of the electric field ("polarity switching"), there is change in the spatial ordering of the particles. This presentation discusses initial results from molecular dynamics simulations that are motivated by these experiments. It is shown that modifying the interaction potential affects the spatial ordering and thermal properties of a dusty plasma. This presentation will also present supporting experimental results on these processes.
*We acknowledge the use of the joint ESA-ROSCOSMOS Experiment «PK-4» on-board the ISS. This work is supported by funding from NASA/JPL, NSF, NSF EPSCOR, and DLR/BMWi.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.21
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