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Published on: November 2, 2020
Fluid modeling of void closure in microgravity noble gas complex plasmas
Victor Land1, Lorin S Matthews, Truell W Hyde
1Center for Astrophysics, Space Physics and Engineering Research, Baylor University, Waco, Texas 76798, USA. victor_land@baylor.edu
This study presents a dusty plasma model including noble gases, analyzing void formation. Results map experimental conditions for void-free crystals or void development in complex plasmas.
Area of Science:
- Physics
- Plasma Physics
- Materials Science
Background:
- Dusty plasmas are complex systems with unique phenomena.
- Void formation is a critical factor in dusty plasma crystal structures.
- Noble gases are increasingly used as carrier gases in plasma experiments.
Purpose of the Study:
- To extend a dusty plasma fluid model to include all noble gases.
- To analyze void closure phenomena in complex plasmas across various experimental parameters.
- To map the parameter space influencing void formation and discharge stability.
Main Methods:
- Development of a self-consistent dusty plasma fluid model.
- Incorporation of all noble gases (Helium, Neon, Argon, Krypton, Xenon) as carrier gases.
- Construction of driving potential-pressure maps to delineate different plasma regimes.
Main Results:
- Identification of parameter ranges for isotropic void-free dust crystal formation.
- Determination of conditions leading to void formation within dust crystals.
- Prediction of regions where the plasma discharge is likely to extinguish.
- The model successfully predicts void closure and formation across diverse noble gases.
Conclusions:
- The extended dusty plasma model provides a comprehensive tool for understanding void dynamics.
- Potential-pressure maps are crucial for designing experiments with controlled void formation.
- This research facilitates the optimization of complex plasma experiments utilizing noble gases.
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