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University of Sydney
School of Mathematics and Statistics
Dr Neil Cramer
School of Physics, University of Sydney
The Physics of Dusty Plasmas
Wednesday, 30th August, 2-3pm, Carslaw 173.
Charged macroparticles such as dust grains are a common component of
laboratory, space and astrophysical plasmas. The presence of these
particles causes significant changes to a plasma's behaviour. A
gaseous plasma made up of ions, electrons and charged macroparticles
is also called a complex plasma, or a colloidal plasma, in analogy
with liquid colloidal suspensions. The particulates may range in size
from nanometres to micrometres, and are usually negatively charged due
to the attachment of some of the background plasma electrons on their
surface. An appreciable fraction of the negative charge in an overall
neutral plasma may reside on the macroparticles, which are coupled to
the ions and electrons in the plasma via electric and magnetic fields.
In discharges, charged dust can accumulate in sheath regions where
electrostatic forces balance the forces due to gravity, ion drag and
gas flow.
Laboratory dusty plasmas are usually strongly coupled, i.e. their
interaction energy is greater than their thermal energy. The particles
can form themselves into an ordered crystal structure known as a
Coulomb crystal, which may provide a macroscopic model for phase
transition studies. The theory and experimental results for dusty
plasmas are reviewed in this talk.
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