Mach Cones in a 2D Dusty Plasma Crystal J. Goree Dept. of Physics and Astronomy, University of Iowa with results from V. Nosenko, Z. Ma, and D. Dubin Supported.

Slides:



Advertisements
Similar presentations
Empirical Rule for Phase Transitions in Dusty Plasma Crystals A.A. Samarian School of Physics, University of Sydney, Sydney, NSW 2006, Australia.
Advertisements

Particle’s Dynamics in Dusty Plasma with Gradients of Dust Charges
Erdem Oz* USC E-164X,E167 Collaboration Plasma Dark Current in Self-Ionized Plasma Wake Field Accelerators
Alex.A. Samarian and Brian.W. James School of Physics, University of Sydney, NSW 2006, Australia Sheath edge location The charge of dust particles in sheath.
Rotating Wall/ Centrifugal Separation John Bollinger, NIST-Boulder Outline ● Penning-Malmberg trap – radial confinement due to angular momentum ● Methods.
Types of Waves Harmonic Waves Sound and Light Waves
Flinders University of South Australia Leon Mitchell Nathan Prior University of Sydney Brian James Alex Samarian Felix Cheung.
Plasmas in Space: From the Surface of the Sun to the Orbit of the Earth Steven R. Spangler, University of Iowa Division of Plasma Physics, American Physical.
electrostatic ion beam trap
Shock wave propagation across the column of dusted glow discharge in different gases. A.S.Baryshnikov, I.V.Basargin, M.V.Chistyakova Ioffe Physico-Technical.
TEST GRAINS AS A NOVEL DIAGNOSTIC TOOL B.W. James, A.A. Samarian and W. Tsang School of Physics, University of Sydney NSW 2006, Australia
Phonons in a 2D Yukawa triangular lattice: linear and nonlinear experiments Dept. of Physics and Astronomy, University of Iowa supported by DOE, NASA,
Chapter 4 Waves in Plasmas 4.1 Representation of Waves 4.2 Group velocity 4.3 Plasma Oscillations 4.4 Electron Plasma Waves 4.5 Sound Waves 4.6 Ion Waves.
F. Cheung, A. Samarian, B. James School of Physics, University of Sydney, NSW 2006, Australia.
Partially ionized gas -contains IONS, ELECTRONS and neutral particles.
Physics of fusion power Lecture 11: Diagnostics / heating.
The Spatiotemporal Evolution of an RF Dusty Plasma: Comparison of Numerical Simulations and Experimental Measurements Steven Girshick, Adam Boies and Pulkit.
Reinisch_ Solar Terrestrial Relations (Cravens, Physics of Solar Systems Plasmas, Cambridge U.P.) Lecture 1- Space Environment –Matter in.
Prof. Reinisch, EEAS / Simple Collision Parameters (1) There are many different types of collisions taking place in a gas. They can be grouped.
Measurement of the Charge of a Particle in a Dusty Plasma Jerome Fung, Swarthmore College July 30, 2004.
Plasma Kinetics around a Dust Grain in an Ion Flow N F Cramer and S V Vladimirov, School of Physics, University of Sydney, S A Maiorov, General Physics.
The Magnetized Dusty Plasma Experiment (MDPX)
Chapter 21 & 22 Electric Charge Coulomb’s Law This force of repulsion or attraction due to the charge properties of objects is called an electrostatic.
Chapter 28 Magnetic Fields Key contents Magnetic fields and the Lorentz force The Hall effect Magnetic force on current The magnetic dipole moment.
4-1 Chap. 7 (Optical Instruments), Chap. 8 (Optical Atomic Spectroscopy) General design of optical instruments Sources of radiation Selection of wavelength.
F. Cheung, A. Samarian, W. Tsang, B. James School of Physics, University of Sydney, NSW 2006, Australia.
ELECTRICITY PHY1013S ELECTRIC FIELDS Gregor Leigh
Physics of Fusion power Lecture4 : Quasi-neutrality Force on the plasma.
F.M.H. Cheung School of Physics, University of Sydney, NSW 2006, Australia.
Transverse optical mode in a 1-D Yukawa chain J. Goree, B. Liu & K. Avinash.
Table Top Plasma Experiments
Electromagnetically Trapped Dusty Plasma Ring R. Sheldon, E. Thomas Jr, D. Gallagher, M. Adrian, M. Abbas, P. Craven & E. Reynolds Wheaton College / National.
Waves and solitons in complex plasma and the MPE - UoL team D. Samsonov The University of Liverpool, Liverpool, UK.
1 Experiments on Shocks and Dust Structures in Dusty Plasmas Robert L. Merlino, Jonathon R. Heinrich, Su-Hyun Kim and John K. Meyer Department of Physics.
Dusty Plasmas in the Laboratory and Space Bob Merlino April 2003 APS Meeting Philadelphia, PA.
Phonon spectrum measured in a 1D Yukawa chain John Goree & Bin Liu.
Complex Plasmas as a Model for the Quark-Gluon-Plasma Liquid
International Microgravity Plasma Facility John Goree The University of Iowa.
Plasmas. The “Fourth State” of the Matter The matter in “ordinary” conditions presents itself in three fundamental states of aggregation: solid, liquid.
Waves: An introduction
Molecular dynamics simulation of strongly coupled QCD plasmas Peter Hartmann 1 Molecular dynamics simulation of strongly coupled QCD plasmas Péter Hartmann.
Direct Numerical Simulations of Non-Equilibrium Dynamics of Colloids Ryoichi Yamamoto Department of Chemical Engineering, Kyoto University Project members:
Crystallisation Experiments with Complex Plasmas M. Rubin-Zuzic 1, G. E. Morfill 1, A. V. Ivlev 1, R. Pompl 1, B. A. Klumov 1, W. Bunk 1, H. M. Thomas.
Molecular Deceleration Georgios Vasilakis. Outline  Why cold molecules are important  Cooling techniques  Molecular deceleration  Principle  Theory.
Dusty plasmas in basic science, astronomy, industry & fusion John Goree The Univ. of Iowa.
Damping of the dust particle oscillations at very low neutral pressure M. Pustylnik, N. Ohno, S.Takamura, R. Smirnov.
Waves in a 2D Dusty Plasma Crystal
Transverse optical mode in a 1-D chain J. Goree, B. Liu & K. Avinash.
Coulomb fission of a charged dust cloud in an afterglow plasma*
LAW OF ELECTRIC CHARGES. WHAT IS AN ELECTRIC CHARGE?
©D.D. Johnson and D. Ceperley MSE485/PHY466/CSE485 1 Scalar Properties, Static Correlations and Order Parameters What do we get out of a simulation?
6E5  Dispersion relation of dust acoustic waves in a DC glow discharge plasma Bob Merlino, Ross Fisher, Univ. Iowa Ed Thomas, Jr. Auburn Univ. Work supported.
--Experimental determinations of radial distribution functions --Potential of Mean Force 1.
Alex Samarian Complex Plasma Laboratory School of Physics, University of Sydney, NSW 2006, Australia
1 Observations of Linear and Nonlinear Dust Acoustic Waves* Bob Merlino, Jon Heinrich Su Hyun Kim and John Meyer Department of Physics and Astronomy The.
Chapter 22 Electric Fields The Electric Field: The Electric Field is a vector field. The electric field, E, consists of a distribution of vectors,
Optically-Excited Waves in 3D Dusty Plasmas John Goree The University of Iowa.
Electrostatics #4 Energy and Electricity Read and Note Pgs Start HW #5.
Non-local Transport of Strongly Coupled Plasmas Satoshi Hamaguchi, Tomoyasu Saigo, and August Wierling Department of Fundamental Energy Science, Kyoto.
Compressional and Shear Wakes in a 2D Dusty Plasma Crystal V. Nosenko, J. Goree & Z.W. Ma Univ. of Iowa A. Piel Univ. of Kiel D. Dubin UCSD.
OPERATED BY STANFORD UNIVERSITY FOR THE U.S. DEPT. OF ENERGY 1 Alexander Novokhatski April 13, 2016 Beam Heating due to Coherent Synchrotron Radiation.
Introduction to Plasma Physics and Plasma-based Acceleration
Participation IAP NAS of Ukraine in understanding of vacuum breakdown phenomena Iaroslava Profatilova, V.Baturin, O. Karpenko.
B. Liu, J. Goree, V. Nosenko, K. Avinash
What is Physics?.
Confining instabilities in a complex plasma S. V. Vladimirov, A. A
Bi-plasma interactions on femtosecond time-scales
X Ray Diffraction © D Hoult 2009.
Chapter 28 Magnetic Fields
Physics 122B Electricity and Magnetism
Presentation transcript:

Mach Cones in a 2D Dusty Plasma Crystal J. Goree Dept. of Physics and Astronomy, University of Iowa with results from V. Nosenko, Z. Ma, and D. Dubin Supported by DOE, NASA, NSF

electrons + ions = plasma What is a dusty plasma? Debye shielding small particle of solid matter becomes negatively charged absorbs electrons and ions

– polymer microspheres –  8  m diameter Particles

Comparison of dusty plasma & pure ion plasmas Similar: repulsive particles Crystals & liquids 2D or 3D suspensions direct imaging laser-manipulation of particles Different - dusty plasma has: gaseous background 10 5  charge no inherent rotation gravity effects Yukawa potential

Gas drag Ion drag Thermophoresis  r 2 Forces Acting on a Particle Coulomb trapping potential inter-particle  r 1 Gravity  r 3

Electrostatic trapping of particles Equipotential contours electrode positive potential electrode With gravity, particles sediment to high-field region  2-D layer possible Without gravity, particles fill 3-D volume QE mg

chamber top-view camera laser illumination side-view camera vacuum chamber

Gas Ar, 15 mTorr RF plasma MHz 20 W Polymer microspheres diameter 8.69  0.17  m Experimental conditions

charge Q  e separation a = 762  46  m Lattice All experiments in this talk: a monolayer of particles  2D physics Triangular lattice with hexagonal symmetry

Pair correlation function  Ordered lattice Many peaks in g(r) Translation order length  9a

Compressional and shear waves

Dispersion relations in 2D triangular lattice

Mach cones (in air) courtesy of D. Dubin Shock wave behind an f-18

Mach cone angle  courtesy of D. Dubin C = U Sin   U

Lateral wake Transverse Wake Wake behind a ship courtesy of D. Dubin

Experimental setup scanning mirror

Data analysis method Trace particle orbits Calculate particle velocity, number density Get top view images of the lattice Determine particle positions

Laser manipulation of particles Ar laser beam W motion of laser spot:  to radiation force direction shown here, || motion is also possible radiation force

Shear wave Mach cone V/C l = 0.51 V

Speed map for compressional Mach cone particle speed v (  m/s)

Lateral wake Transverse Wake Wake behind a ship courtesy of D. Dubin

speed map for compressional Mach cone particle speed v (  m/s)

V/C l = 2.23: compressional wave Mach cone Grey-scale speed map 2 mm Vector velocity map 2 mm  n  t Schlieren map 2 mm  v  vorticity map Big  n/  t  compressional waves small  v  not shear waves

V/C l = 0.51: shear wave Mach cone Grey-scale speed mapVector velocity map  n  t Schlieren map 2 mm  v  vorticity map small  n/  t  not compressional big  v  shear waves

Test of Mach cone angle relation C l = 22.1 mm/s C t = 5.8 mm/s

Comparison to MD simulation MD simulation by Z.W. MaExperiment 2 mm V/C l = 0.51

Compressional & Shear wave Mach cones Scanning parallel to radiation force direction, V/C l = 1.35 Shear wave Mach cone

Theory of wakes in a 2D plasma crystal Dubin, Phys. Plasmas 2000 Wakes with dispersion: c = c(k)   /k Wave equation Phase mixing  cancellation everywhere except where constructive interference occurs (loci of stationary phase)

V/C l > 1: Mach cone and lateral wakes color map experimental  n/  t Schlieren map no fitting parameter  = 1.14 V/C l = 1.21 calculation by Dubin Mach cone lateral

2 mm V/C l < 1: transverse wake transverse  = 1.14 V/C l = 0.51  n/  t Schlieren map

Summary Mach cones were observed in a 2D dusty plasma crystal Shear wave & Compressional Waves Compressional wave: Rich wake structure was observed for both supersonic and undersonic excitation, consisting of multiple lateral and transverse wakes Shear Wave: had a single-cone structure In far field, the wake structure in experiment is comparable to Dubin’s theory of wakes in dusty plasma crystal

Solar system Rings of Saturn Comet tails Basic physics Coulomb crystals Waves Manufacturing Particle contamination (Si wafer processing) Nanomaterial synthesis Who cares about dusty plasmas?

months data in 1999 Dusty plasma publications in APS & AIP journals

Coulomb force –Interparticle interaction is repulsive Coulomb (Yukawa) –External confinement by natural electric fields present in plasma