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Nonideal complex Plasmasin the Universe and in the lab
Michael BonitzInstitut für Theoretische Physik und Astrophysik
Christian-Albrechts-Universität zu Kiel
2nd Summer Institute „Complex Plasmas“, Greifswald, 4 August 2010
PlasmaPlasma
I. Langmuir/L. Tonks (1929): ionized gas - „plasma“
„4th state of matter“: solid fluid gas plasmaideal hot classical gas
made of electrons and ions
= System of many charged particles, dominated by Coulomb interaction
Wikipedia: „More than 99 % of the visible matter in ouruniverse is in the Plasma state“
OccurencesOccurences of Plasmaof PlasmaContemporary Physics Education Project (CPEP)http://www.cpepweb.org/
NonidealLaboratory & astrophysicalplasmas
PlasmaPlasma
I. Langmuir/L. Tonks (1929): ionized gas - „plasma“„4th state of matter“: solid fluid gas plasma
ideal hot classical gasmade of electrons and ions
BUT: there exist unusual („complex“) plasmas which- are „non-ideal“, - often contain non-classical electrons,[- may contain other particles, chemically reactive]
= System of many charged particles, dominated by Coulomb interaction
ContentsContents
1. Introduction: Examples of nonideal plasmas
3. Computer simulations of quantum plasmas
- matter at extreme density
- White dwarf and neutron stars
2. Plasma physics approach to dense matter
Stars in Stars in thethe MilkyMilky wayway
Milky Way Central Bulge, viewed from the inside. It is a vast collection of more than 200 billion stars,
planets, nebulae, clusters, dust and gas.
Stars in Stars in thethe MilkyMilky wayway
Milky Way, Southern part, red emission nebulae, bright star clouds Sagittarius and Scorpius, Red giant Antares
Stars Stars sortedsorted: : schematicschematic
Hertzsprung-Russel-Diagram
Stars Stars sortedsorted: : observationsobservations
22000 stars from the Hipparcos Catalogue together with 1000 low-luminosity stars (red and white dwarfs) from the Gliese Catalogue of Nearby Stars.
Source: Wikipedia
WhyWhy therethere areare different Starsdifferent Stars
• All Stars contain the same matter as we know on Earth
• Origin of different Stars:
- different mixture of elements (composition)- different physical state of matter (temperature, density)- different physical processes (nuclear fusion)
• All Stars undergo similar evolution (only few options)
Compact Stars: Compact Stars: dwarfsdwarfs
• There is a close connection between size R and mass M:
Example water:
R, M 2 R, 8 MconstRM
=ρ
3~
Stars: The smaller a star, the larger its mass!
R, MR/2, 8 M
6
3
~~
−
−
RRM
ρ
White White dwarfsdwarfs• Balance of gravity and Fermi pressure of electrons
3~ −RM
Relativistic electrons
ChandrasekharLimiting mass
Source: Wikipedia
363 10~~
−cmgRM
EARTH
SUNρ
5000km
10000km
0.5M_sun 1.0M_s
Picture of a Picture of a whitewhite dwarfdwarf
White dwarf in the planetary nebula NGC 2440 (“cocoon”)In center of Milky Way. The hottest star? Surface T~200,000KCredit: H. Bond (STSci), R. Ciardullo (PSU), WFPC2, HST, NASA
WhatWhat isis insideinside a a whitewhite dwarfdwarf??
White Dwarf in NGC 2440. 250 time brighter than our Sun Image: Hubble Space Telescope.
• Spectroscopy: Core: carbon, oxygen, …
• Seismology: core crystalline
In In thethe newsnews ((BBC 16 Feb 2004BBC 16 Feb 2004))„Diamond star thrills astronomers“
„Twinkling in the sky is a diamond starof 10 billion trillion trillion carats, astronomers have discovered.“
The cosmic diamond is a chunk of crystallisedcarbon, 4,000 km across, some 50 light-yearsfrom the Earth in the constellation Centaurus. It's the compressed heart of an old star that was once bright like our Sun but has since fadedand shrunk.
Astronomers have decided to call the star "Lucy" after the Beatles song Lucy in the Sky with Diamonds.
White Dwarf BPM 37093,T. Metcalfe, Harvard-Smithsonian
„A diamond that is almost forever“
„The diamond star completely outclassesthe largest diamond on Earth, the 546-carat Golden Jubilee (South Africa).“
DensityDensity of of compactcompact starsstars
• How does matter behave at such extreme densities??
363 10~~
−cmgRM
EARTH
SUNWDρ
The answer is given by plasma physics!
White Dwarfs:(M
OccurencesOccurences of Plasmaof PlasmaContemporary Physics Education Project (CPEP)http://www.cpepweb.org/
White dwarfs
Plasma theory of white dwarfs• Starting in the 1960s: Van Horn, DeWitt, Ichimaru, Chabrier…
• Energy of electron-ion plasma (neutral) in thermodynamic equilibrium:
K – kinetic energy, G – gravitation, U – Coulomb interaction
eiiieeieei UUUGKKH +++++= +
• At extreme densities matter is expected to be fully ionized… (?)
Plasma theory of white dwarfsK – kinetic energy, G – gravitation, U – Coulomb interaction
eiiieeieei UUUGKKH +++++= +U (small)constMnH ≈)]([0
• One-component plasma model (OCP, jellium), TD equilibrium:
[ ]),(1),( ,0 nTKUKUHnTH iiiibacke Γ+=+=−−
Plasma state defined by single „coupling“ parameter
• Electrons exptected to be spatially homogeneous, quantum degenerate, weakly interacting
Thermodynamics of OCP
Classical „one-componentplasma“ (OCP)
Liquid-solid transition below criticaltemperature (above critical couplingstrength).
2D MD simulation of OCP cooling/heating,Periodic b.c., Torben Ott
See lectures by P. Hartmann and T. Ott
rTke
EU
BKIN
2||==Γ
)137:2(175 Dcr ≈Γ
Predicted by Wigner 1934 for theelectron gas in metals.
Wigner crystals in the laboratory
Tne
rTke
EU
BKIN
3/122||∝==Γ
Ways to achieve:
1. cooling
Need: crΓ≥Γ
Ideal gas behavior
Strongly
coupled
plasma
Wigner
(Coulom
b) cryst
al)
White dwarfs
Physically equivalent systems
Ion crystals in traps1987 first realization in Paul trap and laser cooling (Ca, Mg,…)Bollinger et al. (NIST), Walther et al. (true 1-component plasma)
Today many active groups in Innsbruck (Blatt), Aarhus (Drewsen)…
Ions in storage rings, U. Schramm, LMU München
Drewsen
Ion crystals in traps (2)
Applications: atomic physics, quantum optics, collective excitations, quantum computing…
R. Blatt, Uni Innsbruck
Measured oscillation of bi-crystal, Drewsen, Aarhus
Wigner crystals – solution 2
Tne
rTke
EU
BKIN
3/122||∝==Γ
2. Charge increase
Ways to achieve:
1. cooling
Need: crΓ≥Γ
Ideal gas behavior
Strongly
coupled
plasma
Wigner
(Coulom
b) cryst
al)
Trapped ions
White dwarfs
Physically equivalent systems
StronglyStrongly correlatedcorrelated CoulombCoulomb Systems Systems
Trapped ions
Tne
rTke
EU
BKIN
3/122||∝==ΓNeed: crΓ≥Γ
Ways to achieve:
1. cooling
2. Charge increase
„Dusty plasma“
Lectures on Monday, Tuesday
WignerWigner crystallizationcrystallization byby compressioncompression
Trapped ions
Tne
rTke
EU
BKIN
3/122||∝==ΓNeed: crΓ≥Γ
Ways to achieve:
1. cooling
2. Charge increase
3. compression
Dusty plasmas
semiconductors
MesoscopicMesoscopic quantumquantum CoulombCoulombclustersclusters in in quantumquantum dotsdots
quasi-2-dimensional system,
Density increase quantum („cold“) melting of „crystal“
Phys. Rev. Focus (April 2001), Sciences et Avenir, Scientific American, FAZ 1.8. 2001…
First-principle path integral Monte Carlo results
Prediction of electron crystallization: A.Filinov, MB, Yu. Lozovik, PRL 86, 3851 (2001)
compression
Quantum Quantum couplingcoupling parameterparameter3/1
3/2
3/122
~|| −∝∝=Γ n
nne
rEe
EU
FKIN
QNeed: crsB
sQ r
arr ≥∝=Γ
DeBrogliewave length
Tmkh Bπλ 2/=
r
λ
3λχ n=
Quantum degeneracy
Wigner crystal)2(37...34 Dr crs ≈Ceperley et al.,A. Filinov, MB
Ferm
iliq
uid
Ferm
igas
Universality of one-component plasmas
OCP with same coupling parameter(s) show same behavior
M. Bonitz, Physik Journal 7/8 (2002)
„Artificial atoms“ (electrons in quantum dots)
Noneq.-Green functions-Simulation: Lasse Rosenthal (length 0.001mm, T=1K)
„Mendeleyevtable“
Dusty plasmaexperiments byA. Melzer et al.
Length: 10mm,T~300K
Classical 2D finite Coulomb Clusters
Summary: Universal behavior of OCP
• classical plasma described by single parameter• quantum OCP described by two parameters
Application:
Mapping of white dwarf properties on entirely different laboratory plasmas
Γ
But: does the OCP model apply to real plasmas in stars??
Phase diagram of 2-comp. plasmas
Whitedwarfs
Neutronstars
157,000K~1 RydAtoms, molecules
weakly correlated!
Plasma theory of white dwarfs (2)
K – kinetic energy, G – gravitation, U – Coulomb interaction
eiiieeieei UUUGKKH +++++= +
Include: • Dynamics of electrons (no rigid background)• Formation of atoms, molecules; partial ionization• quantum and spin effects of electrons• quantum and spin effects of ions
Need: Selfconsistent first-principle approach to equilibriumproperties quantum Monte Carlo
Ultradense neutral plasmas
157,000K~1 RydAtoms, molecules
Pressure ionizationof atoms (Mott effect)
classical ion crystal +quantum electron gas
Filinov, Bonitz, Fortov, JETP Letters 72, 245 (2000)
ConditionsConditions forfor TCPTCP CoulombCoulomb crystalscrystals
I. strong ion coupling (OCP): )3(100,175 Drr crsshcr
h ≅≥≅Γ≥Γ
II. no Coulomb bound states:
h
e
e
h
e
h
TT
qqZ
mmM =Θ== ,,
Additional parameters in TCP: mass, charge and temperature asymmetry
2.1/ ≅≤= MottsBese rarr,23 Be EkT ≥
Analytical Results: Bonitz et al. PRL 95, 235006 (2005)
1. Classical system:finite temperature range for crystal orminimum charge Z
secr
B
e
rZ
EkT
ΓΘ
≤≤3/22
32
Quantum Quantum TCPTCP CoulombCoulomb crystalscrystals
h
e
e
h
e
h
TT
qqZ
mmM =Θ== ,,mass, charge and temperature asymmetry
AnalyticalAnalytical ResultsResults (2): Quantum system(2): Quantum system
1)(
)(3/4
−=≥e
Motts
crs
ecr
TrZrTMM• Critical mass ratio:
• Maximum temperature: crs
crB
eB
rMZ
ETk
Γ+Θ
=)1(4
2
• Finite density range: Mottcre
Mott nMMnn
3
11⎟⎠⎞
⎜⎝⎛
++
≤≤
Applies to White dwarf stars
White White dwarfdwarf starstar
D. Schneider, LLNL
classicalfluid and crystalin „quantum sea“of electrons
Size ~ our EarthMass ~ our Sun
density:
ERDEρρ610≅
Diamond???Diamond???„Diamond star thrills astronomers“
White Dwarf BPM 37093,T. Metcalfe, Harvard-Smithsonian
„A diamond that is almost forever“
Diamond:Melting point: 3820K
35.3 −≈ gcmρ
White dwarf:
Crystal of bare C6+ nuclei!
3610 −≈ gcmρ
KT 610≈
WhatWhat happenshappens to to thetheplasmaplasma uponupon furtherfurther
compressioncompression??
FromFrom whitewhite dwarfsdwarfs to to neutronneutron starsstars
Quantum Quantum meltingmelting of of ionion crystalcrystalReduce ion mass from M=1856 to M=100to simulate density increase 2/3
3 ~m
nnΛ=χ
Quantum Quantum meltingmelting of of ionion crystalcrystalReduce ion mass to M=25 and M=5
to simulate density increase
2/33 ~
mnnΛ=χ
Ion liquid Ion gas
Neutron Neutron starstarcrystal and quantum fluidof Fe-nuclei
in „quantum sea“of electrons
Radius ~ 10kmMass ~ our Sun
31510 −≅ cmgρ
Source: Coleman, UMD
Ato
ms
Elec
tron
-ion
plas
ma
e &
nuc
lei
(e &
pro
tons
&) n
eutr
ons
3
17.0fmbaryons
N =ρ
MeVTcmfm
C 175101 13
== −
Dwarfstars
Neutronstars
e &
ion
crys
tal
Compression, de-trapping:new states of charged matter
T_c
FromFrom nucleinuclei to to nuclearnuclear mattermatter
CanCan oneone reproducereproducethethe twotwo--componentcomponent plasmaplasmaof of compactcompact starsstars on Earth?on Earth?
OurOur simulationssimulations predictpredictpossiblepossible systemssystems and and
parametersparameters..
PredictedPredicted parametersparameters of of TCP TCP CoulombCoulomb crystalscrystals
][ 3max−cmn ][max KT][ 3min −cmn
+6C Ions(white dwarfs)
91026102 ⋅ 33106.3 ⋅
Are there candidates for laboratory TCP crystals?
TCP TCP CoulombCoulomb crystalscrystals
][ 3max−cmn ][max KT
Protons(hydrogen)
][ 3min−cmn
+6C Ions(white dwarfs)
91026102 ⋅ 33106.3 ⋅
24105⋅ 28100.1 ⋅ 000,66
Laser or ion beam compression experiments (?)
Lecture by Dirk Gericke
TCP TCP CoulombCoulomb crystalscrystalsin in thethe laboratorylaboratory??
][ 3max−cmn ][max KT
Protons(hydrogen)
Semiconductors(M=100)
][ 3min−cmn
+6C Ions(white dwarfs)
91026102 ⋅ 33106.3 ⋅
24105⋅ 28100.1 ⋅ 000,66
0.920102.1 ⋅ 20101.2 ⋅
Phase Phase diagramdiagram of hole of hole crystalcrystal
Bonitz, Filinov, Fortov, Levashov, and Fehske, Phys. Rev. Lett. 95, 235006 (2005)
Re E
kTT23
=3/11 n
ra
r eB
se
∝=
11++
= crMMK
Θ= 2
1Z
α
)2(60),3(83 DDM cr =• for Z=1 (e.g. electron-hole plasma):
Animation: G. Schubert, M=5,12,25,50,100
Band structure& collective
hole behavior
Increase of M: Increasing hole localization
Hole Fermi gas Fermi liquidWigner crystal
Animation: G. Schubert, M=5,12,25,50,100
Early predictions of hole crystal: Halperin/Rice, Abrikosov, ...PIMC simulations Filinov, Bonitz 2005
Experimental verification?High temp. Superconductivity?
Dec 2 2005Deutschlandfunk, NDR
BBC FocusSuperconductor Weekca. 100 online Science pages.......
New Scientist
Our results in the news
„The Hole crystal“
Ato
ms
Elec
tron
-ion
plas
ma
e &
nuc
lei
(e &
pro
tons
&) n
eutr
ons
3
17.0fmbaryons
N =ρ
MeVTcmfm
C 175101 13
== −
Dwarfstars
Neutronstars
e &
ion
crys
tal
Compression, de-trapping:new states of charged matter
FromFrom nuclearnuclear matter to matter to quarksquarks
Qua
rk-g
luon
plas
ma
Nρ)10...5(deconfinement
T_c
Big bang: Big bang: trappingtrapping of of chargedcharged mattermatter
Source: RHIC web site
Quark-gluon plasma realized at:Relativistic Heavy ion collider, BrookhavenLarge Hadron collider, CERN
Crystal of nuclei, ions
Can one verify this experimentally ?
To produce a quark-gluon plasmahuge densities and
particle energies are needed
big particle colliders in the U.S. and Europeaim at producing and studying the properties
of the quark-gluon plasma
G. Baym
G. Baym
G. Baym
Quark-gluon plasma
It is believed that of the quark-gluon plasmahas been seen at RHIC
(Relativistic Heavy Ion Collider) and will soonbe produced at the LHC at CERN
The particles in the QGP plasma interactvia the (color) Coulomb potential
First results were surprising: the QGP is a non-ideal plasma, liquid-like
New applications of non-ideal plasma physics!See e.g. V. Filinov et al., Contrib. Plasma Phys. 49, 536 (2009)
SummarySummary
One-component plasma model: universal phase diagram, Similar plasma behavior in trapped ions, dusty plasmas etc.
Coulomb crystal in neutral/Two-component plasmas:Ion crystal in Fermi sea of electronshole crystal in semiconductors (for M>80), superconductivity?
http://www.theo-physik.uni-kiel.de/~bonitz
Nonideal plasmas: exist in planets, white dwarf and neutron stars, quark-gluon plasma highly organized, collective particle behavior
SummarySummary
Theoretical approaches to nonideal plasmas:Lecture this afternoon
For more information see:
„Introduction to Complex Plasmas“, M. Bonitz, N. Horing and P. Ludwig (eds.), Springer 2010
http://www.theo-physik.uni-kiel.de/~bonitz
PlasmaOccurences of PlasmaPlasmaContentsOccurences of PlasmaPlasma theory of white dwarfs Plasma theory of white dwarfs Thermodynamics of OCPWigner crystals in the laboratoryIon crystals in trapsIon crystals in traps (2)Wigner crystals – solution 2Strongly correlated Coulomb Systems Wigner crystallization by compression Mesoscopic quantum Coulomb clusters in quantum dots�Quantum coupling parameter Universality of one-component plasmas„Artificial atoms“ (electrons in quantum dots) „Mendeleyev table“ Phase diagram of 2-comp. plasmasPlasma theory of white dwarfs (2) Ultradense neutral plasmasConditions for TCP Coulomb crystalsQuantum TCP Coulomb crystalsWhite dwarf starFrom white dwarfs to neutron starsQuantum melting of ion crystalQuantum melting of ion crystalNeutron starFrom nuclei to nuclear matterPredicted parameters of �TCP Coulomb crystalsTCP Coulomb crystalsTCP Coulomb crystals�in the laboratory?Phase diagram of hole crystalBand structure �& collective �hole behaviorOur results in the newsFrom nuclear matter to quarksBig bang: trapping of charged matterCan one verify this experimentally ?Quark-gluon plasma