lecture - superfluidity
DESCRIPTION
Lecture note from Cambrige University.TRANSCRIPT
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Superconductivity andSuperconductivity andQuantum CoherenceQuantum Coherence
Gil Lonzarich Lent Term 2012
Acknowledgements: Christoph Bergemann,John Waldram, David Khmelnitskii,
and, importantly, former students
12 Lectures: Wednesday & Friday 11-12 am, Mott Seminar Room
Three Supervisions, each with one examples sheet
Questions and suggestions are welcome
Complete versions will be made available on the course web site:www-qm.phy.cam.ac.uk/teaching.php
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Superconductivity, once called one of the best understoodmany-body phenomenon in physics, became again 100 yearsafter its discovery a problem full of questions, mysteries and
challenges.
X.-G. Wen, MITQuantum Field Theory of Many Body Systems,
Oxford University Press, 2009
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Literature:Literature:
JF Annett: Superconductivity, Superfluids andCondensates
JR Waldram: Superconductivity of Metalsand Cuprates
AJ Leggett: Quantum Liquids Bose Condensation &Cooper Pairing in Condensed-Matter Systems
R Feynman: Lectures on Physics Volume III
A Altland & B Simons: Condensed Matter Field Theory
CJ Pethick & H Smith: Bose-Einstein Condensation in Dilute Gases
M Tinkham: Introduction to Superconductivity
VV Schmidt: The Physics of Superconductors
GE Volovik: The Universe in a Helium Droplet
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Outline:Outline:
Ginzburg-Landau (GL) Theory of the Superconducting State
Applications of Superconductivity Bose-Einstein Condensates Superfluidity in 4He
Quantum Coherence and Bardeen-Cooper-Schrieffer (BCS) Theory
Unconventional Superconductivityin Advanced Materials
PhenomenologicalGL Theory
MicroscopicBCS Theory
NewDevelopments
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Lecture 1:Lecture 1:
Historical overview Macroscopic manifestation of superconductivity: ,, C/T
Meissner effect and levitation Type-I and type-II superconductivity Superconductivity as an ordered state
introduction to the Ginzburg-Landau theory
Literature: Waldram ch. 4(or equivalent chapters in Annett, Leggett,Schmidt, or Tinkham)
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Timeline:Timeline:
Unconventional superconductors, Unconventional superconductors, includingincludinghigh temperature superconductorshigh temperature superconductors
1970s-now1970s-now
Josephson effect and SQUIDsJosephson effect and SQUIDs1962-641962-64
Superfluidity in Superfluidity in 33HeHe19711971
Ginzburg-Landau theoryGinzburg-Landau theorySuperconducting vorticesSuperconducting vortices
195019501952-571952-57
Prediction of Bose-Einstein condensationPrediction of Bose-Einstein condensation19251925
Superfluidity in Superfluidity in 44HeHeMeissner Meissner effecteffect
1927-381927-3819331933
Cold atomic gases, TopologicalCold atomic gases, Topological phases, phases, 1990s-now1990s-now
BCS & BCS & Bogoliubov Bogoliubov theorytheory19571957
Superconductivity in mercurySuperconductivity in mercury19111911
Liquefaction of HLiquefaction of H22 & & 44He - the crucial stepsHe - the crucial stepsDewar & Dewar & OnnesOnnes
1898-19081898-1908
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Examples of SuperconductorsExamples of Superconductors
24.5 K
39 K
0.5-1.5 K
10 K
9.3 K
4.1 K
UGe2
CeCu2Si2 0.5 KCs3C60 up to ~40 KIron Pnictides up to ~60 KCopper Oxides up to ~160 K
superconducting magnets to ~ 9 TNbTi
superconducting magnets to ~ 20 T
high-Tc s-wave superconductor
Nb3Sn
MgB2
spin-triplet superconductors onthe border of ferromagnetism
Sr2RuO4
highest Tc amongst the elementsNb
first superconductor Tc =Hg
many additional important examples exist
Unconventional spin-singletsuperconductors on border ofMott transitions and/orantiferromagnetism
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Superconducting elements:Superconducting elements:
ww
w.w
ebel
emen
ts.c
om
- e
xam
ple
s sh
eet
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Basic experimental facts:Basic experimental facts:
The resistivity of a superconductor drops to zero below sometransition temperature Tc
Immediate corollary: cant change the magnetic field inside asuperconductor
B = 0 B
Switch on external B:
zero field cooled
0 since ,0 curl curl ==!"!=#
#$$% J
t
B
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What if we cool a superconductor in a magnetic field and thenswitch the field off do we get something like a permanentmagnet?
field cooled
BExperimentally, this does not work even when field cooled, thesuperconductor expels the field!
B
field cooled
This is known as the Meissner effect.Superconductivity arises through athermodynamic phase transition (statedepends only on final conditions, e.g., Tand B).
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The Meissner effect leads to the stunninglevitation effects that underlie many of theproposed technological applications ofsuperconductivity (see examples sheet).
The superconducting state is destroyedabove a critical field Hc
Ideal magnetisation curve
Hc
and so-called type-II superconductivity(which well discuss later)
Hc1 Hc2H
M
NB: These curves apply for amagnetic field along a long rod.
B
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exponential low-Tbehaviour indicative ofenergy gap(explained by BCS)
power-law behaviour atlow-T in unconventionalsuperconductors(to be discussed later)
matching areas means entropy is continuous at Tc: consistentwith second order phase transition
The electronic specific heat around the superconductingtransition temperature Tc:
exponential in simplesuperconductors
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From the form of C/T we find that the entropy S vs. temperaturehas the following form:
T
S
TcThe superconducting state has lower entropy than the normalstate and is therefore the more ordered state. A general theorybased on just a few reasonable assumptions about the orderparameter is remarkably powerful. It describes not justconventional superconductors but also the high-Tcsuperconductors, superfluids, and Bose-Einstein condensates.This is known as Ginzburg-Landau theory.
normal state
superconducting state
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Free energy near a second orderFree energy near a second orderphase transition:phase transition:
For a second order phase transition, the order parametervanishes continuously at Tc. In the conventional description,known as the Landau model, one assumes that sufficiently closeto Tc the free energy density relative to that of the normal statecan be expanded in a Taylor series in the order parameter,
This assumes that the order parameter is real and that the freeenergy density is an even function of the order parameter.
Where is the free energy minimum?
)0(2
42)( >+= !"!
#""f
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Free energy curves:
Pict
ure
cre
dits:
A.
J. S
chofiel
d
> 0 < 0
00
The phase transition takes place at (Tc) = 0. Thus, a powerseries expansion of (T ) around Tc may be expected to havethe following leading form:
f f
0) ( )( >!= aTTa c"
This is consistent, in particular, with a specific heat jump thatcharacterizes most superconductors (examples sheet).
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This is appropriate, e.g., for ferromagnetism where in theuniform magnetization along a given axis. In the Ginzburg-Landau(GL) theory, however, is assumed to be complex rather than realas is the case for a macroscopic wave function. We will see how acomplex order parameter arises naturally from a microscopictheory. The assumptions in the GL theory are:
can be complex-valued
can vary in space but this carries an energy penaltyproportional to
Crucially, couples to the electromagnetic field in the sameway as for an ordinary wavefunction (Feynman III, ch. 21)
Here, A is the magnetic vector potential and q is the relevantcharge, which is found to be q = 2e.
!
"2 # "2
, "4 # "4
2!"
h/iqA!"#"
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This provides the first clue that superconductivity has gotsomething to do with electron pairs.
A final part in the free energy is the relevant magnetic fieldenergy density BM2/20, where BM=B-BE is due to currents in thesuperconductor and BE is due to external sources. (Note thatwhen the material is introduced the total field energy densitychanges from BE2/20 to B2/20, but the part BMBE/0 is taken upby the external sources (Waldram, Ch.6)).
So finally we arrive at the Ginzburg-Landau free energy density:
We have written the free energy so that the gradient terminvolve an effective mass m = 2me , which is consistent withq = 2e. This represents an effective field theory unifyingmatter field & gauge field A (recall B=curlA) in the static limit.
!
f ="#2
+$
2#
4+
1
2m(%ih& + 2eA)# 2+
1
2o( B % BE )
2