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    SUPERCONDUCTIVITY

    OVERVIEW OF EXPERIMENTAL FACTSEARLY MODELS

    GINZBURG-LANDAU THEORY

    BCS THEORY

    Jean Delayen

    Thomas Jefferson National Accelerator Facility

    Old Dominion University

    USPAS June 2008 U. Maryland

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    Historical Overview

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    Perfect Conductivity

    Unexpected result

    Expectation was the opposite: everything should become an isolator at 0T

    Kamerlingh Onnes and van der Waals in

    Leiden with the helium 'liquefactor' (1908)

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    Perfect Conductivity

    Persistent current experiments on rings have measured

    1510s

    n

    s

    s>

    Perfect conductivity is not superconductivity

    Superconductivity is a phase transition

    A perfect conductor has an infinite relaxation time L/R

    Resistivity < 10-23 .cm

    Decay time > 105 years

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    Perfect Diamagnetism (Meissner & Ochsenfeld 1933)

    0B

    t

    = 0B =

    Perfect conductor Superconductor

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    Penetration Depth in Thin Films

    Very thin films

    Very thick films

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    Critical Field (Type I)

    2

    ( ) (0) 1c cc

    T H T H

    T

    -

    Superconductivity is destroyed by the application of a magnetic field

    Type I or soft superconductors

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    Critical Field (Type II or hard superconductors)

    Expulsion of the magnetic field is complete up to Hc1, and partial up to Hc2

    Between Hc1 and Hc2 the field penetrates in the form if quantized vortices or

    fluxoids

    0 e

    pf =

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    Thermodynamic Properties

    Entropy Specific Heat

    Energy Free Energy

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    Thermodynamic Properties

    ( ) 1

    2

    When phase transition at is of order latent heat

    At transition is of order no latent heat

    jump in specific heat

    st

    c c

    nd

    c

    es

    T T H H T

    T T

    C

    < = fi

    = fi

    3

    ( ) 3 ( )

    ( )

    ( )

    electronic specific heat

    reasonable fit to experimental data

    c en c

    en

    es

    T C T

    C T T

    C T T

    g

    a

    =

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    Thermodynamic Properties

    3 3

    2 200

    3

    3

    : ( ) ( )

    (0) 0

    33

    ( ) ( )

    ( ) ( )

    At The entropy is continuous

    Recall: and

    For

    c c

    c s c n c

    T T

    es

    c c

    s n

    c c

    c s n

    T S T S T

    S CS

    T TT T T

    dt dt C T T T T

    T TS T S T T T

    T T S T S T

    a g ga g

    g g

    =

    = =

    fi = = =

    = =

    < >

    Impure metals

    Alloys

    Local electrodynamics

    Pippard superconductors (Type I)

    >>

    Pure metals Nonlocal electrodynamics

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    Material Parameters for Some Superconductors

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    Phenomenological Models (1930s to 1950s)

    Phenomenological model:

    Purely descriptive

    Everything behaves as though..

    A finite fraction of the electrons form some kind of condensate thatbehaves as a macroscopic system (similar to superfluidity)

    At 0K, condensation is complete

    At Tc the condensate disappears

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    Two Fluid Model Gorter and Casimir

    ( )

    ( ) ( ) ( )

    ( )

    ( )

    ( )

    1/2

    2

    2

    1- :

    ( ) = 1

    1

    2

    1

    4

    gives =

    fractionof "normal"electrons

    fractionof "condensed"electrons (zero entropy)

    Assume: free energy

    independent of temperature

    Minimizationof

    c

    n s

    n

    s c

    C

    T T x

    x

    F T x f T x f T

    f T T

    f T T

    TF T x

    T

    g

    b g

    < =

    + -

    = -

    = - = -

    ( ) ( ) ( )

    C

    4

    4

    1/2

    3

    2

    ( ) 1 1

    T

    3 T

    n s

    C

    es

    TF T x f T x f T

    T

    C

    b

    g

    fi = + - = - +

    fi =

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    Two Fluid Model Gorter and Casimir

    ( ) ( ) ( )

    ( )

    4

    1/2

    2

    2

    2

    2

    ( ) 1 1

    ( ) 22

    8

    1

    Superconducting state:

    Normal state:

    Recall difference in free energy between normal and

    superconducting state

    n s

    C

    nC

    c

    C

    TF T x f T x f T T

    TF T f T T

    T

    H

    T

    T

    b

    g

    b

    p

    b

    = + - = - +

    = = - = -

    =

    = -

    ( )2

    2

    1(0)

    c

    c C

    H T T

    H T

    fi = - The Gorter-Casimir model is an ad hoc model (there is no physical basis for the

    assumed expression for the free energy) but provides a fairly accurate

    representation of experimental results

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    Model of F & H London (1935)

    Proposed a 2-fluid model with a normal fluid and superfluid components

    ns :density of the superfluid component of velocity vsnn:density of the normal component of velocity vn

    2

    superelectrons are accelerated by

    superelectrons

    normal electrons

    s s

    s s

    n n

    m eE E t

    J en

    J n e Et m

    J E

    u

    u

    s

    = -

    = -

    =

    =

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    Model of F & H London (1935)

    2

    2 2

    2

    0 = Constant

    = 0

    Maxwell:

    F&H London postulated:

    s s

    s s

    s s

    s

    s

    J n eE

    t m

    BE

    t

    m m J B J B

    t n e n e

    mJ B

    n e

    =

    = -

    fi + = fi +

    +

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    Model of F & H London (1935)

    combine with 0 sB = Jm

    ( ) [ ]

    22 0

    1

    2

    2

    0

    - 0

    exp /

    s

    o L

    L

    s

    n eB B

    m

    B x B x

    m

    n e

    m

    l

    lm

    =

    = -

    =

    The magnetic field, and the current, decay

    exponentially over a distance (a few 10s of nm)

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    ( ) ( )

    1

    2

    2

    0

    4

    1

    4 2

    1

    10

    1

    From Gorter and Casimir two-fluid model

    L

    s

    s

    C

    L L

    C

    m

    n e

    Tn

    T

    T

    T

    T

    lm

    l l

    =

    -

    =

    -

    Model of F & H London (1935)

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    Model of F & H London (1935)

    2

    0

    2

    0, 0

    1

    London Equation:

    choose on sample surface (London gauge)

    Note: Local relationship between and

    s

    n

    s

    s

    BJ H

    A H

    A A

    J A

    J A

    lm

    l

    = - = -

    = = =

    = -

    i

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    Penetration Depth in Thin Films

    Very thin films

    Very thick films

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    Quantum Mechanical Basis for London Equation

    ( ) ( ) ( )

    ( )

    ( )( )

    ( )

    ( )

    2* * *

    1

    0

    2

    2

    0 0 ,In zero field

    Assume is "rigid", ie the field has no effect on wave function

    n n n n n

    n

    e e J r A r r r dr dr

    mi mc

    A J r

    r e J r A r

    m e

    r n

    y y y y y y d

    y y

    y

    r

    r

    = - - - -

    = = =

    = -

    =

    f

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    Pippards Extension of Londons ModelObservations:

    -Penetration depth increased with reduced mean free path

    - Hc and Tc did not change

    - Need for a positive surface energy over 10-4

    cm toexplain existence of normal and superconducting phase in

    intermediate state

    Non-local modification of London equation

    ( ) ( )40

    0

    1-

    3

    4

    1 1 1

    Local:

    Non local:

    R

    J Ac

    R R A r e J r d

    c R

    x

    l

    s upx l

    x x

    -

    =

    = -

    = +

    i

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    London and Pippard KernelsApply Fourier transform to relationship between

    ( ) ( ) ( ) ( ) ( ):4

    andc

    J r A r J k K k A k p

    = -

    ( ) ( )22

    2

    ln 1

    Specular: Diffuse:eff eff o

    o

    dk

    K k k K kdk

    k

    pl l

    p

    = =

    + +

    Effective penetration depth

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    London Electrodynamics

    Linear London equations

    together with Maxwell equations

    describe the electrodynamics of superconductors at all T if: The superfluid density nsis spatially uniform

    The current density Js is small

    2

    2 2

    0

    10s

    J EH H

    t l m l

    = - - =

    0s

    H H J E t

    m = = -

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    Ginzburg-Landau Theory

    Many important phenomena in superconductivity occur

    because ns is not uniform

    Interfaces between normal and superconductors

    Trapped flux

    Intermediate state

    London model does not provide an explanation for the

    surface energy (which can be positive or negative)

    GL is a generalization of the London model but it still

    retain the local approximation of the electrodynamics

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    Ginzburg-Landau Theory

    Ginzburg-Landau theory is a particular case ofLandaus theory of second order phase transition

    Formulated in 1950, before BCS

    Masterpiece of physical intuition

    Grounded in thermodynamics

    Even after BCS it still is very fruitful in analyzing thebehavior of superconductors and is still one of themost widely used theory of superconductivity

    G

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    Ginzburg-Landau Theory

    Theory of second order phase transition is based onan order parameter which is zero above the transition

    temperature and non-zero below

    For superconductors, GL use a complex order

    parameter(r) such that |(r)|2

    represents thedensity of superelectrons

    The Ginzburg-Landau theory is valid close toTc

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    Ginzburg-Landau Equation for Free Energy

    Assume that (r) is small and varies slowly in space

    Expand the free energy in powers of(r) and its

    derivative

    2

    22 4

    0

    1

    2 2 8n

    e hf fm i c

    ba y y y p

    **

    = + + + - + A

    Fi ld F U if C

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    Field-Free Uniform Case

    Near Tc we must have

    At the minimum

    2 4

    02

    nf f ba y y- = +0

    f fn

    -0

    f fn

    -

    0> 0 = -

    2 22

    0(1 )

    8 2

    andcn c

    H f f H t

    ay

    p b

    - = - = - fi -

    2 ay

    b = -

    Fi ld F U if C

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    Field-Free Uniform Case

    At the minimum

    2 4

    02

    nf f ba y y- = +

    20 ( ) ( 1) (1 )t t t b a a y > = - fi -

    22

    0

    2 8(1 )

    (definition of )cn c

    c

    H f f H

    H t

    a

    b p

    - = - = -

    fi -

    2 ayb

    = -

    It is consistent with correlating |(r)|2 with the density of

    superelectrons

    2 (1 ) cnear Tsn tl- -

    which is consistent with ( )20 1c c H H t = -

    Fi ld F U if C

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    Field-Free Uniform Case

    Identify the order parameter with the density of superelectrons

    222

    22 2

    22

    2 22 42

    2 4

    ( )(0)1 1 ( )

    ( ) ( ) (0)

    ( )1 ( )2 8

    ( ) ( )( ) ( )( ) 4 (0) 4 (0)

    since

    and

    Ls

    L L

    c

    c cL L

    L L

    TTn

    T T n

    H TT

    H T H T T Tn T n

    l al l b

    ab p

    l la bp l p l

    Y= Y fi = = -Y

    =

    = - =

    Fi ld F N if C

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    Field-Free Nonuniform Case

    Equation of motion in the absence of electromagnetic field

    221 ( ) 0

    2

    T

    m

    y a y b y y *- + + =

    Look at solutions close to the constant one2 ( )

    whereTa

    y y d y

    b = + = -

    To first order:21 0

    4 ( )m Td d

    a* - =

    Which leads to 2 / ( )r Texd -

    Field Free Non niform Case

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    Field-Free Nonuniform Case

    2 / ( )

    2

    (0)1 2( )

    ( ) ( )2 ( )where

    r T L

    c L

    ne T

    m H T T m T

    x lpd xla

    -**

    = =

    is the Ginzburg-Landau coherence length.

    It is different from, but related to, the Pippard coherence length.( )

    0

    1/22

    ( )1

    Tt

    xx

    -

    GL parameter:( )

    ( )( )

    LT

    TT

    lk

    x=

    ( ) ( )

    ( )

    Both and diverge as but their ratio remains finite

    is almost constant over the whole temperature range

    L cT T T T

    T

    l x

    k

    2 Fundamental Lengths

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    2 Fundamental Lengths

    London penetration depth: length over which magnetic field decay

    Coherence length: scale of spatial variation of the order parameter

    (superconducting electron density)

    1/2

    2( )

    2

    c

    L

    c

    TmT

    e T T

    bl

    a

    * = -

    1/22

    ( ) 4c

    c

    TT m T Tx a*

    = -

    The critical field is directly related to those 2 parameters

    0( )2 2 ( ) ( )

    c

    L

    H TT T

    f

    x l=

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    Surface Energy

    2 2

    2

    2

    1

    8

    :8

    :8

    Energy that can be gained by letting the fields penetrate

    Energy lost by "damaging" superconductor

    c

    c

    H H

    H

    H

    s x lp

    l

    p

    x

    p

    -

    S f1

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    Surface Energy

    2 2

    c

    Interface is stable if >0

    If >0

    Superconducting up to H where superconductivity is destroyed globally

    If >> >

    >

    1

    :2

    1:

    2

    area to volume ratio

    quantized fluxoids

    More exact calculation (from Ginzburg-Landau):

    = Type I

    = Type II

    l

    k x

    lk

    x

    2 21

    8c

    H Hs x lp

    -

    Magnetization Curves

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    Magnetization Curves

    Intermediate State

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    Intermediate State

    Vortex lines in Pb.98In.02

    At the center of each vortex is a

    normal region of flux h/2e

    C iti l Fi ld

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    Critical Fields

    2

    2

    1

    2

    2

    1(ln .008)

    2

    Type I Thermodynamic critical field

    Superheating critical field

    Field at which surface energy is 0

    Type II Thermodynamic critical field

    (for 1)

    c

    c

    sh

    c

    c c

    c

    c

    c

    c

    H

    HH

    H

    H H

    HH

    H

    H

    k

    k

    k k

    k

    =

    +

    Even though it is more energetically favorable for a type I superconductor torevert to the normal state at Hc, the surface energy is still positive up to a

    superheating field Hsh>Hc metastable superheating region in which the

    material may remain superconducting for short times.

    Superheating Field

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    Superheating Field

    0.9

    1

    Ginsburg-Landau:

    for

    The exact nature of the rf critical

    field of superconductors is stillan open question

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    Material Parameters for Some Superconductors

    BCS

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    BCS

    What needed to be explained and what were the clues?

    Energy gap (exponential dependence of specific heat)

    Isotope effect (the lattice is involved)

    Meissner effect

    Cooper Pairs

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    Cooper Pairs

    Assumption: Phonon-mediated attraction between

    electron of equal and opposite momenta located

    within of Fermi surface

    Moving electron distorts lattice and leaves behind a

    trail of positive charge that attracts another electron

    moving in opposite direction

    Fermi ground state is unstable

    Electron pairs can form bound

    states of lower energy

    Bose condensation of overlapping

    Cooper pairs into a coherent

    Superconducting state

    Dw

    Cooper Pairs

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    Cooper Pairs

    One electron moving through the lattice attracts the positive ions.Because of their inertia the maximum displacement will take place

    behind.

    BCS

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    BCS

    The size of the Cooper pairs is much larger than their spacing

    They form a coherent state

    BCS and BEC

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    BCS and BEC

    BCS Theor

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    BCS Theory

    ( )

    0 , 1 ,-

    , : ( , - )

    0 1

    :states where pairs ( ) are unoccupied, occupied

    probabilites that pair is unoccupied, occupied

    BCS ground state

    Assume interaction between pairs and

    q q

    q q

    q qq qq

    qk

    q q

    a b q q

    a b

    q k

    V

    Y = +

    =

    P

    0

    q kif and

    otherwise

    D DV x w x w -

    =

    BCS

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    BCS

    Hamiltonian

    Ground state wave function

    destroys an electron of momentumcreates an electron of momentum

    number of electrons of momentum

    k k qk q q k k

    k qk

    k

    q

    k k k

    n V c c c c

    c k

    c k

    n c c k

    e * *- -

    *

    *

    = +

    =

    H

    ( )0q q q q

    q

    a b c c f* *-Y = +P

    BCS

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    BCS

    The BCS model is an extremely simplified model of reality

    The Coulomb interaction between single electrons is

    ignored Only the term representing the scattering of pairs is

    retained

    The interaction term is assumed to be constant over a

    thin layer at the Fermi surface and 0 everywhere else

    The Fermi surface is assumed to be spherical

    Nevertheless, the BCS results (which include only a veryfew adjustable parameters) are amazingly close to the real

    world

    BCS

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    BCS

    ( )

    ( )

    2

    2 2

    0

    1

    0

    0

    0, 1 0

    1, 0 0

    2 1

    21

    sinh

    0

    Is there a state of lower energy than

    the normal state?

    for

    for

    yes:

    where

    q q q

    q q q

    q

    q

    q

    VDD

    a b

    a b

    b

    e

    V

    r

    x

    x

    x

    x

    ww

    r

    -

    = =

    = -

    + D

    D =

    BCS

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    BCS

    ( )( )

    11.14 exp

    0 1.76

    c D

    F

    c

    kT

    VN E

    kT

    w

    = -

    D =

    Critical temperature

    Coherence length (the size of the Cooper pairs)

    0 .18F

    ckT

    ux =

    BCS Condensation Energy

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    BCS Condensation Energy

    ( ) 20

    2

    0 00

    0

    4

    0

    2

    8

    / 10

    / 10F

    Condensation energy: s n

    F

    V

    E E

    HN

    k K

    k K

    r

    e p

    e

    D

    - = - D

    - D =

    D

    BCS Energy Gap

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    BCS Energy Gap

    At finite temperature:Implicit equation for the temperature dependence of the gap:

    ( )

    ( )

    ( )

    1 22 2

    1 22 20

    tanh / 21

    0

    D kT

    dV

    w e

    er e

    + D = + D

    BCS Excited States

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    BCS Excited States

    0

    2 22k

    Energy of excited states:

    ke x= + D

    BCS Specific Heat

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    BCS Specific Heat

    10

    Specific heat

    exp for < ces

    TC T

    kT

    D -

    Electrodynamics and Surface Impedancei BCS M d l

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    in BCS Model

    ( )

    [ ] ( )

    0

    4

    ,

    , ,

    There is, at present, no model for superconducting

    sur

    is treated as a small pe

    face resistance at high rf

    rturbation

    similar to Pippar

    field

    ex

    ex i i

    ex

    rf c

    R

    l

    H H i t

    e H A r t p

    mc

    HH H

    R R A I R T e J dr

    R

    f

    f f

    w-

    + =

    =

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    Penetration Depth

    ( ) 2

    4

    2( )

    c

    c

    specular

    1Represented accurately by near

    1-

    dkdk

    K k k

    T

    T

    T

    lp

    l

    = +

    Surface Resistance

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    Surface Resistance

    ( )( )

    4

    32 2

    2

    :

    1

    :2

    exp

    -kT

    2

    Temperature dependence

    close to dominated by change in

    for dominated by density of excited states e

    kT

    Frequency dependenceis a good approximation

    c

    c

    s

    tT t

    t

    TT

    AR

    T

    l

    w

    w

    D

    --

    -