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  • 8/19/2019 Theory of Dislocation Mobility in Pure Slip - Lothe1962

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    Theory of Dislocation Mobility in Pure Slip

    Jens Lothe 

    Citation: Journal of Applied Physics 33, 2116 (1962); doi: 10.1063/1.1728907 

    View online: http://dx.doi.org/10.1063/1.1728907  

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    2116

    R O T H M A N f O N E S G R A Y AND

    H A R K N E S S

    rial by Adda

    et

    al. 19 which is about what one would

    expect if their values were slightly increased by dif

    fusion

    l o n g ~ g r i n

    boundaries.20 Adda

    et

    at. did not

    observe any anisotropy; however, visual observation

    of

    autoradiographs of polycrystalline samples is a less

    reliable method of detecting anisotropy than the method

    used by us. Our

    D[lOOJ

    and

    D[ool]

    are factors

    of

    ten and

    twenty or sixty higher than those measured by Resnick

    et

    al.

      l

    on perfect single crystals. This difference

    probably is not due to diffusion along mosaic boundaries

    in our crystals for the reasons given above; the dis

    crepancy is better attributed to the experimental

    uncertainty of the data of Resnick

    et

    al.

    19

    Y.

    Adda, A. Kirianenko, and C. Mairy, Compt. rend. 253,

    445

    (1961).

    20

    R. E. Hoffman and D. Turnbull,

    J.

    Appl. Phys.

    22,

    634 (1951).

    21 R. Resnick and L.

    L. Seigle,

    J. Nuclear Materials 5,5 (1962).

    J O U R N A L OF A P P L I E D

    P H Y S I C S

    CONCLUSIONS

    We conclude that we have measured volume self

    diffusion in alpha uranium, and that it is highly aniso

    tropic, as expected from the structure. Diffusion in the

    corrugated layers, where the jump distances are small

    and the bonding is covalent and strong, is much faster

    than diffusion out

    of

    such layers. However, there are

    indications of fast diffusion between the corrugated

    planes along dislocations.

    ACKNOWLEDGMENTS

    The assistance of M. Essling, E. S. Fisher, A. Hrobar,

    S.

    A.

    Moore, M. H. Mueller, L.

    J.

    Nowicki, M. D. Odie,

    and D. Rokop, and discussions with H. H. Chiswik,

    E. S. Fisher, and

    L

    T. Lloyd are gratefully acknowl

    edged. This project was begun by R. Wei .

    V O L U M E 3 3 . N U M B E R

    6

    J U N E 1962

    Theory of islocation Mobility in Pure Slip

    JENS LOTHE

    Metals Research Laboratory

    Carnegie Institute of

    Technology

    Pittsburgh, Pennsylvania

    (Received July 19, 1961; revised manuscript received November 9,

    1961)

    The mobility during glide of uniformly moving dislocations or dislocation segments supposed not to be

    obstructed by any Peierls' barrier is estimated. For a straight freely moving dislocation, the strong an

    harmonicities in the core region, the thermoelastic (edge dislocation) and the phonon viscosity effect give

    rise to a drag stress

    at

    ordinary temperatures

    T 'fJ,

    f being the Debye temperature, of the order

    ,, ,,-,f.;.XV/c

    in insulators.

    In

    metals the thermoelastic effect is negligible, while the core anharmonicity effect and the

    phonon viscosity effect will be of the same order of magnitude as in insulators. In the above formula,

    E=thermal energy density, V=dislocation velocity, and c=velocity of shear waves. The scattering of

    phonons by the dislocation also causes a drag stress at ordinary temperatures of the order of magnitude

    of

    the above formula.

    All of the above mentioned contributions to the drag stress go rapidly to zero with decreasing temperature.

    However, if the dislocation s constrained by the Peierls' barrier except at freely moving kinks, the kink

    mobility determines the dislocation mobility. It

    is

    shown that the scattering of phonons of a half-wavelength

    longer than the kink width causes a drag stress which may outweigh all other contributions up to ordinary

    temperatures, and which persists with decreasing temperature as

    T

    down to a temperature

    '8b/D,

    where

    b=the lattice spacing constant and D

    is

    the kink width.

    I. INTRODUCTION AND_OUTLINE

    S

    O far, a discussion and interrelation of the various

    theories for dislocation mobility is lacking.

    In

    this

    paper we briefly reconsider the various dissipative

    mechanisms suggested and discuss, in order of magni

    tude, their effect on dislocation mobility. Some estimates

    of the dissipation that result because of the strong

    anharmonicities in the core region are also presented.

    Care is taken to represent the various contributions in

    equations which are easily compared.

    Only dislocations, or dislocation segments, that can

    move freely without thermal activation, will be con-

     

    On leave from Fysisk Institutt, Universitetet, Blindern,

    Oslo,

    Norway.

    sidered. Internal friction experiments in copperl and

    NaCl2 have shown that in these crystals there is a

    modulus defect, quite constant with temperature, with

    an accompanying internal friction that seems to tend

    to zero as the temperature tends to zero, indicating

    either freely moving dislocations or freely moving

    kinks.3.4

    At the end of the paper we shall make some separate

    considerations on kinks.

    t will

    appear that the mobility

    of a smooth dislocation will have a somewhat different

    1 G. A. Alersand D.

    O.

    Thompson, J. Appl. Phys. 32,

    283

    (1961).

    2

    R.

    B.

    Gordon (private communication).

    3

    J.

    Lothe and

    J.

    P. Hirth, Phys. Rev. 115,

    543

    (1959).

    4 J. Lothe, Phys. Rev. 117, 704 (1960).

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    D I SL O C A T I O N M O B I L I T Y IN PUR

    SL I P

    2117

    temperature characteristic than the mobility of a

    dislocation with a kinked core structure.

    We think

    that

    the idea

    of

    some dislocation segments

    being able to move freely, without any activation, need

    not be an approximation. A possible "Peierls' barrier"

    to the motion of a kink in a close-packed metal would

    most likely be

    so

    small

    that it

    would be completely

    obliterated

    by

    zero-point motion. Thus,

    at

    very low

    temperatures,

    we

    would expect the kink to move

    without friction.

    II. RELAXATION EFFECTS

    Relaxation effects in the matrix around the moving

    dislocation leads to heat production. The rate

    of

    heat

    production around the moving dislocation unequiv

    ocally determines the dislocation mobility: The disloca

    tion

    will

    move with constant velocity when the rate

    of

    heat production equals the rate

    of

    energy supply from

    the external mechanism that provides a shear stress

    acting on the dislocation.

    A. ulk

    Relaxations

    Eshelb

    y

    5 has shown

    that

    the thermoelastic effect

    will

    give rise to heat production around a moving disloca

    tion. The thermoelastic effect is appreciable only for

    the moving edge-like dislocation, where irreversible

    heat

    flow will

    take place between the compressional

    and dilatational side. Recently, Mason

    6

    suggested

    that

    pure shear deformations should be accompanied by

    thermal relaxation effects and energy dissipation. This

    effect comes about when the vibrational frequencies in

    a lattice do not change only with volume changes, as

    assumed in the simple Gruneisen theory,

    but

    also

    depend on shear strain. The phonon-viscosity effect,

    as this effect

    was

    termed

    by

    Mason, would

    be

    equally

    effective for both edge and screw dislocations.

    In

    the theories for the thermoelastic effect and the

    phonon viscosity effect

    it is

    necessary to introduce a

    cutoff, defining a cylinder around the dislocation core

    within which the theories do not apply.

    We

    shall

    reconsider what

    is

    the proper cutoff. In particular the

    result for the phonon-viscosity effect depends sensitively

    on the choice of cutoff.

    1. The Thermoelastic Effect

    Eshelby

    5

    calculated the thermoelastic heat production

    per cycle for a vibrating edge dislocation. Because

    of

    a

    term logarithmic in the frequency, it is not obvious

    from Eshelby's result what the stress needed to keep

    the dislocation in uniform motion

    is.

    Weiner

    7

    has

    considered this problem, and for a rigorous analysis

    Weiner's paper should be consulted. In order to get an

    approximate,

    but

    simple and analytical, result

    we

    have

    6 J. D. Eshelby, Proc. Roy. Soc. (London) A197 396 (1957).

    6

    W. P. Mason,

    J.

    Acoust. Soc. Am. 32, 458 (1960).

    7

    J. H. Weiner, J. App . Phys. 29, 1305 (1958).

    calculated the problem by essentially the same pro

    cedure as used

    by

    Eshelby. For simplicity the cutoff

    radius

    1was

    introduced as a cutoff in

    k

    space,

    k

    ma x

    =7r/l.

    The resulting equation for the stress

    u

    needed to move

    the edge dislocation

    at

    a speed

    V is

    with Poisson's

    ration equal to

    i

    1

    IJ b

    Cp C .

    u=- - - - ln 7 rK / lV)XV,

    (1)

    70 K C

    p

    when

    7rK/lV»1.

    Here the symbols are:

    b

    = magni tude of Burgers

    vector; lJ.=shear modulus;

    K=K cp=thermal

    diffusiv

    ity

    (thermal conductivity divided by specific heat per

    unit volume);

    C

    p

     

    c.=specific heats per unit volume

    at

    constant pressure and volume, respectively; and

    1= cutoff radius for the dislocation core.

    An

    asymptotic

    correspondence between Eq. 1) and Eshelby's formula

    8

    as

    1 >

    0

    can easily

    be

    demonstrated.

    The cutoff cannot be smaller than the lattice

    distance b However, the conditions for the macroscopic

    concept of thermoelastic relaxation to apply are not

    satisfied that close to the core. A volume element to

    which

    we

    apply macroscopic thermal concepts must

    have a linear dimension

    at

    least

    as

    large

    as

    the phonon

    mean free

    path

    in an insulator, or the electron mean

    free path in a metal. Thus, it

    is

    natural to put

    l=Ap

    (insulator),

    l=Ae (metal),

    (2)

    where

    Ap

    and

    Ae

    are the phonon mean free

    path

    and

    electron mean free path, respectively. Applying thermo

    elastic theory to closer distances

    of

    the core would,

    for an insulator, lead to heat transmission faster than

    sound, which is not possible.

    Other factors equal, the thermoelastic effect

    is

    strongest in materials

    of

    low thermal conductivity.

    Thus, for an estimate

    of

    the maximum contribution let

    us consider a typical insulator. By making use

    of

    the

    thermodynamic relation

    (3)

    where a

    is

    the volume expansion coefficient and

    B

    the

    bulk modulus, combined with the approximate relations

    (4)

    and

    (5)

    where

    Kp is

    the lattice thermal conductivity and

    'Y'"1.5 is

    Gruneisen's constant,

    we

    can rewrite Eq.

    (1)

    to

    U = ~ ~ C v T ) l n ~ ) x ~ ,

    28Ap

    V

    C

    (6)

    8 In Eshelby's formula (4), reference 5 a factor 1/50 should be

    substituted for the factor 1/10 occurring in

    that

    formula.

    The

    factor 1/50 can be derived from his formula (a24).

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    2118

    J NS LOTHE

    when

    V«c.

    Poisson's ratio has been taken as in the

    relation between J I and B c denotes the velocity of

    sound.

    9

    At ordinary temperatures, in the region 0 to 0/2 it

    is reasonable to put cvT

    /2", E,

    where

    E

    is the thermal

    energy density and

    Ap'" (S-30)b.

    With

    V

    in say the

    region

    "'c/100,

    the estimate of Eq. 6) for

    T ,O

    and

    Ap ,Sb is

    7)

    In

    metals, because of a higher thermal conductivity

    by

    a factor typically of about 30, the thermoelastic

    contribution will be correspondingly smaller.

    2 The Phonon Viscosity Effect

    The

    difference between the adiabatic and isothermal

    bulk modulus is

    (8)

    For an isotropic body the shear modulus

    J I

    is related

    to the bulk modulus B and Poisson's ratio v

    by

    the

    equation

    J.I.= 3(1-2v)B/[2(1+ )].

    (9)

    In

    the elementary theory of Gruneisen's constant the

    vibrational frequencies are taken, on the average, to

    depend on the volume only, 'Y= d InO/d InV. In this

    model

    we

    would have 11J 1 = J.l.ad - J.l.is = 0, corresponding to

    v=

    in Eq. (9) for the change. If, on the other hand,

    we take the frequencies in a wave only to be modified

    by

    longitudinal strain parallel to the wave vector, we

    should rather put

    v=O

    in Eq. (9) to calculate 11J 1 from

    I1B;

    (10)

    Equation (10), thus, is a reasonable upper estimate

    of the difference between the adiabatic and isothermal

    shear modulus. It should be understood that, in this

    context, adiabatic means that energy is not exchanged

    between vibrational modes in the same volume element.

    The additional shear stiffness during adiabatic deforma

    tion comes about because phonons with wave vector

    in the BC' direction become hotter during shear,

    while those in the

    AD'

    direction become "cooler"

    (Fig. 1).

    In terms of three phonon processes it would take

    Umklapp processes to establish equilibrium between

    BC'

    and AD' phonons. Thus, it should be approximately

    A

    B

    FIG. 1. When the volume element

    ABDC

    is sheared

    adiabatically

    to

    take

    the shape

    ABD'C',

    phonons traveling

    in

    the direction

    BC'

    become hotter

    and

    those traveling

    in the

    direction

    AD'

    become

    cooler.

    9

    Because

    of the approximate nature of the

    calculations, we

    will

    denote

    the

    shear wave

    velocity

    as

    well

    as

    the

    average sound

    velocities

    appropriate

    to

    the

    various considerations in this

    paper

    by the same symbol c.

    right, as done

    by

    Mason,6 to determine the relaxation

    time from the equation

    (11)

    where

    Ap is

    given

    by

    Eq.

    (4).

    Then, employing Mason's analysis for the moving

    screw dislocation,

    but

    only for the material outside a

    cylinder of radius Ap around the core, we obtain

    CT=7]b/ 47rAp2)X

    V,

    V«c,

    where

    7]

    is the phonon viscosity

    7]= TI1j t

    (12)

    (13)

    By Eqs. (4), (9), and (11), and with 'Y' 1.5, Eq. (12)

    can be written as

    (14)

    and, in the region T ,O, with the same approximation as

    used for Eq. (7),

    CT 'E/lOXV/c,

    V«c.

    (15)

    The result for an edge dislocation would not be much

    different.

    t must be borne in mind

    that

    Eq. (15), based on

    Eq. (10), is an upper estimate.

    According to Kittel,lO at ordinary temperatures T ,O,

    the relaxation time for phonons is about the same in

    insulators and metals.

    In

    metals the phonon-phonon

    relaxation time

    Tpp

    is about the same as the phonon

    electron relaxation time Tpe. Thus, the phonon mean

    free

    path

    and the phonon viscosity in a metal should

    typically be about the same as in an insulator, and the

    phonon viscosity contribution to dislocation damping

    should not be very different in insulators and metals.

    B. Relaxations in the Core Region

    t remains to estimate the relaxation contributions

    inside the cutoff cylinder or radius

    r=A.

    The contribu

    tions will be divided into two main classes:

    (1) A volume contribution, for which the relaxation

    strengths I1B and 11j.t Eqs. (8) and (10), are supposed

    to apply on the average.

    2) A misfit plane contribution, in which the an

    harmonicities are

    so

    great and of such a nature

    that

    they must be considered separately.

    This division corresponds to the Peierls-Nabarro

    treatment of the dislocation, where two elastic solids

    are joined

    by

    a misfit plane.

    1.

    The

    Core Volume Contribution

    In

    the calculation on the thermoelastic effect for

    an edge dislocation in a metal, only the matter outside

    10

    C. Kittel,

    Introduction to Solid State Physics (John

    Wiley

    Sons, Inc., New York, 1956), 2nd ed., p. 149.

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    DISLOCATION

    MOBILITY

    IN PURE SLIP

    2119

    a cylinder of radius

    r=A.

    was considered. Applying the

    ordinary theory of thermal conduction within this

    cylinder would lead to a phonon relaxation time

    smaller

    than

    Tpe. As at ordinary temperatures T=Ap/c

    "'Tpp'" Tpe, such a procedure must be wrong. Rather,

    the various volume elements in the region we consider

    have a single relaxation time

    Tp •. In

    each volume

    element, phonon energy is transferred to the electron

    gas and carried

    out

    of the region under consideration,

    until equilibrium is established within a time T ' " Ap/ .

    Thus, in analogy with Eq.

    (13),

    we define a bulk

    viscosity

    X,

    X=T .B.

    (16)

    Then, for the region between r=A. and r=Ap for an

    edge dislocation, with

    ,,= t

    and

    'Y' 1.5,

    a simple

    calculation following the treatment on phonon viscosity

    gives, when A.»A

    p

    ,

    1 c.Tb V

    (T '-

    --X- V«c.

    40

    Ap

    C

    (17)

    For relaxations in the region b

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    2120

    J E NS

    LOTHE

    be zero. The second term

    E av

     

    F

    vibr

     

    2v

    2

    ax

    (26)

    gives rise to a change in vibrational energy.

    I f

    the

    oscillator is moved with a velocity

    V,

    F

    vibr

    does work

    at the rate

    Fvibr V=-- V,

    2v

    2

    ax

    (27)

    which goes to increase the energy of vibration. I f the

    increase in vibrational energy radiates out, heat

    is

    supplied to the surrounding matrix. As the average

    vibrational energy of the atoms in the misfit plane is

    constant, the average value of Eq. (27) must determine

    the rate at which heat is produced.

    Each oscillator

    is

    coupled to its neighboring atoms,

    with which vibrational energy

    is

    then exchanged.

    Denote the relaxation time for energy exchange by T.

    Because of the strong coupling to other atoms, the

    relaxation time will only be a

    few

    periods, say roughly,

    (28)

    The differential equation determining the vibrational

    energy of a moving oscillator is then

    dE 1 E av

    2

    =

    - - [E-Eeq T )J+ - - · v ,

    (29)

    dt T 2v

    2

    ax

    where

    Eeq(T)

    is

    the equilibrium value

    Eeq(T) =hv/ (ehplkT -1 .

    (30)

    Now put

    v= vo-ov cos(271 x/b).

    (31)

    By expanding to the first power in ov/vo

    we

    can rewrite

    Eq. (29) as

    dE 1

    EO(

    -+- E-Eo)= 1

    dt T T

    EoehVlkT)OV

    -

    cos(271 vt/b)

    kT Vo

    271 E

    o

    vov

    - -

     

    sin

    (271 vt/b)

    ,

    (32)

    b

    Vo

    where Eo

    is

    Eq. (30) with v= Vo.

    Only that part of the solution of Eq. (32) which is

    in phase with sin (271 vt/b) contributes to the time

    average of Eq. (27). Denoting this part

    oE, we

    obtain

    when

    vT/b

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    D I S L O C T I O N

    MO B I L I T Y IN PURE SLI P

    2121

    sidered to move in an isotropic flux of phonons which

    collide with the dislocation,

    but

    which do not collide

    with each other, i.e., the phonon mean free

    path is

    assumed infinite. For such an approximation to be

    adequate, the phonon mean free

    path

    must at least be

    longer than the dislocation scattering width.

    13

    However,

    no clear criterion for when the approximation of non

    colliding phonons

    is

    valid has been established;

    we

    can

    only assert

    that

    at lower temperatures this picture must

    be right and offers an opportunity for complementary

    and more reliable estimates than the previous core

    considerations based on simple relaxation considera

    tions. Fortunately, it will also turn

    out

    that the high

    temperature values for

    (J

    derived in this picture are of

    the same order of magnitude as the more important

    contributions considered in the first

    part

    of this paper;

    thus not too much ambiguity as to the correct order of

    magnitude of (J

    at

    ordinary temperatures arises. At

    low temperatures some of the effects to be studied give

    a higher value for

    (J

    than the relaxation effects

    and

    should then be the dominant effects.

    Consider a stationary dislocation placed in

    an

    isotropic gas of phonons. The phonons are scattered

    by

    the dislocation;

    sayan

    energy

    W

    is scattered

    out

    radially symmetric about the dislocation per unit time.

    However, if the dislocation

    is

    moving with a velocity V

    the scattered radiation

    is

    asymmetric and gives off a

    net amount of quasi-momentum W/cXV/c per unit

    time to the component parallel to the dislocation

    motion, and thus a stress of the order

    (38)

    is needed

    to

    maintain uniform dislocation motion.4

    The exact coefficient of proportionality in Eq. (38)

    depends on the wavelength dependence of scattering

    cross section. For our purposes, Eq.

    (38) is

    adequate,

    and the problem is then to find W.

    Two important cases

    will

    be studied: 1) the scatter

    ing from a smooth infinite free dislocation, and (2) the

    scattering from a free kink.

    A.

    The Infinite Smooth Dislocation Line

    1 Scattering by Induced Vibrations

    Consider a screw dislocation, and consider

    it

    to

    interact with shear waves only. A shear wave whose

    wave vector if makes an angle with the dislocation will

    induce a wave motion of wave vector k cost?- on the

    dislocation. Thus, if the velocity of a free wave motion

    on the dislocation line

    is

    CD, shear waves for which

    coSt?-

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    2122

    l N S

    LOTHE

    I o e : = = = = = = = = ~ = =

    m

    0.1

    2

    3

    4 5

    6

    7

    8

    O/T

    FIG.

    4. Curve

    I: .IT,

    normalized to 1 for

    eiT.

    Curve

    II: ulT,

    normalized to 1 for eIT=O, u is given by Eq. (43). Curve

    III:

    the constant

    1.

    where

    E w,T)

    iw

    ----

    w=ck.

    e w/kT-1

    (44)

    In the high temperature limit, with

    E w,T)=kT

    and E 'V3kT/b

    3

    ,

    Eq. (43) becomes

    u -'E/10XV/c, 45)

    which is precisely the formula originally given by

    LeibfriedY

    t

    is important to note that

    U

    as given by Eq. (43)

    decreases more slowly with temperature than the

    thermal energy E, which is proportional· to

    ' fokmaxE ck,

    T)k2dk.

    The temperature dependences of

    E

    and

    u

    are compared

    in Fig.

    4.

    f the phonon half-wavelength is small compared with

    the width of the core misfit region, the phonon does not

    tend to move the dislocation core as a whole. Neverthe

    less, we shall expect Eq. (43) to be a fair estimate up

    to higher temperatures because of another equally

    effective scattering mechanism.

    We

    will

    picture the core misfit strip in the glide plane

    as a cut of some width 2a, over which shear stress

    cannot be sustained. Consider shear waves of a wave

    length A

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    D I S L O C T I O N MO B I L I T Y IN PURE SL I P

    2123

    which agrees well with Klemens'

    20

    estimate. With

    k

    m x

    =7r/b and 'Y '1.5, the cross section for phonons of

    highest energy becomes fJ ,b/2.

    However, for dislocations for which the Peierls'

    barrier is negligible, Eq. (46) would not apply to a

    distance

    r ,b

    within the center (see Fig. 2). t is reason

    able

    to

    suppose

    the

    core

    to

    be relaxed within a cylinder

    of radius r '3b, and that the

    perturbation

    potential in

    this region is approximately given by Eq. (46) with 3b

    substituted

    for r. Using

    instead

    of Eq. (46) a

    perturba

    tion potential

    we

    derive a scattering cross section

    fJ='YWk/16(1 k2A2 i,

    (49)

    SO)

    which for the high energy phonons, with A ,3b and

    'Y' 1.5, gives a

    constant

    cross section

    fJ ,b/40.

    (51)

    Thus, with

    j

    of the phonons being scattered, the drag

    stress

    at

    ordinary temperatures will be

    u 'e/60X V/e.

    (52)

    According

    to

    Klemens,20 Eq. (48) may be an under

    estimate

    by

    as much as a factor of the order 10. The

    uncertainty

    is due to lack of precise knowledge about

    the

    anharmonic constants

    and

    the approximations

    involved in the Born scattering formula.

    With

    the same

    uncertainty in Eq. (52), the drag stress due

    to

    strain

    field scattering might be as high as

    u '-'e/5X V/e. 53)

    B. Scattering

    at

    a Kink. Kink Mobilit

    y

    21

    When the Peierls' barrier is significant, the moving

    element will be the kink, which is a short dislocation

    segment taking the dislocation from one Peierls' valley

    to a neighboring valley (Fig. 6). The kink is supposed

    to

    be able to

    translate

    freely along

    the

    dislocation, and

    the

    action of thermal waves of wavelength >./2>D,

    where

    D

    is the kink width, will be

    to

    vibrate the entire

    kink and make it radiate energy.

    Consider a

    kink in

    a screw dislocation.

    The

    action of

    the kink on

    the

    elastic waves, for small kink displace

    ments, can be deduced from a

    Hamiltonian

    22

    20 P. G. Klemens in Solid State Physics, edited

    by

    F. Seitz and

    D.

    Turnbull

    (Academic Press Inc., New York, 1958), Vol. 7,

    p.22.

    21 The author

    acknowledges gratefully

    that Dr.

    Eshelby gave

    him the

    opportunity

    to compare with unpUblished results obtained

    by Dr. Eshelby by methods different from those employed in

    this paper.

    22 t can be shown, by use of the definition of a force on a

    dislocation

    and the

    reciprocal theorem of linear elasticity,

    that

    this procedure is right.

    Peierls

    volle

    Peierls volley

    FIG. 6. A kink of width D brings the dislocation from one Peierls'

    valley into a neighboring one.

    so that the equations of motion for the waves are

    (55)

    Here,

    x

    is the displacement of the kink,

    u

    is the stress

    amplitude of the elastic wave, U is the stress amplitude

    resolved

    onto the

    kink, and

    V

    is the

    total

    volume.

    For

    forced vibrations

    mCY w

    2

    y)=Fo singt,

    (56)

    the rate at which energy is given to the oscillator when

    y=O

    and

    y=O at t=O is, taking the

    dominant

    term,

    F02

    sin(g-w)t

    7rF02

    F · y = -

    - -8 g-w) .

    (57)

    4m g-w 4m

    By treating Eq. (55) this way and summing over all

    shear lattice waves, it is found that for an oscillation

    x= A singt,

    the

    rate of energy radiation is

    (58)

    The

    kink vibrations are caused

    by

    incident thermal

    waves

    (59)

    where mk is the effective kink mass. From Eqs. (58) and

    (59) we deduce that all

    the

    incident waves up to some

    k

    m x

    cause

    the kink

    to radiate at a rate

    (60)

    Considering only waves for which Aj2> D to vibrate the

    kink as a whole,

    we

    must

    put

    (61)

    According to Lothe and Hirth,3 the width of the

    kink is

    7r(

    S

    1

    D=; 21rCTp ,

    (62)

    where S is the line tension and

    Up

    the Peierls' barrier,

    and the kink energy is

    (63)

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    2124

    l N S

    L O T H E

    when

    T>6b/D,

    Eq. 60) becomes

    and the corresponding stress is

    b

    T>f:J

    v'

    b

    T>(}-.

    64)

    (65)

    In a close packed metal, say copper, the Bordoni peak

    experiments

    23

    indicate as typical values

    Wk ' 10-

    2

    j t

    3

    and D , 7b,

    yielding

    (J''''110(3kT/b

    3

    )XV/c,

    T>f:J/7.

    (66)

    An estimate of the effect of thermal waves of half

    wavelength appreciably shorter than

    D

    is needed.

    To

    this end it should be fair to consider the kink as a

    segment of length

    D

    with a velocity normal to itself.

    The

    thermoelastic effect and the phonon viscosity effect

    are negligible for a kink because of the short range of

    the stress field.

    The

    most important damping mecha

    nisms are then those of

    Sec. III A,

    and a likely value of

    the stress due to those sources at a higher temperature is

    ( J ' , ~ ( 3 k T ) ~ X ~

    5 b

    3

    D c'

    67)

    which is seen to be smaller

    than

    Eq. 66)

    by

    a factor

    2/7.

    As

    W

    k

      ,l/D, it is general that Eq. (65) will be the

    more important contribution. This rough estimate of

    the importance of the short wavelength phonons ignores

    that

    the kink is of finite length and

    that

    important

    scattering effects might arise at the transition from the

    kink

    part

    of the dislocation to that

    part

    lying in the

    Peierls' valley. However, the kink width

    D

    will be of the

    same order of magnitude as the wavelength of waves

    of the frequency with which the dislocation vibrates in

    the Peierls' barrier. Thus, elastic waves of shorter

    wavelength will vibrate the dislocation lying in the

    Peierls' valley beyond resonance, i.e., the vibrations

    will be controlled

    by

    the mass and the line tension

    rather

    than

    the Peierls' barrier. t follows

    that

    the

    short wavelength phonons will make the entire disloca

    tion radiate quite uniformly, with little distinction

    between the kink segment and

    that part of

    the disloca

    tion lying in the Peierls' valley, and thus no significant

    scattering effects for short wavelength phonons

    at

    the

    transition between the kink and the Peierls' barrier

    locked dislocation would be expected.

    A satisfactory theoretical treatment

    of

    the effect

    of short wavelength phonons would require a model

    which not only involves the translation of the kink with

    preservation of shape, but which also includes all the

    other degrees of freedom of the entire dislocation.

    23

    D.

    O.

    Thompson and D. K. Holmes

    J

    Appl Phys 30 525

    (1959). • .

    .

    Before such a rather complicated analysis is attempted,

    we cannot do much better

    than

    to introduce a cutoff of

    the order of magnitude of Eq. 61) and estimate the

    effect of phonons of short wavelength in the manner

    explained above.

    Finally, we want to present some considerations on

    the self-consistency of the treatment of kink mobility.

    t

    must be required that the damping stress Eq. 67)

    does not damp the kink to the extent

    that

    for

    k k

    max

    =rr/D the kink motion is not mass controlled. Thus,

    it must be required that

    1(3kT)

    b

    3

    W

    max

    mkWmai>-   X .

    5 b

    3

    D

    c

    68)

    This inequality reduces to

    1>3kTD/j.tb4,

    which is well

    fulfilled up to ordinary temperatures for reasonable

    kink widths, say

    D ,7b

    and

    3kT ,1O-2

    j t

    3

    • Similarly,

    it can be asserted that the direct radiation Eq. 64) is

    much more important than the energy radiation taking

    place because the oscillations are damped

    by

    the

    stress Eq. (67).

    The

    radiation Eq. 58) gives rise to a frequency

    dependent back force on the kink,

    69)

    For this force to be less than the inertial reaction, the

    inequality

    70)

    must be fulfilled. This inequality reduces to

    2c/D>n.

    For

    Qmax=ck

    max

    [Eq

    (61)J,

    this inequality fails to be

    fulfilled by a factor 2/7r. Thus, for Qmax, the oscillations

    are controlled about equally much

    by

    inertia and radia

    tion resistance. This circumstance corresponds to the

    well-known fact that, in the interaction of an electron

    with radiation of a wavelength shorter

    than

    the

    radius

    of

    the electron, the electron motion is radiation

    resistance controlled.

    Taking the effect of radiation resistance on the

    kink oscillations into account would not change the

    order of magnitude of our estimate.

    The

    fact remains

    that the kink oscillations induced

    by

    the waves Qmax

    are largely independent of the effect of shorter wave

    lengths on the kink and give rise to a scattering over

    shadowing the scattering due to the short wavelength

    phonons. The mobility will be proportional to T down

    to

    T ,f:Jb/D.

    IV. SUMMARY, DISCUSSION, AND CONCLUSION

    There is evidence

    that

    under some conditions disloca

    tions can move freely without thermal activation.

    1

    ,2

    This behavior is to be expected when the Peierls'

    barrier for the straight dislocation or for the kink

    segment is broken down by zero-point motion. The

    various factors determining the mobility of dislocations

    experiencing no Peierls' barrier have been discussed in

    some detail.

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    D I S LO C A TI O N

    MO I L I T Y IN P U R E SL I P

    2125

    Two bulk relaxation processes are important: the

    thermoelastic effect and the shear viscosity effect.

    In

    insulators at temperatures of the order the Debye

    temperature

    J

    the thermoelastic effect and the shear

    viscosity effect each give rise to a drag stress of the

    order

    (71)

    but it should be kept in mind that the above estimate

    for the shear-viscosity contribution may be an over

    estimate. In metals the thermoelastic effect

    is

    unimport

    ant, while the shear viscosity effect should be of about

    the same magnitude as in insulators. With decreasing

    temperature these effects go rapidly to zero, as cp

    Ap.

    Estimates of relaxation contributions in or near the

    core, where the theories of thermoelasticity and

    phonon viscosity do not readily apply, have been

    attempted. Only the relaxations associated with the

    strong anharmonicities

    of

    the Peierls-Nabarro structure

    of the slip plane were found to give an appreciable

    contribution, again typically of the order

    (72)

    at ordinary temperatures. This contribution also goes

    rapidly to zero with decreasing temperature.

    The phonon scattering processes can be divided into

    two main types: scattering by the dislocation strain

    field and scattering by dislocation vibrations. The first

    process would cause a drag stress in the region

    E/60X V c