KINEMATICSOF A CONTINUOUSLY DISLOCATED MEDIUM (KINEMATIKA KONTINUAL'NO - DISLOKATSIONNOI SREDY) PMM Vol.
30,No.5,1966, pp. 950-955 V.A.
BABKIN
(Moscow) (Received
November
29, 1965)
The theory of deformation of a medium with a continuous distribution of dislocations is studied. Such a medium will be called continuously dislocated, in contradistinction to a discretely dislocated medium in which the number of dislocations is finite, albeit very large. 1. Def~matiot~. [‘(i
The motion of a point in a solid medium with Lagrangian
= 1, 2, 3) is examined
Cartesian
coordinate
in three-dimensional
system
Euclidean
zi (i = 1, 2, 3). All kinematic
space, properties
coordinates
in which we introduce will be referred
a
to the
&axes. The present
work deals
a small relative
is the total differential ters xs
(tie
with the following
displacement
of the points
with respect
to [’
and certain,
hypothesis:
At a fixed time t,
coordinates
t’
as yet undefined,
and 4’ + d [’
physical
parame-
r ) (S = 1, -em, S ). du =
where n= rc’([i,
xsfcit
Hereinafter,
2)~ t)
summation
By definition,
au ag,
over paired indices
a relative
relative
dci + $-
dx’
3 i is the displacement
displacement dul =
is an elastic
fundamental
with Lagrangian
displacement,
while
of a point in Cartesian
coordinates.
is understood.
with xs = const
au
w
(1.1)
(s = 1, 2, . . . . S)
d$
(1.2)
x8 =comt a relative
displacement
(1.3) is a parametric parameters
(inelastic)
relative
displacement,
because
it is related
to a change
in the
xs.
The physical reason for introducing the parameters x ’ is, that their introduction for the division of small relative displacements into two parts, (1.2) and (1.3). Thus,
1129
allows the
V. A. Babkin
kinematic description becomes more detailed: The the general displacement of the point t’, but also described
by the parameters
at every
accompany
the displacement.
xs which depend on the coordinates must he closely related to the relative
The parameters introduction,
their
which
xs,
x’, t ) indicates not only processes in the medium,
vector u (5 the physic81
[‘ and t, by the very reason displacement, characterizing
point and at every moment. They may he scalars, vectors be found by experiment and from physical considerationa.
generally
reason for introducing x ’ is, that (1.1) in a continuously dislocated medium.
The mathematical relative displacements Let
us rewrite
(1.1)
or tensors,
permits
for it
but they
must
the description
of
in the form
au
ax* dfi =
2-g. Since
da is the total
differential
with
respect
to [‘,
D2u
da is also
and since
the total
differential
we have
I%
04irtgj=----Y-
above),
(1.4)
(1.5)
WD<
with
respect
to 6’
and xs
(see
the hypotheses
we have (1.6)
But it can
be easily
verified
that
(1.7) Hence,
the integral
over
any
closed
contour
C given
by (1.8)
yields, implies
by definition [l that the medium
aod 21, a B urgers under consideration da is given
If the relative displacement contains no dislocations. The
Burgers
vector
may
vector which, in view of (l.?), has continuously distributed
also
be given
by (1.2)
and (1.31,
then,
is non-zero. dislocations.
clearly
This
the medium
by the integral
(1.9)
In the above
formulas,
which takes pect to [‘, is the partial derivative partial derivative. The
components
the symbol
Du/Dt’
into account with respect
of the final
strain
2Pij = pAi,i where fixed
3Ai
form the basis
coordinates.
in moving
denotes
the dependence to [’ considering
tensor :oij
Lagrangian
sre -’
the total partial derivative with resd~,/d~~ of u on x s (5 ‘1. The quantity xs constant. This is the elastic
given 3A,3^j-
coordinates
by
[3] 3”,30j while
(1.10) :Yi
form the basis
in
Kinematics
Utilizing
known methods
and Formula (1.4),
we readily
of a continuously
of expressing obtain,
dislocated
1131
medium
the strain tensor in terms of displacements
in the Cartesian
coordinate
au”
au,
system
au,
3x8
ax8
ax'
[ 33
x’s
---&--$1-~+
auj
au,
a$
ax8
69
au,
au,
au” ai
+qg-gax”-g-asj,xra,i-7,t7 For infinitesimal
aUa ax d a$
ax ax ax’ a~
(1.11)
displacements,
(1.12) The
strains
in (1.12)
may be divided
into elastic
scejij and inelastic,
or parametric
,(PLj p,.. = I+-!. + e(P) 23
13
(1.13)
{j
where ~Wj=;(~+~), Similarly,
= L (-5” 2 ax”
e’qj
the tensor of infinitesimal
rotations
ad
+
$E?$
may be represented
(1.14)
as the sum of two
components
However, 9ij3i3’
neither
the tensor of finite strain
may be split into elastic
eij3f3j
and parametric
parts,
nor the tensor of finite rotation as may be seen,
for example,
from
(1.11). For the medium under investigation u = The velocity
of the point
r -
r. = u (e, x8 (k*, t), t)
au v=E
-I-af
I
p, $=const
The components
(1.16)
4“ is given by
of the strain rate tensor
atI9
zi=const
V(d + +)
(1.17)
=
are given by [ 31
(1.18) Taking
into account
(1.141,
(1.17)
rate tensor from the velocity in case S does not depend explicitly d”i/dx
and (1.18).
when +/&i on t:
we obtain the components does not depend
explicitly
of the strain on xs
and
2. Geometric treatment of strain theory. Let us examine the strains of a continuously dislocated medium, and introduce a moving Lagrangian coordinate system with the basis
1132
Y.A. Babkin
(2.1) If the medium under study is considered
as some space
whose
metric
is
g”tj=3”i3*jr”g”rj”;2&*ij where g*ij = 3O*3OjZiD d 3°iform turns out that the above In fact,
space
it is easily
Rfkl
a basis
-
&2
computation
ari,m
arklm z=.
state
in Euclidean
space,
then it
is Euciideau.
shown by direct m
(2.2)
in the initial
T
that
r,,mrklP-
+
rkpmr 4p G
(2.3)
0
(2.4) Here Rikl m are the components torsion
tensor
The coefficients
of the curvature
are the coefficients
and r*.k
of bktnection
D3^, -= w This transference space, i.e.
result
is entirely
of each point
g(e)
ni j
natura1,
since
the entire
strain
a part of Euclidean
(2.5)
of the body is the result space
into another
dislocated medium under study may be considered g(B)ij3f3j is defined by z
3(e), 3@).
to the tensor
2
of elastic
strains
as motion of the medium will result
Direct
computation
as well
(2.7)
strains,
the metric
coordinates
tensor
by the formulas (2.8)
in the dependence
as through the parameters
in Cartesian
in
(2.6)
Ixs=const
- goij = 2E@)Jj 13
Inasmuch
a space
= ar at’
of
Euclidean
gW ij $e)~$eli = g(e),j 343i
3’
g@) n.,
dinates [‘, explicitly tion are given by
of the
coordinates,
space.
3”‘. I (i = 1, 2, 3) will be called the elastic basis. From (l.lO), (2.6) and (1.141, we find that, for small is related
in Cartesian
r-ijk3^,= riik3,
3W.
&r)tj3i3j
written
by
in the body from one Euclidean
the body remains
But the continuously which the metric tensor
tensor,
of connection
are defined
S.. k are the components v
yields
x ‘,
of
3(“),
the coefficients
on the coorof connec-
Kinematics of a continuousty dislocated
1133
medium
Formulas (2.10) and (2.11) show that s continuously dislocated medium may, from a geometric point of view, be considered as a three-dimensional space with affine connection t cej3 with torsion
tensor
~(e~~~~3~3~3~.
If on the other hand we define a moving reference pondence with a deformable medium by
system
and space
metric
in corres-
(2.12)
g(P)“” ‘ , = 3(~).3(~? * 23
Then we obtain
formulas
similar
~~(P}*j~3~
&$“) n ij 3W
3’
to (2.10)
= (Fiji
_
-
3i 3j
3,=
Z aV L)z?* &r’
Dg’P’
_ $?$.
2
02b:
>
s (P)iikg blksz
~(P)i~k~(~)~~- ~(~)~~~~(~)~~ +
is again found to be a metric
space
with affine
connection
~(p)~~~3~3~3~. By comparing
(2.10)
with (2.14),
we find
‘s(e). .k = 13 Thus, dingly,
the continuously point of view,
from a physical
or inelastic considered located
dislocated
as a space
simultaneously,
It is easily
connection
as either elastic strain
tensor.
L ce13 or L@),,
tensors
a Euclidean of the Lte),
from the
and correspon-
with an incompatible
If the elastic
are compatible,
point of view,
shown that the curvature
and with
(2.16)
medium under study may be considered,
then the total strains
medium is, from a geometric
L(P),
S(P). .k 23
with affine
point of view,
also with an incompatible
(2.15)
r(~)..k~(P)k~ 13
torsion
geometric
(2.14)
flrg@).. 23
and the space tensor
(2.13)
and (2.11)
l+$k)
NP)ts 1 -1 2-g-+--L---(
3t~)i == g(~),j
strain tensor
and inelastic
strains
and the continuously
are dis-
space. and L@)3
spaces
equal zero*
All considerations of this section apply to infinitesimal as well as finite strains. Bowever, for finite strains, the formulas (2.8) do not determine the components of elastic deformation, for clearly, in the case of finite strains, such a tensor cannot, in general, be separated from the strain tensor; instead, they determine the components of what may be called a quasi-elastic tensor. Similarly,
in the case
of finite strains,
p-
the formulas
. . - g”*j ^- 2E@)Aij
(2.17)
x3
determine
the components
The torsion tinuous definition
tensor
dislocations,
of a quasi-parametric ~(e)*~3~3j3~
the tensor
of the dislocation
of the density
density
tensor.
of the L(e)s tensor
[I]
space
is, in terms of the theory of con-
of dislocations
atj3i3P
In fact,
from the
,
(2.18) where S is the surface
supported
on C. By Stokes’ Ct*k3k=e
ilrn
D -7 Dx’
theorem, au ax
(2.18)
yields (2.19)
1134
V.A. Babkin
Whence,
(2.19)
and (2.10)
yield
(2.20) Here
ei?3i3~3,
and eir,3%&3m
to f+ 1) for even permutations similar
to (2.20)
of the indices,
were previously
The formulas
expressing
are given in Cartesian
are antisymmetric
obtained
and to (-
in [ 51
the components
coordinates
this section,
it should
we can introduce
. tensor
in terms of displacements
-& einm-&srn eIij
be noted that a continuously
point of view,
a space
metric
as a space
(2.211 dislocated
with affine
medium
connection
and torsion
rj = gfl,...*cr)^
$l'...'Q)i =
equal
Formulas
by
may be considered, from the geometric different from ,!, cej3 and ,!, @IS. In fact,
of third order,
1) for odd permutations.
of the torsion
SteiijP=: .Scp) jik = In concluding
unit tensors
3% . . . . ‘It,30
ax8 ar as X~=conet T
f...l9
(2.22.l
3
(s = 1, . . ., (S -
q))
(2.23)
m=1,...,p 2sfl,..., ri),,k=
@,....ri).ff_. 13
v
The coefficients
of connection
are given
J+-P);~~
(2.20
by
&p'...'")* =
r(l,...9)*ijk3(l'...,q)k
(2.25)
DQ In passing
to another
according to transformation coefficients of connection. The torsion tensor
by (2.20),
incompatibility, taneously. It is readily L(P) 3, equals
tensor since
coordinate
system,
the coefficients
rft****q)A~~k
transform
formulas of the Christoffel symbols, and therefore they are The proof of the above is similar to that given in [3] .
S@’ “.q)i$F&3~3~ the dislocation
is no longer related
density
tensor,
when all, and not only certain
ones,
seen that the number of spaces
to the dislocation
by definition, of the parameters
with affine connection
xs
3. Equations [6].
t(1***‘@3,
simulincluding
(2.26)
coefficient.
of Equilibrium.
With th e aid of geometric
We repeat identities
and R’e’~j~~3~3~~‘~3~ it is possible theory of dontinuous
complete
change
c~+c~+...+c[i=25 where C, k is the binomial
density
characterizes
dislocations
to obtain [21,
here almost
interrelating
verbatim
the complete
gfe)$&~,
set of static
of Kunin
,$fs)ijk3*3%k
equations
for the
f41 and [61
#e)ij 3i3j= 0, CurI,o(e)ij3i3j = aij3i3j, Di\r Here ru(e)i. sre th e components I
the discussion
the tensors
of the elastic
distortion
#ePi= ~(diiZ7~ w(e)rmj3.1 J tensor
Kinematics of a continuously dislocated
,(e)i,
CC_
=
(3.2)
ad
3
The operations
1135
medium
of Curl and Div on a tensor
ai%+3j
are defined
by
Rakm
Curl aij3i3j=
cilm Dz’
3,3,
,,$ Div cii3i3j= The known tensor
of the density
3
(3.3)
3j
of dislocations
atj3tgj
should
be subjected
to the
condition Divai’3i3j Clearly, interrelating
however,
we may obtain
similar
= 0 results
(3.4) with the aid of geometric
identities
the tensors g(nl,j
Curl w(P)ij a,$
=
a’j3i3j,
-
R(P)
S(o)ijk3t3j3k,
3”$,
Div p(oltj
. l . ijk Bia3Bkal
p(pjij =
3, 3j = 0,
h(rr’tjlrn ,@lm
(3,5)
Here ,(p)i
are the components If both systems is permissible
of the parametric of equations
since
.3
aui
ax’
a$
azf
distortion
tensor.
are combined,
the equations
are linear,
Curl Wij3,3j
combining
Divpij3i3j =O, .. PI3 = h(eliilm m(e) Im + The first equation
in (3.7)
is satisfied
of equilibrium
equations,
which
Jj = W’“‘ij + uwj pij =
(3.7) are the equations
corresponding
we obtain
0,
z
(3.6)
#e)ti
@)iilm
identically;
and equations
+
#P)fj
(3.7)
,(p)I,
the second
of state,
and third equations
in
respectively.
If the medium is in a state of static equilibrium, then the parameters of the medium must satisfy all three systems of equations simultaneously, from which it follows that in a medium with dislocations defined
by (3.2),
there must exist
but also the parametric
not only the elastic
stress
tensor
The system of equations (3.7) is not complete. dynamic system will be obtained in future work.
stress
p(P)ij3i3j,
A complete
In conclusion, the author expresses thanks to L.D. interest in this work and for their valuable advice.
tensor
defined
p(P)ij3,3j,
by (3.5).
set of equations
Sedov and V.V.
Lokhin
for a for their
BIBLIOGRAPHY 1.
Eshelby J., Kontinual’naia vo inostr. liter., M., 1963.
2. Landau L.D. and Lifshits M., 1965.
teoriia
dislokatsii
E.M., Teoriia
(Theory
uprugosti
of continuous
(Theory
dislocations).
of elasticity).
Izd-vo
IzdNauka,
V.A.
1136
Babkin
3.
Sedov L.D., Vvedenie v mekhaniku solids). Fizmatgiz, M., 1962.
4.
Kosevich A.M., Dinamicheskaia lJFN, Vol. 84, No. 4, 1964.
5.
Kondo K., Memoirs of unifying study of the basic problems in engineering geometry, I. II. Tokyo, Cakujutsu Bunken Fukyn-Kai, 1955, 19.58.
6.
Kunin
I.A.,
Teoriia
dislokatsii
sploshnoi
teoria
(Theory
sredi
dislokatsii
(Introduction
(Dynamic
to the mechanics
theory
of dislocations). Dopolnenie Tenzomyi analiz
(Supplement to the monograph) by Skhouten, J.A., analysis for physicists). Izd-vo Nauka. M., 1965.
Translated
of
of dislocations).
by means
k monografii dlia fizikov
by H.H.
of
(Tensor