Scripta M E T A L L U R G I C A
Vol. II, pp. 477-484, Printed ~n the United
1977 States
Pergamon
Press,
Inc.
ELASTIC STRAIN ENERGY AND INTERACTIONS OF THIN SQUARE PLATES WHICH HAVE UNDERGONE A SIMPLE SHEAR Jong K. Lee and William C. Johnson Department of M e t a l l u r g i c a l E n g i n e e r i n g Michigan Technological University Houghton, Michigan 49931 (Received March 28, 1977) (Revised April 22, 1977)
The elastic strain energy of and the elastic strain interaction energies between thin precipitate plates which have undergone a simple shear parallel to their broad faces is of great interest in connection with respect to twinning and martensitic phase transformations. Although the elastic strain energy associated with an equivalently sheared ellipsoidal precipitate has been exactly formulated by Eshelby (I), the interaction energy between two such precipitates has not been computed due to the considerable amount of numerical calculation involved. On the other hand, it has been shown that the calculation of harmonic and blharmonic functions and their derivatives can be performed without difficulty for any point of interest inside or outside a right rectangular parallelepiped (2). Utilizing this mathematical characteristic, we investigate in this Letter, the elastic strain energy and the interaction energies of thin square plates which have undergone a simple shear under the simplifying assumption that the matrix and precipitates are elastically isotropic and have the same elastic constants. Let an infinitely v, be subjected domain
extended matrix,
to a uniform
of a precipitate,
the constrained
V.
with shear modulus
stress-free
displacement
of u ci(~)
pTkj is the stress derived
Green's
functions
Gik(~ , ~'),
is given by (1,3)
u (~) = P j where
transformation
In terms of the elastic
~ and Polsson's ratio T strain e.. Ij within the
j(~, r')dV(r')
from the stress-free
(i)
transformation
T strain eij
using Hooke's law. Here the usual tensor suffix notation is employed. A repeated suffix is to be summed over the values i, 2 and 3. Suffixes preceded by a comma denote d i f f e r e n t i a t i o n with respect to Cartesian coordinates. For the isotropic form (3):
case,
the elastic
÷ Gik(r' where
Green's
function
i ~ik ~') - ~-~U I~-~' I
6ik is the Kronecker
delta
function.
i 16~(l-v)U
the r e s u l t i n g
for the constrained
strain eCij" " = (u~,jl + u~j,l.)/2: T
~)
relationship
,klij
Eq.
with respect
- 2ve~k¢(~)
T + ejk~(r),ki}]
22 ÷ + ~xi~x k r-r'l
Substituting
and d i f f e r e n t i a t i n g
e~ij (~) : I • ~[ekl~(
Gik(~ , ~') is given in the
,ij
(2) into Eq.
(2) (i)
to xi, one obtains
- 2(l-v)
T (~) {eik~ ,kj (3)
477
478
STRAIN ENERGY OF SHEARED THIN PLATES
Vol, ii, No, 6
where
(4)
¢(~) = f f f dV(~') v
Ir-r'l
and
dV(~').
~(~) = f f f l ~ - ~ ' J V
¢(~) is the ordinary harmonic harmonic potential function.
potential
function
while
(5) ¢(~)
is
called
the
bi-
Now we c o n s i d e r a right rectangular parallelepiped whose center is taken as the origin and whose edges are parallel to the Cartesian coordinate axes. Let the edges of the p a r a l l e l e p i p e d be 2a, 2b and 2c. For a d i l a t a t i o n a l stressfree t r a n s f o r m a t i o n Faivre
strain e T T ~ ~ 0 if i = J, otherwise ei~ T = 0), (i.e., ei~ ij c (~) by i n t e g r a t i n g Eqo (i) and (4) obtained the c o n s t r a i n e d strain ei~
d i f f e r e n t i a t i n g the e q u a t i o n thus obtained with respect to x i.
In a different
approach, Sass, Mura and Cohen (5) expressed the d i s p l a c e m e n t a s s o c i a t e d with a cube p r e c i p i t a t e in the Fourier series. In this study, we assume that the T stress-free t r a n s f o r m a t i o n strain ei~J is a simple shear in the Xl-X 3 plane T T (= x - z plane), i.e., el3 = e31 ~ 0 and all other components are zero. The elastic strain energy per unit volume of a precipitate, is given by (i): w
IH ( Tj -
=
V
T ~e13
= a~
{8abc
W, in an infinite matrix
ij
T
el3 - f
c
f
b
a c
+
/ el3(r')dx'dy'dz').
(6)
-c -b -a For the elastic
strain interaction energy between two precipitates,
we consider,
as shown in Figure i, an identical p r e c i p i t a t e whose center is at ~. For s~mpllcity, let the edges of the second p r e c i p i t a t e also be parallel to the Cartesian coordinate axes and I~] be sufficiently large so that there is no contact between the two precipitates. The interaction energy becomes (6):
Eint
l = -fffP j B>e j A
dV,
VA z+c
=
T -4~em3
f
y+b x+a
f
z-cy-bx-a
f
e lc 3 ~. -( ~ ' ) d x ' d y ' d z ' ,
where P icj (B) is the c o n s t r a i n e d stress due to the p r e c i p i t a t e whose center is T at the origin and e .(A) is the stress-free transformation strain of the ij p r e c i p i t a t e whose center is at ~.
(7)
Vol.
II, No.
6
STRAIN ENERGY OF SHEARED THIN PLATES
479
[o01] Z,X3
~ / / /...... /L
F;/
FIG. ]_ Sketch o f the orientation relationships between two square plates. The square plate at ~he orizin is denoted as B while the other one is designated as A.
1/ ~Y,X 2
[010]
/ X,X, [100] The harmonic biharmonic MacMillan.
function ~(~) has been obtained by MacMillan
(2) and the
function ~(~) is derived using techniques similar to those of Employing, with Faivre (4), the fol!owin~ notation: [f(x,y,z)] x2'y2'z2 -Xl,Yl,Z I
one obtains Cor a right rectangular ~(~) = [xy~n(r+z)
(8)
(-l)i+j+kf(xi,Yj ,z k) i,j,k=l parallelepiped:
+ yz%n(r+x)
+ zx~n(r+y)
o ] - 1 {x~tan - . ( y z ) xr
+ y2 tan-].(~_~) x y ~ xs +Jx_a, a , y +y_b, b , z +z_c c zx + z 2 t ~~ . - i t~-~j
(9)
and ~(~) = [~xyzrl ÷ ~l{(r2 x2)yzZn(r+x)
+ (r2_y2)zxgn(r+y)
+ (r2_z2)xy~n(r+z)}_~{x4tan-l(x_~)yz
+ Y4~-an-l'zx~,
]x+a,y+b,z+c + z4tan-l(z~r)}~x_a,y_b,z_c ' where r 2 = x 2 + y2 + z 2. e
e ]e3 ( r ) -~
From Eq.
(lO)
(3), el3( c ~) becomes:
T
]3 [ ~b ( ~) , ] - 1 3 3 = ~TF~-(T2b-]7
._ ( t _ v ) { ~ ( ~ ) 1
] + ~(~) , 33}]
T
f k~ --.
~ - ,I- ( 1 - v ) { t , a . ~ - - ( ~ } ;
+ ta, n - l ( ~ - t ~ ; ] - I
x-'a,?'~4b,z-'-a
'"
480
STRAIN ENERGY
The fo].lowing integration found to give: I(~)
=
OF SHEARED
which
THIN PLATES
is required
Vol.
in ca!culat~.ng
gint(~)
11, No.
is also
z+c y+b x+a ~ ~ ~ [ uw~ + (l_v){tan -I uv _ -l,wv~u+a,v+b,w+c z-c y-b x-a p(v2-p 2) (wP) + ~an ~J;]u-a,v-b,w-c
= [[(l-v)xyz{tan-l(~zY)
+ tan-l(x~)}
+ ~-~{x(y2_z2)£n
6
dudvdw
r-x
+ z(y2-x2)£n r-z _ ¼z(r2_y2)~nr7 y r+z r+y + where
2
£
, 2,~x+a,y+b,z+c]x+a,y+b,z+c 6{(6-3v)y 2 - (3-v)r IJx_a,y_b,z_c~x_a,y_b,z_c
= u 2 + v 2 + w 2.
(12)
We note that T 2 ~(e13) W = ab--~{8abc
I(~=O) } - 4n(l-v)
(13)
and
T
÷ Eint(r) For a squar e plate
2
U(el3) = - ~--~-v~-- I(~).
(14)
for which a = b = c/8,
W becomes:
2 f(B) 3 ) {I - 4 ~ ( l _ v ) g }
W = 2~(e
(15)
where f(B)
= 8(l-v)B{tan-l(
1
_4(2_v)B2tanh-1
) + tan-l(
1 l~+B~
B
)} + 4{v + (2-v)B2}tanh -I
i
4 ~{v + (3-v)B2} 2~+B2
+ ~{v + 2(3-~)B2} l + ~ B2 - ~(3-v)B 3 + v{2£n/~-1 + 4 ' ~ - 1 ) } ~+1
In Figure
2, the constrained
8 : 0.i is plotted different
strain
as a function
directions,
[I00],
C +
el3(r)
(Eq.
(Ii))
of the distance
[010],
and
[001].
whether
it is inside
We note
changes
sign from negative
For comparison, (ellipsoid
to positive
at
is calculated,
in the
that
(6),
of position
[00!]
the results
calcu-
the e~o~r) ~J
with an ellipsoidc!
using
with in three
out by Eshelby
is a function
I~I=I3B
the el3c (~) field associated
of revolution)
plate
center
In all of the numerical As pointed
a precipitate.
"
of a square
from the plate
lations, Poisson's ratio v is taken to be 1/3. c the el3(r) field associated with a square plate or outside
(16)
3"
f~e!d
direction. precioitate
of Eshe!by
(3).
Vol.
II, No.
6
STRAIN ENERGY OF SHEARED THIN PLATES
The aspect ratio,
i.e., the ratio of minor axis to m a j o r axis,
tb be 0.i, and the results are p l o t t e d
in Figure
3.
481
is again taken
c (~) field in the The el3
[001] d i r e c t i o n d i m i n i s h e s more r a p i d l y in the case of a square plate than in that of an e l l i p s o i d while in the other two directlons, [I00] and [010], the situation is reversed.
ioi.... , 1 ~oo~]
I
oo /
-~-
/I
FIG. C
o,
]
06
÷
The el3(r)
2
field a s s o c i a t e d with a
square plate (B=0.1) vs. distance from the center in the three d i r e c t i o n s [i00], [010], and [001].
~o4 03
0.1 0 -0.1 ''
-O2
O
L
02
L
0.4
I
I
I
I
0.6 08 10 12 Distance f r o m Center, r l a
1.4
16
O7r I
0.8 0 7
1001,[010]
II
k
O 5
810.1
FIG. O10]
~o.4 O3 0.2
~'
,~,oo]
j
-o.1 ~
C
02
04
06 0.8 10 1.2 Dlstancg f r o m Center, r f a
3
c (~) field a s s o c i a t e d with an The el3 e l l i p s o i d a l precipitate (B=0.1) vs. distance from-the center in the three d i r e c t i o n s [100], [010] and [001].
14
•~
482
STRAIN ENERGY
OF SHEARED
THIN PLATES
Vol,
II~ No,
6
Figure 4 shows the elastic strain energy a s s o c i a t e d with a square plate (Eq. (15)) as a function of B (= c/a). Again, for comparative purposes, Eshelby's results on the ellipsoidal p r e c i p i t a t e (i) are included in this figure. When B~0.35, the ellipsoidal p r e c i p i t a t e has a smaller elastic shear strain energy than the square plate while the situation is reversed for B~0.35. The ratio of W c u b e / W s p h e r e is found to be 0.94. 0.7
0,6
Sphere
~./~ /
0,5
Square P'°'"
~-- 0 . 4
FIG.
~ 0.3
/~/// 0.2
~):113
111II
0.1
%
o!~ o!4 o!6 o!8
,!o 12~........ 14 ,6
The (self) elastic shear strain energy per unit volume of a precipitate vs. the aspect ratio, B. The solid line shows the strain energy a s s o c i a t e d with a square plate while the dashed line indicates that of an ellipsoidal precipitate.
Figures 5 and 6 show the ratio of the interaction energy
(Ein t) to the
total (self) elastic shear strain energy (2VW) as a function of distance between the centers of the two square plates. In Figure 5, ~ is 0.01 while Figure 6 shows the results when ~=0.i. As one might expect, the m a x i m u m interaction energy occurs when the centers are aligned along the [001] d i r e c t i o n and the two p r e c i p i t a t e s are nearly in contact; the ratio of Ein t to 2VW is 0.71 when B=0.01 and 0.45 for B=0.1. Figure 7 shows the m a x i m u m possible interaction energy, in the same terms, as a continuous function of B. In the other directions, the i n t e r a c t i o n energy diminishes rapidly with i n c r e a s i n g distance relative to the d i m e n s i o n of the plate in that direction. We note that in the i n t e r a c t i o n energy calculation, transformation
the same stress-free
strain e~. Hence, if the centers of ij is assumed for both plates. the two square plates are aligned along the [001] direciton, and their transformation strains are simple shears of opposite sign in the x-z plane, the m a g n i t u d e s of their elastic interaction energies are the same but the signs are reversed. Thus, when B=0.1, the elastic interaction energy can decrease the total (self) shear strain energy of plates aligned in the [001] d i r e c t i o n by a factor of 0.48.
Vol.
Ii, No.
6
STRAIN
ENERGY
OF SHEARED
THIN
PLATES
483
080 070 060 /3:001 050 040
~Tn.
030
The
e4 ~O2O
ratio
center
5
E i n t / 2 V W , vs.
distance,
where
the
inter-
Ein t is the
shear i n t e r a c t i o n e n e r g y and V W is the self shear s t r a i n e n e r g y a s s o c i a t e d w i t h a square p l a t e , 6=0.01.
01
-01 -0.2' -0 30~Inter-center di.~tance, rla
0.8
i
i
1.0
0.7
09
06 08
0.5
/3=01 07
0.4 >0.6 >~0.3
E
e,l
~e5
jO.2
,2
~01]
"~04 w
0.1
03
0 -0.,
[010}-/&~O]
02 0.1
-0.2 -0"30
1
3
012
4
Inter-center distQnce, rio
FZG. The ratio, center
6
E i n t / 2 V W , vs.
distance,
where
0 4J
#
FIG. the
inter-
Ein t is the
s h e a r i n t e r a c t i o n e n e r g y and V W is the self shear s t r a i n e n e r g y a s s o c i a t e d w i t h a s q u a r e plate. 6 = 0.i.
I __ 10 L 0.8
016
--1.2
7
The p o s s i b l e m a x i m u m ratio, E i n t / 2 V W , vs. the a s p e c t r a t i o , 6. These v a l u e s are d e v e l o p e d at the [001] o r i e n t a t i o n w i t h T an el3 s i m p l e shear.
484
STRAIN ENERGY OF SHEARED THIN PLATES
Vol.
II, No.
Acknowledsements This work was supported by the Divsion of Materials Research of the National Science Foundation under Grant DMR76-06855 for which much appreciation is expressed. The authors are indebted to Professor H. I. Aaronson for introducing us to this problem and his invaluable discussions of this work and to Professors D. M. Barnett and K. C. Russell for their helpful comments. References i. 2. 3. 4. 5. 6.
J. D. Eshelby, Proc. Roy. Soc. A241, 376 (1957). W. D. MacMillan, The Theory of the Potential, p. 78, McGraw-Hill, (1930). J. D. Eshelby, Proc. Roy. Soc. A252, 561 (1959). G. Faivre, Phys. Stat. Sol. 35, 2-~-9 (1964). S. L. Sass, T. Mura and J. B__Cohen, Phil. Mag., 16, 679 (1967). J. D. Eshelby, Progress in Solid Mechanics, 2, 89-~1961).
New York
6