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all the forces
δ(ξ
,x
)
a
j
,j
=
1
,
2
,
3 for three-dimensional problems and
j
=
1
,
2 for two-
dimensional problems, can be written as
u
i
=
u
ji
a
j
(9.68)
In the rectangular coordinate system,
1
=
when
i
j
a
i
a
j
=
δ
=
ij
0
when
i
=
j
Then
u
ji
=
u
i
a
j
. From Eq. (9.58b),
g
i,kk
−
g
k,ik
a
j
=
(
1
1
u
ji
=
g
i
a
j
)
,kk
−
g
k
a
j
)
,ik
−
ν)
(
2
(
1
−
ν)
2
(
1
Since, from Eqs. (9.64) and (9.66),
g
i
=
ga
i
so that
g
i
a
j
=
ga
i
a
j
=
g
δ
ij
. Thus
1
u
ji
=
g
,kk
δ
−
−
ν)
g
,ik
δ
(9.69)
ij
kj
(
2
1
For three-dimensional problems, substitute Eq. (9.64) into Eq. (9.69) to obtain
1
1
u
ji
=
−
ν)
g
,kk
δ
−
g
,ik
δ
=
[2
(
1
−
ν)
r
,kk
δ
−
r
,ik
δ
kj
]
(9.70)
ij
kj
ij
2
(
1
16
π
G
(
1
−
ν)
The derivatives of
r
are taken with reference to the coordinates of
x
i
,
i.e.,
r
,i
=
∂
r
r
,j
=
∂
r
(9.71a)
∂
x
i
∂
x
j
and
∂
∂
(
x
i
−
ξ
)
r
i
r
i
(
r
,i
=
(
x
k
−
ξ
)
2
=
2
=
(9.71b)
k
x
i
x
k
−
ξ
k
)
where
r
i
=
(
x
i
−
ξ
)
is the projection of
r
on the
x
i
axis. From the relationships of Eq. (9.71),
i
r
2
r
∂
r
2
r
2
r
i
∂
1
r
i
r
i
∂
r
−
x
i
=
x
i
−
=
∂
∂
∂
x
i
r
3
Hence
3
3
2
r
r
2
r
k
∂
−
2
r
r
,kk
=
x
k
=
=
∂
r
3
k
=
1
k
=
1
Also
∂
r
i
r
r
∂
2
r
∂
∂
r
∂
∂
1
r
2
r
i
r
i
∂
r
r
,ik
=
x
k
=
=
=
x
k
−
∂
x
i
∂
∂
x
k
∂
x
i
x
k
∂
∂
x
k
i.e.,
1
−
r
r
,i
r
,k
when
i
=
k
r
,ik
=
1
r
(
−
)
=
1
r
,i
r
,i
when
i
k
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