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It is cle
ar that th
is matrix reduces to the stiffness matrix for an Euler-Bernoulli matrix as
ε
=
Then
A
=
4
,B
=
2
,D
=
of Eq. (11.51) permit
the formation of stiffness matrices expressed in terms of polynomials in
|
N
0
|
/
EI
→
0
.
0
.
The expansions in
ε
ε
,
rather than in
terms of transcendental functions.
The applied distributed loading
p
i
0
p
i
0
can be
obtained by integration of Eqs. (11.23) or from a power series expansion. Loading functi
on
s
for several distributed loadings are listed in Tables 4.4 and 11.1. See Example 11.5 for
p
i
0
for some prescribed imperfections.
of the basic relationship
p
i
k
i
v
i
=
−
Bar in Tension
(
N
0
>
0)
.
−
N
a
u
a
EA
/
0
0
EA
/
0
0
2
.
w
a
V
a
(
A
+
B
)
+
D
]
EI
/
3
−
(
A
+
B
)
/
−
(
A
+
B
)
+
D
]
EI
/
3
−
(
A
+
B
)
/
2
[2
EI
0
[2
EI
.
M
a
θ
a
A
EI
A
+
B
)
2
B
EI
/
0
(
EI
/
/
=
......
.
...
.........
.........
N
b
u
b
.
EA
/
0
0
V
b
w
b
.
A
+
B
)
+
D
]
EI
3
A
+
B
)
2
Symmetric
[2
(
/
(
EI
/
M
b
θ
b
A
EI
/
p
i
k
i
v
i
(11.52)
=
where
ε(
ε
−
ε
ε)
sinh
cosh
2
15
ε
11
6300
ε
2
4
A
=
A
=
+
−
+···
4
2
(
cosh
ε
−
1
)
−
ε
sinh
ε
ε(ε
−
ε)
sinh
1
30
ε
13
12 600
ε
2
4
B
=
B
=
−
+
−···
2
(
ε
−
)
−
ε
ε
2
cosh
1
sinh
2
ε
(
1
−
cosh
ε)
1
10
ε
1
1400
ε
2
4
A
+
B
=
A
+
B
=
6
+
−
+···
2
(
cosh
ε
−
1
)
−
ε
sinh
ε
N
EI
D
=
ε
2
2
=
−
ε
3
sinh
ε
6
5
ε
1
700
ε
2
4
(
A
+
B
)
+
D
=
(
A
+
B
)
+
D
=
+
−
+···
2
2
12
2
(
cosh
ε
−
1
)
−
ε
sinh
ε
(11.53)
|
Note that the axial force
N
occurs in both the matrix
k
i
EI
) and
the force vector
p
i
. Use of this matrix in a stability study of frames is discussed later in this
chapter.
The corresponding load vectors are readily calculated, or can be taken from Tables 11.1
or 4.3.
The parameters
A
,B
,A
+
(through
ε
=
N
0
|
/
B
,D
,
2
A
+
B
)
±
D
,
are plotted in Fig. 11.14 as functions
(
of
ε
(Chwalla, 1959).
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