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The eigenvalues (principal stresses) of T are the three real roots of the cubic equation
given by Eq. (1.82)
3
2
|
T
λ
I
| =− λ
+
I 1 λ
I 2 λ +
I 3 =
0
(1.87)
where
I 1
= σ
+ σ
+ σ
x
y
z
2
xy
2
yz
2
xz
I 2
= σ
σ
τ
+ σ
σ
τ
+ σ
σ
τ
x
y
y
z
x
z
yz
xz
xy
I 3
= σ
σ
σ
σ
τ
σ
τ
σ
τ
+
2
τ
τ
τ
yz
Since the principal stresses must be independent of the choice of the coordinate system,
the coefficients of this cubic polynomial are uniquely determined. This means that the
quantities I 1 ,I 2 ,I 3 , called stress invariants , have the same values regardless of the choice of
axes x, y, z in which the state of stress is given. If, in particular, these axes are chosen to be
a set of principal axes, then the shear stresses are all zero and the invariants are expressed
in terms of the principal stresses
x
y
z
x
y
z
xy
xz
σ 1 ,
σ 2 ,
σ 3 as
I 1
= σ
+ σ
+ σ
1
2
3
I 2
= σ
σ
+ σ
σ
+ σ
σ
(1.88)
1
2
2
3
1
3
= σ
σ
σ
I 3
1
2
3
1.7.2 Extreme Shear Stresses
The extreme values assumed by the shear stresses as cutting plane orientation varies will
be determined in this section. The calculations are simplified if the x, y, z axes are chosen
to be a set of principal axes at the point in question. We relabel these axes 1 , 2 , 3, and write
the stress vectors on coordinate planes as
σ 1
= σ
1 e 1
σ 2
= σ
2 e 2
3 e 3
These are the stress vectors of Eq. (1.77) expressed along the principal axes for which the
corresponding shear stresses are zero. As in Eq. (1.79), the stress vector on a plane whose
unit normal is the vector a is written as
σ 3
= σ
3 e 3
The stress vector σ a can be decomposed into two orthogonal components σ a
σ a
=
a 1
σ
1 e 1
+
a 2
σ
2 e 2
+
a 3
σ
·
a and a shear
τ.
component of magnitude
Then, this shear component is given by
a 1 σ
3 2
τ 2
2
a 1 σ
2
1
a 2 σ
2
2
a 3 σ
2
3
a 2 σ
a 3 σ
=
σ a
·
σ a
(
σ a
·
)
=
+
+
+
+
a
1
2
A more convenient, equivalent expression for calculating extreme values is
2
2 a 1
a 2 +
2 a 2
a 3 +
2 a 3
a 1
τ
=
σ
)
σ
)
σ
)
(1.89)
1
2
2
3
3
1
For
τ
to attain an extreme value the function
λ a 1 +
1
2
a 2 +
a 3
F
(
a 1 ,a 2 ,a 3 ) = τ
in which
λ
is a Lagrange multiplier that must assume its extremum. The conditions
F
F
F
F
∂λ =
a 1 =
0
a 2 =
0
a 3 =
0
0
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