18. chapter 18- geometric nonlinearities _a4
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CHAPTER 8
GEOMETRIC NONLINEARITIES
The geometric nonlinear behavior is usually associated with thin, flexible
structures, subjected to simultaneous bending and compression. Thus,
structural components as frame columns or diaphragms are dangerously
exposed to the buckling effect. Common materials used in civil engineering,
as masonry, concrete or steel are quite stiff, with rather large values of the
elasticity modulus. Thus, the geometric nonlinearities due to a very
deformable medium are rarely encountered.
Generally, the geometric nonlinearity is an approach based on the
structures geometry changes, occurring when the structure deforms under
the applied loading conditions. When displacements are no longer
negligible, the stiffness matrix K is not a constant matrix any more, but
becomes a function of displacement . The geometric nonlinearities are
associated with shape changes and overall rotations.
Two types of geometric nonlinearities are discussed below:
- large stains the strains are no longer negligible, shape changes and
rotations occur;- large deflections mechanism type of deformation, with large
rotations but small strains (when structural components exhibit a
quasi solid body motion).
1. Large strains
During a large strain deformation, the applied loads make the solid move
from the undeformed position to the deformed one. The loading points are
also following the same displacement. Both initial and final locations are
represented by the corresponding position vector: X for the undeformed
state and xfor the deformed state (see figure 18.1). The displacement vector
is computed as:
Xx = (18.1)
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Fig. 18.1Position vectors during the motion of the deforming body
The deformation gradient written in terms of the displacement is defined as:
X
I
X
xF
+=
= (18.2)
The deformation gradient includes the volume change, the rotation and the
shape change. The volume change, with V0and Vthe initial and the current
volumes respectively, is
Fdetdd
0
=VV (18.3)
The deformation gradient can be separated into a rotation and a shape
change:
RUF= (18.4)
with Rthe rotation matrix and Uthe shape change (or stretch) matrix. Once
the stretch matrix is known, a logarithmic strain measure can be defined as:
U ln= (18.5)
Equation (18.5) is determined by spectral decomposition of U:
x
yxX
Undeformed Deformed
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Tiii ee =
3
1ln (18.6)
with ithe eigenvalues and eithe eigenvectors of Urespectively.
The evaluation of is made by incremental approximation, n being the
current load step and n - 1the previous one:
= n d (18.7)
with
nn
U = ln (18.8)
The increment of the stretch matrix Unis computed from the incremental
deformation gradient:
nnn URF = (18.9)
where 11= nnn FFF .
The approximate method starts with
mmn
T
mn RR ,= (18.10)
with Rm the rotation matrix computed from the deformation gradient
evaluated at the midpoint position:
X
IURF
+== mmmm (18.11)
and the midpoint displacement
( )12
1= nnm (18.12)
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The midpoint strain increment is also computed from the midpointconfiguration:
nmmn B = , (18.13)
The total strain of the current load step is computed by adding the strain
increment to the previous load step strain:
nnn += 1 (18.14)
On element level, the large strain formulation is represented by a tangent
stiffness matrix with two components: the usual stiffness matrix and thegeometric stiffness contribution:
iii GKK += (18.15)
2. Large deflections
The large deflection hypothesis with large rotations and small mechanical
strain - is seldom encountered in civil engineering, except for assemblage
details of prefabricated structural components. It is more suitable for
machineries or mechanism type of structural parts.
In case of large deflection theory, the logarithmic scale measure (18.5) isreplaced by the small strain measure:
IU = (18.15)
where Uis the stretch matrix and Ithe identity matrix.
To implement large deflections, a corotational approach is used. The
nonlinearities are enclosed in the strain-displacement relationship, which
takes a special form:
nvn TBB =
(18.16)
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where Bv is the usual strain-displacement relationship in the originalelement coordinate system and Tn the orthogonal transformation matrix,
relating the original element coordinates to the rotated element coordinates.
Tn can be computed directly or in realationship with the rotation of the
element coordinate system Rn
nvn RTT = (18.17)
with Tvthe original transformation matrix.
The rotated coordinates differ from the original coordinates by the amount
of rigid body rotation. Therefore Tn is computed by separating the rigid
body rotation from the total deformation n using equation (18.4). Thedisplacement field can be divided into a rigid body translation, a rigid body
rotation and a component which causes strains
dr += (18. 18)
where r is the rigid body motion and
d the deformational displacement,
containing both translational and rotational DOF. The translational
component can be computed from the displacement field with:
( ) vvnd xxR += (18.19)
with xvthe original element coordinates in the global coordinate system and
the displacement vector in the same global coordinates. The rotational
components are extracted by subtracting the nodal rotations from the
element rotations given by r.
The elemental tangent stiffness matrix yields:
VnvT
vV
T
ne dTEBBTK = (18.20)
The elastic strain is computed from:
d
nv
el
n B = (18.21)
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withd
n the element deformation producing straining.
The modeling of large deflection can be summarized in the following steps:
1. Computation of the updated transformation matrix Tn for eachelement.
2. Extraction of the updated displacements dn from the total element
displacement nfor computing the stresses and the restoring forces.3. Updating the nodal rotations with the appropriate rotational
increments .