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THEORY
OF
STRUCTURES
Theory of Structures
Revision of De Saint Venant's Problem 14-09-20
Consider an elastic node with any possible shape section that must be constant over the length
DSV considers a reference system centered in the geometric centroid of the section (⟶ we need a geometric analysis to find it)
Properties of centre of gravity:
Sx = ∫ y dA = 0
Sy = ∫ x dA = 0
First order moments
In order to have a principal reference system we need that
Ixy = ∫ xy dA = 0
Mixed moment of inertia
In addition we define also:
Ix = ∫ y2 dA > 0
Iy = ∫ x2 dA > 0
Moments of inertia
Properties of DSV's Problem
Linear-elastic homogeneous isotropic material
Small strain & displacement
No thermal strain (⟶ no inelastic effects)
No body forces (e.g. gravity)
⟶ body forces are distributed over the volume
No forces on the lateral surface ⟶ we can only have forces on initial and end sections
No extreme constraints ⟶ body is completely free ⟶ global equilibrium must be neglected
⟶ We know the resultant actions on the extreme sections
Def: Cauchy's Stress Components Gxx, Gxy, Gxz ⟶ direct components Normal stress = δxx Shear stress = τxy, τxz - refer to 1:2 x-axis
⟶ Triangular components (equilibrium of a small volume element) refers to the 1:2 y-axis and 1:2 z-axis
Balance Equations:
∫ Gxa dA = N
∫ x Gya dA = Mx
∫ y Gxa dA = My
N.B. For an open section: we not consider shear center
Consider xc - yc dA = M + Tx - Ty
Note: External constraint is a combination of displacements something reduction in increments. DSV solve the problem in the absence of any external constraint
on Γ boundary conditions
Initial Hypothesis (Gx, Gy, Zxy = 0) are ok because all equations are satisfied
Knowing stress tensor, once we have the stress fields we can easily compute the strain field (εj, εt).
Now, we want to focus on the problem of PURE TORSION
DSV hypotheses (Gx, Gy, Zxy) are zero; then M = only torque → Σi, Σip = 0
To have an analytical solution we have to consider what happens to Σzx, Σyp
We take into account last equation of independent equation system m which is → equilibrium equation in A
and we manipulate the two remaining compatibility equations m which E + Ey - σy = 0
They can be summarised in a single differential equation
From boundary conditions on Γ we obtain: equilibrium on Γ
We can obtain Σzx, Σyp solving the linear differential problem of 2 equations and 2 unknowns.
Equilibrium in A
Compatibility in A
+ boundary condition in strong form on Γ
+ boundary condition in weak form
Next it to compute CONSTANT C
cos: it is a well-posed problem that admits a unique solution
Applying the constitutive law:
χxx=⟨χxx⟩C=Gβ∂⟨yG⟩C/∂x∂y
χyy=⟨χyy⟩C=Gβ∂⟨yG⟩C/∂y2
Let's see now if they are in agreement with governing equations:
- COMPATIBILITY EQUATION:
∂2χxx/∂x = ∂2yG/∂y = C
⇒ GP ( ∂2φ/∂x∂y + ... + 1) = C
- EQUILIBRIUM EQUATION:
∂2χxx/∂x + ∂2yG/∂y = 0
⇒ GP ( ∂2χxx/∂x2 + ∂2χyy/∂y2 ) = 0
we obtained the well-known LAPLACE OPERATION:
∇2yG = 0
if I take also the harmonic problem I can compute the warping function
- BOUNDARY CONDITION:
m STRONG FORM
⟨χxx⟩m + ⟨χyy⟩m My = 0 ⇒ (∂yG/∂x) Mx + (∂yG/∂y) My = 0
yG = ymx - xmy
∇2yG = 0
∂yG/∂m = ymx - xmy
NEUMANN-DIRICHLET PROBLEM
HR is a boundary condition on a normal derivative
it admits a solution, but the solution is not unique This is due to the fact that boundary condition is expressed in terms of the derivative of something (yG)
So we can always add a constant to yG without altering the governing equation.
This is due to the fact that boundary condition is not affected.
We can add to yG a constant that is that the rigid body rotation the solution is not unique because of these reasons BUT the dimensions of φ are unique
Continue with thin-walled open sections
We have seen STATICS.
C2B = 2 Mt, m / J
Jw = 4/3 ∫ b3 ds
From the stress distribution we observed that the maximum shear is in correspondence of the boundary for m maximum and m = m1 ± b2.
When section is not uniform along the mean line, the maximum tangential stress is where the thickness b is the greatest.
τcmax = 2 Mt b(s) / J
For KINEMATICS an important parameter is β ( Mt / 4GJ )
L way in which torsional rotation increases along the axis, but it is not sufficient to describe the whole kinematic field.
Remember that we defined (if centroid is the reference point):
- SX = βxy
- SY = βxz
Once we have computed, β we can obtain SX, SY.
To have an approximate solution we assume γ0 constant across the thickness of the profile, because thickness is very small.
We focus our attention on the warping function on the mean line only γ6(s)
For computing the warping function on the mean line we can consider the following procedure:
- Try to compute the moment of the warping function along the mean line: dγ6 / ds
From differential geometry we can compute it as:
dγ6 = ∂γ∂x . ∂x∂s + ∂γ∂y . ∂y∂s
We are assuming that the mean line is a PARAMETRICAL curve - the points are modelled through the curve as a function of parameters, and then we have x(s), y(s).
If we know the shape of the mean line we can compute the two terms ∂x/∂s, ∂y/∂s that are functions of s.
Remember that the tangent vector to the mean line is given by ts = d2d1(from differential geometry)
Remember also that tangent vector is orthogonal to normal vector tn . m
Angle warping function for a closed profile is given by:
Consider an axial path.
b(s) ds.
From a point and do the whole loop of the parameter, and arrive to the certain point.
compatibility equation.
Start from a point and do the whole loop of the parameter, and arrive to the certain point.
OSS:
By comparing two found expression of
we can easily compute
Torsional inertia for a closed section
from the basis of geometry