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Principle of Virtual Work
Degrees of Freedom
Associated with the concept of the lumped-mass approximation is the idea of the NUMBER
OF DEGREES OF FREEDOM.
This can be defined as
“the number of independent co-ordinates required to specify the configuration of the
system”.
The word “independent” here implies that there is no fixed relationship between the coordinates, arising from geometric constraints.
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Degrees of Freedom of Special Systems
A particle in free motion in space has 3 degrees of freedom
z
particle in free motion in space
has 3 degrees of freedom
r
y
x
3
If we introduce one constraint – e.g. r is fixed then the number of degrees of freedom reduces to 2.
note generally:
no. of degrees of freedom = no. of co-ordinates –no. of equations of constraint
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Rigid Body
y
P1
P3
This has 6 degrees of
freedom
3 translation
3 rotation
P2
.
x
3
e.g. for partials P1, P2 and P3 we have 3 x 3 = 9 co-ordinates but the distances between
these particles are fixed – for a rigid body – thus there are 3 equations of constraint.
The no. of degrees of freedom = no. of co-ordinates (9) - no. of equations of constraint (3)
= 6.
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Formulation of the Equations of Motion
Two basic approaches:
1. application of Newton’s laws of motion to free-body diagrams
Disadvantages of Newton’s law approach are that we need to deal with vector quantities
– force and displacement.
thus we need to resolve in two or three dimensions – choice of method of resolution
needs to be made. Also need to introduce all internal forces on free-body diagrams
– these usually disappear when the final equation of motion is found.
2. use of work
with work based approach we deal with scalar quantities – e.g. work – we can develop
a routine method – no need to take arbitrary decisions.
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Free body diagram
θ
T
mg
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Principle of Virtual Work
The work done by all the forces acting on a system, during a small virtual displacement is
ZERO.
Definition A virtual displacement is a small displacement of the system which is compatible
with the geometric constraints.
P2
P1
b
a
b
P1 aδθ
P2 bδθ
a
e.g.
This is a one-degree of freedom system, only possible movement is a rotation.
work done by P1 = P1(- aδθ)
work done by P2 = P2(bδθ)
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Total work done = P1(- aδθ) + P2(bδθ) = δW
By principle of Virtual Work
δW = 0
therefore:
P1 (- aδθ) + P2(bδθ) = 0
- a P1 + b P2 = 0
P1a = P2b
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D’Alembert’s Principle
Consider a rigid mass, M, with force FA applied
A = &x&
FA
M
(acceleration)
From Newton’s 2nd law of motion
F A = Ma = M&x&
or
F A − M&x& = 0
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Now, the term ( − M&x& ) can be regarded as a force – we call it an inertial force, and denote it FI – thus
we can then write:
F I = − M&x&
FA + FI = 0
In words – the sum of all forces acting on a body (including the inertial force) is zero – this is a statics principle.
In fact all statics principles apply if we include inertial forces, including the Principle of Virtual Work.
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Virtual Work and Displacements
Using the concept of virtual displacements, and virtual work, we can derive the equations of
motion of lumped parameter systems.
Example 1
Mass/Spring System
x
k
m
Here number of degrees of freedom =1
Co-ordinate to describe the motion is x
Now consider free-body diagram, at some time t
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Total _ force : −m&x& − kx
δW = (− m&x& − kx )δx = 0
Hence
− m&x& − kx = 0
or
m&x& + kx = 0
R (reactive force)
m
m
inertial force
− m&x&
restoring force kx
mg (gravity force)
General one degree of freedom system
If q1 is the co-ordinate used to describe the movement then the general form of δW is as follows:
δ W = Q 1 δ q1
we call δq1 – generalised displacement
Q1 – generalised force.
δW
From principle of virtual work
= Q 1 δ q1 = 0
∴ Q1 = 0
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Example
Referring to the mass/spring system again
x= q1
k
m
x
δ W = (− m q&&1 − kq 1 )δ q1 = 0
∴ Q1 = − m q&&1 − kq 1 = 0
m q&&1 + kq 1 = 0
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Example 2
Simple pendulum
− mlθ& 2
(inertial force –radial)
0
θ
− mlθ&&
(inertial force – tangential)
P
mg
This is another one degree of freedom system.
During a virtual displacement, δθ, the virtual work done is
δW =
(−ml&θ& − mg sin θ) lδθ = 0
δW = 0 (PVW)
∴ ml&θ& + mg sin θ = 0
&θ& + g sin θ = 0
l
or
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Example 3 – two degrees of freedom system
x1
k
x2
k
m
m
free-body diagrams.
kx1
-mx1
m
k(x2-x1)
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-mx2
m
14
For LH mass:
[− kx1 − m&x&1 + k (x2 − x1 )]δx1 = δW1
[− k (x2 − x1 ) − m&x&2 ]δx2 = δW2
δW = δW1 + δW2 = (Q1 )δx1 + (Q2 )δx2
For δW = 0 for all
δx1 , δx2
the Qi quantities must be zero.
Hence:
m&x&1 + kx1 − k ( x2 − x1 ) = 0
m&x&2 + k ( x2 − x1 ) = 0
or
m 0   &x&1   k
 0 m  &x&  + − k

 2  
− k   x1  0
=
k   x2  0
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n degree of freedom systems
Having discussed single and two degree of freedom systems, and introduced the concept of
generalised forces we can now consider the general case of an n degree of freedom system.
A virtual displacement must be consistent with the constraints on the system. The motion can be
described by n independent, generalised co-ordinates, q1 , q2 ,...., qn .
Hence a virtual displacement can be represented by small changes in these co-ordinates:-
δ q1 , δ q 2 ,..., δ qn
Suppose only one co-ordinate,
qi (1 ≤ i ≤ n ) is given a small, imaginary displacement,
δ qi . As a
result every particle in the system will be, in general, displaced a certain amount. The virtual work
done will be of the form
acting on the system.
δW = Qiδ qi where Qi is an expression relating directly to the forces
Qi is the generalised force associated with qi .
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From the principle of virtual work
δW = Qiδ qi = 0
Since,
δ qi
is finite, we get
Qi = 0
This must be true for
i = 1,2,..., n.
Q1 = 0
I.e.
Q2 = 0
M
Qn = 0
these are the equations
of motion of the system
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The generalised forces have component parts
1)
2)
3)
4)
5)
inertial forces (mass x acceleration)
elastic or restraining forces
damping forces (energy dissipation)
external forces
constraint forces
δW = Qiδqi =δWI +δWE +δWD +δWA
inertial
elastic
damping external
(
)
= QiI + QiE + QiD + QiA δ qi
(Noting, as before, that the constraint forces do no virtual work)
Then the equations of motion are:
QiI + QiE + QiD + QiA = 0
i = 1,2,..., n
These are the n equations of motion.
We will examine each of these components now, in more detail. The aim is to
relate these component forces to the generalised co-ordinates
q1 , q2 ,...., qn .
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Inertial Forces (See also Handout)
The position of the ith particle of mass, in the system, is, in general, related to the
n generalised co-ordinates, and time (if the constraints are independent of time)
then the position of the ith particle depends only on the n generalised coordinates. Thus
r r
ri = ri (q1, q2 ,...,qn , t)
(1)
Now we suppose that the system is in motion and that we represent the inertial
force on the ith particle (using D’Alembert’s Principle) as
r
− mi &r&i
(2)
We now give the system an arbitrary virtual displacement – this can be
represented in terms of generalised co-ordinates by δq1 , δq2 ,..., δqn . The virtual
displacement of the Ithparticle can be represented by
r
δr
(3)
and the virtual work done by the inertia force on the Ith particle is simply
r&
r
&
(−mi ri ). δri
(4)
(note that this is a scalar product). From this result we get the total virtual work as
r
r
δW I = ∑ (−mi &r&i ). δri
i
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(5)
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Using equation (1) we have
r
n
∂ri
r
δri = ∑
⋅ δq j
∂
q
i =1
j
(6)
Hence
r
r& n ∂ri
&
δW = ∑ (− mi ri ) ⋅ ∑
⋅ δq j
∂
q
i
j =1
j
I
(7)
and re-arranging


n
(
r
)
δW I = ∑ δq j ∑ − mi &r&i ⋅
j =1
i
∂ri 

∂rj 
(8)
However, the generalised inertial forces, Qj, are effectively defined by
r
n
δW I = ∑ (− mi &r&i ) ⋅ ∑ Q Ij δq j
j =1
i
(9)
Comparing (8) and (9) we have
r
r&& ∂ri
Q = ∑ (− mi ri ) ⋅
∂q j
i
I
j
(10)
It is shown in the handout notes that
Q Ij = −
∂ ∂T
(
∂t ∂q& j
)+
∂T
∂q j
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(11)
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where T is the total KE
T =
∑
i
1
r r
m i r&i ⋅ r&i
2
(12)
Elastic Forces
Consider a simple spring:
←FS
•
FE
x
For static equilibrium
FE = FS
(external force)
= (internal spring force)
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Suppose we define the POTENTIAL ENERGY, V, as the work done by the
external force to extend the spring a distance χ
κχ
FE
χ
external work done =
1 2
kx = V
2
∴ V = f (x) =V(x)− a function of
Here
V =
extension of
spring
x
1 2
kx
2
The work done by the internal spring force, W, is equal and opposite to V
1
W = −V = − kx 2
2
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Now consider a small, virtual displacement,
and V are as follows:
δx . Corresponding changes to W
δV
δV = ⋅ δx = −δW
δx
Comparing with standard form
δ W = Q E1 δ q1
then
( q1 = x , here )
Q1E = −
∂V
∂V
= −
∂ q1
∂x ⋅
Generally,
V = V ( q1 , q 2 ,...., q n )
δ V = −δ W =
∂V
δq j
∑
∂
q
j =1
j
n
Compare with
δW
∴
∑
=
Q
E
j
Q
= −
E
j
δq
j
∂V
∂q j
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Lagrange’s equation
Suppose that no damping forces are present, and there are no externally
applied forces. Then
QiD = QiA = 0
(i = 1,2,...,n)
We have found that
QiI = −
∂  ∂T  ∂T

+
∂t  ∂q&i  ∂qi
QiE = −
∂V
∂qi
(i = 1,2,...,n)
If we collect these results we get
∂  ∂T  ∂T ∂V
−

+
=0
∂t  ∂q& i  ∂qi ∂qi
(i = 1,2,..., n )
This is LAGRANGE’s EQUATION
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If we define
L=T-V
And assume that V does not depend on the
be written as:
q&i ’s, then Lagrange’s equation can
∂  ∂L  ∂L

 −
=0
∂t  ∂q&i  ∂qi
Example 1- mass/spring system
x
k
m
Here
∂T
=0
∂q1
This is a single degree of freedom system. Here
q1 = x
and
∂  ∂T  ∂

 = (Mq&1 ) = Mq&&1
∂t  ∂q&1  ∂t
∂V
= kq1
∂q1
1
m q& 12
2
1
V =
kq 12
2
T =
Hence
mq&&1 + kq1 = 0
The Lagrange equation is (n=1 so only one equation)
∂  ∂T  ∂T ∂V
−

+
=0
∂t  ∂q&1  ∂q1 ∂q1
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Example 2-simple pendulum
1
θ
q1 = θ
Here
In terms of
l
m
q1
we have
T=
1
2
m (l q& 1 )
2
V=
mgl(1 − cos q1 )
Hence
∂  ∂T  ∂

 =
ml 2 q&1 = ml 2 q&&1
∂t  ∂q&1  ∂t
(
)
∂T
=0
∂q1
∂V
= mgl sin q1
∂q1
ml 2 q&&1 + mgl sin q1 = 0
or
q&&1 +
g
sin q1 = 0
l
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