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Section 8.6
Solid Mechanics Part I Kelly268
8.6 The Principle of Minimum Potential Energy
The principle of minimum potential energy follows directly from the principle of
virtual work (for elastic materials).
8.6.1 The Principle of Minimum Potential Energy
Consider again the example given in the last section; in particular re-write Eqn. 8.5.15 as
0
22
2
2
22
1
11













 BB u
L
AE
L
AE
Pu (8.6.1)
The quantity inside the curly brackets is defined to be the total potential energy of the
system,  , and the equation states that the variation of  is zero – that this quantity does
not vary when a virtual displacement is imposed:
0 (8.6.2)
The total potential energy as a function of displacement u is sketched in Fig. 8.6.1. With
reference to the figure, Eqn. 8.6.2 can be interpreted as follows: the total potential energy
attains a stationary value (maximum or minimum) at the actual displacement ( 1u ); for
example, 0 for an incorrect displacement 2u . Thus the solution for displacement
can be obtained by finding a stationary value of the total potential energy. Indeed, it can
be seen that the quantity inside the curly brackets in Fig. 8.6.1 attains a minimum for the
solution already derived, Eqn. 8.5.17.
Figure 8.6.1: the total potential energy of a system
To generalise, define the “potential energy” of the applied loads to be extWV   so that
VU   (8.6.3)
The external loads must be conservative, precluding for example any sliding frictional
loading. Taking the total potential energy to be a function of displacement u, one has
0
)(


 u
du
ud
 (8.6.4)
)(u
1u
1u
2u
2u
Section 8.6
Solid Mechanics Part I Kelly269
Thus of all possible displacements u satisfying the loading and boundary conditions, the
actual displacement is that which gives rise to a stationary point 0/  dud and the
problem reduces to finding a stationary value of the total potential energy VU  .
Stability
To be precise, Eqn. 8.6.2 only demands that the total potential energy has a stationary
point, and in that sense it is called the principle of stationary potential energy. One can
have a number of stationary points as sketched in Fig. 8.6.2. The true displacement is one
of the stationary values 321 ,, uuu .
Figure 8.6.2: the total potential energy of a system
Consider the system with displacement 2u . If an external force acts to give the particles
of the system some small initial velocity and hence kinetic energy, one has K0 .
The particles will now move and so the displacement 2u changes. Since  is a
minimum there it must increase and so the kinetic energy must decrease, and so the
particles remain close to the equilibrium position. For this reason 2u is defined as a
stable equilibrium point of the system. If on the other hand the particles of the body were
given small initial velocities from an initial displacement 1u or 3u , the kinetic energy
would increase dramatically; these points are called unstable equilibrium points. Only
the state of stable equilibrium is of interest here and the principle of stationary potential
energy in this case becomes the principle of minimum potential energy.
8.6.2 The Rayleigh-Ritz Method
In applications, the principle of minimum potential energy is used to obtain approximate
solutions to problems which are otherwise difficult or, more usually, impossible to solve
exactly. It forms one basis of the Finite Element Method (FEM), a general technique
for solving systems of equations which arise in complex solid mechanics problems (and
which is discussed in Book III).
Example
Consider a uniaxial bar of length L, young’s modulus E and varying cross-section
)/1(0 LxAA  , fixed at one end and subjected to a force F at the other. The true

1u 2u 3u
Section 8.6
Solid Mechanics Part I Kelly270
solution for displacement to this problem is    LxEAFLu /1ln/ 0  . To see how this
might be approximated using the principle, one writes
Lx
L
uFdx
dx
du
EAVU 






 
2
0
2
1
(8.6.5)
First, substituting in the exact solution leads to
0
2
0
2
00
0
2
2ln
2ln
/1
1
)/1(
2 EA
LF
EA
FL
Fdx
LxEA
F
Lx
EA L







  (8.6.6)
According to the principle, any other displacement solution (which satisfies the
displacement boundary condition 0)0( u ) will lead to a greater potential energy  .
Suppose now that the solution was unknown. In that case an estimate of the solution can
be made in terms of some unknown parameter(s), substituted into Eqn. 8.6.5, and then
minimised to find the parameters. This procedure is known as the Rayleigh Ritz
method. For example, let the guess, or trial function, be the linear function xu   .
The boundary condition leads to 0 . Substituting xu  into Eqn. 8.6.5 leads to
LFLEALFdxLxEA
L
  
2
0
0
2
0
4
3
)/1(
2
1
(8.6.7)
The principle states that   0/   dd , so that
00
0
3
2
3
2
0
2
3
EA
Fx
u
EA
F
FLLEA
d
d




(8.6.8)
The exact and approximate Ritz solution are plotted in Fig. 8.6.3.
Figure 8.6.3: exact and (Ritz) approximate solution for axial problem
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.2 0.4 0.6 0.8 1
x
0EA
FL
Lx /
exact
approximate
Section 8.6
Solid Mechanics Part I Kelly271
The total potential energy due to this approximate solution 03/2 EAFx is, from Eqn.
8.6.5,
0
2
3
1
EA
LF
 (8.6.9)
which is indeed greater than the minimum value Eqn. 8.6.6 ( 0
2
/347.0 EALF ).
■
The accuracy of the solution 8.6.9 can be improved by using as the trial function a
quadratic instead of a linear one, say 2
xxu   . Again the boundary condition
leads to 0 . Then 2
xxu   and there are now two unknowns to determine. Since
 is a function of two variables,
  0, 





 



 (8.6.10)
and the two unknowns can be obtained from the two conditions
0,0 






(8.6.11)
Example
A beam of length L and constant Young’s modulus E and moment of inertia I is supported
at its ends and subjected to a uniform distributed force per length f. Let the beam undergo
deflection )(xv . The potential energy of the applied loads is
dxxfvV
L

0
)( (8.6.12)
and, with Eqn. 8.5.19, the total potential energy is
dxvfdx
dx
vdEI
LL
 






00
2
2
2
2
(8.6.13)
Choose a quadratic trial function 2
xxv   . The boundary conditions lead to
)( Lxxv   . Substituting into 8.6.13 leads to
6/2 32
LfEIL   (8.6.14)
With   0/   dd , one finds that
Section 8.6
Solid Mechanics Part I Kelly272
2
232
2424
)(
24
x
EI
fL
x
EI
fL
xv
EI
fL
 (8.6.15)
which compares with the exact solution
43
3
241224
)( x
EI
f
x
EI
fL
x
EI
fL
xv  (8.6.16)
■
8.6.3 Problems
1. Consider the statically indeterminate uniaxial problem shown below, two bars joined
at Lx  , built in at 0x and Lx 2 , and subjected to a force F at the join. The
cross-sectional area of the bar on the left is 2A and that on the right is A. Use the
principle of minimum potential energy in conjunction with the Rayleigh-Ritz method
with a trial displacement function of the form 2
xxu   to approximate the
exact displacement and in particular the displacement at Lx  .
2. A beam of length L and constant Young’s modulus E and moment of inertia I is
supported at its ends and subjected to a uniform distributed force per length f and a
concentrated force P at its centre. Use the principle of minimum potential energy in
conjunction with the Rayleigh-Ritz method with a trial deflection  Lxv /sin  , to
approximate the exact deflection.
3. Use the principle of minimum potential energy in conjunction with the Rayleigh-Ritz
method with a trial solution xu  to approximately solve the problem of axial
deformation of an elastic rod of varying cross section, built in at one end and loaded
by a uniform distributed force/length f, and a force P at the free end, as shown below.
The cross sectional are is )/2()( 0 LxAxA  and the length of the rod is L.
F
L L
f
P

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08 energy 06_minimum_potential_energy

  • 1. Section 8.6 Solid Mechanics Part I Kelly268 8.6 The Principle of Minimum Potential Energy The principle of minimum potential energy follows directly from the principle of virtual work (for elastic materials). 8.6.1 The Principle of Minimum Potential Energy Consider again the example given in the last section; in particular re-write Eqn. 8.5.15 as 0 22 2 2 22 1 11               BB u L AE L AE Pu (8.6.1) The quantity inside the curly brackets is defined to be the total potential energy of the system,  , and the equation states that the variation of  is zero – that this quantity does not vary when a virtual displacement is imposed: 0 (8.6.2) The total potential energy as a function of displacement u is sketched in Fig. 8.6.1. With reference to the figure, Eqn. 8.6.2 can be interpreted as follows: the total potential energy attains a stationary value (maximum or minimum) at the actual displacement ( 1u ); for example, 0 for an incorrect displacement 2u . Thus the solution for displacement can be obtained by finding a stationary value of the total potential energy. Indeed, it can be seen that the quantity inside the curly brackets in Fig. 8.6.1 attains a minimum for the solution already derived, Eqn. 8.5.17. Figure 8.6.1: the total potential energy of a system To generalise, define the “potential energy” of the applied loads to be extWV   so that VU   (8.6.3) The external loads must be conservative, precluding for example any sliding frictional loading. Taking the total potential energy to be a function of displacement u, one has 0 )(    u du ud  (8.6.4) )(u 1u 1u 2u 2u
  • 2. Section 8.6 Solid Mechanics Part I Kelly269 Thus of all possible displacements u satisfying the loading and boundary conditions, the actual displacement is that which gives rise to a stationary point 0/  dud and the problem reduces to finding a stationary value of the total potential energy VU  . Stability To be precise, Eqn. 8.6.2 only demands that the total potential energy has a stationary point, and in that sense it is called the principle of stationary potential energy. One can have a number of stationary points as sketched in Fig. 8.6.2. The true displacement is one of the stationary values 321 ,, uuu . Figure 8.6.2: the total potential energy of a system Consider the system with displacement 2u . If an external force acts to give the particles of the system some small initial velocity and hence kinetic energy, one has K0 . The particles will now move and so the displacement 2u changes. Since  is a minimum there it must increase and so the kinetic energy must decrease, and so the particles remain close to the equilibrium position. For this reason 2u is defined as a stable equilibrium point of the system. If on the other hand the particles of the body were given small initial velocities from an initial displacement 1u or 3u , the kinetic energy would increase dramatically; these points are called unstable equilibrium points. Only the state of stable equilibrium is of interest here and the principle of stationary potential energy in this case becomes the principle of minimum potential energy. 8.6.2 The Rayleigh-Ritz Method In applications, the principle of minimum potential energy is used to obtain approximate solutions to problems which are otherwise difficult or, more usually, impossible to solve exactly. It forms one basis of the Finite Element Method (FEM), a general technique for solving systems of equations which arise in complex solid mechanics problems (and which is discussed in Book III). Example Consider a uniaxial bar of length L, young’s modulus E and varying cross-section )/1(0 LxAA  , fixed at one end and subjected to a force F at the other. The true  1u 2u 3u
  • 3. Section 8.6 Solid Mechanics Part I Kelly270 solution for displacement to this problem is    LxEAFLu /1ln/ 0  . To see how this might be approximated using the principle, one writes Lx L uFdx dx du EAVU          2 0 2 1 (8.6.5) First, substituting in the exact solution leads to 0 2 0 2 00 0 2 2ln 2ln /1 1 )/1( 2 EA LF EA FL Fdx LxEA F Lx EA L          (8.6.6) According to the principle, any other displacement solution (which satisfies the displacement boundary condition 0)0( u ) will lead to a greater potential energy  . Suppose now that the solution was unknown. In that case an estimate of the solution can be made in terms of some unknown parameter(s), substituted into Eqn. 8.6.5, and then minimised to find the parameters. This procedure is known as the Rayleigh Ritz method. For example, let the guess, or trial function, be the linear function xu   . The boundary condition leads to 0 . Substituting xu  into Eqn. 8.6.5 leads to LFLEALFdxLxEA L    2 0 0 2 0 4 3 )/1( 2 1 (8.6.7) The principle states that   0/   dd , so that 00 0 3 2 3 2 0 2 3 EA Fx u EA F FLLEA d d     (8.6.8) The exact and approximate Ritz solution are plotted in Fig. 8.6.3. Figure 8.6.3: exact and (Ritz) approximate solution for axial problem 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.2 0.4 0.6 0.8 1 x 0EA FL Lx / exact approximate
  • 4. Section 8.6 Solid Mechanics Part I Kelly271 The total potential energy due to this approximate solution 03/2 EAFx is, from Eqn. 8.6.5, 0 2 3 1 EA LF  (8.6.9) which is indeed greater than the minimum value Eqn. 8.6.6 ( 0 2 /347.0 EALF ). ■ The accuracy of the solution 8.6.9 can be improved by using as the trial function a quadratic instead of a linear one, say 2 xxu   . Again the boundary condition leads to 0 . Then 2 xxu   and there are now two unknowns to determine. Since  is a function of two variables,   0,             (8.6.10) and the two unknowns can be obtained from the two conditions 0,0        (8.6.11) Example A beam of length L and constant Young’s modulus E and moment of inertia I is supported at its ends and subjected to a uniform distributed force per length f. Let the beam undergo deflection )(xv . The potential energy of the applied loads is dxxfvV L  0 )( (8.6.12) and, with Eqn. 8.5.19, the total potential energy is dxvfdx dx vdEI LL         00 2 2 2 2 (8.6.13) Choose a quadratic trial function 2 xxv   . The boundary conditions lead to )( Lxxv   . Substituting into 8.6.13 leads to 6/2 32 LfEIL   (8.6.14) With   0/   dd , one finds that
  • 5. Section 8.6 Solid Mechanics Part I Kelly272 2 232 2424 )( 24 x EI fL x EI fL xv EI fL  (8.6.15) which compares with the exact solution 43 3 241224 )( x EI f x EI fL x EI fL xv  (8.6.16) ■ 8.6.3 Problems 1. Consider the statically indeterminate uniaxial problem shown below, two bars joined at Lx  , built in at 0x and Lx 2 , and subjected to a force F at the join. The cross-sectional area of the bar on the left is 2A and that on the right is A. Use the principle of minimum potential energy in conjunction with the Rayleigh-Ritz method with a trial displacement function of the form 2 xxu   to approximate the exact displacement and in particular the displacement at Lx  . 2. A beam of length L and constant Young’s modulus E and moment of inertia I is supported at its ends and subjected to a uniform distributed force per length f and a concentrated force P at its centre. Use the principle of minimum potential energy in conjunction with the Rayleigh-Ritz method with a trial deflection  Lxv /sin  , to approximate the exact deflection. 3. Use the principle of minimum potential energy in conjunction with the Rayleigh-Ritz method with a trial solution xu  to approximately solve the problem of axial deformation of an elastic rod of varying cross section, built in at one end and loaded by a uniform distributed force/length f, and a force P at the free end, as shown below. The cross sectional are is )/2()( 0 LxAxA  and the length of the rod is L. F L L f P