The principle of minimum total potential energy
is a fundamental concept used in physics
, and engineering
. It asserts that a structure or body shall deform or displace to a position that minimizes the total potential energy, with the lost potential energy being dissipated as heat. For example, a marble placed in a bowl will move to the bottom and rest there, and similarly, a tree branch laden with snow will bend to a lower position. The lower position is the position for minimum potential energy: it is the stable configuration for equilibrium. The principle has many applications in structural analysis
and solid mechanics
The tendency to minimum total potential energy is due to the second law of thermodynamics, which states that the entropy of a system will maximize at equilibrium. Given two possibilities - a low heat content and a high potential energy, or a high heat content and low potential energy, the latter will be the state with the highest entropy, and will therefore be the state towards which the system moves.
The principle of minimum total potential energy should not be confused with the related principle of minimum energy which states that for a system that changes
without heat transfer, the total energy will be minimized.
Note that in most complex systems there is one global minimum and many local minima (smaller dips) in the potential energy. These are called metastable states. A system may reside in a local minimum for a long time — even an effectively infinite period of time.
The total potential energy, , is the sum of the elastic strain energy, U, stored in the deformed body and the potential energy, V, of the applied forces:
This energy is at a stationary position
when an infinitesimal
variation from such position involves no change in energy:
The principle of minimum total potential energy may be derived as a special case of the virtual work principle for elastic systems subject to conservative forces.
The equality between external and internal virtual work (due to virtual displacements) is:
- = vector of displacements
- = vector of distributed forces acting on the part of the surface
- = vector of body forces
In the special case of elastic bodies, the right-hand-side of (3) can be taken to be the change, , of elastic strain energy U due to infinitesimal variations of real displacements.
In addition, when the external forces are conservative forces, the left-hand-side of (3) can be seen as the change in the potential energy function V of the forces. The function V is defined as:
where the minus sign implies a loss of potential energy as the force is displaced in its direction. With these two subsidiary conditions, (3) becomes:
This leads to (2) as desired. The variational form of (2) is often used as the basis for developing the finite element method in structural mechanics