Minimum total potential energy principle

The minimum total potential energy principle is a fundamental concept used in physics, chemistry, biology, 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.

A binding energy is the energy that must be exported from a system for the system to enter a bound state at a negative level of energy. Negative energy is called "potential energy".[1] A bound system has a lower (i.e., more negative) potential energy than the sum of its parts—this is what keeps the system aggregated in accordance with the minimum total potential energy principle. Therefore, a system's binding energy is the system's synergy. This, in its turn, implies that the minimum total potential energy principle is the maximum total synergy principle.

Some examples

Structural Mechanics

The total potential energy,  \boldsymbol{\Pi} , is the sum of the elastic strain energy, U, stored in the deformed body and the potential energy, V, associated to the applied forces:

 \boldsymbol{\Pi} = \mathbf{U} + \mathbf{V} \qquad \mathrm{(1)}

This energy is at a stationary position when an infinitesimal variation from such position involves no change in energy:

 \delta\boldsymbol{\Pi} = \delta(\mathbf{U} + \mathbf{V}) = 0 \qquad \mathrm{(2)}

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:

 \int_{S_t} \delta\ \mathbf{u}^T \mathbf{T} dS + \int_{V} \delta\ \mathbf{u}^T \mathbf{f} dV = \int_{V}\delta\boldsymbol{\epsilon}^T \boldsymbol{\sigma} dV \qquad \mathrm{(3)}

where

 \mathbf{u} = vector of displacements
 \mathbf{T} = vector of distributed forces acting on the part  S_t of the surface
 \mathbf{f} = vector of body forces

In the special case of elastic bodies, the right-hand-side of (3) can be taken to be the change,  \delta \mathbf{U} , 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:

 \mathbf{V} = -\int_{S_t} \mathbf{u}^T \mathbf{T} dS - \int_{V} \mathbf{u}^T \mathbf{f} dV

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:

 -\delta\ \mathbf{V} = \delta\ \mathbf{U}

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.

References