While the Föppl–von Kármán equations are of interest from a purely mathematical point of view, the physical validity of these equations is questionable. Ciarlet states: The two-dimensional von Karman equations for plates, originally proposed by von Karman , play a mythical role in applied mathematics. While they have been abundantly, and satisfactorily, studied from the mathematical standpoint, as regards notably various questions of existence, regularity, and bifurcation, of their solutions, their physical soundness has been often seriously questioned. Reasons include the facts that
the theory depends on an approximate geometry which is not clearly defined
a given variation of stress over a cross-section is assumed arbitrarily
there is a confusion between reference and deformed configurations which makes the theory inapplicable to the large deformations for which it was apparently devised.
Conditions under which these equations are actually applicable and will give reasonable results when solved are discussed in Ciarlet.
The three Föppl–von Kármán equations can be reduced to two by introducing the Airy stress function where Then the above equations become
Pure bending
For the pure bending of thin plates the equation of equilibrium is, where is called flexural or cylindrical rigidity of the plate.
Kinematic assumptions (Kirchhoff hypothesis)
In the derivation of the Föppl–von Kármán equations the main kinematic assumption is that surface normals to the plane of the plate remain perpendicular to the plate after deformation. It is also assumed that the in-plane displacements are small and the change in thickness of the plate is negligible. These assumptions imply that the displacement field in the plate can be expressed as in which is the in-plane displacement. This form of the displacement field implicitly assumes that the amount of rotation of the plate is small.
The components of the three-dimensional Lagrangian Green strain tensor are defined as Substitution of the expressions for the displacement field into the above gives For small strains but moderate rotations, the higher order terms that cannot be neglected are Neglecting all other higher order terms, and enforcing the requirement that the plate does not change its thickness, the strain tensor components reduce to the von Kármán strains The first terms are the usual small-strains, for the mid-surface. The second terms, involving squares of displacement gradients, are non-linear, and need to be considered when the plate bending is fairly large. These first two terms together are called the membrane strains. The last terms, involving second derivatives, are the flexural strains. They involve the curvatures. These zero terms are due to the assumptions of the classical plate theory, which assume elements normal to the mid-plane remain inextensible and line elements perpendicular to the mid-plane remain normal to the mid-plane after deformation.
Stress–strain relations
If we assume that the Cauchy stress tensor components are linearly related to the von Kármán strains by Hooke's law, the plate is isotropic and homogeneous, and that the plate is under a plane stress condition, we have = = = 0 and Expanding the terms, the three non-zero stresses are
Stress resultants
The stress resultants in the plate are defined as Therefore, the elimination of the in-plane displacements leads to and Solutions are easier to find when the governing equations are expressed in terms of stress resultants rather than the in-plane stresses.
Equations of Equilibrium
The weak form of the Kirchhoff plate is here Ω denotes the mid-plane. The weak form leads to The resulting governing equations are
Föppl–von Kármán equations in terms of stress resultants
The Föppl–von Kármán equations are typically derived with an energy approach by considering variations of internal energy and the virtual work done by external forces. The resulting static governing equations are When the deflections are small compared to the overall dimensions of the plate, and the mid-surface strains are neglected, The equations of equilibrium are reduced to