Kirchhoff plate theory is the straightforward generalization of Euler-Bernoulli beam theory to plates. We abandon the plane situation in which all derivatives in \(y\)-direction vanish. The weak boundary conditions then become
\begin{align} \label {eq:beamweakforcex} Q_x(x,y) &= \int _h \dif z\, \tau _{xz}(x, y, z) \\ \label {eq:beamweakforcey} Q_y(x,y) &= \int _h \dif z\, \tau _{yz}(x, y, z) \\ \label {eq:beamweakmomentxx} M_{xx}(x, y) &= \int _h \dif z\, z \sigma _{xx}(x, y, z) \\ \label {eq:beamweakmomentyy} M_{yy}(x, y) &= \int _h \dif z\, z \sigma _{yy}(x, y, z) \\ \label {eq:beamweakmomentxy} M_{xy}(x, y) &= \int _h \dif z\, z \tau _{xy}(x, y, z), \end{align}
where the integral is over the height \(h\) of the plate. \(Q_x\) and \(Q_y\) are called shear forces, \(M_{xx}\) and \(M_{yy}\) are bending moments and \(M_{xy}\) is the torsional moment.
Note that employing static equilibrium \(\sigma _{ij,j}=0\) we obtain
where the last equality holds because \(\tau _{xz}(x,y,h/2)=-\tau _{xz}(x,y,-h/2)\). The condition for static equilibrium \(\sigma _{ij,j}=0\) therefore becomes
in the weak form. Note that this can be written in the compact form \(Q_{i,i}=-p\) and \(M_{ij,j}=Q_i\).
As in the Euler-Bernoulli case, we assume that the components \(\sigma _{xx}\), \(\sigma _{yy}\) and \(\tau _{xy}\) vary linearly with \(z\). We can write
\begin{align} \sigma _{xx}(x, y, z) &= \frac {M_{xx}(x, y)}{I} z \\ \sigma _{yy}(x, y, z) &= \frac {M_{yy}(x, y)}{I} z \\ \tau _{xy}(x, y, z) &= \frac {M_{xy}(x, y)}{I} z \end{align}
with \(I=\int dz\, z^2=h^3/12\). The remaining components of the stress tensor are obtained from static equilibrium. Static equilibrium yields
Integration under the condition that the loads on top and bottom surface of the plate balance, \(\sigma _{zz}(x,h/2)=-\sigma _{zz}(x,-h/2)\), gives
\begin{equation} \label {eq:platestresszz} \sigma _{zz}(x, y, z) = \frac {p(x, y)}{2I} \left (\frac {h^2}{4} - \frac {z^2}{3}\right ) z. \end{equation}
At the top and bottom of the plate we find \(\sigma _{zz}(x,h/2)=-\sigma _{zz}(x,-h/2)=p(x,y)/2\).
10.2 Displacements
Now that we know the stress inside the plate, we can again compute the displacements from Hooke’s law. In the full three-dimensional case, Hooke’s law,
We now only consider the displacement at the surface, \(w(x,y)\equiv u_z(x,y,h/2)\). Since the surfaces are traction free, all terms involving \(\tau _{xz}\) and \(\tau _{yz}\) vanish. Hence
We now plug Eqs. \eqref{eq:plateMxx}, \eqref{eq:plateMyy} and \eqref{eq:plateMxy} into the equilibrium conditions Eqs. \eqref{eq:plateeq2} and \eqref{eq:plateeq3}. This yields