Flexural rigidity

In a beam or rod, flexural rigidity (defined as EI) varies along the length as a function of x shown in the following equation:

${\displaystyle \ EI{dy \over dx}\ =\int _{0}^{x}M(x)dx+C_{1}}$

where ${\displaystyle E}$ is the Young's modulus (in Pa), ${\displaystyle I}$ is the second moment of area (in m⁴), ${\displaystyle y}$ is the transverse displacement of the beam at x, and ${\displaystyle M(x)}$ is the bending moment at x.

Flexural rigidity has SI units of Pa·m⁴ (which also equals N·m²).

In the study of geology, lithospheric flexure affects the thin lithospheric plates covering the surface of the Earth when a load or force is applied to them. On a geological timescale, the lithosphere behaves elastically (in first approach) and can therefore bend under loading by mountain chains, volcanoes and other heavy objects. Isostatic depression caused by the weight of ice sheets during the last glacial period is an example of the effects of such loading.

The flexure of the plate depends on:

1. The plate elastic thickness (usually referred to as effective elastic thickness of the lithosphere).
2. The elastic properties of the plate
3. The applied load or force

As flexural rigidity of the plate is determined by the Young's modulus, Poisson's ratio and cube of the plate's elastic thickness, it is a governing factor in both (1) and (2).

Flexural Rigidity[1] ${\displaystyle D={\dfrac {Eh_{e}^{3}}{12(1-\nu ^{2})}}}$

${\displaystyle E}$ = Young's Modulus

${\displaystyle h_{e}}$ = elastic thickness (~5–100 km)

${\displaystyle \nu }$ = Poisson's Ratio

Flexural rigidity of a plate has units of Pa·m³, i.e. one dimension of length less than the same property for the rod, as it refers to the moment per unit length per unit of curvature, and not the total moment. I is termed as moment of inertia. J is denoted as 2nd moment of inertia/polar moment of inertia.

• Bending stiffness
• Lithospheric flexure