Pierre-Simon, marquis de Laplace
20 (1749–1827) was a French scientist and politician (
Fig. 2). He made significant contributions in mechanics, calculus, and theory of probability. In Treaty of Celestial Mechanics (Original title in French:
Traité de Mécanique Céleste),
21 Laplace described a mathematical relationship, Laplace's Law, originally intended to quantify the liquid surface tension in a capillary.
To predict wall stress (
σ), Laplace's Law can be applied to a uniform isotropic hollow sphere with thickness
t and radius
r, under internal pressure
p (
Fig. 3).
22 It is important to note that the thin shell assumption is applied in Laplace's Law, which postulates that there is no circumferential stress (stress tangential to the surface of corneoscleral shell) variation through the wall thickness. A common way to derive such a formula is to perform a balance of forces between the internal pressure (
p) and the resulting wall stress. By examining the cross-section of the sphere, the total force due to the internal pressure is the product of
p and the cross-sectional area (
πr2) while the aggregate circumferential tension is the product of
σ,
t and the cross-sectional circumference (2
πr). Equating the two quantities and rearranging them leads to
When applied to the corneoscleral shell, Laplace's law is intuitive in many ways: Bigger eyes (larger
r) and/or thinner corneoscleral tissue layers (smaller
t) will exhibit larger wall stress. In addition, stress increases proportionally to IOP (larger
p). Laplace's Law can be derived in other ways, and presented in various formulations such as using the radius of curvature instead of the spherical radius.
22 In this work we will discuss Equation 1, as it is the most commonly used formulation in ophthalmology.