To analyze laser power loss at the interface between two different refractive index materials, we used the Fresnel equation at the normal incident, given by the following formula
14:
\begin{equation}R = {\left| {\frac{{{n_t} - {n_i}}}{{{n_t} + {n_i}}}} \right|^2}\end{equation}
where
R is the reflectance, and
ni and
nt are the refractive indices of the first and second material, respectively, when the laser travels. In the simulation, three boundaries for reflection (air/anterior cornea, posterior cornea/OVDs, and OVDs/lens) should be considered; however, we did not include the reflection at air/anterior cornea because we filled OVDs in the anterior chamber without affecting the air/anterior cornea boundary. If the reflectance at the first boundary (between posterior cornea and OVD) is
R1 and the remaining 1 −
R1 travels to the second boundary (between the OVD and the lens), the total reflectance at the two boundaries,
RT, is a simple sum of two reflections, as follows:
\begin{equation}{R_T} = {R_1} + \left( {1 - {R_1}} \right){R_2} = {R_1} + {R_2} - {R_1}{R_2}\end{equation}
where
R2 is the reflectance at the second boundary.
As the reflectance of light depends on the incident angle as well, the spherical shape of the cornea changes the reflectance depending on the radial distance from the spherical center of the cornea. When
R = 6.8
mm, the radius of curvature of the cornea,
13 and
D = 6
mm, which is a diameter cut by cataract surgery, we get the maximum 26° incident angle variation by a simple geometric formula,
\({\theta _i} = {\sin ^{ - 1}}\frac{D}{{2{\rm{R}}}}\). The reflectance with the incident angle can be simulated from the following angle-dependent Fresnel equations
14:
\begin{equation}{R_ \bot } = {\left| {\frac{{\sin \left( {{\theta _i} - {\theta _t}} \right)}}{{\sin \left( {{\theta _i} + {\theta _t}} \right)}}} \right|^2}{\rm{\ }}\end{equation}
\begin{equation}{R_\parallel } = {\left| {\frac{{\tan \left( {{\theta _i} - {\theta _t}} \right)}}{{\tan \left( {{\theta _i} + {\theta _t}} \right)}}} \right|^2}\end{equation}
where
R⊥,
R∥ are the reflectances perpendicular and parallel to the incident plane, and θ
i and θ
t are the angles of incidence and refraction, respectively. With a given incident angle (θ
i), the refractive angle (θ
t) can be calculated from Snell's law (
nisin θ
i =
ntsin θ
t, where
ni and
nt are the refractive indices of the incident and refractive domains, respectively). Consequently,
Equations 3 and
4 are the functions of one variable, θ
i.