The experimental protocol for inflation testing the posterior scleral shell has been fully described in our previous reports.
14,16,19,33 Briefly, the posterior scleral shells were cleaned of intra- and extraorbital tissues immediately post mortem, and individually mounted on a custom-built pressurization apparatus (
Fig. 1, left). Each eye was blotted dry, covered with a white contrast medium (ProCAD Contrast Medium; Ivoclar, Schaan, Lichtenstein), and then immediately immersed in PBS at room temperature (
Fig. 1, left). Preconditioning loads were applied in the form of 20 pressurization cycles from 5 to 30 mm Hg at a rate of 5 mm Hg per second, and then the scleral shell was allowed to recover for 15 minutes. A starting pressure of zero could not be used because the posterior scleral shell of NHPs does not maintain its shape unless pressurized to at least 2 mm Hg and exhibits geometric nonlinearities up to 4 mm Hg, so a starting pressure of 5 mm Hg was used. The scleral shells were inflated from 5 to 45 mm Hg in small steps of 0.01 to 0.2 mm Hg using an automated system with computer feedback control. Scleral surface displacements were recorded after the sclera had reached equilibrium at each pressure step (∼30 seconds) using a commercial electronic laser speckle interferometer (ESPI; Q-100, Dantec Dynamics A/S, Skovlunde, Denmark) (
Fig. 1; right, top). In a recent study, we assessed the displacement measurement uncertainty of this ESPI system in inflation testing conditions similar to those used herein, and the average measurement uncertainty was ±16 nm at the 95% confidence level.
32 As in previous studies (Fazio MA, et al.
IOVS 2014;55:ARVO E-Abstract 4552),
14,16,19,33 all inflation testing was performed at room temperature to avoid artifacts from convection currents in the saline bath that interfere with the laser displacement measurements.
A customized B-spline fitting system
37 was used to obtain continuous and differentiable analytical functions that define the 3D displacement field over the entire posterior third of the scleral surface as described previously.
33 The 3D deformation of the infinitesimally thin outer layer of the sclera was obtained by analytical differentiation of the fitting system functions, which allows direct calculation of the mechanical strain without any intermediate finite element or analytical modeling. The strain formulation is reported in
Equations 1 and
2, as described in our previous studies,
16,18,33 and the 3D strain tensor was computed using an approximated formulation as follows:
ESPI displacements in Cartesian space were fit to continuous, differentiable, analytical functions
∪Display Formula\(\def\upalpha{\unicode[Times]{x3B1}}\)\(\def\upbeta{\unicode[Times]{x3B2}}\)\(\def\upgamma{\unicode[Times]{x3B3}}\)\(\def\updelta{\unicode[Times]{x3B4}}\)\(\def\upvarepsilon{\unicode[Times]{x3B5}}\)\(\def\upzeta{\unicode[Times]{x3B6}}\)\(\def\upeta{\unicode[Times]{x3B7}}\)\(\def\uptheta{\unicode[Times]{x3B8}}\)\(\def\upiota{\unicode[Times]{x3B9}}\)\(\def\upkappa{\unicode[Times]{x3BA}}\)\(\def\uplambda{\unicode[Times]{x3BB}}\)\(\def\upmu{\unicode[Times]{x3BC}}\)\(\def\upnu{\unicode[Times]{x3BD}}\)\(\def\upxi{\unicode[Times]{x3BE}}\)\(\def\upomicron{\unicode[Times]{x3BF}}\)\(\def\uppi{\unicode[Times]{x3C0}}\)\(\def\uprho{\unicode[Times]{x3C1}}\)\(\def\upsigma{\unicode[Times]{x3C3}}\)\(\def\uptau{\unicode[Times]{x3C4}}\)\(\def\upupsilon{\unicode[Times]{x3C5}}\)\(\def\upphi{\unicode[Times]{x3C6}}\)\(\def\upchi{\unicode[Times]{x3C7}}\)\(\def\uppsy{\unicode[Times]{x3C8}}\)\(\def\upomega{\unicode[Times]{x3C9}}\)\(\def\bialpha{\boldsymbol{\alpha}}\)\(\def\bibeta{\boldsymbol{\beta}}\)\(\def\bigamma{\boldsymbol{\gamma}}\)\(\def\bidelta{\boldsymbol{\delta}}\)\(\def\bivarepsilon{\boldsymbol{\varepsilon}}\)\(\def\bizeta{\boldsymbol{\zeta}}\)\(\def\bieta{\boldsymbol{\eta}}\)\(\def\bitheta{\boldsymbol{\theta}}\)\(\def\biiota{\boldsymbol{\iota}}\)\(\def\bikappa{\boldsymbol{\kappa}}\)\(\def\bilambda{\boldsymbol{\lambda}}\)\(\def\bimu{\boldsymbol{\mu}}\)\(\def\binu{\boldsymbol{\nu}}\)\(\def\bixi{\boldsymbol{\xi}}\)\(\def\biomicron{\boldsymbol{\micron}}\)\(\def\bipi{\boldsymbol{\pi}}\)\(\def\birho{\boldsymbol{\rho}}\)\(\def\bisigma{\boldsymbol{\sigma}}\)\(\def\bitau{\boldsymbol{\tau}}\)\(\def\biupsilon{\boldsymbol{\upsilon}}\)\(\def\biphi{\boldsymbol{\phi}}\)\(\def\bichi{\boldsymbol{\chi}}\)\(\def\bipsy{\boldsymbol{\psy}}\)\(\def\biomega{\boldsymbol{\omega}}\)\(\def\bupalpha{\unicode[Times]{x1D6C2}}\)\(\def\bupbeta{\unicode[Times]{x1D6C3}}\)\(\def\bupgamma{\unicode[Times]{x1D6C4}}\)\(\def\bupdelta{\unicode[Times]{x1D6C5}}\)\(\def\bupepsilon{\unicode[Times]{x1D6C6}}\)\(\def\bupvarepsilon{\unicode[Times]{x1D6DC}}\)\(\def\bupzeta{\unicode[Times]{x1D6C7}}\)\(\def\bupeta{\unicode[Times]{x1D6C8}}\)\(\def\buptheta{\unicode[Times]{x1D6C9}}\)\(\def\bupiota{\unicode[Times]{x1D6CA}}\)\(\def\bupkappa{\unicode[Times]{x1D6CB}}\)\(\def\buplambda{\unicode[Times]{x1D6CC}}\)\(\def\bupmu{\unicode[Times]{x1D6CD}}\)\(\def\bupnu{\unicode[Times]{x1D6CE}}\)\(\def\bupxi{\unicode[Times]{x1D6CF}}\)\(\def\bupomicron{\unicode[Times]{x1D6D0}}\)\(\def\buppi{\unicode[Times]{x1D6D1}}\)\(\def\buprho{\unicode[Times]{x1D6D2}}\)\(\def\bupsigma{\unicode[Times]{x1D6D4}}\)\(\def\buptau{\unicode[Times]{x1D6D5}}\)\(\def\bupupsilon{\unicode[Times]{x1D6D6}}\)\(\def\bupphi{\unicode[Times]{x1D6D7}}\)\(\def\bupchi{\unicode[Times]{x1D6D8}}\)\(\def\buppsy{\unicode[Times]{x1D6D9}}\)\(\def\bupomega{\unicode[Times]{x1D6DA}}\)\(\def\bupvartheta{\unicode[Times]{x1D6DD}}\)\(\def\bGamma{\bf{\Gamma}}\)\(\def\bDelta{\bf{\Delta}}\)\(\def\bTheta{\bf{\Theta}}\)\(\def\bLambda{\bf{\Lambda}}\)\(\def\bXi{\bf{\Xi}}\)\(\def\bPi{\bf{\Pi}}\)\(\def\bSigma{\bf{\Sigma}}\)\(\def\bUpsilon{\bf{\Upsilon}}\)\(\def\bPhi{\bf{\Phi}}\)\(\def\bPsi{\bf{\Psi}}\)\(\def\bOmega{\bf{\Omega}}\)\(\def\iGamma{\unicode[Times]{x1D6E4}}\)\(\def\iDelta{\unicode[Times]{x1D6E5}}\)\(\def\iTheta{\unicode[Times]{x1D6E9}}\)\(\def\iLambda{\unicode[Times]{x1D6EC}}\)\(\def\iXi{\unicode[Times]{x1D6EF}}\)\(\def\iPi{\unicode[Times]{x1D6F1}}\)\(\def\iSigma{\unicode[Times]{x1D6F4}}\)\(\def\iUpsilon{\unicode[Times]{x1D6F6}}\)\(\def\iPhi{\unicode[Times]{x1D6F7}}\)\(\def\iPsi{\unicode[Times]{x1D6F9}}\)\(\def\iOmega{\unicode[Times]{x1D6FA}}\)\(\def\biGamma{\unicode[Times]{x1D71E}}\)\(\def\biDelta{\unicode[Times]{x1D71F}}\)\(\def\biTheta{\unicode[Times]{x1D723}}\)\(\def\biLambda{\unicode[Times]{x1D726}}\)\(\def\biXi{\unicode[Times]{x1D729}}\)\(\def\biPi{\unicode[Times]{x1D72B}}\)\(\def\biSigma{\unicode[Times]{x1D72E}}\)\(\def\biUpsilon{\unicode[Times]{x1D730}}\)\(\def\biPhi{\unicode[Times]{x1D731}}\)\(\def\biPsi{\unicode[Times]{x1D733}}\)\(\def\biOmega{\unicode[Times]{x1D734}}\)\({(\theta ,\varphi )}\) =
Display Formula\(\left\{ {{{u}_{\theta }}{(\theta ,\varphi ),\ }{{u}_{\varphi }}{(\theta ,\varphi ),\ }{{u}_{r}}{(\theta ,\varphi )}} \right\}\) for the meridional
Display Formula\(\theta \in \left[ {0,{\pi \over 2}} \right]\), circumferential
Display Formula\(\varphi \in \left[ {0,2\pi } \right]\), and radial directions, respectively. The analytical function defines the displacement field over the two-thirds of the outer surface of the posterior pole of each eye. Five (
Display Formula\({{\varepsilon }_{{\theta \theta }}}\),
Display Formula\({{\varepsilon }_{{\theta \varphi }}}\),
Display Formula\({{\varepsilon }_{{\varphi \varphi }}}\),
Display Formula\({{\varepsilon }_{{r\varphi }}}\),
Display Formula\({{\varepsilon }_{{r\theta }}}\)) out of nine components of the full strain tensor (
Equation 1) were computed by direct mathematical differentiation of the analytical displacement functions, and by assuming that the displacement components tangent to the scleral surface do not vary in the radial direction. A recent study by Tang and Liu
38 showed that variation of the meridional and circumferential components of displacement in the radial direction is minimal in the infinitesimally thin outer layer of the sclera where strain was calculated in this study. So, meridional and circumferential displacement variation in the radial direction,
Display Formula\({{\partial {{u}_{\theta }}} \over {\partial r}}({\theta },{\varphi })\) and
Display Formula\({{\partial {{u}_{\varphi }}} \over {\partial r}}({\theta },{\varphi })\) in
Equation 2, respectively, was assumed to be zero, and the sensitivity of the reported outcomes to this assumption was quantified and reported to be very low in our previous study.
16
Three components of the strain tensor
Display Formula\({{\varepsilon }_{{\varphi \theta }}}\),
Display Formula\({{\varepsilon }_{{\theta r}}}\), and
Display Formula\({{\varepsilon }_{{\varphi r}}}\) were computed by strain compatibility equations, and the final component,
Display Formula\({{\rm{\varepsilon }}_{{\rm{rr}}}}\), was numerically computed by assuming tissue incompressibility, thereby imposing
Display Formula\(det{[}{\bf{\varepsilon }} + {\mathop{\rm I}\nolimits} {]} = 1\) (where
Display Formula\({\mathop{\rm I}\nolimits} \) is the Identity Matrix).
\begin{equation}\tag{1}{\rm{Strain\ Tensor}} = \varepsilon {\rm{(\theta ,\varphi )}} = \left\{ {\matrix{ {{{\rm{\varepsilon }}_{{\rm{\theta \theta }}}}}&{{{\rm{\varepsilon }}_{{\rm{\theta \varphi }}}}}&{{{\rm{\varepsilon }}_{{\rm{\theta r}}}}} \cr {{{\rm{\varepsilon }}_{{\rm{\varphi \theta }}}}}&{{{\rm{\varepsilon }}_{{\rm{\varphi \varphi }}}}}&{{{\rm{\varepsilon }}_{{\rm{\varphi r}}}}} \cr {{{\rm{\varepsilon }}_{{\rm{r\theta }}}}}&{{{\rm{\varepsilon }}_{{\rm{r\varphi }}}}}&{{{\rm{\varepsilon }}_{{\rm{rr}}}}} \cr } } \right\}{\rm ,}\end{equation}
where
\begin{equation}\tag{2}\left\{ \matrix{ {{\varepsilon }_{{\theta \theta }}}{ = }{{1} \over {r}}{(}{{\partial {{u}_{\theta }}} \over {\partial {\theta }}}{ + }{{u}_{r}}{)} \hfill \cr {{\varepsilon }_{{\varphi \varphi }}}{ = }{{1} \over {{rsin\theta }}}{(}{{\partial {u\varphi }} \over {\partial {\varphi }}}{ + }{{u}_{r}}{sin\theta + }{{u}_{\theta }}{cos\theta )} \hfill \cr {{\varepsilon }_{{\theta \varphi }}}{ = }{{1} \over {{2r}}}{(}{{1} \over {{sin\theta }}}{{\partial {{u}_{\theta }}} \over {\partial {\varphi }}}{ + }{{\partial {{u}_{\varphi }}} \over {\partial {\theta }}}{ - }{{u}_{\varphi }}{cot\theta )} \hfill \cr {{\varepsilon }_{{r\theta }}}{ = }{{1} \over {2}}{(}{{1} \over {r}}{{\partial {{u}_{r}}} \over {\partial {\theta }}}{ + }{{\partial {u\theta }} \over {\partial {r}}}{ - }{{{u\theta }} \over {r}}{)} \hfill \cr {{\varepsilon }_{{r\varphi }}}{ = }{{1} \over {2}}{(}{{1} \over {{rsin\theta }}}{{\partial {{u}_{r}}} \over {\partial {\varphi }}}{ + }{{\partial {{u}_{\theta }}} \over {\partial {r}}}{ - }{{{{u}_{\varphi }}} \over {r}}{)} \hfill \cr} \right.\end{equation}
The maximum principal tensile strain (
Display Formula\({\varepsilon _I}\),
Equation 3) was computed over the entire scleral surface from the spectral decomposition of the full strain tensor:
\begin{equation}\tag{3}{{\bf{\varepsilon }}^{{Eig}}}{ = }\left\{ {\matrix{ {{{\varepsilon }_{I}}}&{0}&{0} \cr {0}&{{{\varepsilon }_{{II}}}}&{0} \cr {0}&{0}&{{{\varepsilon }_{{III}}}} \cr } } \right\}\end{equation}
The radius of the spherical coordinate system was computed by best-fitting 3D coordinates of ∼2500 points on the outer surface of the posterior sclera. These points were acquired using a 3D digitizer with a nominal resolution of ∼200 μm (MicroScribe G2X, Immersion; San Jose, CA, USA), while the sclera was pressurized to 10 mm Hg with PBS. A pressure of 10 mm Hg was chosen to reduce the potential for deformation of the sclera with the digitizer tip so as to get the best possible scleral surface geometries. The difference in shape of the sclera when pressurized at 10 mm Hg compared to 5 mm Hg is negligible as compared to the intrinsic 200-μm resolution of the digitizer. Also, while the strain is a function of the radius of the sphere defining the coordinate system, the sensitivity of the strain to an error in the sphere radius is negligible.
16