A spherical radial deformation is , with and . Differentiation gives the displayed symmetric gradient. Its radial eigenvalue is and its two tangential eigenvalues are ; when these are positive, they are the principal stretches. The determinant is . Positivity distinguishes an orientation-preserving radial elastic deformation from a map that collapses an interior sphere.
For a radial deformation with positive radial derivative, put and . The principal nominal stresses are and . Radial equilibrium reads . Since , substitution cancels the terms proportional to , leaving . Strict convexity of and positivity of force a constant positive determinant .
Integration of gives . Two spherical boundary radii fix uniquely. A positive increasing cube-radius interpolation verifies positivity of and , so the algebraic solution is an admissible smooth radial equilibrium. The result is restricted to this energy family and radial class; strict convexity of its determinant term alone does not imply uniqueness among arbitrary three-dimensional deformations.
Consider an orientation-preserving classical radial deformation of an elastic solid on a connected spherical annulus. If its nonnegative energy is zero everywhere and the material is isotropic with strict Baker-Ericksen inequalities, every gradient is a natural state, so . Thus and .
A separate rigidity argument applies when the zero wells are , with finitely many positive definite symmetric . The radial gradient is positive symmetric; if , then , so uniqueness of the positive square root gives . The rotation well similarly gives . Hence the continuous ratio takes values in a finite set of eigenvalues and must be constant on the connected radial interval. Differentiating finishes the proof. This version needs neither material isotropy nor Baker-Ericksen inequalities and does not require an assumed continuity of beyond the radial-map regularity used for the ratio.
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