Shallow shell theory of the buckling energy barrier: from the Pogorelov state to softening and imperfection sensitivity close to the buckling pressure

Abstract

We study the axisymmetric response of a complete spherical shell under homogeneous compressive pressure $p$ to an additional point force. For a pressure $p$ below the classical critical buckling pressure $p_c$, indentation by a point force does not lead to spontaneous buckling but an energy barrier has to be overcome. The states at the maximum of the energy barrier represent a subcritical branch of unstable stationary points, which are the transition states to a snap-through buckled state. Starting from nonlinear shallow shell theory we obtain a closed analytical expression for the energy barrier height, which facilitates its effective numerical evaluation as a function of pressure by continuation techniques. We find a clear crossover between two regimes: For $p/p_c\ll 1$ the post-buckling barrier state is a mirror-inverted Pogorelov dimple, and for $(1-p/p_c)\ll 1$ the barrier state is a shallow dimple with indentations smaller than shell thickness and exhibits extended oscillations, which are well described by linear response. We find systematic expansions of the nonlinear shallow shell equations about the Pogorelov mirror-inverted dimple for $p/p_c\ll 1$ and the linear response state for $(1-p/p_c)\ll 1$, which enable us to derive asymptotic analytical results for the energy barrier landscape in both regimes. Upon approaching the buckling bifurcation at $p_c$ from below, we find a softening of an ideal spherical shell. The stiffness for the linear response to point forces vanishes $\propto (1-p/p_c)^{1/2}$; the buckling energy barrier vanishes $\propto (1-p/p_c)^{3/2}$. In the Pogorelov limit, the energy barrier maximum diverges $\propto (p/p_c)^{-3}$ and the corresponding indentation diverges $\propto (p/p_c)^{-2}$. Numerical prefactors for proportionalities both in the softening and the Pogorelov regime are calculated analytically.