Abstract
An open question in studying normal grain growth concerns the asymptotic state to which microstructures converge. In particular, the distribution of grain topologies is unknown. We introduce a thermodynamic-like theory to explain these distributions in two- and three-dimensional systems. In particular, a bending-like energy is associated to each grain topology , and the probability of observing that particular topology is proportional to , where is the order of an associated symmetry group and is a thermodynamic-like constant. We explain the physical origins of this approach, and provide numerical evidence in support.
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