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 thermodynamiclike theory to explain these distributions in two- and three-dimensional systems. In particular, a bendinglike 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 thermodynamiclike constant. We explain the physical origins of this approach and provide numerical evidence in support.
- Received 28 May 2019
- Revised 17 May 2020
- Accepted 9 June 2020
DOI:https://doi.org/10.1103/PhysRevLett.125.015501
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