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 Ei is associated to each grain topology ti, and the probability of observing that particular topology is proportional to [1/s(ti)]e-βEi, where s(ti) is the order of an associated symmetry group and β is a thermodynamiclike constant. We explain the physical origins of this approach and provide numerical evidence in support.
Original language | English |
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Article number | 015501 |
Journal | Physical Review Letters |
Volume | 125 |
Issue number | 1 |
DOIs | |
State | Published - 3 Jul 2020 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy