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In Section 4, we discuss our results and implications for the evolution of grain size distribution.
Annealing twin boundaries are important in the evolution of grain boundary engineered materials.
Liffman and Clayton (1989) calculate the evolution of grain size distributions by taking into account grain growth and shock destruction.
There is a qualitative difference in the evolution of grain size distribution between αf = 2.3 and 4.3.
Starting with the size distribution of SNe II dust grains in N07, H10 solve the shattering equation to calculate the evolution of grain size distribution.
An example application of the model simulating the evolution of grain boundary porosity in nuclear fuel is shown on a representative tetrakaidecahedron-shaped fuel grain.
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The outlet pictures show the evolution of grains along the central plane of the 3D simulation.
The governing mechanism in the evolution of grains is an interplay of surface energy anisotropy and growth kinetics.
In order to gain insights into the microstructural processes, we visualize the evolution of grains along the central plane for the three grain sizes.
We simulate the evolution of grains in two geometries that are similar to experimental systems that have been studied.
We compare the evolution of grains along the central plane of the 3D setup (3D-CP) with the 2D simulation (in which the initial grain distribution is identical to that of 3D-CP).
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