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6 Perspectives

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Development of both faster computing processors and efficient simulation algorithms have expanded the range of atomistic simulations and narrowed down their discrepancies with experiments. Simulations would nonetheless benefit from improved accuracy. As becoming more common, the best way to achieve this goal is to perform first‐principles MD calculation from beginning to end. Although such calculations made with standard quantum mechanical codes remain difficult when dealing with a large number of atoms, progress should result from the use of the so‐called order‐N and linear scaling methods, which have developed vigorously during the past decade. For oxide glasses, recent codes such as SIESTA or CONQUEST now have the potential ability to handle systems of around one thousand atoms with a supercomputer whereas calculations for systems ten times bigger should become feasible in the next decade. Alternatively, better classical potentials can be derived from the energy data yielded by ab‐initio methods as well illustrated by the Tuneyuki and BKS potentials used for silica glass that were based on the simple Buckingham function [4]. Whereas parameter fitting of these potential models was handmade, automatic fitting by machine learning methods is becoming popular since a huge number of data can be sampled on potential energy surfaces yielded by first‐principles calculations to derive better interatomic potentials. And even if the simulation remains based on classical mechanics, the shell, polarizable, charge‐equilibrium, and other models will be more widely used to reproduce better structures and properties [4].

The two other main limitations of numerical simulations currently concern the space‐ and timescales considered. To cope with them, combinations of two different techniques may be used as already described in Section 3 for RMC methods. Besides, MC algorithms can be integrated into MD calculations to speed up simulation of too slow structural relaxation as is the case for the formation of boroxol rings in B2O3 [11]. Of more general use, however, is a combination of classical and first‐principles MD simulations [20] whereby the former yield a preliminary structure that is subsequently optimized in the latter before spectroscopic or other properties are finally derived from the first‐principles simulations.

The “coarse‐graining” methods are also promising as multi‐scale simulation procedures. By lumping groups of atoms into larger entities referred to as particles, which interact according to newly parametrized effective interaction potentials, they have been successfully used for polymers to describe slow dynamic modes and to investigate the cooperative motions and fluctuations observed in the intermediate‐ and long‐range regions. For oxide glasses, however, their application is hampered by the difficulty of assigning appropriate structural fragments to coarse‐grained units.

Finally, it is important for glass scientists to share their know‐how on simulation techniques and interatomic potentials. One of such activities takes place in the TC‐3 Technical committee of the International Commission on Glass (ICG) where round‐robin tests are made to compare experimental data and calculated results on standard glass samples. Such an activity will provide useful information to other glass scientists on agreement and discrepancy between experiments and atomic simulations. Another activity is conducted in TC‐27 whose members discuss future directions of atomistic simulations, promote standardization of atomistic techniques, and provide information on these techniques to the glass community (e.g. [21]). In addition, ICG has published an educational textbook, which includes one chapter on atomistic simulations [22].

In a near future, we strongly expect that any macroscopic property will be explained in terms of microscopic structure by atomistic and first‐principles simulations. In addition, computational design of glass materials will advance rapidly in good harmony with experimental studies.

Encyclopedia of Glass Science, Technology, History, and Culture

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