Encyclopedia of Glass Science, Technology, History, and Culture. Группа авторов

Encyclopedia of Glass Science, Technology, History, and Culture - Группа авторов


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results for systems ten times bigger. The second method, which will now be described in some detail, is the density functional theory (DFT).

      2.2 Density Functional Theory

      The DFT formalism exploits certain ground‐state properties of many‐electron systems in an external field, thus in our case the Coulomb field of the nuclei. Following up ideas proposed by Thomas and Fermi in the 1930s, it has been rigorously established by Hohenberg, Kohn, and Sham in the early 1960s [2], who showed that the total energy of the system is a functional of the electronic density. DFT gets rid of the many‐body wavefunction, which depends on 3n electronic spatial coordinates, and replaces it by the simpler electronic density ρ(r) that only depends on three spatial coordinates:

      (3)equation

      Kohn and Sham [3] showed that this density can be written as a sum of the density of noninteracting particles, images, where ϕi are the fictitious one‐particle Kohn–Sham (KS) orbitals, and thus the ground‐state density ρ0(r) is given by the sum of the ground states of these particles. Hence, the total energy of the system can be expressed as

      (4)equation

      (5)equation

      Even for such a simple model system, the expression of the correlation energy has to be calculated numerically with Monte‐Carlo methods. A more advanced approximation, the so‐called “generalized gradient approximation” or GGA, is based on a more complex operator making use of the density gradient of mth order:

      (6)equation

      However, this higher approximation does not necessarily give more reliable results so that it is a priori not clear which exchange‐correlation functional should be used [2]. Despite this problem one can say that the KS approach and reasonable (simple) approximations for the exchange‐correlation term have opened the door to the calculations of the electronic structure for many‐atom systems relevant to the study of real materials.

      Although expressing the full quantum mechanical problem in the language of DFT leads to a significant reduction of the computational effort for calculating the forces on the nuclei, in practice this task is still extremely demanding when dealing with more than a few tens of atoms. Therefore, one usually makes the further approximation that all the core electrons of an atom are lumped together so that their effect is replaced by an effective potential, the so‐called “pseudo‐potential,” for the remaining valence electrons which are described by a pseudo‐wavefunction [2]. The physical motivation for this approximation is that the chemical bonds between two atoms are usually related to the outer valence electrons and thus depend only weakly on the inner core electrons.

      2.3 Computational Limitations

      So far, we have discussed how DFT allows one to obtain the forces between the nuclei due to their surrounding electrons. These forces can now be used to solve the equations of motion for the nuclei:

      Although the CPMD approach allows to obtain the correct equilibrium properties of a system, the introduction of the fictive dynamics for the electronic degrees of freedom makes that the motion of the system in configuration space is not completely realistic [2]. Despite this shortcoming, CPMD simulations are still widely used to study complex systems by means of computer simulations (cf. software available at http://www.psi‐k.org/codes.shtml). This problem can, however, be avoided with the so‐called Born–Oppenheimer molecular dynamics (BOMD) in which one solves at each time step the electronic problem. This approach thus allows to give a correct dynamics but at the cost of an increased computational load. Only in the last few years the numerical algorithms have been improved to such an extent that today it is possible to simulate within BOMD several hundreds of particles [5, 6].

      This brief description of the ab initio simulations should make it clear that in practice the codes for such simulations must be extremely optimized in order to keep the necessary computer time within a reasonable limit. This is why, in contrast to simulations performed with effective potentials, first‐principles calculations are not made with “homemade” codes but with one of the very sophisticated and highly optimized packages that have been developed over the years. Various groups use different approaches to maintain and develop these packages, the most popular ones being CPMD, VASP, Quantum Espresso, CP2K, Siesta, CASTEP, etc. (see on http://www.psi‐k.org/codes.shtml for a more extended list). Each of them has advantages and disadvantages regarding the scaling of computational effort with system size, accuracy, ensembles that can be simulated (microcanonical, canonical, constant pressure, etc.), quantities that can be calculated, etc., and therefore the best choice will depend on the application.


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