Abstract

The most important characteristic of glass transition is a jump in the specific heat . Despite its significance, no standard theory exists to describe it. In this study, first-principles molecular-dynamics simulations are used to describe the glass transition of silica glass. The novel view that state variables are extended to include the equilibrium positions of atoms is fully used in analyzing the simulation results. Decomposing the internal energy into three components (structural, phonon, and thermal expansion energies) reveals that the jump of silica glass is entirely determined by the component of structural energy. The reason for the small is its high glass-transition temperature, which makes the fluctuation in the structural energy insensitive to the temperature change. This significantly affects how the Prigogine-Defay ratio Π is interpreted, which was previously unknown. The ratio Π represents the ratio of the total energy change to the contribution of thermal expansion energy at the glass transition. The general property, Π> 1, of glasses indicates that glass transitions occur mainly via the change in the structural energy. Silica glass is an extreme case in that the transition occurs entirely through the change in internal structure, such as the distribution of the bending angle of Si–O–Si bonds.

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