Computer simulation and modeling the metal to insulating transition of liquid mercury via pair, empirical, and many-body potentials

In this study, Monte Carlo simulations were carried out to detect the metal–insulator transition in liquid mercury by changing the static properties at the microscopic scale. In the simulations pair, empirical, and many-body potentials govern metal–metal interactions in the canonical ensemble. The s...

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Veröffentlicht in:Journal of molecular modeling 2022-12, Vol.28 (12), p.377-377, Article 377
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description In this study, Monte Carlo simulations were carried out to detect the metal–insulator transition in liquid mercury by changing the static properties at the microscopic scale. In the simulations pair, empirical, and many-body potentials govern metal–metal interactions in the canonical ensemble. The structural and thermodynamic changes over a wide temperature range from 773 to 1773 K are described in the first coordination shell and residual internal energy, respectively. The results reveal that during the simulated heating process, the properties undergo significant change at 1673 K, which is in connection with the metal-nonmetal transition in the liquid. These findings coincide with the experimental observations of this thermodynamic phenomenon. Notably, the free energy of association that renders the system to this thermodynamic state is estimated. Graphical Abstract
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subjects Characterization and Evaluation of Materials
Chemistry
Chemistry and Materials Science
Computer Appl. in Life Sciences
Computer Applications in Chemistry
Computer simulation
Free energy
Internal energy
Metal-insulator transition
Molecular Medicine
Original Paper
Residual energy
Theoretical and Computational Chemistry
Thermodynamics
title Computer simulation and modeling the metal to insulating transition of liquid mercury via pair, empirical, and many-body potentials
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