Corresponding States for Volumes of Elemental Solids at Their Pressures of Polymorphic Transformations

Many non-molecular elemental solids exhibit common features in their structures over the range of 0 to 0.5 TPa that have been correlated with equivalent valence electron configurations. Here, it is shown that the pressures and volumes at polymorphic transitions obey corresponding states given by a s...

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Bibliographic Details
Main Author: Oliver Tschauner
Format: Article
Language:English
Published: MDPI AG 2022-11-01
Series:Crystals
Subjects:
Online Access:https://www.mdpi.com/2073-4352/12/12/1698
Description
Summary:Many non-molecular elemental solids exhibit common features in their structures over the range of 0 to 0.5 TPa that have been correlated with equivalent valence electron configurations. Here, it is shown that the pressures and volumes at polymorphic transitions obey corresponding states given by a single, empirical universal step-function V<sub>tr</sub>/L = −0.0208(3) · P<sub>tr</sub> + N<sub>i</sub>, where V<sub>tr</sub> is the atomic volume in Å<sup>3</sup> at a given transformation pressure P<sub>tr</sub> in GPa, and L is the principal quantum number. N<sub>i</sub> assumes discrete values of approximately 20, 30, 40, etc. times the cube of the Bohr radius, thus separating all 113 examined polymorphic elements into five discrete sets. The separation into these sets is not along L. Instead, strongly contractive polymorphic transformations of a given elemental solid involve changes to different sets. The rule of corresponding states allows for predicting atomic volumes of elemental polymorphs of hitherto unknown structures and the transitions from molecular into non-molecular phases such as for hydrogen. Though not an equation of state, this relation establishes a basic principle ruling over a vast range of simple and complex solid structures that confirms that effective single-electron-based calculations are good approximations for these materials and pressures The relation between transformation pressures and volumes paves the way to a quantitative assessment of the state of very dense matter intermediate between the terrestrial pressure regime and stellar matter.
ISSN:2073-4352