Extension of finite-strain equations of state to ultra-high pressure

•A four-parameter equation of state (EoS) is proposed for solids, applicable in the ultra-high pressure regime.•The isothermal EoS, a broken power-law density, is tested with high-pressure data sets of copper extending up to 60 TPa.•The range of applicability of Eulerian and Lagrangian finite-strain...

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Bibliographic Details
Published inPhysics letters. A Vol. 393; p. 127185
Main Author Tomaschitz, Roman
Format Journal Article
LanguageEnglish
Published Elsevier B.V 26.03.2021
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ISSN0375-9601
1873-2429
DOI10.1016/j.physleta.2021.127185

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Summary:•A four-parameter equation of state (EoS) is proposed for solids, applicable in the ultra-high pressure regime.•The isothermal EoS, a broken power-law density, is tested with high-pressure data sets of copper extending up to 60 TPa.•The range of applicability of Eulerian and Lagrangian finite-strain expansions of the EoS is determined.•The third-, fourth- and fifth-order Birch-Murnaghan EoSs are recovered from the Eulerian finite-strain expansion of the EoS.•A closed-form expression of the free energy is obtained, covering densities up to the Thomas-Fermi free-electron limit. Eulerian and Lagrangian finite-strain expansions are extended into the ultra-high pressure range by way of an isothermal closed-form EoS, a broken power-law density depending on four parameters determined by least-squares regression. The EoS is put to test with high-pressure data sets of copper up to 60 TPa and can be used to extrapolate data sets obtained in the GPa range to ultra-high densities approaching the Thomas-Fermi free-electron regime. In the low and intermediate pressure range up to a few hundred GPa, the EoS admits finite-strain ascending series expansions, which coincide with the third-, fourth- and fifth-order Birch-Murnaghan and Lagrangian EoSs, subject to the finite-strain expansion parameter used. The pressure evolution of the compression modulus of copper is obtained from the regressed EoS. A closed-form expression of the free energy over the full pressure range up to the Thomas-Fermi limit is derived and compared with finite-strain theory.
ISSN:0375-9601
1873-2429
DOI:10.1016/j.physleta.2021.127185