Anton–Schmidt equation of state
Template:Short description The Anton–Schmidt equation is an empirical equation of state for crystalline solids, e.g. for pure metals or intermetallic compounds.[1] Quantum mechanical investigations of intermetallic compounds show that the dependency of the pressure under isotropic deformation can be described empirically by
- .
Integration of leads to the equation of state for the total energy. The energy required to compress a solid to volume is
which gives
- .
The fitting parameters and are related to material properties, where
- is the bulk modulus at equilibrium volume .
- correlates with the Grüneisen parameter .[2][3]
However, the fitting parameter does not reproduce the total energy of the free atoms.[4]
The total energy equation is used to determine elastic and thermal material constants in quantum chemical simulation packages.[4][5]
The equation of state has been used in cosmological contexts to describe the dark energy dynamics.[6] However its use has been recently criticized since it appears disfavored than simpler equations of state adopted for the same purpose.[7]
See also
References
- ↑ Template:Cite journal
- ↑ Otero-de-la-Roza, et al., Gibbs2: A new version of the quasi-harmonic model code. Computer Physics Communications 182.8 (2011): 1708-1720. Template:Doi
- ↑ Jund, Philippe, et al., Physical properties of thermoelectric zinc antimonide using first-principles calculations., Physical Review B 85.22 (2012) Template:ArXiv.
- ↑ 4.0 4.1 Atomic Simulation Environment documentation of the Technical University of Denmark, Department of Physics [1]
- ↑ Gilgamesh chemical software documentation of the Department of Chemical Engineering of Carnegie Mellon University Template:Cite web
- ↑ Salvatore Capozziello, Rocco D'Agostino, Orlando Luongo, Cosmic acceleration from a single fluid description, Physics of the Dark Universe 20 (2018) 1-12, Template:ArXiv.
- ↑ Kuantay Boshkayev, Talgar Konysbayev, Orlando Luongo, Marco Muccino, Francesco Pace, Testing generalized logotropic models with cosmic growth, Physical Review D 104 (2021) 2, 023520, Template:ArXiv.