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1992
The gas inside a star consists of a mixture of molecules, atoms and electrons. At temperatures higher than a few times 104 K, the atoms have lost part of their electrons (or all their electrons), and are said to be (partly) ionized. The remaining atom is then called an ion.
Claude Doom, C. De Loore
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The gas inside a star consists of a mixture of molecules, atoms and electrons. At temperatures higher than a few times 104 K, the atoms have lost part of their electrons (or all their electrons), and are said to be (partly) ionized. The remaining atom is then called an ion.
Claude Doom, C. De Loore
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2001
Having introduced the necessary statistical technique, we are now in a position to establish routes from statistical mechanics to thermodynamics, i.e. to observable macroscopic properties. There are three such routes, provided by energy pressure (virial) compressibility equations of state.
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Having introduced the necessary statistical technique, we are now in a position to establish routes from statistical mechanics to thermodynamics, i.e. to observable macroscopic properties. There are three such routes, provided by energy pressure (virial) compressibility equations of state.
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EQUATIONS OF STATE AS CONSERVATION EQUATIONS [PDF]
Chemical Engineering Communications, 1983 Equations of state are shown to be mathematically equivalent to conservation equations, when the distance-time plane is replaced by the pressure-temperature plane. The Clapeyron equation is consequently developed, as a “shock condition“, based on the discontinuity in molar volume between phases at equilibrium.
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Reviews in Mineralogy and Geochemistry, 2000
Diffraction experiments at high pressures provide measurement of the variation of the unit-cell parameters of the sample with pressure and thereby the variation of its volume (or equivalently its density) with pressure, and sometimes temperature. This last is known as the ‘Equation of State’ (EoS) of the material.
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Diffraction experiments at high pressures provide measurement of the variation of the unit-cell parameters of the sample with pressure and thereby the variation of its volume (or equivalently its density) with pressure, and sometimes temperature. This last is known as the ‘Equation of State’ (EoS) of the material.
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Thermodynamic Properties and Equation of State for Solid and Liquid Copper
International journal of thermophysics, 2023N. Kozyrev
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Physical Review B, 1988
The "universal" equation of state recently proposed by Vinet, Ferrante, Rose, and Smith is numerically equivalent, to leading order in finite strain, to several well-established two-parameter equations of state. Notably, it is in accord with the Birch-Murnaghan equation that is derived from Eulerian finite-strain theory, and hence is applicable to ...
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The "universal" equation of state recently proposed by Vinet, Ferrante, Rose, and Smith is numerically equivalent, to leading order in finite strain, to several well-established two-parameter equations of state. Notably, it is in accord with the Birch-Murnaghan equation that is derived from Eulerian finite-strain theory, and hence is applicable to ...
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1991
It was shown in Chapter 11 that both the internal energy and the entropy of a closed hydrostatic system can be determined completely when the equation of state and one principal heat capacity are known. This knowledge then gives complete information about the thermodynamic behaviour of the system.
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It was shown in Chapter 11 that both the internal energy and the entropy of a closed hydrostatic system can be determined completely when the equation of state and one principal heat capacity are known. This knowledge then gives complete information about the thermodynamic behaviour of the system.
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2010
Studying the motions of complex fluid media involves determining how local quantities that characterize the behavior of single- or multicomponent, homogeneous or heterogeneous media evolve over time and space.
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Studying the motions of complex fluid media involves determining how local quantities that characterize the behavior of single- or multicomponent, homogeneous or heterogeneous media evolve over time and space.
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