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Thermodynamic Properties of Shock-Compressed Plasmas Based on a Chemical Picture

  • V. K. Gryaznov
  • I. L. Iosilevskiy
  • V. E. Fortov
Part of the High-Pressure Shock Compression of Condensed Matter book series (SHOCKWAVE)

Abstract

Calculation of an equation of state and thermodynamic functions is the starting point for a whole set of calculations of thermophysical properties of a substance under strong shock compression and heating [1–6]. Thermodynamic calculation is also an inherent part of hydrodynamic simulation of shock compression. The feature of this interrelation is that the thermodynamic data employed as input information for a very wide and important class of hydrodynamic flows such as adiabatic flows (irreversible shock compression, reversible isentropic compression and expansion, throttling, etc.) are limited in principle by the use of a reduced caloric equation of state that is incomplete from the thermodynamic point of view. This equation of state is an expression for the internal energy (or enthalpy) as a function, U(P, V), of the conjugate thermodynamic variables, pressure and specific volume.

Keywords

Partition Function Chemical Model Shock Compression Grand Canonical Ensemble Caloric Equation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media New York 2004

Authors and Affiliations

  • V. K. Gryaznov
  • I. L. Iosilevskiy
  • V. E. Fortov

There are no affiliations available

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