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Shock waves and equations of state of matter

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Abstract

The physical properties of hot dense matter over a broad domain of the phase diagram are of immediate interest in astrophysics, planetary physics, power engineering, controlled thermonuclear fusion, impulse technologies, enginery, and several special applications. The use of intense shock waves in dynamic physics has made the exotic high-energy density states of matter a subject of laboratory experiments and enabled advancing by many orders of magnitude along the pressure scale to range into the megabars and even gigabars. The present report reviews the contribution of shock-wave methods to the problem of the equation of state (EOS) at extreme conditions. Experimental techniques for high-energy density cumulation, the drivers of intense shock waves, and methods for the fast diagnostics of high-energy matter are considered. It is pointed out that the available high pressure and temperature information covers a broad range of the phase diagram, but only irregularly and, as a rule, is not thermodynamically complete; its generalization can be done only in the form of a thermodynamically complete EOS. As a practical example, construction of multi-phase EOS for iron is presented. The model’s results are shown for numerous shock-wave data, the high-pressure melting and evaporation regions and the critical point of iron.

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  1. Institute of Problems of Chemical Physics RAS, Prosp. Akad. Semenova, 1, Chernogolovka, 142432, Moscow, Russia

    V. E. Fortov & I. V. Lomonosov

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Communicated by K. Takayama.

The paper was submitted upon invitation from the Editor-in-Chief.

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Fortov, V.E., Lomonosov, I.V. Shock waves and equations of state of matter. Shock Waves 20, 53–71 (2010). https://doi.org/10.1007/s00193-009-0224-8

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