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This article is cited in 3 scientific papers (total in 3 papers)
Possible negative value of the Grüneisen coefficient of hydrogen in the pressure range from 40 to 75 GPa and temperature range from 3500 to 7500 K
A. B. Medvedevab a Institute of Experimental Physics (VNIIEF), Russian Federal Nuclear Center, Sarov, 607188, Russia
b Department of the National Research Nuclear University "MEPhI", Institute of Physics and Technology, Sarov, 607186, Russia
Abstract:
Experimental data on single and double shock compression of initially liquid and gaseous (compressed by initial pressure) hydrogen isotopes (protium and deuterium) at pressures of $\approx$ 10–180 GPa and temperatures of $\approx$ 3000–20000 K are considered. The mean values of the measured variables (pressure, density, internal energy, and temperature) show that hydrogen at a pressure of $\approx$ 41 GPa in the temperature interval of $\approx$ 3500–5700 K and at a pressure of $\approx$ 74 GPa in the temperature interval of $\approx$ 5000–7500 K is characterized by a negative value of the Grüneisen coefficient. Such an anomaly may play a key role in some processes, including those proceeding in the Jupiter gas shell, which mainly consists of protium ($\approx$ 90%) and helium ($\approx$ 10%). In the range of pressures (depths) of its manifestation, convection in the protium shell is forbidden with an increase in temperature in the shell with increasing pressure. Possibly, a comparatively moderate fraction of helium does not suppress the anomaly, and it serves as a barrier for large-scale convection in the Jupiter shell. Experiments are required to confirm this anomaly.
Keywords:
hydrogen, protium, deuterium, equation of state, pressure, temperature, density, energy, Grüneisen coefficient, shock adiabat, isentrope, convection, Jupiter.
Received: 26.06.2017 Revised: 21.07.2017
Citation:
A. B. Medvedev, “Possible negative value of the Grüneisen coefficient of hydrogen in the pressure range from 40 to 75 GPa and temperature range from 3500 to 7500 K”, Fizika Goreniya i Vzryva, 54:2 (2018), 98–113; Combustion, Explosion and Shock Waves, 54:2 (2018), 216–230
Linking options:
https://www.mathnet.ru/eng/fgv495 https://www.mathnet.ru/eng/fgv/v54/i2/p98
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