RUS  ENG
Full version
JOURNALS // Fizika Goreniya i Vzryva // Archive

Fizika Goreniya i Vzryva, 2018 Volume 54, Issue 2, Pages 98–113 (Mi fgv495)

This article is cited 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.

UDC: 532.593+523.45

Received: 26.06.2017
Revised: 21.07.2017

DOI: 10.15372/FGV20180211


 English version:
Combustion, Explosion and Shock Waves, 2018, 54:2, 216–230

Bibliographic databases:


© Steklov Math. Inst. of RAS, 2024