Kimura T, Ozaki N, Sano T, Okuchi T, Sano T, Shimizu K, Miyanishi K, Terai T, Kakeshita T, Sakawa Y, Kodama R
Geodynamics Research Center, Ehime University, 2-5 Bunkyo-cho, Matsuyama, Ehime 790-8577, Japan.
Graduate School of Engineering, Osaka University, Suita, Osaka 565-0871, Japan.
J Chem Phys. 2015 Apr 28;142(16):164504. doi: 10.1063/1.4919052.
Pressure, density, and temperature data for H2O were obtained up to 260 GPa by using laser-driven shock compression technique. The shock compression technique combined with the diamond anvil cell was used to assess the equation of state models for the P-ρ-T conditions for both the principal Hugoniot and the off-Hugoniot states. The contrast between the models allowed for a clear assessment of the equation of state models. Our P-ρ-T data totally agree with those of the model based on quantum molecular dynamics calculations. These facts indicate that this model is adopted as the standard for modeling interior structures of Neptune, Uranus, and exoplanets in the liquid phase in the multi-Mbar range.
利用激光驱动冲击压缩技术,获得了高达260吉帕斯卡的水的压力、密度和温度数据。冲击压缩技术与金刚石对顶砧相结合,用于评估主雨贡纽态和非雨贡纽态的P-ρ-T条件下的状态方程模型。模型之间的对比使得对状态方程模型进行清晰的评估成为可能。我们的P-ρ-T数据与基于量子分子动力学计算的模型完全一致。这些事实表明,该模型被用作在多兆巴范围内对海王星、天王星和系外行星液相内部结构进行建模的标准。