首页> 外文学位 >Viscosity of planetary fluids and the amorphization of crystals at high pressure.
【24h】

Viscosity of planetary fluids and the amorphization of crystals at high pressure.

机译:行星流体的粘度和高压下晶体的非晶化。

获取原文
获取原文并翻译 | 示例

摘要

Transport properties of solids and fluids change by orders of magnitude as a function of different pressure and temperature. Such properties in large part dictate the mass and heat transport in planetary interiors, so their measurement at high pressures and temperatures is important. While these properties are often well constrained at room pressure, there is a dearth of measurement on fluids of all types at high pressure and temperature. The viscosity, in particular, is poorly known for many materials above 0.5 to 1.0 GPa, or at high compression (rho/rho0 ∼ 1.5-2.0).;To determine how the viscosity of different materials changes with pressure, the diamond-cell was used as a high-pressure rolling-sphere viscometer. Measurements on organic fluids reveal large changes in viscosity as a function of both temperature and pressure, with activation energies increasing significantly as the density increases. In contrast, water has only a small increase in viscosity with large increases in density, and an activation energy that remains almost constant. For both organic liquids and water, several scaling relations derived from different physical arguments fit the data equally well. This makes it difficult to reliably extrapolate viscosity data, as different models tend to diverge significantly from each other at high pressure and temperature.;X-ray diffraction measurements on the pressure-induced amorphization of tin-iodide show a small increase in transition pressure as a function of temperature. Contrary to previous interpretations, the amorphization does not need to be a two-step process, as some of the samples amorphize without converting to a second crystal phase. Large variability in the number of crystal phases, location of the glass transition pressure, and crystal volumes were observed as a function of sample loading. This may be due to the potential for extreme sensitivity of the sample to even small deviatoric stresses in the sample chamber.
机译:固体和流体的传输特性会随压力和温度的变化而变化几个数量级。这些特性在很大程度上决定了行星内部的质量和热传递,因此在高压和高温下进行测量非常重要。尽管这些特性通常在室温下受到很好的约束,但缺乏在高压和高温下对所有类型流体的测量。特别是对于在0.5至1.0 GPa以上或在高压缩率(rho / rho0〜1.5-2.0)的许多材料而言,粘度是未知的。为了确定不同材料的粘度如何随压力变化,金刚石电池是用作高压滚动球粘度计。对有机流体的测量表明,粘度随温度和压力的变化很大,活化能随密度的增加而显着增加。相反,水的粘度仅具有很小的增加,而密度却有较大的增加,并且活化能几乎保持恒定。对于有机液体和水,从不同物理参数得出的几个比例关系都很好地拟合了数据。由于在高压和高温下不同的模型趋于彼此大相径庭,因此难以可靠地推断粘度数据.X射线衍射测量在压力引起的碘化锡非晶化上的变化表明,随着压力的升高,转变压力小幅增加。温度的函数。与先前的解释相反,非晶化不需要分两步进行,因为一些样品可以非晶化而无需转换为第二晶相。观察到晶体相数,玻璃化转变压力的位置和晶体体积的较大变化是样品加载的函数。这可能是由于样品对样品室中很小的偏斜应力具有极高的敏感性的缘故。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号