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Practical Determination of Gas Densities from the Speed of Sound Using Square-Well Potentials

机译:使用平方阱势从声速实际确定气体密度

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The relationships between the first three density virial coefficients (B, C, and D) and the first four acoustic virial coefficients (β_a, γ_a, δ_a, and ε_a) are rederived and a published error relating D to δ_a is corrected. We observe that even if the nth and higher-density virial coefficients of a hypothetical gas are identically zero, the nth and higher acoustic virial coefficients are not zero; they depend on the temperature derivatives of the 1st through (n — 1)th density virial coefficients. Thus, two density virial coefficients may suffice for a fit to acoustic data with a cubic pressure dependence. These results are exploited by extending the pressure range of fits to previously published speed-of-sound data without either introducing additional parameters or degrading the fits. We deduce gas densities from fits to speed-of-sound data with acoustic virial coefficients having the temperature dependencies calculated from square-well potentials. The estimated densities differ from independent measurements by a few tenths of a percent in an important range of conditions. These estimates require no p-ρ—T data whatsoever.
机译:重新获得前三个密度维里系数(B,C和D)与前四个声维里系数(β_a,γ_a,δ_a和ε_a)之间的关系,并校正与D关联的已公布误差。我们观察到,即使假设气体的第n个和更高密度的维里系数等于零,第n个和更高的声维里系数也不为零;它们取决于第1到第(n_1)个密度维里系数的温度导数。因此,两个密度维里系数可以满足与立方压力相关的声数据的拟合。通过将拟合的压力范围扩展到以前发布的声速数据,而无需引入其他参数或降低拟合,可以利用这些结果。我们从拟合度到声速数据推论出气体密度,而声维里系数具有根据平方阱电势计算出的温度依赖性。在重要的条件范围内,估计的密度与独立的测量值相差百分之几。这些估计不需要任何p-ρ-T数据。

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