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Light scattering from a binary liquid mixture above its critical consolute point

机译:Light scattering from a binary liquid mixture above its critical consolute point

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Light scattering measurements were performed on the binary liquid mixture carbon tetrachloridendash;perfluoromethylcyclohexane at its critical concentration and immediately above its critical consolute temperature. Measurements of time averaged intensities as a function of scattering angle and temperature distance from the critical consolute temperature,Tminus;Tc, yielded the critical parameters ggr; = 1.220plusmn;0.018, xgr;0= 2.28plusmn;0.21 Aring;, and ngr; = 0.626plusmn;0.013. Here ggr; describes the temperature dependence of the susceptibility khgr; according to the relation khgr;prop;egr;minus;ggr;, where egr; = (Tminus;Tc)/Tc. xgr;0and ngr; characterize the correlation length with xgr; = xgr;0egr;minus;ngr;, which is a measure of the spatial extent of local concentration fluctuations. These values of ggr; and ngr; agree well with the scaling and universality hypothesis. Time dependence of the intensity as a function of scattering angle and ofTminus;Tcwas determined by measuring the photocurrent autocorrelation function. These measurements yielded decay rates for concentration fluctuations. Combination of decay rates, correlation lengths, and viscosities allowed a direct comparison with the modendash;mode coupling theory of Kawasaki. Excellent coincidence of theory and experiment was found except in the vicinity ofKxgr; = 1, where decay rates were high when compared to theory.Kis the magnitude of the momentum transfer vector. Sources of error in the critical parameters obtained from light scattering intensity measurements were analyzed in detail. A useful equation is derived which relates the actual scattering angle inside a cylindrical cell to eight experimental parameters including five rsquo;rsquo;alignmentrsquo;rsquo; parameters which are subject to error. Graphical criteria are presented for estimating uncertainties in critical parameters ggr;, xgr;0, ngr;, and eegr;.

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