Abstract
Experimental results for six binary mixtures of Ne and Kr obtained in a two-bulb apparatus operated at 77.6 K and 308 K are presented. The composition dependence of α T is compared with the results of the Chapman-Enskog theory. The empirical potential of Kestin, Ro and Wakeham is able to explain the experimental dependence of α T on the composition at our working temperature. The same comparison with the results of other authors, at around room temperature, indicates an equally good agreement.
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