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Critical Temperature for Phase Separation of the Solid Solutions of Rare Gases

✍ Scribed by HALSEY, G. D.; FREEMAN, MARK P.

Book ID
109590513
Publisher
Nature Publishing Group
Year
1956
Tongue
English
Weight
306 KB
Volume
178
Category
Article
ISSN
0028-0836

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πŸ“œ SIMILAR VOLUMES

Temperature variation of the radiative r
Temperature variation of the radiative recombination spectrum of the solid rare gases
✍ F. Coletti; A.M. Bonnot πŸ“‚ Article πŸ“… 1978 πŸ› Elsevier Science 🌐 English βš– 284 KB

We present detailed spectra of the electron excited solid rare gases in the esciton region. The variatipn of the temperature gves a redshift of the structures when the temperature increases. This evolution for Xe, Kr and Ar can be-related to the variation of the lattice parameter.

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Calculations were performed on the basis of a generalized Gibbs energy of mixing G~, which is the sum of the Gibbs energy of mixing of the stagnant system and Es, the energy stored in the system during stationary flow. With increasing shear rate )), the demixing temperatures shift to lower values (s