Phase equilibria in the ternary system isobutyl alcohol+isobutyl acetate+1-hexanol and the binary systems isobutyl alcohol+1-hexanol, isobutyl acetate+1-hexanol at 101.3kPa

2005 ◽  
Vol 235 (1) ◽  
pp. 64-71 ◽  
Author(s):  
R. Muñoz ◽  
J.B. Montón ◽  
M.C. Burguet ◽  
J. de la Torre
2000 ◽  
Vol 65 (12) ◽  
pp. 1833-1838
Author(s):  
Jaroslav Nývlt

Of correlation methods for solubility in ternary systems, the method of expansion of relative activity coefficients and the hydration analysis are based on the thermodynamic condition of phase equilibria. Both of them require only reliable solubility data in the ternary system and corresponding binary systems. Correlation parameters of both of these methods are interrelated and the methods are compared on the system K2SO4-H2SO4-H2O at 50 °C.


2006 ◽  
Vol 71 (7) ◽  
pp. 843-847 ◽  
Author(s):  
Dusko Minic ◽  
Dragan Manasijevic ◽  
Dragana Zivkovic ◽  
Z. Zivkovic

Binary thermodynamic data, successfully used for phase diagram calculations of the binary systems In-Sb, Bi-Sb and In-Bi, were used fort the prediction of phase equilibria in the ternary system In-Sb-Bi at 300?C. The predicted equilibria were compared with the results of SEM-EDX analysis.


2004 ◽  
Vol 19 (8) ◽  
pp. 2298-2305 ◽  
Author(s):  
Yee-wen Yen ◽  
Sinn-wen Chen

Phase equilibria of the Ag–Sn–Cu ternary system have been determined experimentally as well as using the calculation of phase diagram (CALPHAD) method. Various Ag–Sn–Cu alloys were prepared to study the isothermal sections of the Ag–Sn–Cu ternary system at 240 and 450 °C. No ternary compounds were found and all the binary compounds had only limited ternary solubility. The ∈1–Cu3Sn phase is a very stable phase. It is in equilibrium with the Ag, ζ–Ag4Sn, ∈2–Ag3Sn, η–Cu6Sn5, and Cu phases at 240 °C, and is in equilibrium with the Ag, ζ, ∈2, L, and δ–Cu4Sn phases at 450 °C. Thermodynamic models of the Ag–Sn–Cu ternary system were developed based on available thermodynamic models of the constituent binary systems without introducing ternary interaction parameters. The isothermal sections at 240 and 450 °C were calculated, and the results were in good agreement with those determined experimentally. In addition to the isothermal sections, stability diagrams of Sn and Cu were calculated as well.


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