Quasi-equilibrium evaporation characteristics of oxygen in the liquid–vapor interfacial region

Author(s):  
Zhongqi Zuo ◽  
Wenbing Jiang ◽  
Pingan Pan ◽  
Xujin Qin ◽  
Yonghua Huang
2006 ◽  
Vol 110 (12) ◽  
pp. 6101-6109 ◽  
Author(s):  
Nicolas Glandut ◽  
Andrew D. Malec ◽  
Michael V. Mirkin ◽  
Marcin Majda

Author(s):  
Aaron P. Wemhoff ◽  
Van P. Carey

Molecular dynamics (MD) simulations of liquid-vapor interfaces were performed to determine mean property variations and property fluctuations in the liquid-vapor interfacial region at various reduced temperatures. The interfacial region typically has a thickness on the order of a few nanometers for systems of practical interest. The system’s initial conditions were specified as a bulk liquid region sandwiched between two bulk vapor regions. Simulations were run using a Lennard-Jones 6-12 potential function between the atoms with appropriate parameters for Argon atoms. As the simulation was performed, interfacial region property data was collected over time. The resulting property data are shown to establish trends similar to those indicated by theoretical and experimental results reported elsewhere. The peak fluctuations of mass density and free energy density were determined to be approximately equal in magnitude when normalized with the difference in their respective bulk values at a given temperature. These fluctuations were found to increase rapidly with temperature. The fluctuations in the interfacial thickness and interfacial position follow a functional dependence on temperature similar to that exhibited by the mean value of interfacial thickness. In addition to exploring fluctuations in the interfacial region, two new methods were developed to determine interfacial tension through methods involving integration of excess free energy density across the interfacial region. These techniques were shown to yield mean results similar to theoretical predictions and those using conventional techniques. In addition, the time required for computation using the new techniques is significantly reduced due to less computational time per step and fewer required steps for convergence to a mean value.


Author(s):  
Aaron P. Wemhoff ◽  
Van P. Carey

Surface tension prediction of liquid-vapor interfaces of polyatomic fluids using traditional methods in molecular dynamics simulations has shown to be difficult due to the requirement of evaluating complex intermolecular potentials even though these methods provide accurate predictions. In addition, the traditional methods may only be performed during a simulation run. However, analytical techniques have recently been developed that determine surface tension by using the characteristics of the density profile of the interfacial region between the bulk liquid and vapor regions. Since these characteristics are a standard result of many liquid-vapor interfacial region simulations, these data may be used in a post-simulation analysis. One such method, excess free density integration (EFEDI), provides results from the post-simulation analysis, but the expansion from monatomic to polyatomic fluids is not straightforward [1]. A more general and powerful approach to surface tension involves the application of a Redlich-Kwong-based mean-field theory [2], which has resulted in a single equation linking the surface tension of a fluid, σlv, with the density gradient at the center of the interfacial region, σlv=0.1065(1−T/Tc)−0.34Li2dρ^dzz=0aR0NA2bRNAT1/2ln1+ρ^lbRNA1+ρ^vbRNA(1) where z is the position normal to the interfacial region and is zero at its center, ρ^l and ρ^v are the liquid and vapor molar densities, respectively, TC is the critical temperature, NA is Avogadro’s number, Li is a characteristic length given by Li=kBTCPC1/3(2) and aR0 and bR are the coefficients in the Redlich-Kwong equation of state, P=NkBTV−bRN−aR0N2T1/2V(V+bRN)(3) Furthermore, PC is the critical pressure for the fluid. Reference [2] shows that the relation provided by Equation 1 provides a approximate prediction of surface tension for argon fluid using data from molecular dynamics simulations. The derivation of Equation 1 is based on the assumption that the density profile in the interfacial region follows ρ^−ρ^vρ^l−ρ^v=1e4z/δzi+1(4) where δzi is the interfacial region thickness,. Note that Equation 4 is more commonly expressed in the equivalent form ρ^(z)=12(ρ^l+ρ^v)−12(ρ^l−ρ^v)tanh2zδzi(5) Wemhoff and Carey [1] have recommended the use the fit curve relation given by Equation 5 for the liquid-vapor interfacial region of a diatomic nitrogen system. Therefore, Equation 1 may be used to predict the surface tension for diatomic nitrogen at various temperatures.


2017 ◽  
Vol 09 (08) ◽  
pp. 1750111 ◽  
Author(s):  
B. V. Librovich ◽  
A. F. Nowakowski ◽  
F. C. G. A. Nicolleau ◽  
T. M. Michelitsch

A new mathematical model for non-equilibrium evaporation/condensation including boiling effect is proposed. A simplified differential-algebraic system of equations is obtained. A code to solve numerically this differential-algebraic system has been developed. It is designed to solve both systems of equations with and without the boiling effect. Numerical calculations of ammonia–water systems with various initial conditions, which correspond to evaporation and/or condensation of both components, have been performed. It is shown that, although the system evolves quickly towards a quasi-equilibrium state, it is necessary to use a non-equilibrium evaporation model to calculate accurately the evaporation/condensation rates, and consequently all the other dependent variables.


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