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Calculation of Surface Tension
Surface tension is a thermophysical property
closely related to the bulk thermodynamic properties of the material.
It is important to understand the surface tension properties as it can
have a big influence on the way in which alloys solidify. In particular
it affects the solerability
solderability. In conventional solders lead had a particularly
desirable property of
reducing the surface tension. Understanding how the addition of
impurities affect the surface tension of lead free solders is important
in attempts to remove the use of lead from electronic
interconnections. Measurements of surface tension has been
carried out systematically within the COST531 Action resulting in the
Surdat
database developed by Moser and colleagues. The Figure below
shows a key of measurements carried out on the surface tension of pure
Sn [W Gasior, Z Moser, J Pstrus, J. Phase Equil. 2001, 221(1), 20-25].

Surface tension
of Sn from the work of Gasior et al.
While surface tension is not a thermodynamic
property of the bulk material it is neverthless a reflection of the
thermodynamic
properties of the atoms near the surface. For a pure material, of
course, the surface has the same composition as that of the bulk
material. However when it comes to an alloy the different component
elements have different tendencies to be surface active causing the
composition of the surface to be quite different from that of the bulk
material.
Tanaka [99Tan] has attempted to model the surface
tension of a wide range of materials, both ionic and metallic melts, by
using an equation developed by Butler [32But] which seeks to express
the surface tension in terms of an equilibrium between the bulk
material and a surface layer.
Tanaka expressed the Butler equation as:

Butler equation
for surface tension expressed by Tanaka
Where the surface tension of the material, σ, is
related to the surface tension of the individual components
σ1 and σ2,
the relative surface areas occupied by the components A1 and A2, the
composition expressed as mole fraction and the excess partial Gibbs
energies of the components in the bulk and the surface layer. While
this is expressed for two components these equalities would hold for
any number of components.
These equations can be transformed into: 
which expresses the fact the chemical potential of
the components is equal in the bulk and surface layer or alternatively that there is
chemical equilibrium between the bulk and the surface layer. The right
hand side of the above equations relate to the bulk thermodynamic
properties while on the left hand side of the equations relate to the
surface. The thermodynamic properties of the bulk are, of course, well
represented by standard thermodynamic models and data as stored in comprehensive thermodynamic databases such as the
SOLDERS database. The surface thermodynamic properties are given by:
relative to the pure elements in the liquid phase.
The surface area contributions, A1 and A2, to the surface properties
could be related to the volumes of the pure elements in then the
liquid:
where N0 is the Avogadro number and V1 the molar
volume of the first element.
Tanaka calculated the surface tension for a number of metallic systems
and found an empirical relationship relating Gmix , the excess Gibbs
energy of mixing, for the surface and Gmix for the bulk:
It is now possible to calculate the equilibrium
between the bulk material and the surface layer. The unknown surface
tension, σ, of the liquid for a particular composition is calculated to
be the value which just brings the surface into equilibrium with the
bulk. This could be seen as analogous to a procedure for calculating
the pressure required to bring a new phase into equilibrium with a
chosen phase.
While the empirical relationship above derived by
Tanaka is useful in the absence of any other information it may be more
useful to derive the excess properties for the surface layer from any
experimental surface tension data available.
The way in which this problem is now formulated means that the approach
can easily be generalised to any number of components. Indeed the most
practical way to introduce a capability for calculating surface tension
is to create a database for the thermodynamic properties of the
surface.
The figure below shows the calculated surface tension of Bi-Sn liquids with
experimental points superimposed. 
The composition of the surface can
also be calculated at the same time as shown in the next figure and this shows
how Bi is markedly more surface active than Sn. 
The next figure shows the calculated surface tension
of Ag-Sn alloys at 1000ºC. 
While the actual value of the surface
tension is important, it is often more important to know how the
surface tension changes with temperature. Computational thermochemistry
provides this capability as shown in the next figure where the
temperature dependence of the surface tension is predicted to change
sign.

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