In the analysis of slug flow under gravity conditions surface tension
is usually neglected. The liquid slug is treated as a homogeneous mixt
ure and the liquid film adjacent to the wall, in the Taylor bubble zon
e behind the slug, is treated using the one-dimensional approach (chan
nel flow theory). Although the use of the one-dimensional approach is
not accurate, especially close to the bubble cap, it is considered as
a valid approximation and it yields reasonable results for the modelin
g of pressure drop, bubble length and void fraction in slug flow. Sinc
e for the case of microgravity flow, surface tension is expected to be
a dominant force that should not be overlooked, one may be tempted to
use the same procedure for the analysis of slug flow under microgravi
ty conditions with the surface tension included (this can be done also
for non-microgravity conditions). In this work,it is shown that the i
nclusion of the surface tension in the one-dimensional approach for th
e film analysis leads to erroneous and unacceptable results near the b
ubble cap that cannot be used even as an approximation. It is also sho
wn that far away from the cap the solution with and without the surfac
e tension is practically the same. Thus, a simplified model for slug f
low in microgravity is suggested that assumes a spherical shape of the
bubbles at the nose that is matched with the conventional one-dimensi
onal viscous solution far downstream. In this procedure the effect of
surface tension at the nose is in fact taken into account indirectly b
y the imposition of a spherical cap. That is, the assumption that the
bubble nose behaves similar to the behavior of small size bubbles that
are controlled by surface tension.