Direct numerical simulations of interface dynamics to link capillary pressure and total surface energy

Details

Serval ID
serval:BIB_DC67D8D71762
Type
Article: article from journal or magazin.
Collection
Publications
Institution
Title
Direct numerical simulations of interface dynamics to link capillary pressure and total surface energy
Journal
Advances in Water Resources
Author(s)
Ferrari A., Lunati I.
ISSN-L
0309-1708
Publication state
Published
Issued date
2013
Peer-reviewed
Oui
Volume
57
Pages
19-31
Language
english
Notes
Ferrari2013
Abstract
The flow of two immiscible fluids through a porous medium depends
on the complex interplay between gravity, capillarity, and viscous
forces. The interaction between these forces and the geometry of
the medium gives rise to a variety of complex flow regimes that are
difficult to describe using continuum models. Although a number of
pore-scale models have been employed, a careful investigation of
the macroscopic effects of pore-scale processes requires methods
based on conservation principles in order to reduce the number of
modeling assumptions. In this work we perform direct numerical simulations
of drainage by solving Navier-Stokes equations in the pore space
and employing the Volume Of Fluid (VOF) method to track the evolution
of the fluid-fluid interface. After demonstrating that the method
is able to deal with large viscosity contrasts and model the transition
from stable flow to viscous fingering, we focus on the macroscopic
capillary pressure and we compare different definitions of this quantity
under quasi-static and dynamic conditions. We show that the difference
between the intrinsic phase-average pressures, which is commonly
used as definition of Darcy-scale capillary pressure, is subject
to several limitations and it is not accurate in presence of viscous
effects or trapping. In contrast, a definition based on the variation
of the total surface energy provides an accurate estimate of the
macroscopic capillary pressure. This definition, which links the
capillary pressure to its physical origin, allows a better separation
of viscous effects and does not depend on the presence of trapped
fluid clusters.
Create date
25/11/2013 15:33
Last modification date
20/08/2019 16:01
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