A New Approach to Instability Theory in Porous Media

1985 ◽  
Vol 25 (05) ◽  
pp. 765-779 ◽  
Author(s):  
R.G. Bentsen

Abstract Early work in the area of instability theory is limited in that it is based on first-order perturbation theory and the concept of a velocity potential. Thus, while it can deal with an incipient finger, it cannot deal with the subsequent growth of a finger. This paper develops a new approach to the instability theory that overcomes this limitation. The new approach, like earlier work, is based on the assumption that the immiscible displacement of one fluid by another can be treated as a moving-boundary problem. Therefore, two solutions arise, one for each side of the plane interface that initially separates the two fluids. plane interface that initially separates the two fluids. Because the new approach makes use of a force potential rather than a velocity potential, it is possible to impose several new conditions on these two solutions. As a consequence, further extensions to the stability theory have been obtained. In particular, it is now possible to predict the steady-state velocity at which a finger propagates and, consequently, the breakthrough recovery obtained not only when the displacement is stable, but also when it is pseudostable. pseudostable. Introduction It has been recognized for some time 1 that viscous fingering can play a significant role in the immiscible displacement of one fluid by another. This led a number of people to attempt a theoretical description of viscous fingering. Many of these attempts are based on first-order perturbation theory. When this approach is taken, it is usual to postulate the existence of a velocity potential. Then, if the divergence of the perturbation velocity is identically equal to zero, the postulated velocity potential will satisfy Laplace's equation. There are several problems with this approach. First, a velocity potential exists only for fields of flow involving a fluid of constant density and viscosity and a porous medium that is homogeneous and isotropic throughout. Thus it is debatable whether results based on the concept of a velocity potential have any application when the porous medium is not ideal. Second, the concept of a porous medium is not ideal. Second, the concept of a velocity potential has only kinematical significance and gives no insight whatsoever into the dynamic properties of the flow. As a consequence, when a velocity potential is used, one cannot infer how variations in rock and fluid properties might affect the perturbation velocity. properties might affect the perturbation velocity. Finally, the divergence of the perturbation velocity is zero only when a plane interface separates the displaced fluid from the displacing fluid. As soon as the interface is perturbed, two fluids will occupy a region where there was previously only one, and the divergence of the perturbation velocity will no longer be zero. Rather, the perturbation velocity will no longer be zero. Rather, the divergence of the sum of the perturbation velocities, one for each fluid, will be zero. Thus, while first-order perturbation theory can deal with an incipient finger, it perturbation theory can deal with an incipient finger, it cannot deal with the subsequent growth of the finger. The purpose of this paper is to develop a theory for viscous purpose of this paper is to develop a theory for viscous fingering that does not suffer from the aforementioned limitations that arise from the use of a velocity potential. The new theory, which is based on the concept of a force potential, not only explicitly accounts for the dynamic flow potential, not only explicitly accounts for the dynamic flow properties of both fluids, but also is capable of delineating properties of both fluids, but also is capable of delineating the entire life-span of the growing finger. Theory Fluid Displacement. To develop the theory presented in subsequent sections, it is necessary to have a working model of how one fluid displaces another. Such a model must be simple to keep the mathematics tractable. Consequently, it is usual to assume that the displaced and displacing fluids are separated initially by a plane interface and that the porous medium is ideal. If the porous medium is truly ideal (in the sense that the size and shape of all flow paths are identical), the displaced and displacing fluids will continue to be separated during the course of a displacement by a saturation discontinuity (or shock), provided the displacement is stable. 4 Thus stable provided the displacement is stable. 4 Thus stable displacements of this kind can be treated as a moving boundary problem. However, any real porous medium will contain a distribution of pore sizes. As a consequence, different parts of an initially plane interface will move at different parts of an initially plane interface will move at different velocities through the porous medium; i.e., a distribution of saturations will evolve to separate that part of the porous medium where only displacing fluid is flowing from that where only displaced fluid is flowing. The length and shape of this transition zone will depend not only on the pore-size distribution of the porous medium, but also on pore-size distribution of the porous medium, but also on the balance between viscous, gravity, and capillary forces that exists at each point along the saturation profile during the course of the displacement. Moreover, the shape of the saturation profile can be predicted by conventional displacement theory "if the displacement is stable. Even in an ideal porous medium, the displacement front separating the fluids may become unstable under certain conditions. Consequently, a distribution of saturations will evolve again to separate the two regions where only one fluid is flowing. However, the length and shape of this transition region will differ markedly from that which results from a distribution of pore sizes. SPEJ P. 765

1975 ◽  
Vol 53 (23) ◽  
pp. 2590-2592
Author(s):  
J. Cejpek ◽  
J. Dobeš

The reaction processes in which a one-step transition is forbidden are analyzed from the point of view of the first order perturbation theory. The interference between two competing two-step reaction paths is found to be always constructive. A qualitative explanation of the experimentally observed reaction intensities is presented.


Author(s):  
D. Semkat ◽  
H. Fehske ◽  
H. Stolz

AbstractWe investigate quantum many-body effects on Rydberg excitons in cuprous oxide induced by the surrounding electron-hole plasma. Line shifts and widths are calculated by full diagonalisation of the plasma Hamiltonian and compared to results in first order perturbation theory, and the oscillator strength of the exciton lines is analysed.


1993 ◽  
Vol 08 (18) ◽  
pp. 1691-1700 ◽  
Author(s):  
GEORGE TRIANTAPHYLLOU

In view of the recent interest in the decays of mesons into a pair of light leptons, a computation of the QED radiative corrections to the decay of π0 into an electron-positron pair is presented here. The analysis is based on the soft-photon resummation method, which, unlike first-order perturbation theory, allows for very strict invariant-mass cuts on the final electrons. When combined with the theoretical estimates for the non-radiatively corrected decay rate, the results of the present paper could help to determine if new physics affect this decay.


Author(s):  
Shyeh Tjing Loi ◽  
John C B Papaloizou

Abstract Observations of pressure-gravity mixed modes, combined with a theoretical framework for understanding mode formation, can yield a wealth of information about deep stellar interiors. In this paper, we seek to develop a formalism for treating the effects of deeply buried core magnetic fields on mixed modes in evolved stars, where the fields are moderate, i.e. not strong enough to disrupt wave propagation, but where they may be too strong for non-degenerate first-order perturbation theory to be applied. The magnetic field is incorporated in a way that avoids having to use this. Inclusion of the Lorentz force term is shown to yield a system of differential equations that allows for the magnetically-affected eigenfunctions to be computed from scratch, rather than following the approach of first-order perturbation theory. For sufficiently weak fields, coupling between different spherical harmonics can be neglected, allowing for reduction to a second-order system of ordinary differential equations akin to the usual oscillation equations that can be solved analogously. We derive expressions for (i) the mixed-mode quantisation condition in the presence of a field and (ii) the frequency shift associated with the magnetic field. In addition, for modes of low degree we uncover an extra offset term in the quantisation condition that is sensitive to properties of the evanescent zone. These expressions may be inverted to extract information about the stellar structure and magnetic field from observational data.


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