3.2 Geometric Observables
[page 376, §1]
[376.1.1] Well defined geometric observables are the basis for
the geometric characterization of porous media.
[376.1.2] A perennial problem in all applications is to identify
those macroscopic geometric observables that are
relevant for distinguishing between classes of microstructures.
[376.1.3] One is interested in those properties of
the microstructure that influence the macroscopic physical
behaviour.
[376.1.4] In general this depends on the details of the physical
problem, but some general properties of the microstructure
such as volume fraction or porosity are known to
be relevant in many situations.
[376.1.5] Hadwigers theorem [16] is an example of
a mathematical result that helps to identify an
important class of such general geometric properties of porous media.
[376.1.6] It will be seen later, however, that there exist
important geometric properties that are not
members of this class.
[376.2.1] A geometric observable f is a mapping (functional) that
assigns to each admissible pore space P a real number
fP=fP∩S
that can be calculated from P without solving a physical
boundary value problem.
[376.2.2] A functional whose evaluation requires the solution of a physical
boundary value problem will be called a physical observable.
[376.3.1] Before discussing examples for geometric observables
it is necessary to specify the admissible geometries P.
[376.3.2] The set R of admissible P is defined as
the set of all finite unions of compact convex sets
[16, 43, 41, 40].
[376.3.3] Because R is closed under unions and
intersections it is called the convex ring.
[376.3.4] The choice of R is convenient for applications
because digitized porous media can be considered as
elements from R
and because continuous observables defined for
convex compact sets can be continued to all of R.
[376.3.5] The set of all compact and convex subsets of Rd
is denoted as K.
[376.3.6] For subsequent discussions the
Minkowski addition of two sets A,B⊂Rd
is defined as
Multiplication of A with a scalar is defined by
aA=ax:x∈A for a∈R.
[376.4.1] Examples of geometric observables are the volume of P
or the surface area of the internal
∂P=∂M=P∩M.
[376.4.2] Let
denote the d-dimensional Lebesgue volume
of the compact convex set K.
[376.4.3] The volume is hence a functional Vd:K→R on K.
[376.4.4] An example of a compact convex
[page 377, §0]
set is the unit ball
Bd=x∈Rd:x≤1=Bd0,1
centered at the origin 0 whose volume is
[377.0.1] Other functionals on K can be constructed from the volume
by virtue of the following fact.
[377.0.2] For every compact convex K∈K and every
ε≥0 there are numbers VjK,j=0,…,d
depending only on K such that
VdK+εBd=∑j=0dVjKεd-jκd-j | | (5) |
is a polynomial in ε.
[377.0.3] This result is known as Steiners formula [16, 43].
[377.0.4] The numbers VjK,j=0…,d define functionals on
K similar to the volume VdK.
[377.0.5] The quantities
are called quermassintegrals [40].
[377.0.6] From (5) one sees that
limε→01εVdK+εBd-VdK=κ1Vd-1K, | | (7) |
and from (4) that κ1=2.
[377.0.7] Hence Vd-1K may be viewed as half the surface area.
[377.0.8] The functional V1K is related to the mean width wK
defined as the mean value of the distance between a pair of
parallel support planes of K.
[377.0.9]
The relation is
which reduces to V1K=wK/2 for d=3.
[377.0.10] Finally the functional V0K is evaluated from
(5) by dividing with εd and taking
the limit ε→∞.
[377.0.11] It follows that V0K=1 for all K∈K∖∅.
[377.0.12] One extends V0 to all of K by defining
V0∅=0.
[377.0.13] The geometric observable V0 is called Euler characteristic.
[377.1.1] The geometric observables Vi have several important properties.
[377.1.2] They are Euclidean invariant (i. e. invariant under rigid motions),
additive and monotone.
[377.1.3] Let Td≅(Rd,+) denote the group of translations with
vector addition as group operation and let SOd be
the matrix group of rotations in d dimensions [3].
[377.1.4] The semidirect product Ed=Td⊙SOd is the Euclidean
group of rigid motions in Rd.
[377.1.5] It is defined as the set of pairs a,A
with a∈Td and A∈SOd and group operation
[377.1.6] An observable f:K→R is called euclidean invariant
or invariant under rigid motions
if
[page 378, §0]
holds for all a,A∈Ed and all K∈K.
[378.0.1] Here AK=Ax:x∈K denotes the rotation
of K and a+K=a+K its translation.
[378.0.2] A geometric observable f is called additive
if
f∅ | =0 | | (11) |
fK1∪K2+fK1∩K2 | =fK1+fK2 | | (12) |
holds for all K1,K2∈K with K1∪K2∈K.
[378.0.3] Finally a functional is called monotone if for K1,K2∈K
with K1⊂K2 follows fK1≤fK2.
[378.1.1] The special importance of the functionals ViK arises from
the following theorem of Hadwiger [16].
[378.1.2] A functional f:K→R is euclidean invariant,
additive and monotone if and only if it is a linear
combination
with nonnegative constants c0,…,cd.
[378.1.3] The condition of monotonicity can be replaced with
continuity at the expense of allowing also negative ci,
and the theorem remains valid [16].
[378.1.4] If f is continuous on K, additive and euclidean invariant
it can be additively extended to the convex ring R [41].
[378.1.5] The additive extension is unique and given by the
inclusion-exclusion formula
f⋃i=1mK1=∑I∈Pm-1I-1f⋂i∈IKi | | (14) |
where Pm denotes the family of nonempty subsets
of 1,…,m and I is the number of elements
of I∈Pm.
[378.1.6] In particular, the functionals Vi have a unique additive extension
to the convex ring R[41], which is again be denoted by Vi.
[378.2.1] For a threedimensional porous sample with P∈R the extended
functionals Vi lead to two frequently used geometric observables.
[378.2.2] The first is the porosity of a porous sample S defined as
ϕP∩S=ϕ3P∩S=V3P∩SV3S, | | (15) |
and the second its specific internal surface area
which may be defined in view of (7) as
[378.2.3] The two remaining observables
ϕ1P∩S=V1P∩S/V3S and
ϕ0P∩S=V0P∩S/V3S have received less attention
in the porous media literature.
[378.2.4] The
[page 379, §0]
Euler characteristic V0 on R coincides with
the identically named topological invariant.
[379.0.1] For d=2 and G∈R one has
V0G=cG-c′G where cG is the number
of connectedness components of G, and c′G denotes
the number of holes (i. e. bounded connectedness components
of the complement).
3.3 Definition of Stochastic Porous Media
[379.1.1] For theoretical purposes the pore space P is frequently
viewed as a random set [43, 22].
[379.1.2] In practical applications the pore space is usually discretized
because of measurement limitations and finite resolution.
[379.1.3] For the purpose of discussion the set S⊂R3 is a
rectangular parallelepiped whose sidelengths are M1,M2
and M3 in units of the lattice constant a (resolution)
of a simple cubic lattice.
[379.1.4] The position vectors
ri=ri1…id=ai1,…,aid
with integers 1≤ij≤Mj are used to
label the lattice points, and ri
is a shorthand notation for ri1…id.
[379.1.5] Let Vi denote a cubic volume element (voxel)
centered at the lattice site ri.
[379.1.6] Then the discretized sample may be represented
as S=⋃i=1NVi.
[379.1.7] The discretized pore space P~, defined as
is an approximation to the true pore space P.
[379.1.8] For simplicity it will be assumed that the
discretization does not introduce errors,
i. e. that P~=P, and that
each voxel is either fully pore or fully matrix.
[379.1.9] This assumption may be relaxed to allow
voxel attributes such as internal surface or
other quermassintegral densities.
[379.1.10] The discretization into voxels reflects the limitations arising
from the experimental resolution of the porous structure.
[page 380, §0]
[380.0.1] A discretized pore space for a bounded sample belongs
to the convex ring R if the voxels are convex and
compact.
[380.0.2] Hence, for a simple cubic discretization the pore
space belongs to the convex ring.
[380.0.3] A configuration (or microstructure) Z of a
2-component medium may be represented
in the simplest case by a sequence
Z=Z1,…,ZN=χPr1,…,χPrN | | (18) |
where ri runs through the lattice points and N=M1M2M3.
[380.0.4] This representation corresponds to the simplest discretization
in which there are only two states for each voxel indicating
whether it belongs to pore space or not.
[380.0.5] In general a voxel could be characterized
by more states reflecting the microsctructure within
the region Vi.
[380.0.6] In the simplest case there is a one-to-one correspondence
between P and Z given by (18).
[380.0.7] Geometric observables fP then correspond to functions
fZ=fz1,…,zN.
[380.1.1] As a convenient theoretical idealization it is frequently
assumed that porous media are random realizations
drawn from an underlying statistical ensemble.
[380.1.2] A discretized stochastic porous medium is
defined through the discrete probability density
p(z1,…,zN)=Prob{(Z1=z1)∧…∧(ZN=zN)} | | (19) |
where zi∈0,1 in the simplest case.
[380.1.3] It should be emphasized that the probability density p
is mainly of theoretical interest.
[380.1.4] In practice p is usually not known.
[380.1.5] An infinitely extended medium or microstructure
is called stationary or
statistically homogeneous if p is invariant under
spatial translations.
[380.1.6] It is called isotropic if p is invariant under rotations.
3.4 Moment Functions and Correlation Functions
[380.2.1] A stochastic medium was defined through
its probability distribution p.
[380.2.2] In practice p will be even less accessible than the
microstructure P=Z itself.
[380.2.3] Partial information about p can be obtained
by measuring or calculating expectation values
of a geometric observable f. These are defined as
fz1,…,zN=∑z1=01…∑zN=01fz1,…,zNpz1,…,zN | | (20) |
where the summations indicate a summation over all configurations.
[380.2.4] Consider for example the porosity ϕS defined in (15).
[380.2.5] For a stochastic medium ϕS becomes a random variable.
[380.2.6] Its expectation is
ϕ | =V3PV3S=1V3S∫S⟨χP(r)⟩d3r | |
| =1V3S∑i=1N⟨zi⟩V3(Vi)=1N∑i=1N⟨zi⟩ | |
| =1N∑i=1NProb{zi=1}=1N∑i=1NProb{ri∈P}. | | (21) |
[380.2.7] If the medium is statistically homogeneous then
⟨ϕ⟩=Prob{zi=1}=Prob{ri∈P}=⟨χP(ri)⟩ | | (22) |
independent of i.
[380.2.8] It happens frequently that one is given only a single
sample, not an ensemble of samples.
[380.2.9] It is then necessary to invoke an ergodic hypothesis
that allows to equate spatial averages with ensemble
averages.
[380.3.1] The porosity is the first member in a hierarchy of
moment functions.
[380.3.2] The n-th order moment function is defined generally as
Snr1,…,rn=χPr1…χPrn | | (23) |
for n≤N.
[page 381, §0]
[381.0.1] For stationary media
Snr1,…rn=gr1-rn,…,rn-1-rn
where the function g depends only on n-1 variables.
[381.0.2] Another frequently used expectation value is the correlation function
which is related to S2.
[381.0.3] For a homogeneous medium it is defined as
Gr0,r=Gr-r0=χPr0χPr-ϕ2ϕ1-ϕ=S2r-r0-S1r02S1r01-S1r0 | | (24) |
where r0 is an arbitrary reference point, and ϕ=S1r0.
[381.0.4] If the medium is isotropic then Gr=Gr=Gr.
Note that G is normalized such that G0=1 and G∞=0.
[381.1.1] The hierarchy of moment functions Sn, similar to p,
is mainly of theoretical interest.
[381.1.2] For a homogeneous medium Sn is a function of n-1
variables.
[381.1.3] To specify Sn numerically becomes impractical
as n increases.
[381.1.4] If only 100 points are required along each coordinate axis
then giving Sn would require 102dn-1 numbers.
[381.1.5] For d=3 this implies that already at n=3 it becomes economical
to specify the microstructure P directly rather than
incompletely through moment or correlation functions.
3.5 Contact Distributions
[381.2.1] An interesting geometric characteristic introduced and
discussed in the field of stochastic geometry are
contact distributions [11, 43, p. 206].
[381.2.2] Certain special cases of contact distributions have appeared
also in the porous media literature [13].
[381.2.3] Let G be a compact test set containing the origin 0.
[381.2.4] Then the contact distribution is defined as the conditional
probability
HGr=1-Prob0∉M+-rG|0∉M=1-Prob{M∩rG=∅}ϕ. | | (25) |
[381.2.5] If one defines the random variable R=infs:M∩sG≠∅
then HGr=ProbR≤r|R>0 [43].
[381.3.1] For the unit ball G=B0,1 in three dimensions HB
is called spherical contact distribution.
[381.3.2] The quantity 1-HBr is then the distribution
function of the random distance from a randomly chosen
point in P to its nearest neighbour in M.
[381.3.3] The probability density
pr=ddr1-HBr=-ddrHBr | | (26) |
[page 382, §0]
was discussed in [39] as a well defined alternative
to the frequently used pore size distrubution from mercury
porosimetry.
[382.1.1] For an oriented unit interval G=B10,1;e
where e is the unit vector one obtains the linear
contact distribution.
[382.1.2] The linear contact distribution written as
Lre=ϕ1-HB10,1;er
is sometimes called lineal path function [48].
[382.1.3] It is related to the chord length distribution pclx
defined as the probability that an interval in the intersection
of P with a straight line containing B10,1;e
has length smaller than x [22, 43, p. 208].
3.6 Local Porosity Distributions
[382.2.1] The idea of local porosity distributions is to measure
geometric observables inside compact convex subsets
K⊂S, and to collect the results into empirical
histograms [19].
[382.2.2] Let Kr,L denote a cube of side length L centered at the
lattice vector r.
[382.2.3] The set Kr,L is called a measurement cell.
[382.2.4] A geometric observable f, when measured inside a measurement
cell Kr,L, is denoted as fr,L and called a local
observable.
[382.2.5] An example are local Hadwiger functional densities
f=∑i=0dciψi with coefficients ci
as in Hadwigers theorem (13).
[382.2.6] Here the local quermassintegrals are defined using
(6) as
ψiP∩Kr,L=WiP∩Kr,LVdKr,L | | (27) |
for i=0,…,d.
[382.2.7] In the following mainly the special case d=3 will be of interest.
[382.2.8] For d=3 the local porosity is defined by setting i=0,
Local densities of surface area, mean curvature and Euler
characteristic may be defined analogously.
[382.2.9] The local porosity distribution, defined as
gives the probability density to find a local porosity ϕr,L
in the measurement cell Kr,L.
[382.2.10] Here δx denotes the Dirac δ-distribution.
[382.2.11] The support of μ is the unit interval.
[382.2.12] For noncubic measurement cells K one defines
analogously μϕ;K=δϕ-ϕK where
ϕK=ϕP∩K is the local observable in cell K.
[382.3.1] The concept of local porosity distributions
was introduced in [19] and
has been generalized in two directions [22].
[382.3.2] Firstly by admitting more than one measurement cell,
and secondly by admitting more than one geometric observable.
[382.3.3] The general n-cell distribution function is defined as [22]
| μn;f1,…,fmf11,…,f1n;…;fm1,…,fmn;K1,…,Kn= | | (30) |
| δf11-f1K1…δf1n-f1Kn…δfm1-fmK1…δfmn-fmKn | |
[page 383, §0]
for n general measurement cells K1,…,Kn
and m observables f1,…,fm.
[383.0.1] The n-cell distribution is the probability density to find
the values f11 of the local observable f1 in cell
K1 and f12 in cell K2 and so on until fmn
of local observable fm in Kn.
[383.0.2] Definition (30) is a broad generalization
of (29).
[383.0.3] This generalization is not purely academic, but was
motivated by problems of fluid flow in porous media
where not only ψ0 but also ψ1 becomes
important [20].
[383.0.4] Local quermassintegrals, defined in (27),
and their linear combinations (Hadwiger functionals)
furnish important examples for local observables
in (30), and they have recently been measured
on real sandstone samples [28].
[383.1.1] The general n-cell distribution in (30) is very general indeed.
[383.1.2] It even contains p from
(19) as the special case m=1,f1=ϕ and n=N with
Ki=Vi=Kri,a.
More precisely one has
μN;ϕϕ1,…,ϕN;V1,…,VN=pϕ1,…,ϕN | | (31) |
because in that case ϕi=zi=1 if Vi∈P and
ϕi=zi=0 for V∉P.
[383.1.3] In this way it is seen that the very definition of a stochastic
geometry is related to local porosity distributions
(or more generally local geometry distributions).
[383.1.4] As a consequence the general n-cell distribution
μn;f1,…,fm is again mainly of theoretical
interest, and usually unavailable for practical computations.
[383.2.1] Expectation values with respect to p
have generalizations to averages with respect to μ.
[383.2.2] Averaging with respect to μ will be denoted by an overline.
[383.2.3] In the special case m=1,f1=ϕ and Ki=Vi=Kri,a
with n<N one finds [22]
ϕr1,a⋯ϕrn,a¯ | =∫01…∫01ϕ1⋯ϕnμn;ϕϕ1,…,ϕn;V1,…,Vndϕ1⋯dϕn | |
| =∫01…∫01ϕ1⋯ϕnμN;ϕϕ1,…,ϕN;V1,…,VNdϕ1⋯dϕN | |
| =∫01…∫01ϕ1⋯ϕnδϕ1-ϕr1,a⋯δϕN-ϕrN,adϕ1⋯dϕN | |
| =ϕr1,a⋯ϕrn,a | |
| =χPr1…χPrn | |
| =Snr1,…,rn | | (32) |
thereby identifying the moment functions of order n
as averages with respect to an n-cell distribution.
[383.3.1] For practical applications the 1-cell local porosity
distributions μr,L and their analogues for other
quermassintegrals are of greatest interest.
[383.3.2] For a homogeneous medium the local porosity distribution obeys
μϕ;r,L=μϕ;0,L=μϕ;L | | (33) |
[page 384, §0]
for all lattice vectors r, i. e. it is independent of
the placement of the measurement cell.
[384.0.1] A disordered medium with substitutional disorder [49]
may be viewed as a stochastic geometry obtained by placing
random elements at the cells or sites of a fixed regular
substitution lattice.
[384.0.2] For a substitutionally disordered medium
the local porosity distribution μr,L
is a periodic function of r whose
period is the lattice constant of the substitution
lattice.
[384.0.3] For stereological issues in the measurement of μ
from thin sections see [45].
[384.1.1] Averages with respect to μ are denoted by an overline.
[384.1.2] For a homogeneous medium the average local porosity is found as
ϕ¯r,L=∫01μϕ;r,Ldϕ=ϕ=ϕ¯ | | (34) |
independent of r and L.
[384.1.3] The variance of local porosities for a homogeneous medium
defined in the first equality
σ2L=ϕL-ϕ¯2¯=∫01ϕL-ϕ¯2μϕ;Ldϕ=1L3ϕ1-ϕ1+2L3∑ri,rj∈Kr0,Li≠jGri-rj | | (35) |
is related to the correlation function as given in the
second equality [22].
[384.1.4] The skewness of the local porosity distribution is defined
as the average
[384.2.1] The limits L→0 and L→∞ of small and large
measurement cells are of special interest.
[384.2.2] In the first case one reaches the limiting resolution
at L=a and finds for a homogeneous medium [19, 22]
μϕ;a=ϕ¯δϕ-1-1-ϕ¯δϕ. | | (37) |
[384.2.3] The limit L→∞ is more intricate because it requires
also the limit S→R3.
[384.2.4] For a homogeneous medium (35)
shows σL→0 for L→0 and this suggests
[384.2.5] For macroscopically heterogeneous media, however,
the limiting distribution may deviate from this result
[22].
[384.2.6] If (38) holds then in both limits the geometrical
information contained in μ reduces to the single number
ϕ¯=ϕ.
[384.2.7] If (37) and (38) hold there exists a special
length scale L* defined as
L*=minL:μ0;L=μ1;L=0 | | (39) |
[page 385, §0]
at which the δ-components at ϕ=0 and ϕ=1
vanish.
[385.0.1] The length L* is a measure for
the size of pores.
[385.1.1] The ensemble picture underlying the definition of a stochastic
medium is an idealization.
[385.1.2] In practice one is given only a single realization and has
to resort to an ergodic hypothesis for obtaining an estimate
of the local porosity distributions.
[385.1.3] The local porosity distribution may then be estimated by
μ~ϕ;L=1m∑rδϕ-ϕr,L | | (40) |
where m is the number of placements of the measurement
cell Kr,L.
[385.1.4] Ideally the measurement cells should be far apart or at
least nonoverlapping, but in practice this restriction
cannot be observed because the samples are not large enough.
[385.1.5] The use of μ~ instead of μ can lead to deviations due to
violations of the ergodic hypothesis or simply due to oversampling
the central regions of S [6, 7].
3.7 Local Percolation Probabilities
[385.2.1] Transport and propagation in porous media are controlled
by the connectivity of the pore space.
[385.2.2] Local percolation probabilities characterize the connectivity
[19].
[385.2.3] Their calculation requires a threedimensional pore space
representation, and early results were restricted to samples
reconstructed laboriously from sequential thin sectioning [24].
[385.2.4] In this section a relationship between the Euler characteristic
and the local percolation probabililties is established for the
first time.
[385.3.1] Consider the functional Λ:K×K×R→Z2=0,1
defined by
ΛK0,K∞;P∩S=1: if K0↝K∞ in P0: otherwise | | (41) |
where K0⊂R3,K∞⊂R3 are two compact
convex sets with K0∩P∩S≠∅ and
K∞∩P∩S≠∅,
and “K0↝K∞ in P” means that
there is a path connecting K0 and K∞ that lies
completely in P.
[385.3.2] In the examples below the sets K0 and K∞ correspond to
opposite faces of the sample, but in general other choices
are allowed.
[385.3.3] Analogous to Λ, which is defined for the whole sample, one defines
for a measurement cell
Λαr,L=ΛK0α,K∞α;P∩Kr,L=1: if K0α↝K∞α in P0: otherwise | | (42) |
where α=x,y,z and K0x,K∞x denote those two faces of
Kr,L that are normal to the x direction.
[385.3.4] Similarly K0y,K∞y,K0zK∞z denote the faces of Kr,L
normal to the y- and z-directions.
[385.3.5] Two additional percolation observables Λ3 and Λc
are introduced by
| Λ3r,L=Λxr,LΛyr,LΛzr,L | | (43) |
| Λcr,L=sgnΛxr,L+Λyr,L+Λzr,L. | | (44) |
[page 386, §0]
Λ3 indicates that the cell is percolating in
all three directions while Λc indicates
percolation in x- or y- or z-direction.
[386.0.1] The local percolation probabilities are defined as
λαϕ;L=∑rΛαr,Lδϕ,ϕr,L∑rδϕ,ϕr,L | | (45) |
where
δϕ,ϕr,L=1: if ϕ=ϕr,L0: otherwise. | | (46) |
[386.0.2] The local percolation probability λαϕ;L gives
the fraction of measurement cells of sidelength L with
local porosity ϕ that are percolating in the “α”-direction.
[386.0.3] The total fraction of cells percolating along the “α”-direction
is then obtained by integration
pαL=∫01μϕ;Lλαϕ;Ldϕ. | | (47) |
[386.0.4] This geometric observable is a quantitative measure for the number
of elements that have to be percolating if the pore
space geometry is approximated by a substitutionally
disordered lattice or network model.
[386.0.5] Note that neither Λ nor Λα are additive
functionals, and hence local percolation probabilities
are not covered by Hadwigers theorem.
[386.1.1] It is interesting that there is a relation between
the local percolation probabilities and the local Euler
characteristic V0P∩Kr,l.
[386.1.2] The relation arises from the observation that the voxels
Vi are closed, convex sets, and hence for any two voxels
Vi,Vj the Euler characteristic of their intersection
V0Vi∩Vj=1: if Vi∩Vj≠∅0: if Vi∩Vj=∅ | | (48) |
indicates whether two voxels are nearest neighbours.
[386.1.3] A measurement cell Kr,L contains L3 voxels.
[386.1.4] It is then possible to construct a L3+2×L3+22-matrix
B with matrix elements
Bii,j | =V0Vi∩Vj | | (49) |
Bij,i | =-V0Vi∩Vj | | (50) |
where i,j∈0,1,…,L3,∞ and the
sets V0=K0 and V∞=K∞ are two opposite
faces of the measurement cell.
[386.1.5] The rows in the matrix B correspond to voxels while
the columns correspond to voxel pairs.
[386.1.6] Define the matrix A=BBT
[page 387, §0]
where BT is the transpose of B.
[387.0.1] The diagonal elements Aii give the number of
voxels to which the voxel Vi is connected.
[387.0.2] A matrix element Aij differs from zero
if and only if Vi and Vj are connected.
[387.0.3] Hence the matrix A reflects the local
connectedness of the pore space around a single voxel.
[387.0.4] Sufficiently high powers of A provide information about the global
connectedness of P.
[387.0.5] One finds
ΛK0,K∞;P∩Kr,L=sgnAm0∞ | | (51) |
where Am0∞ is the matrix element in the upper right
hand corner and m is arbitrary subject to the condition m>L3.
[387.0.6] The set P∩Kr,L can always be decomposed uniquely
into pairwise disjoint connectedness components (clusters)
Bi whose number is given by the rank of B.
[387.0.7] Hence
V0P∩Kr,L=∑i=1rankBV0Bi | | (52) |
provides an indirect connection between the local
Euler characteristic and the local percolation probabilities
mediated by the matrix B.
)
[387.1.1] The theoretical concepts for the geometric characterization
of porous media discussed here are also useful in effective
medium calculations of transport parameters such as conductivity
or permeability [19, 20, 22].
[387.1.2] The resulting parameterfree predictions agree well with
the exact result [46, 47].