Stroke. 1996;27:1072-1083
(Stroke. 1996;27:1072-1083.)
© 1996 American Heart Association, Inc.
Risk of Intracranial Arteriovenous Malformation Rupture Due to Venous Drainage Impairment
A Theoretical Analysis
George J. Hademenos, PhD
Tarik F. Massoud, MD
From the Endovascular Therapy Service, Department of Radiological
Sciences, University of California at Los Angeles School of Medicine.
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Abstract
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Background and Purpose Increased resistance in the
venous drainage
of intracranial arteriovenous malformations (AVMs) may
contribute
to their increased risk of hemorrhage. Venous
drainage impairment
may result from naturally occurring
stenoses/occlusions, or
if draining veins (DVs) undergo
occlusion before feeding arteries
during surgical removal, or after
surgery in the presence of
"occlusive hyperemia." We
employed a detailed biomathematical
AVM model using electrical network
analysis to investigate theoretically
the
hemodynamic consequences and the risk of AVM rupture
due
to venous drainage impairment.
Methods The AVM model consisted of a noncompartmentalized
nidus with 28 vessels (24 plexiform components and 4 fistulous
components), 4 arterial feeders, and 2 DVs. An expression
for the risk of AVM nidus rupture was derived on the basis of
functional distribution of the critical radii of component vessels.
Risk was calculated from biomathematical simulations of volumetric flow
rate with both DVs patent and for four stages of venous drainage
obstruction: (1) 25%, (2) 50%, (3) 75%, and (4) 100%. Each stage of
occlusion was applied to each DV while the other DV was patent and then
to the patent DV while the other DV was totally occluded.
Results For flow through the AVM when both DVs were
unobstructed, the baseline risk of AVM nidus rupture ranged from 4.4%
to 91.2%. Theoretical rupture occurred in nidus components proximal to
the DVs when the risk exceeded 100%, as was observed with the
obstruction of DV1 and a patent DV2. The ranges for risk of rupture
across the nidus for the four stages were (1) 4.7% to 90.5%, (2)
5.9% to 86.9%, (3) 0% to 98.4%, and (4) 0% to 106.3%,
respectively. Rupture was observed for an 86% occlusion of DV1 (ie,
the DV fed by the intranidal fistula) and DV2 patent, primarily because
of the dramatic shift in the hemodynamic burden toward
the weaker plexiform nidus vessels.
Conclusions On theoretical grounds, venous drainage
impairment was predictive of AVM nidus rupture and was strongly
dependent on AVM morphology (presence of intranidal fistulas and their
spatial relation to DVs) and hemodynamics.
Specifically, stenosis/occlusion of a high-flow DV induces
a rapid redistribution of blood into the weak plexiform vessels of the
opposing region of the nidus, causing a hemodynamic
overload and an increased risk of rupture. These findings should be
carefully considered among all factors affecting the natural history of
intracranial AVMs and the mechanisms implicated in their spontaneous
rupture. They may also provide a theoretical rationale for some of the
hemorrhagic complications that occur during and after surgical
treatment.
Key Words: cerebral arteriovenous malformations cerebral hemorrhage hemodynamics models, theoretical
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Introduction
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Preoperative evaluation
and management of intracranial AVMs
are based primarily on the natural
history, diagnostic presentation
and interpretation, and clinical
status of the patient.
1 Because
the majority of AVMs are
symptomatic lesions,
2 an aggressive
therapeutic approach
should be implemented on diagnosis. Attempts
to accurately assess nidus
stability and risk of impending rupture
have been proposed on the basis
of a number of factors such
as perfusion arterial
pressure,
3 4 nidus size,
5 intranidal
aneurysms,
6 7 8 angioarchitecture,
9 10 11 12 and
other structural characteristics,
including morphological and
hemodynamic features of their DVs.
13 14 15 16
The influence of venous drainage impairment as seen in clinical
observations, ie, the presence of stenosis or occlusion, on the risk of
spontaneous AVM rupture has been controversial.17 18 19
Although factors such as type of venous drainage (central, peripheral,
or mixed) and number and IVP of the DVs have been studied, the
influence of venous drainage impairment and the resultant altered
hemodynamics on the risk of nidus hemorrhage have not been investigated
adequately. Venous drainage impairment has been described as the
"most critical determinant of what happens within and surrounding an
AVM nidus."20 It thus becomes important to
qualitatively and quantitatively assess intranidal hemodynamics in
relation to venous drainage impairment.
One method of theoretical investigation of intranidal hemodynamics of
an AVM involves the use of biomathematical models.21 22 23 24
This technique may be extended to assess the intranidal stability and
risk of AVM rupture as a direct result of venous drainage impairment.
In this article, a novel biomathematical model of a normal intracranial
AVM based on network analysis was used to quantify and visualize
hemodynamic processes within the nidus after simulated venous drainage
impairment. The observed hemodynamic parameters, combined with
biomechanical, anatomic, and histopathological information of the
involved vessels, were then used to theoretically determine the
intranidal stability and predict risk of hemorrhage of the AVM, as may
occur either spontaneously or during/after surgical treatment of human
AVMs.
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Materials and Methods
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A Biomathematical Model of an AVM
A biomathematical model based on network
analysis
25 26 27 was
used to qualitatively and
quantitatively investigate the altered
hemodynamics of
venous drainage impairment of an intracranial
AVM and the corresponding
risk of hemorrhage. The details of
this AVM model are described
elsewhere.
28 In brief, the AVM
network, nestled within a
simulated circulatory network of the
head and neck, consisted of four
AFs, two DVs, and a nidal angioarchitecture
with a randomly distributed
array of 28 interconnected plexiform
and fistulous components, as shown
in Fig 1

. This structure
of the AVM model was developed
to accurately characterize anatomic
landmarks and features clinically
observed in human AVMs. Twenty-four
of the nidus vessels were
plexiform, and four nidus vessels
were fistulous. The plexiform vessels
were held constant at
a length of 2.0 cm and a radius of 0.05
cm,
29 whereas the length
and radius of the fistulous
components were 4.0 cm and 0.10
cm, respectively. Two AFs (AF1 and AF2)
were considered major
feeders, and AF3 and AF4 (a simulated transdural
supply) were
minor feeders. Both DVs drained into the intracranial
venous
sinuses.

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Figure 1. Schematic diagram of the electrical network
describing the biomathematical AVM hemodynamic model. CCA indicates
common carotid artery; ECA, external carotid artery; ICA, internal
carotid artery; SCA, subclavian artery; VA, vertebral artery; PCA,
posterior cerebral artery; ACA, anterior cerebral artery; MCA, middle
cerebral artery; E, electromotive force; N, node; and L, loop. The
fistulous vessels are designated by the following components of the
circuit: i13, i18, i25, and
i36. Reproduced with permission.28
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The hemodynamics within an AVM can be described by
Poiseuille's formula:
 | (1) |
where Q is the volumetric flow rate,

P is the
pressure
gradient, R is the inner radius of the vessel, L is the length
of
the vessel, and

is the blood viscosity (

=3.5 cp). Equation
1

can be further simplified as
 | (2) |
where R
v is the vascular
resistance
by the vascular bed given by
 | (3) |
To determine
the hemodynamic
quantities within each vessel of the vascular
array from a simulation,
network analysis of the loops and nodes
constituting the AVM
model circuit was performed to yield 41
linear equations corresponding
to the 41 vessels and distinct
values of volumetric flow rate. The 41
derived linear equations
were solved simultaneously by
expanding Equation 2

into matrix
form. The matrices corresponding to
pressure and resistance
were created using a spreadsheet application
(Microsoft Excel)
and transported to an advanced mathematical
computation program
(Mathematica) for solution of the flow rate values
for all 41
vessels.
Once the volumetric flow rate (Q) was determined for each simulation,
it was then possible to calculate other hemodynamic
parameters such as IVP gradient ([
P]nv)
and biomechanical stress (S). Using the resistance for each nidus
vessel, the IVP gradient was quantified according to
(
P)nv=(Q)nv(Rv)nv,
where nv refers to the particular nidus vessel. The IVP gradient was
used to calculate the biomechanical stress from the relation S=
P
R/t, where R is the radius of the vessel and t is the vessel wall
thickness.
DV Occlusion Schemes
The occlusion schemes adopted for the AVM simulations consisted
of systematic impairment of the DVs, assuming underlying normal flow
through a normal AVM nidus. Hemodynamic characteristics
were first assessed through the AVM with both DVs patent. After this
normal simulation, four sets of hemodynamic simulations
were performed for various stages of venous drainage impairment. In the
first set, with DV2 fully patent, hemodynamic
simulations were performed with the progressive occlusion of DV1 by
25%, 50%, 75%, and 100%. Each simulation is described in Fig 2
, with corresponding circles denoting the stage of
occlusion for each DV. The shaded portion of the DV refers to vessel
occlusion, and the unshaded area refers to vessel patency. Each stage
of occlusion was represented by its calculated value of
resistance with the exception of 100%. Total occlusion of a vessel
corresponded to an infinite resistance and was represented
in the calculations by the largest value of resistance that could be
registered in its corresponding cell of the matrix. The second set of
simulations involved keeping DV1 fully patent and performing similar
simulations for DV2. In the third set, DV1 was 100% occluded and DV2
was occluded systematically by 25%, 50%, 75%, and 100%; the final
set consisted of hemodynamic simulations with DV2
totally occluded and DV1 progressively occluded by 25%, 50%, 75%,
and 100%.

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Figure 2. Tabular description of the state of venous drainage
occlusion for each simulation. Shaded area of the circles
representing the DVs corresponds to vessel occlusion, and
the unshaded area corresponds to vessel patency. The value ranges for
the risk of rupture correspond to those seen in all nidus vessels of
the AVM. Risk values 100% represent nidus rupture.
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Risk of AVM Hemorrhage
The highly tortuous, structurally weak intranidal vessels
coupled with the continual impingement of large
hemodynamic forces make the AVM highly susceptible to
hemorrhage. The precise location or region of rupture is
extremely difficult to observe angiographically and to detect
histologically, and it remains a source of speculation
in the assessment of AVMs. It is commonly believed that, on the basis
of biomechanical properties of the intranidal vessels, rupture occurs
when the cumulative hemodynamic stresses of the vessel
wall exceed its elastic modulus.
In static equilibrium, the distribution of forces acting on the
cylindrical vessel can be explained by Laplace's law. In effect,
Laplace's law equates a radial force, P, produced by the transmural
blood pressure over the cross-sectional area of the lumen, which
distends it to a circumferential force, T, that compensates for the
distension. In mathematical form, Laplace's law for a cylinder is
 | (4) |
where R is the radius
of curvature. The stress within the vessel
wall can be determined
by
 | (5) |
where t is the wall thickness. Equation 5

is only
valid,
however, for thin-walled vessels, ie, t

R. On the basis
of
biomechanical reasoning, a relation most likely exists between
the wall
thickness and radius of the vessel, eg, wall thickness
decreases for a
corresponding increase in radius. The exact
relation is unknown and,
therefore, in this study, has been
approximated by a fixed value. The
integral factors that influence
the wall stress can be shown by taking
the differential of Equation
5

:
 | (6) |
The circumferential wall stress, given in Equation
5

, can also
be expressed as
 | (7) |
where

is the circumferential
strain and E is the elastic
modulus of the vessel under physiological
conditions.
The circumferential strain can be expressed as the ratio

R/R,
where

R is the change in radial length between the relaxed
and
strained states and R is the radial length in the unstrained
state.
Assuming that changes in the radial length are infinitesimal,
Equation 7

can be expressed in differential form as
 | (8) |
equating
Equations 6 and 8 as
 | (9) |
The condition of vessel rupture
or blowout can be derived by
determining the differential relation
between the radius and pressure:
dR/dP. Dividing both sides
of Equation 9

by dP and solving for dR/dP,
 | (10) |
Expressing
Equation 10

in terms of volume can be accomplished by
 | (11) |
where
dV/dP is referred to as volume distensibility and V is the
volume
of a cylinder (

R
2L). Thus,
or
 | (12) |
Assuming that E is
constant, the rate of volume expansion will
continually increase
with increasing pressure to the state where
E/R=P/t. Solving
for R yields the critical radius,
R
c,
 | (13) |
Equation 13

describes
the critical radius of the blood vessel.
Any increase or decrease
in the state variables that would upset
this equality could
possibly induce rupture. Evaluation of the risk of
rupture is
based on the functional distribution of the critical radius
with
respect to the theoretical blood pressure extremes encountered
by
the nidus and is given by
 | (14) |
where Pmin and Pmax are the CVP and the
"maximum intranidal pressure," respectively, and Pexp
is the pressure of the nidus vessel determined at simulation. In this
study, Pmin=6.6x103 dyne/cm2
(equivalent to a CVP of 5 mm Hg). The upper limit of
arterial pressure experienced by the nidus microvessels
before rupture is likely to occur during considerable systemic
hypertension (ie, blood pressure that is then transmitted to the AFs
and the nidus). It has been observed that systemic hypertension to a
mean value of 118 mm Hg does not precipitate AVM
hemorrhage.4 The influence of higher levels of
systemic hypertension on the propensity of AVMs to rupture is unknown.
Therefore, in our calculations it is assumed that the normally
low-pressure AFs may reach a maximum value of 74 mm Hg during mean
systemic hypertensive levels of 118 mm Hg (derived by assuming a linear
relationship between these two parameters30 ).
Therefore, 74 mm Hg (equivalent to 9.8x104
dyne/cm2) was chosen as the upper limit of blood pressure
(Pmax) possibly encountered by nidus vessels before
rupture. This value of pressure is acknowledged as a conservative
estimate, since it has not been observed clinically or determined
experimentally. In reality, selection of this pressure value is of
secondary importance for the risk calculations because this does not
affect the principles conveyed by our theoretical study. We consider
the value of 74 mm Hg to be an adequate approximation for the purpose
of our calculations. It is noted that maximal AF pressures obtained by
Young et al30 on systemic hypertensive challenges reached
values close to 74 mm Hg.
Because the variables E and t cannot be determined quantitatively
from in vivo imaging techniques, they are assumed constant and factored
from the equation for risk of rupture. Evaluation of Equation 14
yields
the following expression for risk of AVM nidus rupture:
 | (15) |
The expression given in Equation 15

represents the
normalized
probability or risk of rupture and is multiplied by 100% to
present
the results as a percentage of risk of rupture. The
denominator
or normalization constant is the integrated distribution of
critical
radii for the maximum possible transnidal pressure gradient.
It
can be seen that, on a qualitative basis, as the IVP of the
nidus
vessels reaches that of the "maximum intranidal pressure,"
the
risk of rupture approaches 100%, implying certain rupture.
Conversely,
for IVPs closer to that of CVP, the risk of rupture
decreases
accordingly. Fig 3

shows the influence of intranidal
vessel
pressure on the risk of rupture. Risk of rupture is lowest at
values
closest to those of CVP and increases in an exponential fashion
to
a maximum value at pressures equal to or greater than the maximum
intranidal
pressure.
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Results
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The range of risk of rupture for all nidus vessels during all
simulations
are displayed in Fig 2

. The wide range of values observed
for
each simulation is a reflection on the high variability of risk
within
the multitude of interconnected nidus vessels. The upper limit
of
each range is of paramount importance because, should this risk
value
exceed 100%, then the whole nidus is deemed to have ruptured.
Fig 4
displays the results of the
hemodynamic simulations with the AVM in its normal
state, ie, both DVs patent. Fig 5
depicts the IVP
gradient, biomechanical stress, and risk of rupture displayed in each
column occurring as a result of the systematic occlusion of DV1 with
DV2 patent displayed according to row. This particular series of
simulations was chosen for graphical display primarily because of the
dramatic hemodynamic effects induced by the occlusion
of the DV fed by the fistulous component. The
hemodynamic results from the AVM simulations
presented in Figs 4
and 5
show the individual values of IVP
gradient, biomechanical stress, and risk of rupture within each nidus
vessel mapped onto the AVM model network. In addition, regions or areas
of abnormal hemodynamics induced by the systematic
occlusion of the DVs can readily be observed. For example, in the case
of normal flow through the AVM shown in Fig 4
, one would expect values
of low pressure, biomechanical stress, and risk of rupture within the
plexiform vessels of the nidus. Conversely, high values of pressure
gradient, biomechanical stress, and risk of rupture would be expected
through the fistulous component of the nidus. For the venous occlusion
simulations represented in Fig 5
, a region of low
hemodynamic significance can be seen in the immediate
area of the minor AFs, since they are small contributors of blood flow
to the AVM. This region is generally consistent throughout all
simulations and all stages of occlusion. In contrast, a region of high
hemodynamic values can be seen around DV1 where the
fistula makes a direct connection. As one DV becomes occluded, the
nidus vessels constituting the opposite side of the nidus compensate
with increasing hemodynamic values. As DV1 becomes
occluded, IVP in the upper portion of the nidus increases in response.
The same behavior is observed in the occlusion of DV2 with DV1 patent.

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Figure 4. Schematic diagram of the nidus portion of the
biomathematical AVM model depicting the intranidal values of IVP
gradient (A), biomechanical stress (B), and risk of rupture (C) with
both DVs patent (simulation 1).
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Figure 5. (facing page). Schematic diagram of the nidus portion
of the biomathematical AVM model depicting the intranidal values of IVP
gradient (A), biomechanical stress (B), and risk of rupture (C) with
DV1 occluded 25%, 50%, 75%, and 100% and DV2 patent. The numbers
along the left-hand column refer to the simulation
numbers.
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Simulation series A (consisting of simulations 2 through 5 and 10
through 13) and series B (consisting of simulations 6 through 9 and 14
through 17) represent a continuous series of systematic venous
drainage occlusion in which series A begins with the occlusion of DV1
(simulations 2 through 5) followed by the occlusion of DV2 with DV1
totally occluded (simulations 10 through 13), and series B begins with
the occlusion of DV2 (simulations 6 through 9) followed by the
occlusion of DV1 with DV2 totally occluded (simulations 14 through 17).
Each simulation and its corresponding range of risk of rupture values
are summarized in Fig 2
. Fig 6
shows the variation of
the IVP gradient, biomechanical stress, and risk of rupture for each
AVM nidus vessel with respect to stage of occlusion for the systematic
impairment of DV1 with a patent DV2, represented by
simulations 2 through 5. This set of simulations was chosen for display
in Fig 6
because of the definitive observation of AVM rupture. In Fig 6
, increases in pressure gradient, biomechanical stress, and risk of
rupture are observed at the nidus vessels in close proximity to the DVs
and, on a much smaller scale, at nidus vessels near the major AFs (AF1
and AF2). In fact, at 100% occlusion of DV1, rupture was shown to
occur at nidus vessel 34. Decreases in pressure gradient, biomechanical
stress, and risk of rupture are noted at the nidus vessels near the
minor AFs (AF3 and AF4) and the vessels composing the central core or
region of the AVM nidus. In comparison with the results in Fig 6
,
similar trends in the hemodynamic values are observed
in the remaining set of simulations in series A, with increases in the
nidus vessels near the DVs and rupture continuing to be seen in nidus
vessel 34. In contrast to DV1, occlusion of DV2 produces relatively
minor increases of pressure gradient, biomechanical stress, and risk of
rupture at the nidus vessels closest to the DVs, with little to no
decrease in parameters elsewhere. The pressure gradient,
biomechanical stress, and risk of rupture revealed a gradual increase
in the nidus vessels directly connected to the venous drainage (DV1 and
DV2). Risk of rupture in nidus vessel 35 increases to approximately
88.7%, whereas the risk in nidus vessel 37 remains at 91.4% before
reaching a plateau, even throughout total occlusion of DV1, before
sharply decreasing to zero for both DVs occluded. For both DV1 and DV2
totally occluded, the pressure gradient, biomechanical stress, and risk
of rupture dropped dramatically to extremely low values, presumably
because of a theoretical stagnant flow through the nidus; however,
nidus rupture occurs before this possibility.

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Figure 6. Three-dimensional line graphs showing the
variation of the intranidal values of IVP gradient (A), biomechanical
stress (B), and risk of rupture (C) for each AVM nidus vessel with DV1
occluded 0%, 25%, 50%, 75%, and 100% and DV2 patent.
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The critical value of stenosis is defined in the literature as
the degree of occlusion that shows a pronounced decrease in flow. To
elucidate the critical value of stenosis at which this drop in
flow occurs and reasons for a substantial decrease in risk of rupture
for total occlusion of both DVs, the risk of rupture was plotted
against stage of occlusion for the six nidus vessels adjoining the DVs
(nidus vessels 32 through 37) for series A and is presented in
Fig 7
. The risk of rupture for the only ruptured nidus
vessel (nidus vessel 34) exceeded 100% with the combination of 80%
occlusion of DV1 and DV2 patent (point 1) and remains high before
decreasing and reaching 100% on the opposing end of this range (point
2) at the combination of 62.5% occlusion of DV2 and DV1
totally occluded. Points 1 and 2 are represented in Fig 7
by the line segments bisecting the line at 100% risk of rupture. These
values for stage of occlusion were obtained by extrapolating from the
points defining the above range downward to the x axis. The
risk of rupture past this range sharply decreases to values of 0%.
Thus, the range of critical venous drainage impairment (causing
rupture) for this specific AVM model occurs as a result of combinations
that yield 80% to 100% stenosis in DV1 plus 0% to 62.5%
stenosis in DV2 (ie, higher stenoses or even occlusion
in DV1 are poorly tolerated by the nidus and thus induce
rupture).

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Figure 7. Graph showing the variation of risk of rupture for
the nidus vessels adjacent to the DVs (nidus vessels 32, 33, 34, 35,
36, and 37) over the gradual stages of occlusion in which DV1 is
occluded before DV2.
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Discussion
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Venous Drainage Impairment
Several studies over the last decade have brought attention
to the
possibility that characteristics of venous drainage in
cerebral AVMs
may be important factors in the pathophysiology
of spontaneous nidus
rupture.
13 15 19 31 However, not all are
in agreement
regarding the role of venous factors in the generation
of AVM
hemorrhage, and this topic remains controversial. Other
recent
accounts suggest that the importance of the venous system
in the
natural history of cerebral AVMs may have been
overstated.
32 In this study, we have adopted a novel
biomathematical AVM
model for further theoretical characterization and
study of
the influences of venous drainage impairment on an adjacent
AVM
nidus, particularly in relation to its consequent risk of rupture.
Characteristics of venous drainage that have been reported previously
to influence the risk of spontaneous AVM nidus rupture include (1)
venous drainage impairment (stenosis or occlusion of DVs), (2)
number of DVs, (3) the location of DVs (deep, superficial, or a
combination of both), and (4) the presence of venous aneurysms
or varices. The role of the number of veins draining an AVM in relation
to the risk of nidus rupture remains unclear, with conflicting accounts
in the literature.11 13 14 31 In our theoretical
analysis, we chose not to investigate the effect of varying the
number of DVs because this would have also added considerably to the
complexity and number of the AVM models required and the mathematical
calculations entailed. This important analysis will
nevertheless be the subject of a future communication. Regarding the
location of the DVs, previous results indicate that despite the high
improbability that the hemodynamics of deep venous
drainage are significantly different from that of more superficial
drainage,33 there may be a higher risk of bleeding from
AVMs with deep venous drainage.10 14 These factors cannot
be examined using our model until the data resulting from direct
intraoperative or endovascular pressure sampling of both superficial
and deep veins become available.
Venous drainage impairment results from stenoses or occlusions
in the veins draining an AVM. Previously, a stenosis has been
considered to be a reduction of greater than 50%15 31 or
greater than three fifths34 of any AVM DV in two
angiographic views. Because of this nonuniform definition of a venous
stenosis, we investigated the effects of various (0% to 100%)
degrees of narrowing in the DVs on the risk of nidus rupture.
Stenoses are most often seen at the junction of major DVs as
they enter a dural sinus, eg, at the junction of the vein of Galen and
the straight sinus or the junction of a cortical vein with the superior
sagittal sinus.31 Complete obliteration of the galenic
system was also observed by Viñuela et al19 in 10
patients with AVMs. The exact etiology of a venous
stenosis/occlusion is unclear, although several suggestions
have been made. Albert et al13 have explained these
stenoses as mere common variations in the width of veins or as
a consequence of radiographic projection. Local damage
to the venous endothelium due to turbulent flow has
been proposed by Viñuela et al19 on the basis of
previous observations by Fry35 that such intimal damage
results from the mechanical action of pressure and shearing stress on
the endothelial surface and the change in the
electrochemical characteristics of the endothelial
membrane produced by convective properties of flow. This may result in
subsequent thrombosis and luminal narrowing. Quisling and
Mickle36 suggested that some instances of venous narrowing
may not be rigidly atretic or fibrotic but rather represent a
vasoconstrictive response to increased shunt volume or
elevated venous pressure; it is known, for instance, that cerebral
veins possess both myogenic and neurogenic
vasoconstrictive properties.37 Willinsky
et al12 have also postulated that mechanical kinking of
veins at the edge of the tentorium may be one of the precipitating
factors in the high incidence of hemorrhage from temporal and
posterior fossa AVMs.
The site of a typical AVM rupture has never been demonstrated
histologically but has been postulated to occur at the
venous end of the nidus.20 The mechanisms responsible for
this in the presence of venous drainage impairment have been thought to
occur because of retrograde venous hypertension yielding regional
intranidal hypertension with consequent rupture of delicate AVM
vessels.9 19 The presence of significant
prestenotic DV hypertension has been confirmed by Miyasaka
et al16 during intraoperative measurements in three
patients with marked segmental stenoses and a history of AVM
rupture. They found an average prestenotic mean pressure of
34 mm Hg (ie, considerably above normal cortical pressures and normal
AVM DV pressures28 ), whereas pressure measurements in
poststenotic sites approached normal values. From a
clinical standpoint, however, conflicting results are available
regarding the association of venous drainage impairment and a history
of hemorrhage in patients harboring AVMs. Thus, in four
series,15 18 19 31 hemorrhage was found to occur
in 48% to 94% of AVMs with venous drainage impairment. Willinsky et
al12 found that 52% of patients with AVM
hemorrhage had venous stenosis. Young et
al,30 on the other hand, found no relationship between
venous factors and AVM hemorrhage. Similarly, Patel et
al18 showed no clear evidence that venous restrictive
changes promote hemorrhage. Our own recent experience in
correlating angioarchitectural features of cerebral AVMs with a
clinical presentation of intracranial hemorrhage
has demonstrated no significant association between the presence of
venous drainage impairment and nidus rupture: stenosis was
present in 25 of 40 patients (62%) with AVM hemorrhage
versus 33 of 60 patients (55%) without AVM
hemorrhage.11
Risk of AVM Nidus Rupture
To adequately and properly investigate the previously mentioned
conflicting clinical observations, a biomathematical AVM model was used
to theoretically study the changes in AVM intranidal
hemodynamics in response to progressive occlusion of
its DVs. In addition, the risk of AVM nidus rupture was determined on
the basis of the critical radii of intranidal microvessels. With use of
a biomathematical model of an AVM, the results of theoretical
simulations are well within expected values from clinical observations
and biophysical principles. However, there are several issues involving
the AVM model that bear further discussion.
The expression for the risk of rupture used in this research is based
on the transnidal distribution of pressure and normalized to the
pressure gradient between Pmax (maximum intranidal
pressure) and Pmin (CVP). One could raise the following
questions: (1) Is pressure the sole variable responsible for risk
of rupture? and (2) Why is the risk of rupture normalized to a pressure
gradient spanning the two extremes encountered by the nidus? The first
issue can be addressed by considering the possible influence of an
autoregulatory capacity of an AVM. The lack of autoregulation, which is
not implemented in this AVM model, assumes that nidus vessels are
viewed as fixed vascular conduits and that increases in
arterial blood pressure are transmitted directly to the AVM
nidus vessels and to the DVs.38 Because the basis for risk
of rupture is the critical radius of a cylindrical vessel described by
biomechanical constants typical of a nidus vessel, pressure is at least
a complicating if not precipitating factor in the stability and
prediction of rupture of the nidus vessels. An increase in pressure
translates to increased biomechanical stress of the vessel. According
to Laplace's law, the biomechanical stress increases to the point of
the elastic limit of the vessel, beyond which the vessel ruptures. The
simulation results of normal flow in Fig 5
reflect a range of risk of
rupture for nidus components from 4.4% to 91.2%. Because risk of
rupture values do not exceed 100%, rupture does not always occur under
normal circumstances. However, as venous drainage becomes impaired, the
risk of rupture changes as the intranidal pressure redistributes itself
to compensate for the venous occlusion. Increases in risk of AVM nidus
rupture are observed particularly in close proximity to the DVs. In the
event of nidus rupture, vessels closest to the venous drainage were
shown to exhibit a substantial increase in the risk of rupture, and
nidus vessel 34 was shown to rupture. The occurrence of rupture at the
DV end of the nidus is due presumably to the increased pressure buildup
in the nidus vessels feeding into the stenosed DVs experienced at the
site of occlusion and is supported by current clinical hypotheses.
These findings are clearly visualized from simulation 5 of Fig 6C
.
Interestingly, these observations appear to provide a theoretical
biophysical basis for the commonly held supposition that AVMs rupture
near the origin of their DVs.20
With regard to the second issue, it is tempting to describe the risk of
rupture in terms of the baseline transnidal pressure gradient (ie, that
in the presence of normal systemic blood pressure) between the AFs and
DVs or to state that any nidus vessel whose IVP gradient exceeds the
baseline normal pressure of the AF is prone to rupture. However, AVM
physiology, particularly within the nidus, is much more complex. In an
AVM with multiple AFs and DVs, as simulated in our model, pressures
from each feeding and draining pedicle contribute to the distribution
of pressure within the nidus. Thus, the total pressure entering the
nidus is starkly different in both magnitude and direction from the
pressure exiting the nidus. Because pressure is a physical vector
quantity, it stands to reason that the pressure from multiple feeders
translates into an intranidal pressure that could possibly exceed the
pressure within some AFs, without rupture. It is, however, impossible
that the intranidal pressures will exceed those within the feeder with
the highest blood pressure. Therefore, for the purpose of our
calculations, the maximum intranidal pressure was assumed to be
equivalent to the highest values achievable for blood pressure in
adjacent AFs, ie, those occurring during systemic hypertension.
The range in risk of rupture for the simulations progressed in
continuous trends depending on the state of intranidal and transnidal
hemodynamics, with the exception of the simulation for
DV1 occluded 50% with DV2 patent. In the preceding simulations where
DV1 is patent or occluded 25%, the risk-of-rupture ranges are
4.4% to 91.2% and 4.7% to 90.5%, respectively. When DV1 was
occluded 50%, a decrease in the range of values for risk of rupture
was observed before the continual progression of these values with
further venous drainage impairment. DV1 is fed by the fistula and
assumes the majority of the hemodynamic forces. As DV1
is occluded, this reduces the biomechanical stress and hence risk of
rupture on adjacent nidus vessels. Although this change in stress
translates into an increase in pressure in surrounding nidus vessels,
it is well within the upper limit of biomechanical stress of these
nidus vessels and can thus easily be accommodated without the incidence
of rupture.
A primary limitation of the AVM simulations is that a constant
(nonpulsatile) blood pressure was assumed corresponding to the absence
of a temporal effect. Because hemodynamic alterations
are a time-dependent phenomenon, the risk of nidus rupture will
depend on the rate of venous drainage occlusion, ie, abrupt or gradual.
Since intracranial AVMs are also drained by a myriad of
angiographically occult venules of less than 50 µm,34 it
is hypothesized that gradual occlusion may more readily accommodate the
hemodynamic and vasodilatatory adaptation of these AVM
veins and thus translate into a reduced risk of nidus rupture compared
with abrupt occlusion. These important temporal/dynamic factors will be
addressed in future analyses using this model.
Critical Stenosis of AVM DVs
The remaining points of interest raised by the results from this
study are interrelated in that they are based on the
hemodynamic consequences of a stenosis, and
they bear further discussion. With respect to this research, the
hemodynamics at a DV stenosis (and particularly
a critical stenosis) are important primarily for two reasons:
(1) to quantitatively and qualitatively investigate the resulting
alterations in intranidal hemodynamics and (2) to help
explain why rupture was evident in series A, in which DV1 was occluded
first, yet was not observed in series B, in which the reverse was
performed. The basis for the hemodynamics described in
the model simulations was Poiseuille's law, which in effect states a
linear relationship between volumetric flow rate and pressure gradient
under normal circumstances. One is then left to consider quantitative
values of flow rate as the pressure continually increases in the nidus.
The linear relationship holds true only as a first-order effect and
is valid only to a point where the hemodynamic
relationship becomes nonlinear or drastically changes in form. The
reasons for this change in form include non-Newtonian viscosity of
blood, turbulence, pulsatile driving pressures, kinetic energy
transformations, and distensibility of vessels.39 This
point corresponds to the transition from laminar flow to turbulent
flow. As the stenotic region of a vessel becomes pronounced,
the flow rate decreases, the pressure gradient across the
stenosis decreases, and the flow velocity increases, as
illustrated by Bernoulli's principle. In addition, there is a buildup
of excess pressure proximal to the stenosis. The trends of
these hemodynamic parameters continue until
a critical stenosis is reached. The critical stenosis
is unique to vessel geometry and hemodynamics but has
been shown to generally occur at about 75% to 80% obstruction of the
major vessels in the human vasculature.40 41 42 43 At the point
of critical stenosis, a sharp decrease of flow rate is observed
that is due to the increased turbulence prior to the stenosis.
As the stenosis totally occludes the vessel, the pressure
drop across the stenosis reaches 100% of the maximum and
the flow rate is zero. In addition, the prestenotic
pressure is equal in magnitude to that at the source or the location
just prior to the vessel with the occlusion. As an illustrative example
of Newton's third law, the stenosis exerts an equal yet
opposite force against the hemodynamic forces generated
by the AF driving the blood through the nidus. At 100%
stenosis, the pressure gradient is not exactly zero because of
the additional energy losses. However, no relations, experiments, or
adequate explanations exist that elucidate and accurately
characterize these energy losses, leading one to approximate the
pressure gradient.43
Hemodynamics before, within, and beyond a critical
stenosis are crucial to understanding intranidal
hemodynamics during venous drainage impairment.
However, the most important issue is the use of this knowledge to
explain the reasons behind the observation of rupture during occlusion
of DV1 followed by DV2 and nonrupture of the AVM nidus in the reverse
case. It is tempting to believe that, on the basis of basic
hydrodynamics and clinical experience, total occlusion of either DV
would induce definite nidus rupture. This was shown to not necessarily
always be the case. Occlusion of the DV fed by the fistulous component
transfers an enormous hemodynamic burden to the
high-resistance plexiform vessels for exit through DV2.
Interestingly, it was noted that as DV1 was totally occluded a sharp
increase in pressure was observed at vessels 35 and 26, both of which
feed into vessel 34 via N26. It was the physical combination of the
marked pressure increases from these two vessels that contributed to
the substantial increase in pressure and thus rupture of vessel 34 (ie,
rupture at the venous end of the nidus). This can readily be seen in
Fig 6
. In contrast to DV1, occlusion of DV2 (fed entirely by plexiform
nidus vessels) places a relatively minor hemodynamic
burden on the vessels feeding into DV1. The only increase in pressure
and hence risk of rupture was noted in nidus vessel 35, together with
the relatively constant high risk of rupture in nidus vessel 37 at
91.4%, but within the biomechanical stresses of the vessel wall. Thus,
although the IVP gradient was high in both nidus vessels, the two
vessels were able to withstand the increased
hemodynamic burden in concert without rupture in either
vessel.
One would expect that as both DVs became totally occluded the IVP
gradient and hence the risk of nidus rupture would increase
accordingly. This is reflected in the well-established
clinical/angiographic finding that interruption of the venous outlet of
a plexiform pial AVM causes nidus rupture and not simple stagnation of
flow within the nidus.44 45 However, the model displays
results from simulations at discrete points; therefore, once rupture
has occurred, simulations beyond that stage of occlusion become
meaningless. One might speculate that if the nidus vessels were strong
enough to withstand the increasing risk of rupture, as shown by the
sharp slope increase in Fig 7
, then intranidal flow stagnation would
eventually occur (as depicted by the simulation results) when the
values for the critical-stenosis range in the DVs are
surpassed. Indeed, this may well provide the
hemodynamic rationale for the safety and efficacy of
the transvenous (endovascular or surgical46 47 48 ) treatment
(ie, total occlusion) of single-hole or multichannel dural
arteriovenous fistulas. It is hypothesized that under these
circumstances the much stronger site of shunting (direct fistula
surrounded by dura, as opposed to delicate nidus microvessels) is able
to withstand the upslope of the rupture-risk curve in Fig 7
,
without rupturing, to be followed by the precipitous drop in pressure
gradient, biomechanical stress, and risk of rupture, signifying blood
stagnation and effective therapeutic interruption of the fistula.
Nidus Rupture as a Surgical Complication
The above findings may also help explain the biophysical and
hemodynamic mechanisms for some complications related
to AVM surgery. Occlusion of AFs before DVs is a conventional technique
that is followed by most neurosurgeons during operative removal of
intracranial AVMs. This respect for the venous drainage of AVMs dates
from Dandy's49 description of catastrophic nidus rupture
that occurred when DVs were ligated initially. More recently, however,
the idea has emerged50 that, under certain circumstances,
it may be safe to occlude, transect, and mobilize a DV (using it as a
handle) as a first step toward dissection of the AVM core (Malis
procedure51 ). It has been stated that this is permissible
(safe) only in the presence of multiple veins draining an AVM, so as
not to impair its total drainage with consequent nidus rupture. The
results of our study concur in part with this concept, and they provide
a theoretical hemodynamic rationale for the safety of
the Malis procedure but only under certain circumstances. In the
particular theoretical model we have chosen, total occlusion of one AVM
vein that drains the fistulous vessels does result in nidus rupture. On
the other hand, occlusion of the vein draining the plexiform vessels
did not cause rupture. Therefore, our theoretical simulations
demonstrate that the Malis procedure may not be safe if any single vein
is transected. Instead, careful angiographic analysis may be
necessary beforehand to avoid initial occlusion of the vein carrying
the most drainage, lest AVM rupture does occur. Should more than one DV
be totally occluded before AFs during surgery, then the risk of
immediate rupture would depend on the ratio of number of DVs to AFs for
that particular AVM. However, adopting the Malis procedure as
originally conceived, ie, occlusion of only one vein (the most
hemodynamically appropriate) in the presence of
multiple veins, would ensure as low a risk as possible of rupturing the
AVM. Emerging from our results also is the proviso that, should the
Malis procedure be performed using one vein, careful angiographic
scrutiny of the remaining DVs would then be necessary to detect any
naturally occurring stenosis(es) that may help tip the balance
of overall venous drainage impairment toward critical nidus rupture.
Venous restrictive disease has also been implicated recently in the
hyperemic complications associated with endovascular or
surgical treatment of AVMs.52 Thus, Al-Rodhan et
al52 have proposed the concept of "occlusive
hyperemia" to explain the morbidity that may occur after
resection of high-flow intracranial AVMs. It was suggested that
these complications may occur on surgical resection because of outflow
obstruction in veins draining an AVM, which also implicates the normal
drainage from brain surrounding the AVM, thus resulting in passive
engorgement in normal brain tissue. Should a portion of the nidus be
retained after surgery, this venous overload (occlusive
hyperemia) may become "malignant" because of a concurrent
arterial overload within the retained nidus.20
Our experimental simulations therefore also provide a theoretical
rationale for events leading to possible retained nidus rupture in the
presence of venous drainage impairment and occlusive hyperemia.
The results of this study demonstrate that, for the particular
configuration and hemodynamics of AVM that were
simulated, nidus rupture occurs within a certain range of critical
venous drainage impairment. It is conceivable that overall equivalent
degrees of impairment may follow incomplete surgery, resulting in
rupture of retained nidus.
Conclusions
In conclusion, we have shown using our biomathematical AVM model
that AVM rupture as a result of venous drainage impairment occurs in
nidus vessels at the venous end of the AVM and is dependent on the
nidus angioarchitecture and hemodynamics. Specifically,
these results, based on theoretical analysis, suggest that the
risk of nidus rupture depends on the relative distribution of
hemodynamic load within the DVs before
stenosis/occlusion. Stenosis/occlusion of a
high-flow DV induces a significant redistribution of blood into the
weak plexiform vessels of the opposing region of the nidus, causing a
hemodynamic overload and an increased risk of rupture.
These findings should be carefully considered among all factors
affecting the natural history of intracranial AVMs and the mechanisms
implicated in their spontaneous rupture. They may also provide a
theoretical rationale for some of the hemorrhagic complications that
occur during and after surgical treatment.
 |
Selected Abbreviations and Acronyms
|
|---|
| AF |
= |
arterial feeder |
| AVM |
= |
arteriovenous malformation |
| CVP |
= |
central venous pressure |
| DV |
= |
draining vein |
| IVP |
= |
intravascular pressure |
|
 |
Acknowledgments
|
|---|
This work was supported in part by National Institutes of Health
grant
1-RO1-HL/NS52352-01A1. The authors gratefully acknowledge the
assistance
of Lynne Olson for the artistic preparation and
presentation
of the illustrations and of Kelly Hademenos
and Susan Massoud
for the management of the data for the AVM model
simulations.
 |
Footnotes
|
|---|
Reprint requests to George J. Hademenos, PhD, Division of Medical
Imaging-172115, Department of Radiological Sciences, UCLA School
of Medicine, 10833 Le Conte Ave, Los Angeles, CA 90024-1721.
E-mail hademeno@endeavor.radsci.ucla.edu.
Received November 20, 1995;
revision received February 22, 1996;
accepted February 28, 1996.
 |
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