South Carolina Children's Heart Center, Medical University of
South Carolina, Charleston, South Carolina 29425
Laplace's law constrains how thin the ventricular wall may be
without experiencing excessive stress. The present study
investigated constraints, imposed by myocardial viscosity (resistance
to internal rearrangement), on how thick the wall may be. The ventricle
was modeled as a contracting, spherical shell. The analysis
demonstrated that viscosity generates stress and energy dissipation
with inverse fourth- and eighth-power dependence, respectively, on
distance from the cavity center. This result derives from the
combination of squared dependence of viscous forces on shearing
velocity gradients and the greater shear rearrangement required for
inner layers of a contracting sphere. These predictions are based
solely on geometry and fundamentals of viscosity and are independent of material properties, cytoskeletal structure, and internal structural forces. Calculated values of energy and force required to overcome viscosity were clearly large enough to affect the extent of thickening of the left ventricle. It is concluded that load-independent viscous resistance to contraction is an important factor in cardiac mechanics, especially of the thickened ventricles of concentric hypertrophy.
 |
INTRODUCTION |
ONE RESPONSE OF THE LEFT
VENTRICLE to prolonged arterial hypertension is the development
of concentric hypertrophy (2, 13). This adaptation lowers
the stress experienced by the ventricular wall and normalizes the
elevated stress resulting from increased pressure. Laplace's law of
the heart relates wall stress to pressure in terms of the ratio of wall
thickness to lumen radius. Lower ratios (relatively thin walls) result
in greater internal stress. Because of this pattern of stress
increases, there is a lower limit to the thickness of the myocardial
wall at a particular operating pressure (2, 21).
Investigators have found that normal wall thickness-to-radius ratios
are nearly constant over a group of mammalian species that are widely
disparate in size but relatively close in blood pressure (5,
19). Ratios that are much lower than this normal value are
indicative of pathological eccentric hypertrophy, which results in
elevated wall stress at normal pressures. It is not clear, however,
what is constraining the ratio in the opposite direction.
A small amount of nonobstructive hypertrophy would lower wall stress,
and this is believed to be one benefit of exercise (9). It
is, therefore, not obvious why concentric hypertrophy often regresses
after developing in response to transient conditions such as pregnancy
(22) or repaired valve stenosis (4). The stress reduction is apparently not enough of an advantage for the mild
hypertrophy to be maintained. It is unclear what disadvantages may
result from concentric hypertrophy that would counterbalance the
advantage of stress reduction.
Recently suggested counteracting factors have included problems in
perfusion observed in the endocardial layers of concentrically hypertrophied ventricles (15, 24), nonischemic decrease in myocardial function (12), and the increased oxygen demand
due to greater deformation occurring at the endocardium
(1). Whereas the significant cellular and biochemical
issues underlying cardiac function have been extensively investigated,
comparatively less attention has been directed toward analysis of the
purely physics-based factors that may play a role (3, 11, 18, 21,
29). Because deformation or internal rearrangement of the
myocardium, whether achieved by slippage between layers or by cellular
distortion, occurs in a viscous medium, the effects of viscosity are a
possible factor in determining chamber geometry and behavior. This
study is an examination of the magnitude and patterns of predicted
viscous effects in a thick-walled chamber such as the left ventricle. These effects are 1) stresses that resist contraction
(viscous drag) and 2) extra energy consumed to overcome
these stresses (viscous energy losses).
Glossary
|
Proportionality constant between lumen radius r and
intermediate radius
|
A |
Chemical affinities
|
|
Proportion of total wall volume inside intermediate radius
|
C |
Circumference at intermediate radius
|
ij |
Kroneker delta
|
|
Viscosity coefficient
|
| h |
Wall thickness
|
|
Intermediate radius within the myocardium
|
| P |
Hydrostatic pressure
|
| r |
Radius of the lumen (endocardial radius)
|
| R |
Radius at epicardium
|
[S] |
Entropy production
|
| T |
Temperature
|
| vc |
Circumferential components of velocity
|
| vi |
Components of velocity
|
v |
Radial components of velocity
|
| Vw |
Wall (myocardial) volume
|
w |
Reaction rates
|
| Wj |
Heat flow
|
ij |
Components of the stress tensor
|
x |
Distance along intermediate radius
|
 |
METHODS |
Geometric model.
The model selected for analysis was a homogeneous, thick-walled
spherical shell. This model was chosen to elucidate the patterns of
viscous effects that are due only to bulk geometry and the fundamental
laws of hydrodynamics. Whereas the actual left ventricle of the heart
has a much greater complexity than that of the model, the ventricle
must still, in the mean, behave within the boundaries established by
the fundamental physics of this model. More specifically, whereas
patterns of fibrous structure, layering, and particular cytoskeletal
structure within the wall may change the absolute level of viscous
effects, the overall pattern of stress and energy losses across the
thickness of the wall will be determined by the constraints of geometry
and hydrodynamics.
The behavior of a contracting spherical shell can be described in terms
of circumferential and radial velocities. The circumferential component
velocities in the present analysis should not be equated directly to
the velocities of contraction of the sarcomeres. As has been shown
(3), the varying helical arrangement of fibers in the
myocardium allows for nearly homogeneous contraction along fiber
directions. This pattern of contraction does not alter the geometric
necessity of increasing net velocity gradients along the purely
circumferential directions (partially or completely across fibers). If
these gradients did not occur, the shell would not be able to contract
due to the constraints of the geometry. As the fibers contract along
their length, rearrangements and distortions also have to occur across
the direction of the fibers. The mean net effect of these movements
must be to produce the motion prescribed by a shell with a thick,
constant-volume wall.
Stresses within a thick-walled shell.
There will be components of stress (force per unit area) due to
viscosity stemming from any gradient in velocities of contraction between adjacent elements in a mass (shearing). These stresses are
expressed counter to the direction of motion of the mass element. The
stress components are proportional to the first spatial derivatives of
the velocities taken in directions normal to the velocities themselves
(10)
|
(1)
|
Here P is hydrostatic pressure and
ij
is the Kroneker delta, which equals unity when i =
j; it is zero otherwise. Note that the double subscript, as used
here, does not indicate summation but signifies the row and column of
an overall stress tensor. Eq. 1 can be split into diagonal
(
ij = 1) and off-diagonal
(
ij = 0) terms
|
(2)
|
Note that the sign convention used here requires that
, the
viscosity coefficient, be positive so that the viscous stress component
will be counter to the direction of motion. Most importantly, note also
that Eq. 2, right, as well as Eq. 2,
left, second term, represents stress components that occur
independently of external loads or internal restoring forces. They
occur with all contractions, even those generating no transmural pressure.
Although there are undoubtedly variations in contraction velocities
occurring at different sites over the surface of the ventricle (29), the present approach uses a simplified model in
which the rates of contraction are homogeneous over the circumference of a ventricle modeled as a thick-walled sphere. This model allows a
qualitative analysis of the endocardial-to-epicardial variation in
viscous effects, which is the object of the investigation. In a
nonhomogeneous contraction, specific areas would be contracting at
higher and lower velocities to achieve the same overall rate of
contraction. The present model may thus be viewed as an analysis of
mean behavior.
For this model, there are two components of velocity that may have
gradients across the wall thickness. The first is the radial velocity
toward the contracting lumen. The second is that of different structures moving with respect to one another along circumferences. This second motion is modeled as a completely balanced net contraction, with no net circumferential displacement. Each unit of volume of
myocardium stays in the same angular position while decreasing in
circumferential dimension.
This model is completely general with respect to the fine structure of
the thick shell itself, the myocardium. The overall geometry requires a
particular fundamental pattern of net circumferential and radial
velocities. Different patterns of fiber direction, spiral and helical
layer rearrangements, or restoring forces undoubtedly exist within the
myocardium. Although these factors may achieve more efficient
contraction, the net displacement must still lie within the constraints
of geometry.
Viscous energy losses.
In any system, some portion of the total energy flux is lost as heat
(dissipated) in entropy production. The equation for total net energy
losses,
[S], in a nonequilibrium system such as myocardium is
(10, 14)
|
(3)
|
In this equation, Wj is heat flow, T is
temperature,
ij is the components of the
stress tensor, vi is the components of velocity,
A
is the affinities of the chemical
reactions, and w
is the reaction rates. The
first term represents entropy produced due to temperature gradients and
heat flows. The second term is the contribution due to chemical
affinity, a function of changes in chemical potential, and chemical
flow. The third term represents the entropy increase due to velocity
gradients and stress. This last term is the viscous energy loss
addressed in the present study.
 |
RESULTS |
General framework of analysis.
The first part of RESULTS addresses the patterns of motion
that are dictated by the geometry of contraction of a thick shell with
constant wall volume. The analysis in the section below shows that the
constancy of wall volume, combined with shell geometry, requires that
inner and outer regions must behave in fundamentally differing ways for
contraction to take place. Compared with the outer regions, the inner
regions of the wall are subject to much greater rearrangements in both
the radial and circumferential directions during contraction.
Accordingly, the spatial rates of change (gradients) in displacement
and velocity are also much greater toward the inner surface of the shell.
The second part of RESULTS is an accounting of the stresses
and viscous energy losses that are predicted as a result of the patterns of velocity in a contracting shell. The most important aspect
of this accounting results from the dependence of energy loss on the
square of the gradient of velocities in a fluid medium. In a
contracting shell, the magnitude of energy loss is very sensitive to
radius as a result of the shell velocity patterns combined with the
dependence on the square of the gradient.
The final part of RESULTS is a calculation of levels of
stress and energy loss based on a typical set of ventricular proportions.
Patterns of stress and dissipation across the wall.
Viscous stresses in a deforming mass are determined by the gradients in
motion of adjacent mass elements. To determine what these gradients are
in the present model, one can define an intermediate radius
, within
the myocardium, that represents the position of a particular physical
fiber throughout contraction of a thick-walled spherical shell (see
Fig. 1). This fiber will be positioned at a changing radius within which is enclosed a constant proportion
of
total wall volume, Vw. The radius of the lumen itself,
r, is related to
, the intermediate radius, by a variable
factor,
, that depends on r itself and the proportion
.

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Fig. 1.
Cross-sectional diagram of the spherical shell model used
for analysis. R and r, radii of the outer and
inner surfaces, respectively; , intermediate radius that encloses a
constant proportion of the total volume of the shell.
|
|
As shown in the APPENDIX, equations can be derived for the
spatial gradients in velocity at an instantaneous value of lumen radius
r
|
(4)
|
Equation 4 shows that the rates of change of velocity,
and consequently the absolute resultant velocities, are much greater at
lower values of
, i.e., near the endocardium. Substitution of these
results into the expressions for viscous stress (Eq. 2)
gives radial and circumferential stresses
|
(5)
|
Equation 5, left, shows the radial viscous
drag (stress-resisting contraction) acting in parallel with pressure
during contraction. The direction of the circumferential component,
expressed in Eq. 5, right, is arbitrary. Both
equations show the rapid increase in viscous drag as
, the relative
distance from the center of the lumen, decreases.
The APPENDIX also shows the derivation of an expression for
viscous energy losses in terms of radial and circumferential velocities (v
and vc,
respectively)
|
(6)
|
This result indicates the nonlinear (quadratic) sensitivity of
viscous loss to gradients in radial and circumferential velocity across
the thickness of the wall. The expressions for velocity gradients
(Eq. 4) within a thick-walled shell can be substituted to
produce
|
(7)
|
This equation displays the consequences of combining the effects
of 1) the quadratic dependence of viscous energy loss on velocity gradients and 2) the magnified strain (distortion)
and rate of strain generation near the inner surface necessary for the
contraction of a constant-volume shell. Together, these two factors
result in an expression that includes terms up to an inverse eighth
power of the radial coordinate
. It is worth stating again that the
terms in Eqs. 5 and 7 that do not include
pressure are independent of external load. They represent the stresses
and energy losses that will occur even when contraction is against zero
transmural pressure.
To see what Eqs. 5 and 7 predict for a
"typically proportioned" ventricle, a sphere can be defined with a
Vw of 4/3
(1)3 or 4.19 cubic
units. Typical mammalian thickness-to-radius ratios are obtained by
using wall thicknesses of 0.33 and 0.55 units at average minimum and
maximum contraction, respectively. These points correspond roughly to
end diastole and end systole, respectively. Based on the relationship
between h and lumen radius for a thick-walled sphere
|
(8)
|
the end-diastolic radius will be 0.84 units, with a corresponding
volume of 2.44 cubic units. The end-systolic values are 0.49 and 0.48 units. This gives an ejection fraction of 0.80 and a shortening
fraction of 0.42. Using these numbers in Eq. 5 gives the
results shown in Table 1, which
demonstrate the extent of variation in viscous stresses due to velocity
gradients in the course of a typical ventricular contraction. As can be
seen, the differences are dramatic.
When these typical ratios are used to determine energy losses
(Eq. 7), the results are even more dramatic (Table
2). At an extent of contraction
corresponding to a normal end systole, the energy used to overcome
circumferential viscous resistance to rearrangement is >400 times
greater at the endocardium than at the epicardium.
Relative magnitudes of viscous stress and energy losses (dissipation)
are shown graphically in Figs. 2 and
3, respectively. The units on the
x-axis are in terms of the endocardial radius so that the
thickness of the ventricular wall is represented as extending from
unity to a larger value, depending on relative contraction of the
chamber. The endocardial end-diastolic stress or dissipation value is
defined as 1.0. The simplifying assumption has been made that the
values at the epicardium remain constant. The lowest curve in Fig.
2A represents the relative values of pressure-independent
radial stress (2nd term in Eq. 5) across the wall at end
diastole, with the wall extending between 1 and 1.4. At end systole,
the plot shows that the wall is thickened relative to the lumen and
that the endocardial radial stress is 3.4 times higher than it was at
end diastole. If the wall thickens to the relative proportion seen in
hypertrophy, the relative stress rises to almost nine times that seen
at normal end diastole.

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Fig. 2.
A: plots of the relative magnitudes of radial (rad)
stress due to viscous drag at different radii and at different
proportional wall thicknesses typical of end diastole (ED), end systole
(ES), and end systole in a hypertrophic (hypert) ventricle. The
endocardium is defined as being at a radius of 1, and the magnitude at
the epicardium is assumed to remain constant. B: plots of
circumferential (cir) stress due to viscous drag.
|
|

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Fig. 3.
A: plots of the relative magnitudes of dissipation of
energy resulting from radial stress due to viscous drag at different
radii and at different proportional wall thicknesses typical of end
diastole, end systole, and end systole in a hypertrophic ventricle. The
endocardium is defined as being at a radius of 1, and the magnitude at
the epicardium is assumed to remain constant. B: plots of
dissipation of energy resulting from circumferential stress due to
viscous drag.
|
|
The predictions for circumferential stress are more pronounced than for
radial stress, as shown in Fig. 2B. Endocardial
circumferential stress increases by ~5 and 18 times at end systole
for normal and proportionately greater contractions, respectively.
Figure 3 shows the relative energy dissipation across the wall
for normal and hypertrophic contractions. The increase in relative rate
of loss at the endocardium is quite pronounced, as is the localization
of the greatest losses at the inner layers of the wall.
Are energy losses large enough to be significant?
Whereas the stress and entropy equations have terms that behave
qualitatively in ways that would explain observed limits to myocardial
thickening, it is not established whether these quantities are of
sufficient magnitude to be significant in cardiac function and
pathology. To determine a possible answer to this question, the present
study investigated possible sizes of energy losses rather than the more
difficult estimation of local stress values.
It was estimated how much heat would be generated in myocardium based
on published values of viscosity coefficients and calculated gradients
in velocity of contraction. The resulting estimates were compared with
published estimates of myocardial total losses to entropy (i.e., from
all three terms of Eq. 1: heat flow, chemical reaction, and
viscosity). These estimates were based on comparisons between heat
generated in isometric contractions and the corresponding pressure-volume areas (27, 28).
Modeling of viscoelastic properties of the myocardium (6, 7, 25,
26) has been done in terms of series and parallel elastic
elements. Chiu et al. (6, 7) made estimates of parallel and series viscous coefficients by using the model in Fig.
4. An iterative procedure of viscosity
estimates was used to fit empirical results, giving values of 39 and
0.15 mN · s
1 · Lmax
1
(where Lmax is maximim length), respectively,
for a muscle 6 mm long and 0.92 mm2 in cross section.
Converting to centipoise gives 3,815 and 14.7 cP, respectively. Because
the series contribution is negligible, it will be dropped from the
following estimations.

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Fig. 4.
Lumped model used by Chiu et al. (6, 7) for
modeling viscosity in myocardium. CE, contractile element; PE, parallel
elastic element; SE, series elastic element; V, viscous elements.
|
|
The heat output from any level of viscosity varies with the distance
between sliding elements. At an effective distance of 10 µm between
elements (~1/2 the thickness of a myocyte) and viscosity of 3,815 cP,
the heat output would be 156.26 ergs · cm
3 · s
1 · K
1.
These estimates are found by using 293K and a velocity of 0.3 mm/s for
the series element in an 8-mm muscle (26).
Based on observations of carbon granule motion on the muscles and of
the microscopic behavior of sarcomeres, Chiu et al. (6, 7)
concluded that only a portion of the elastance that they observed
resulted in internal shear. If this fraction were low, say 1/10, the
velocity differences would be reduced by 10. This would decrease the
overall heat calculated by a factor of 100 (keeping 3,815 cP as the
viscosity coefficient and 10 µm as the distance), leading to 1.56 ergs · cm
3 · s
1 · K
1
as the estimate.
The total heat measured by Mast and
Elzinga (20) during isometric contraction was
112.29 ergs · cm
3 · s
1 · K
1.
According to their regression analysis, this heat averaged ~5% above
the energy represented by the pressure-volume areas, or 5.6 ergs · cm
3 · s
1 · K
1.
This 5% is the excess energy expended that did not contribute to the
pressure increase during the contraction. Based on the error inherent
in the estimated slope of the regression line (95% confidence
interval), the excess might have been as high as 20%, or 22.5 ergs · cm
3 · s
1 · K
1.
Accordingly, these calculations lead to an estimated range of viscous
contributions to total entropy losses from 7% (1.56-22.5 ergs · cm
3 · s
1 · K
1)
to 28% (1.56-5.6
ergs · cm
3 · s
1 · K
1).
The viscous losses would amount to 1.4% (1.56-112.29
ergs · cm
3 · s
1 · K
1)
of the total energy used (losses plus work). This percentage is the
level that occurs in a linearly contracting piece of papillary muscle
with no magnification of distortion due to thick-shell geometry. This
linear result can be taken as approximating the percentage of losses
near the epicardium (where contraction is closest to linear) at end
systole. As shown in Table 2, the losses near the endocardium would be
400 times higher after normal systolic thickening, far exceeding the
total of losses plus work at the epicardium. Relative thickening to the
extent observed in hypertrophic ventricles would result in an increase
of >4,000 times. This calculation of viscous losses does not include
the losses due to gradients in radial velocity (1st and 2nd terms in
Eq. 7; Table 2) for which no empirical results were available.
This result strongly suggests that the inner layers of muscle somehow
avoid being subjected to either the full velocity gradients imposed by
spherical shell geometry or the full observed viscosity coefficient.
The existence of helical- and spiral-oriented layers, angular torsion,
or nonhomogeneous contraction may allow gradients of velocity to be
redirected largely across spaces between layers in which the effective
viscosity was much lower than within muscle bundles. Displacements
along the borders between layers could be such that the vectorial
components of displacement in the circumferential direction were of a
magnitude required for shell contraction. In this fashion, the net
deformation required for contraction could still be achieved (by
sliding between low-viscosity layers) while avoiding runaway viscous losses.
However, to reduce the overall energy loss by a factor of 4,000 would
require that the average viscosity both between and within layers be at
or lower than the viscosity of water (1 cP). Such a lowering seems
clearly unreasonable to expect within the myocardium. Further
hypertrophy would lead to further eighth-power increases in losses.
This pattern appears to represent a sharp energetic barrier to the
development of hypertrophy beyond the upper limit of what is observed physiologically.
 |
DISCUSSION |
The preceding analysis demonstrates that the interaction of
myocardial geometry and viscosity is a qualitatively and quantitatively significant factor in constraining the maximum relative thickness of
the left ventricular myocardium. This interaction is thus strongly implicated in the limitations observed in the extent and persistence of hypertrophy.
The constraint imposed by viscosity on ventricular geometry is the
opposite of the minimum thickness constraint imposed by Laplace's law.
The overall picture is one of a balance between load increases at
higher relative distensions (eccentric hypertrophy) due to the Laplace
law and load increases at lower relative distensions (concentric
hypertrophy) due to viscosity. This pattern of variation results in a
minimum total load at some particular ratio of wall thickness to lumen
radius. Such a minimum indicates a mechanism for the observed small
variation in end-systolic relative wall thickness over large ranges of
ventricular mass, both within and between mammalian species (5,
19). Systolic thickening beyond a certain point will result in a
cost, in total stress and energy dissipation, that will exceed the
benefit to be gained in cardiac output or mechanical advantage against
pressure. Thus there would be no net advantage to be gained by
maintenance of concentric hypertrophy after load is normalized, such as
after pregnancy or after valve repair.
The nonisotropic structure of the actual myocardium could change the
quantitative levels of stress and energy loss but not the overall
epicardial-endocardial pattern set by physics and demonstrated in
RESULTS. It is certainly reasonable to assume that
some aspects of the microstructure of the myocardium have reduction of
viscosity as their function. Due to the extreme steepness of the
increase in viscous effects with thickening, it is clear that only
relatively small, overall increments in thickening could be achieved
without large increases in stress and energy loss.
The extent of similarity of mammalian relative wall thicknesses at
systole may be further determined, not only by the existence of a
minimum load as indicated in RESULTS, but also by the
steepness of the increase in viscous stress and energy loss with
further contraction. The eighth-power dependence contained in
Eq. 7 presents a sharply defined barrier to further
contraction, which will occur within a tight range of the relative
extent of contraction. Due to the steepness of the function, the
variations in velocity, cytoskeletal mechanics, and viscosity that
undoubtedly occur between species would have minimal effects on the
particular proportional extent of contraction that marks the limits of
what is physiologically attainable. It would be interesting to
investigate whether significant variations in overall geometry, such as
the elongated geometry in the ferret heart, are accompanied by
significant variations in the thickness-to-radius ratio.
The widely observed dysfunction of the endocardial layers during
tachycardia in hypertrophy (12, 15, 24) is completely consistent with the predictions of the currently presented analysis. Indeed, the marked endocardial-epicardial difference in energy dissipation would suggest that dysfunction may occur without any other
underlying pathologies, such as impeded blood flow (15, 24) or Ca2+-ATPase (12) levels. Much
more oxygen must be consumed at the endocardium than at the epicardium
to overcome local viscous resistance to contraction. The selective
ischemia (15, 24) and the greater oxygen demand
(1) observed at the endocardium agree with this physics-based pattern of energy demand.
The predictions of the present study agree with the observations of
Young et al. (29). Their results, obtained using magnetic resonance tagging, suggest that greater mechanical work is expended in
wall shearing (as opposed to lumen reduction) in hypertrophic than in
normal hearts. Additionally, these studies show that, as approximated
by the present circumferentially homogenous model, radial strain is
maximal and total strain along the fibers is minimal (i.e., little
change in angular position is observed).
The increase in the endocardial shear with contraction (as shown
graphically in Figs. 2 and 3) may indeed result in the attainment of a
point of maximum load beyond which sarcomeres cannot proceed. As
successively greater thicknesses of the endocardial myocardium reach
this point of limiting viscous load from shear, more and more of the
lumen pressure load must be born by the remaining outer layers of
muscle. Indeed, this is the pattern observed by Aoyagi et al.
(1) with increasing dobutamine administration. After a
certain point, only the velocity of the contraction increases and not
the extent of the contraction, a result the investigators attribute to
the load imposed by increased distortion necessary at greater extents
of contraction. As demonstrated here, such increased distortion would
result in increased viscous resistance to contraction and increased
energy lost to overcoming viscosity.
The results of LeGrice et al. (17) with a tachycardia
model are also in agreement with the present results. Whereas their work does not address concentric hypertrophy, it does demonstrate the
mismatch between oxygen supply and demand that occurs at the endocardium and not the epicardium. Considering the
epicardium-to-endocardium gradient in predicted energy dissipation even
at normal systole, as shown in Fig. 3, it is reasonable to expect that
the extra stress of tachycardia would affect the endocardium much
sooner than the epicardium. The greater overall velocities of
contraction would increase the energy dissipation in all layers, but
the endocardial layers would be more likely to exceed physiological
limits because these layers are already functioning at a greater level
of viscous loss.
The present results apparently contradict those of Izzi et al.
(16), who were not able to find differences in efficiency between normal and hypertrophic hearts. If more energy were wasted overcoming viscosity in hypertrophic hearts, it would be expected that
these hearts would display lower energetic efficiency. However, the
study contained relatively large standard deviations in the results,
such that an existing difference in efficiencies may not have been
detected. Calculation of the statistical power (8) of the
t-test that was used to compare regression slopes gives a
result of 0.10 (1-tailed test,
= 0.05). This means that there was only a 10% probability that a real difference of the size observed
would indeed have produced a statistically significant result in a
given experiment. In fact, a real difference as large as 40% between
the efficiencies of the two groups of hearts would still have had a
20% probability of producing a statistically nonsignificant
t-value in a given experiment. Additionally, the hearts were
studied under isovolumic conditions; therefore, not all viscous
properties would have been observable. Considering these factors, a
real and substantial difference might have existed between the normal
and hypertrophic hearts in this study in agreement with the present analysis.
Limitations of the present study.
The geometry of the left ventricle is much more closely approximated by
an ellipsoidal shell than a spherical shell. The choice was made to
present the analysis in terms of a sphere due to the much simpler
mathematics involved. The qualitative pattern of the results also
applies to ellipsoids and even cylinders. If the analysis is carried
out in terms of a cylinder, the inverse eighth- and sixth-power terms
are replaced by inverse sixth- and fourth-power terms, respectively. An
ellipsoidal ventricular geometry may be represented as something
between these two models, implying that the dependence of viscous
losses, while possibly not inverse eighth power, are at least on the
order of inverse seventh power. Such a dependence would not change any
of the implications of the present work.
There may be inaccuracies in the values used in this study for
viscosity coefficients, separation of contracting elements, and
contraction velocity. However, the values used are all in the range of
what is physiologically reasonable and hence demonstrate that the
effects of viscosity are clearly not orders of magnitude too small for
significant impact. Due to the eighth-order (or perhaps seventh-order)
increase in the magnitude of the circumferential (shear) dissipative
losses with radius, even a much smaller set of values would still give
physiologically significant results. In fact, as discussed in
RESULTS, the magnitudes predicted for typical ventricular
proportions are almost certainly too large to exist in the myocardium.
Such magnitudes would require all of the energy in the endocardial
layers to be lost to viscous drag, even at normal end systole.
In summary, the mechanical and thermodynamic analysis presented
in this study strongly suggests that the basic geometry and material
properties of the left ventricle are a sufficient basis, by themselves,
for constraints on the extent to which hypertrophy can progress and for
the selective dysfunction often observed in the endocardium. Whereas
biochemical, cellular, and physiological mechanisms are most certainly
not excluded by this analysis, the implication is that such factors act
in addition to, or on top of, the more fundamental geometric and
hydrodynamic principles.
To determine velocity gradients in a thick-walled, spherical
shell, an intermediate radius
was defined to represent the position
of a particular physical fiber throughout contraction. This radius
encloses a constant proportion
of total wall volume Vw.
The lumen radius r is related to
by a factor
,
depending on r and
. The outer radius of the sphere is
R (Fig. 1)
Because there are no spatial changes in velocity
along the dimensions parallel to the surface (x2
and x3), the derivatives along these directions
are zero, and these terms drop out