 |
INTRODUCTION |
Simple lipid bilayers have been a challenge for
quantitative structure determination. For example, experimental values
for the average area per lipid
A
for fully hydrated
dipalmitoylphosphatidylcholine (DPPC) at 50°C have ranged from 56 to
72 Å2 (Nagle, 1993
), with corresponding uncertainty in the
average thickness of the hydrocarbon core,
2
DC
. The same range of uncertainty has
come from the two primary experimental methods, namely x-ray diffraction and NMR. Recently, primary emphasis has been on the x-ray
technique, where
ADPPC
= 62.9 ± 1.3 Å2 was obtained (Nagle et al., 1996
). This result was in
agreement with a reanalysis of NMR order parameter data, which gave
ADPPC
= 62 ± 2 Å2
(Nagle, 1993
). However, it was emphasized in that reanalysis that there
were assumptions that could and should be tested with simulations. This
paper carries forward that program.
Simulations give a much more detailed view than any experiments on
lipid bilayers (Tobias et al., 1997
; Tieleman et al., 1997
). However,
given the uncertainties in force fields and the restriction to
nanosecond time scales, one should not necessarily expect simulations to obtain accurate values for all quantities of interest. The use of
simulations that we envision is to test relations between simulated
microscopic quantities that cannot be obtained from experiment. Such
relations are commonly used to obtain quantities of interest from raw
data. Simulations can also inspire new relations, as we show in this
paper. This use of simulations does not require that all of the force
fields be exactly correct or that the simulated quantities of
experimental interest agree perfectly with experiment. The interplay of
simulations that is envisioned is that simulations will help guide
experimental analysis, which will then provide more accurate quantities
of interest, which will then help tune the force fields used in the simulations.
The main relation studied in this paper is between the average order
parameters
Sn
and the average travel per
methylene
Dn
along the normal to the
bilayer. The conventional relation (Schindler and Seelig, 1975
;
Thurmond et al., 1991
; Nagle, 1993
) can essentially be written as
|
(1)
|
where DM is the maximum possible travel. A
different relation has also been used (De Young and Dill, 1988
):
|
(2)
|
However, a recent simulation (Berger et al., 1997
) shows (their
figure 7) that neither relation is especially good, and this paper
reports essentially the same result for a different simulation. Even
though the values of
A
that were obtained in their
simulation using the method of Nagle (1993)
were in fairly good
agreement with the actual simulated
A
, it is important
to elucidate the errors, including fortuitous compensations.
The simulation we analyze in this paper has been described previously
(Tu et al., 1995
). Briefly, the simulation was performed at constant
number, pressure, and temperature (NPT), with N = 32
DPPC lipids per monolayer and nW = 28 waters/lipid, P = 0, and T = 50°C, using a
Nose-Hoover thermostat. The SPC/E water potential and an all-atom
description of the lipids were used in the CHARMM program, with Ewald
sums for long-range interactions. Since publication (Tu et al., 1995
)
the simulation has been continued to 2 ns.
 |
METHYLENE TRAVEL |
The first main result is illustrated in Fig.
1, which plots the conventional
CD2 order parameters Sn
versus the travel of the nth methylene along the bilayer
normal. Each simulated data point in this figure gives molecular
dynamical averages for one specific methylene, with the different
points corresponding to different carbon numbers n,
different chains (sn-1 and sn-2), and different monolayers (upper and
lower) in the simulated bilayer. The solid straight line shows that the
conventional prediction (Nagle, 1993
) works fairly well for values of
the order parameter
Sn
0.2 that are
close to the experimental plateau region, but the slope of the data is
clearly smaller than the conventional slope. This point has previously
been made for a different simulation by Berger et al. (1997)
; they
presented essentially this type of figure (except that they plotted the
molecular order parameter instead of
Sn
)
with very similar results. Our first main result is the derivation of a
new formula that gives the result shown by the solid curve in Fig. 1.

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FIGURE 1
Symbols: simulated average order parameters
Sn versus average molecular travel
Dn (in Å). Curved solid line: New Eq. 24.
Straight solid line: conventional Eq. 1. Dashed line: Eq. 2. Dotted
line: Eq. 14.
|
|
The derivation of the new formula was inspired by detailed results of
the simulation that have not previously been presented. As with any
fluctuating statistical mechanical ensemble, one should consider
distribution functions. A fairly general one that we have analyzed for
the hydrocarbon chains is denoted
pn(z, D). The discrete index
n is the carbon number, which goes from 2 for the methylene
next to the carbonyl to 16 for the terminal methyl. The continuous
variable z is the distance along the bilayer normal, where
z = 0 is the center of the bilayer and with the
positive sign for the direction toward the headgroup region for that
chain. The instantaneous position of carbon n is denoted by
zn. The continuous variable D is the
methylenic travel; for carbon number n the instantaneous travel Dn is defined by
|
(3)
|
as illustrated in Fig. 2. From the
distribution function pn(z, D) the
average position of carbon n is given as
|
(4)
|
Fig. 3 shows that
zn
has upward curvature. This corresponds
to Dn decreasing with n, which
conforms to the expectation that the chains become more disordered near
the terminal methyl end.

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FIGURE 2
For the nth CH2 group,
D defines the travel along the bilayer normal z,
defines the local methylenic tilt, and defines the rotation
about the local methylene axis z'. Note that the local axis
is generally different for each carbon n.
|
|
For many purposes it suffices to consider only the reduced distribution
function
|
(5)
|
For example, the average travel of carbon n,
irrespective of where it is, is then given by
|
(6)
|
It is also important to consider the mean square
travel,
|
(7)
|
These quantities are shown in Fig.
4.
To consider averages of the order parameter Sn,
it is necessary to consider another variable in the probability
distribution functions. Fig. 2 shows the local axis z' that
goes through carbons n
1 and n + 1
and makes the angle
with the bilayer normal along z.
Rotation around the local axis z' is measured by the angle
. A straightforward calculation (see Eq. 3a; Nagle, 1993
) gives the
combined order parameter Sn of both deuterons on
the nth methylene corresponding to this orientation:
|
(8)
|
where cos
= Dn/DM involves only the
previous variable Dn and the maximum travel
along the z axis, which is DM = 2.54 Å for undistorted saturated hydrocarbon chains. The additional
variable is sin2
, for which average values for narrow
ranges of D are given by
|
(9)
|
Fig. 5 shows values of
sin2
n(D)
for two values of
n for the upper and lower monolayers separately. The fact
that
sin2
n(D)
is closer to
0.4 for the upper monolayer and closer to 0.5 for the lower monolayer
indicates incomplete thermal equilibration. This variable was
considered by van der Ploeg and Berendsen (1983)
, with the suggestion
that
sin2
n(D)
was less than
0.5.

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FIGURE 5
Simulated
sin2 n(D) as a function of
D for n = 6 ( , ) and n = 12 ( , ) averaged over sn-1 and sn-2 chains. , , The
upper monolayer; , , the lower monolayer.
|
|
After integration of Eq. 8 over
, the average order parameter
|
(10)
|
becomes
|
(11)
|
Fig. 6 shows simulation results that
have been binned according to the values of D, for both the
upper monolayer and the lower monolayer. Fig. 6 also shows theoretical
curves for
Sn(D)
that were
obtained from Eq. 11 for different values of
sin2
n(D)
. Clearly, the
curve using a random distribution
sin2
n(D)
= 0.5 fits quite
well for 1.5 Å < D < DM, where the
counting statistics are good (see p(D) curves in Fig. 6),
and even reasonably well for smaller values of D, where the
statistics are much poorer, because there are few groups with large
negative values of D; such groups have been called
upturns (Nagle, 1993
). (The occurrence of values of
D greater than DM is due to molecular
distortions caused by thermal fluctuations and intermolecular
interactions.)

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FIGURE 6
Simulated S(D) averaged over all
carbons in the lower monolayer ( ) and the upper monolayer ( ) are
compared to Eq. 11.  , the result for
sin2 (D) = 0.50; - - -, the results
for 0.46 and 0.54. The curves labeled p(D) show the
probability distribution function for the lower monolayer ( ) and
the upper monolayer (- - -).
|
|
Based on Fig. 6, we now adopt the approximation
sin2
n(D)
= 0.5. Then,
|
(12)
|
Further integration over D yields the usual average
order parameters,
|
(13)
|
The consistency of Eq. 13 is tested in Fig.
7, which shows that the results for the
direct simulation of Sn are very close to the
values of
Sn
obtained from Eq. 13 and
direct simulation of
n.
Equation 12 emphasizes that
Sn(D)
is a quadratic function
of D, so that
Sn
is a function
of
Dn2
=
n2 rather
than of
Dn
2. This just
reflects the well-known fundamental fact that the order parameter is a
second-order Legendre polynomial, whereas the travel is first order.
One might nevertheless consider approximating
Dn
by
n:
|
(14)
|
where the equality comes from inverting Eq. 13. This is a poor
approximation, as shown first by Fig. 4, which compares
Dn
and
n, and, more
importantly, by the lower curved line in Fig. 1. The reason for this is
that
n is generally greater than
Dn
because
pn(D) has a nonzero width
n:
|
(15)
|
Because
n2 > 0, the methylenic travel given by
Eq. 14 is overestimated. This is a basic mathematical problem. Upturns,
defined as groups with D < 0, are involved, in so far
as they broaden the distribution and increase
n for
larger n, as indicated by the increasing difference between
n and
Dn
in Fig. 4, but
they are not the fundamental problem.
To calculate Dn from
n, we need a
way to estimate the mean square deviation
n. Such a way
is suggested by considering the distribution function
pn(D) in Fig.
8, which shows that, over the most
significant range of D, pn(D) behaves
roughly exponentially:
|
(16)
|
The relevant parameter is the decay length
n, and
the parameter
n is just a normalization factor. It may
be noted that the decay length
n increases with the
carbon number n in Fig. 8. Furthermore, secondary peaks in
pn(D) occur near maximally negative
values of D; these are clearly deviations from the
functional form in Eq. 16. These are due to upturns, which are
infrequent for small n, but become more numerous, although
they are still less than 10%, for large n.

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|
FIGURE 8
Number distributions
pn(D) for n = 3
(smallest decay length) to n = 15 (largest decay
length).
|
|
Assuming Eq. 16, we have
|
(17)
|
|
(18)
|
With no further approximation, Eq. 17 can be solved numerically to
give
n. However, analytical expressions are more
appealing, and for this reason we extend the above integrals from
DM to 
(valid for
n
DM). Then,
|
(19)
|
|
(20)
|
|
(21)
|
Solving for
n in terms of
n yields
|
(22)
|
|
(23)
|
The square roots above are imaginary for
n2 < DM2/2, and this sets a limit to the
applicability of Eq. 23. For such small values of
n2
most of our previous approximations are questionable. In this limit,
n would be on the order of DM/2,
meaning a broad pn(D), which is
poorly modeled by Eq. 16. For carbons at the end of the chain we may
expect more complicated probability distributions. As shown by the
simulations, the maximum in pn(D)
deviates from DM, and peaks at negative values
of D start to develop because of upturns. However, for
another comparison note that a constant (isotropic) distribution
between
DM and DM gives
n2 = DM2/3; this is
only a little less than the applicability limit, so the restriction
n2 > DM2/2 is not so severe.
Assuming that the approximations hold, we can combine Eq. 23 with Eq. 13 to give our final expression of
Dn
as a
function of
Sn
:
|
(24)
|
where the corresponding limiting point of applicability is
Sn
=
1/8 =
0.125. In these
simulations, only
S15
is close to this
limit, as can be seen in Fig. 1, which plots Eq. 24 and compares to
direct simulations. The usual way to compare is shown in Fig.
9, which compares the direct simulation
results for
Dn
with those obtained from
Eq. 24, using the simulation results for
Sn
. These two results deviate for large
n because the exponential form used in Eq. 16 is not
accurate for methylenes near the terminal methyl, as shown in Fig. 8.
Moreover, the approximation
n
DM used to obtain Eq. 19 breaks down for
n > 10. The standard Eq. 1, shown in Fig. 9, deviates
at both high n and low n.

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FIGURE 9
Solid squares show directly simulated
Dn (in Å). Estimates using Eq. 24 are
shown with open circles, and the + symbols show estimates from Eq. 1.
|
|
 |
AVERAGE CHAIN LENGTH |
In this section we extend the results for methylenic travel to
longer segments of the hydrocarbon chain. Of particular interest is the
average length of the entire hydrocarbon chain. This length is a little
awkward conceptually because it should include a poorly defined piece
beyond the terminal methyl n = 16. A more precisely defined length will be called L*C, which
is defined to be the average distance along the bilayer normal between
the first methylene carbon and the terminal methyl carbon:
|
(25)
|
For the present simulation
z2
= 13.78
Å and
z16
= 1.32 Å, giving
L*C
= 12.46 Å. To estimate the
average full length of the chain
LC
, we
first add 0.547 Å to
L*C
to
account for half of the projected distance from the first methylene to the carbonyl carbon. We then add
1.5
z15
z16
to account for
the extra length of the terminal methyl; the rationale for this is that
the terminal methyl volume VCH3 is about
twice as large as methylene volume VCH2
(Nagle and Wiener, 1988
; Petrache et al., 1997
). The estimated chain
length obtained directly from the simulations is then
LC
= 13.99 Å.
To obtain chain lengths from NMR requires using either our new Eq. 24
or the conventional Eq. 1. We first report results for
L*C
, which are simply obtained by
summing
Dn
over all odd values of
n from 3 to 15. The result from Eq. 24 is
L*C
= 12.49 Å, and the result
from Eq. 1 is
L*C
= 12.42 Å.
Despite the deviations in Fig. 9, both approximate results from
Sn
agree well with the direct result,
L*C
= 12.46 Å. However, the
result from our new Eq. 24 uses
D15
, which
is right at the limit where the square root becomes imaginary, and so
it probably gives a too small value, which happens to compensate for
the positive deviations in Fig. 9. The conventional result involves
even more accidental cancellations, as shown in Fig. 9.
We next estimate the full chain length
LC
,
using
|
(26)
|
where
D2
was estimated by
D3
, and where the extra
D15
term estimates the extra contribution
from the n = 16 terminal methyl end. These conventions
are identical to those used two paragraphs above to obtain
LC
= 13.99 Å. The value obtained using
Eq. 26 and the direct simulation results for
Dn
is
LC
= 14.01 Å. Using Eq. 24 and the simulated
Sn
yields
LC
= 14.0 Å, and using Eq. 1 yields
LC
= 14.1 Å. It therefore appears that, for these simulations,
either the old or the new formula gives good estimates of
LC
.
It is also worth considering such quantities for different simulations.
Berger et al. (1997)
reported relative positions of C4,
C9, and C14 for three different simulation runs
of fluid-phase DPPC. They also reported the order parameters for each
run. Our test of Eq. 24 for their best run (no. 2) is presented in
Table 1. Feller et al. (1997)
reported
similar results, which are also used to test Eq. 24 in Table 1.
Comparison values are also shown for the present simulation. In the
plateau region, n = 4-9, the new Eq. 24 gives superior
values for the travel when compared to the conventional Eq. 1. In the
extended region, n = 4-14, the conventional Eq. 1 does
better, but the relative error in Eq. 24 is less than 3%.
 |
HYDROCARBON THICKNESS |
To obtain a better understanding of chain packing, it is
especially interesting to compare the average length of the hydrocarbon chains
LC
with half the thickness of the
hydrocarbon chain region
DC
. The latter
quantity is defined by
|
(27)
|
where
A
is the average area per molecule, which
is 61.8 Å2 in this simulation, and
VC is the volume of both hydrocarbon chains,
which has been determined to be 862 Å2 for this
simulation, using the procedure of Petrache et al. (1997)
. Using Eq. 27
then gives
DC
= 13.95 Å. The consistency
of this procedure is indicated in Fig.
10, which shows where
DC
falls on a profile of the hydrocarbon
probability distribution function:
|
(28)
|
where Vn = VCH2
for n = 2-15 and V16 = VCH3. (The flatness of the hydrocarbon
probability distribution in the region
8 Å < z < 8
Å, where the headgroups and water are absent, is the criterion used to
obtain the ratio
VCH3/VCH2, and
then VCH2 comes from the simulated density
of hydrocarbon in this region (Petrache et al., 1997
).) Fig. 10 shows
where
z16
and
z2
fall for the upper monolayer, as well
as the probability distributions for these carbons.

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FIGURE 10
Probability distribution of hydrocarbon chains, using
VCH2 = 26.94 Å3 and
VCH3 = 53.80 Å3. Thick
solid line: Contribution from both monolayers. Dashed
line: Upper monolayer only. Crosses: Average positions
z2 and z16 .
Thin solid lines: Probability distributions for n = 2 and n = 16 (terminal methyl) in the upper
monolayer. Dotted line: Headgroup (including carbonyls,
glycerol, and phosphatidylcholine) probability distribution in the
lower monolayer.
|
|
A major and unexpected result of this simulation is that
LC
determined in the previous section is
numerically very close to
DC
. Although
this result has often been implicitly assumed, it is not a priori
correct, as emphasized by Nagle (1993)
. This point is illustrated in
Fig. 11, which shows three caricatures, each of which packs four chains, two in each monolayer. Because of this
simplicity, the average chain length in these caricatures is just
LC
= (L1 + L2)/2. The distinguishing feature of model I is early
chain termination of chain 1, so L1 < DC, which makes
LC
less
than
DC
. Model I has decreasing order with
increasing n because the terminal methyl end of chain 2 is
more disordered than the carbonyl end, whereas chain 1 is equally
disordered along the chain. The distinguishing feature of model II is
interdigitation across the midplane, which makes
LC
greater than
DC
, and which results in increasing order
with increasing n. Because the experimental order parameter
decreases with increasing n, model I is clearly superior to
model II. However, for this simulation, which has
LC
=
DC
,
model I must be wrong. This has led us to propose model III in Fig. 11.
Model III has both early chain terminations and interdigitation, the
order parameter decreases with increasing n, and
LC
=
DC
, so
model III is the best model for characterizing these simulations.

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FIGURE 11
Three simplified caricatures, labeled I, II, and III,
of packing geometry. For simplicity, only four chains are shown for
each model, but more realistic distribution functions can easily be
envisioned. The four numbered boxes represent the volumes occupied by
each of the four chains. Ignoring upturns, the chains start from the
headgroup end at z = ±DC and end in the
z = 0 region. The order parameter is larger when the
vertical cross section of the box is smaller. Note that these
caricatures are not meant to designate sn-1 versus sn-2 chains.
|
|
 |
AREA PER MOLECULE |
For the present simulation,
A
= 61.8 Å2 is obtained simply by dividing the total area of either
monolayer by the number of lipid molecules in that layer. The issue is
whether this value of
A
can be obtained using the NMR
order parameters. For this simulation, which conforms to chain packing
model III in Fig. 11, this is easily accomplished using Eq. 27 and the
preceding estimates of
LC
for
DC
; this gives the satisfactory result
A
= 862 Å3/14.0 Å = 61.6 Å2.
Because model III may not apply to all bilayers, it is also of interest
to evaluate a different way to obtain
A
that uses only
the low carbon numbers in the so-called plateau region. The usual
formula for this is
|
(29)
|
where VCH2 = 26.94 Å3 is
the volume per methylene group in this simulation, and the factor of 4 accounts for two chains per lipid and for a factor of 2 in
Dn, which, as defined, is really twice the
travel per methylene. Fig. 12 shows the
results from Eq. 29 for
An
versus
n. These values are all too low in the plateau region
n = 3-8.

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FIGURE 12
Estimate of An, using Eq. 29
( ) and Eq. 31 ( ). The horizontal line indicates the actual
simulated area A = 61.8 Å.
|
|
There is a basic mathematical flaw in Eq. 29, which is corrected by
taking the average of the instantaneous area,
An = 4VCH2/Dn; this gives
(Brown, 1996
)
|
(30)
|
The relation
|
(31)
|
shows that
1/Dn
is larger than
1/
Dn
because
Dn2
is larger than
Dn
2. The order parameters are
used to obtain
Dn
(Eq. 24) and
Dn2
(Eq. 13). Fig. 12 shows that
An
obtained using Eq. 31 in the plateau
region is in reasonable agreement with the actual
A
if
one averages
An
over a plateau region
defined to be n = 3-8.
Although the average over n = 3-8 gives the correct
A
, it is important to understand why there is a slope
in
An
. Fig. 3 shows the average positions
zn
, and Fig. 10 shows that there is a
significant fraction of the headgroups at values of
zn
for n = 3-5. Because
these headgroups take up volume and area that is not accounted for by
Eq. 30, this accounts for the smaller values of
An
in Fig. 12. The probability of
headgroups decreases sharply at
zn
for
larger values of n, but Fig. 10 shows that the probability
of terminal methyls increases. These early chain terminations mean that
there is more total area that is shared by fewer chains, which is also
not taken into consideration in Eq. 30; this accounts for the larger
values of
An
in Fig. 12. The chain
termination consideration was known previously (Nagle, 1993
), and this
motivated considering only the plateau region. This simulation shows
that the headgroups must also be considered and that there is hardly
any region that can be said to be free of both artifacts. Although one
can obviously define a plateau region that works for this simulation,
it is not clear if this will be universal for other simulations or for
real lipid bilayers.
 |
DISCUSSION |
The main result in this paper has been the development of Eq. 24,
which gives a new approximation for obtaining methylenic travel
Dn
from NMR order parameters
Sn
. As shown in Fig. 1, this formula fits
the results of this simulation better than older approximations. Of
course, the derivation of Eq. 24 used detailed results of the
probability distribution shown in Fig. 8, and so Eq. 24 can only be
expected to be as good as the simulation. There are results that show
that the
angle for the chains did not come to equilibrium in the
simulation (Fig. 5), although this seems to make only a minor
difference in the tests in Figs. 6 and 7. Furthermore, the results from
the different simulation of Berger et al. (1997)
are in quantitatively
good agreement, and results for chain fragments from three simulations
(Table 1) are in good agreement. Finally, the use of Eq. 24 to predict the chain length is in excellent agreement with the actual chain length
LC
. Nevertheless, Eq. 24 is a sufficiently
radical departure from standard practice that it should be tested on
new and independent simulations of bilayers.
A major surprise is the simulation result that half the mean thickness
of the hydrocarbon chain region
DC
is
numerically close to the average chain length
LC
. Even though this has been an implicit
assumption in NMR studies (Schindler and Seelig, 1975
; Thurmond et al.,
1991
), it is not a priori necessary. In particular, the occurrence of
early chain terminations (model I in Fig. 11) would, by itself, require
LC
to be smaller than
DC
. However, the effect of early chain
terminations appears to be canceled by the effect of interdigitation,
as illustrated by model III in Fig. 11.
The result
DC
=
LC
leads to a simple way of estimating
area per molecule
A
using Eq. 27. This reproduces the
actual
A
in this simulation. This would be a very nice
result, except that it leads to a disagreement. This procedure gave
ADPPC
= 71.7 Å2 for DPPC at
50°C (Thurmond et al., 1991
). Of course, the NMR study used the older
Eq. 1, but we have shown in the third section of this paper that, for
this simulation, the significant deviations in this formula for
individual carbons n (see Fig. 9) average out, so that the
total chain length
LC
is quite well
approximated by either Eq. 1 or Eq. 24. Therefore, the results in this
paper support the method used by Thurmond et al. (1991)
. However, their result for
ADPPC
is 14% larger than the
value
ADPPC
= 62.9 Å2
obtained from x-ray studies (Nagle et al., 1996
).
We have examined this disagreement further for DMPC. Two recent studies
have agreed that
ADMPC
= 59.6 ± 0.5 Å2 for DMPC at T = 30°C. Our study
(Petrache et al., 1998
) used the same x-ray method as used for DPPC.
The other study (Koenig et al., 1997
) combined x-ray and NMR results,
but only changes in
LC
were obtained from
NMR order parameters because of the concern that no formula was
adequate to give absolute numbers. Because these two studies used quite
different methods and assumptions, we believe that the common value of
ADMPC
that was obtained is a reliable
benchmark for testing present NMR formulae.
We used the order parameters obtained by Koenig et al. (1997)
at
T = 30°C in Eqs. 24 to estimate
Dn
, which were then added up, using Eq. 26, to obtain
LC
= 11.95 Å. We then
assumed that
DC
=
LC
in Eq. 27. We also used
VC = 782 Å3, which was
obtained by subtracting the headgroup volume VH = 319 Å3 (Sun et al., 1994
) from the lipid volume
VL = 1101 Å3 (Nagle and Wilkinson,
1978
). The result obtained with Eq. 27 is
ADMPC
= 65.4 Å2, 10% higher
than obtained previously. Using the conventional Eq. 1 instead of Eq. 24 reduces this marginally to
ADMPC
= 64.3 Å2. Using the plateau method described in the previous
section and averaging
An
over n = 3-8 gives
ADMPC
= 65.2 Å2. Therefore, for DMPC, the methods that work so well for
this simulation give values for
ADMPC
that
are too large.
The resolution of this disagreement may involve several issues. The
first and most obvious is whether this simulation is misleading. Clearly, other simulations should be analyzed with NMR interpretation in mind. This involves testing Eq. 24, which also has implications for
changes in chain length used by Koenig et al. (1997)
. It also involves
testing
LC
=
DC
and Eq. 27. Of course, it is possible that all simulations will give the same but not the correct answer to
the issue of equality of
LC
and
DC
because chain packing, as contrasted
with chain conformational order, does not equilibrate in the nanosecond
time range. In this regard NMR studies indicate slower, collective
motions (Nevzorov et al., 1998
). It may be noted that the simulation
studied in this paper was a particularly long one, although a new
hybrid Monte Carlo/molecular dynamics method may, in the future,
overcome some equilibration barriers (Clark et al., 1999
). Perhaps one
might also question whether, because of subtle effects of relative time
scales (Brown, 1996
), NMR may not measure the same instantaneous order
parameters that are obtained straightforwardly from simulations.
Measured NMR order parameters that are only ~10% too low would also
account for the disagreement.
We have not yet achieved the desired goal of being able to advocate an
analysis method that can use NMR order parameters to quantitate bilayer
structure. Nevertheless, flaws in previous