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Biophys J, May 1999, p. 2479-2487, Vol. 76, No. 5

Analysis of Simulated NMR Order Parameters for Lipid Bilayer Structure Determination

Horia I. Petrache,* Kechuan Tu,# and John F. Nagle*§

 *Department of Physics and  §Department of Biological Sciences, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, and  #Department of Pharmacological Chemistry, University of California, San Francisco, California 94143 USA

    ABSTRACT
TOP
ABSTRACT
INTRODUCTION
METHYLENE TRAVEL
AVERAGE CHAIN LENGTH
HYDROCARBON THICKNESS
AREA PER MOLECULE
DISCUSSION
REFERENCES

The conventional formula for relating CD2 average order parameters < Sn> to average methylenic travel < Dn> is flawed when compared to molecular dynamics simulations of dipalmitoylphosphatidylcholine. Inspired by the simulated probability distribution functions, a new formula is derived that satisfactorily relates these quantities. This formula is used to obtain the average chain length < LC> , and the result agrees with the direct simulation result for < LC> . The simulation also yields a hydrocarbon thickness 2< DC> . The result < LC>  = < DC> is consistent with a model of chain packing with both early chain termination and partial interdigitation of chains from opposing monolayers. The actual simulated area per lipid < A> is easily obtained from the order parameters. However, when this method is applied to NMR order parameter data from dimyristoylphosphatidylcholine, the resulting < A> is 10% larger than the currently accepted value.

    INTRODUCTION
TOP
ABSTRACT
INTRODUCTION
METHYLENE TRAVEL
AVERAGE CHAIN LENGTH
HYDROCARBON THICKNESS
AREA PER MOLECULE
DISCUSSION
REFERENCES

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
⟨D<SUB><UP>n</UP></SUB>⟩/D<SUB><UP>M</UP></SUB>=(1−2⟨S<SUB><UP>n</UP></SUB>⟩)/2, (1)
where DM is the maximum possible travel. A different relation has also been used (De Young and Dill, 1988):
⟨D<SUB><UP>n</UP></SUB>⟩/D<SUB><UP>M</UP></SUB>=(1−4⟨S<SUB><UP>n</UP></SUB>⟩)/3. (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
TOP
ABSTRACT
INTRODUCTION
METHYLENE TRAVEL
AVERAGE CHAIN LENGTH
HYDROCARBON THICKNESS
AREA PER MOLECULE
DISCUSSION
REFERENCES

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>  approx  -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(zD). 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
D<SUB><UP>n</UP></SUB>=z<SUB><UP>n−1</UP></SUB>−z<SUB><UP>n+1</UP></SUB>, (3)
as illustrated in Fig. 2. From the distribution function pn(zD) the average position of carbon n is given as
⟨z<SUB><UP>n</UP></SUB>⟩=<LIM><OP>∬</OP></LIM>zp<SUB><UP>n</UP></SUB>(z, D)<UP>d</UP>z <UP>d</UP>D.  (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, theta  defines the local methylenic tilt, and psi  defines the rotation about the local methylene axis z'. Note that the local axis is generally different for each carbon n.



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FIGURE 3   Average carbon position < zn> (solid squares, in Å) for all chains.

For many purposes it suffices to consider only the reduced distribution function
p<SUB><UP>n</UP></SUB>(D)=<LIM><OP>∫</OP></LIM>p<SUB><UP>n</UP></SUB>(z, D)<UP>d</UP>z. (5)
For example, the average travel of carbon n, irrespective of where it is, is then given by
⟨D<SUB><UP>n</UP></SUB>⟩=<LIM><OP>∫</OP></LIM>Dp<SUB><UP>n</UP></SUB>(D)<UP>d</UP>D. (6)
It is also important to consider the mean square travel,
&Dgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>≡⟨D<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>⟩=<LIM><OP>∫</OP></LIM>D<SUP>2</SUP>p<SUB><UP>n</UP></SUB>(D)<UP>d</UP>D. (7)
These quantities are shown in Fig. 4.



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FIGURE 4   Simulated data for Delta n () and < Dn> (open circle ) averaged for all chains.

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 theta  with the bilayer normal along z. Rotation around the local axis z' is measured by the angle psi . 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:
S<SUB><UP>n</UP></SUB>=½<UP>sin</UP><SUP>2</SUP>&psgr;−½(1+<UP>sin</UP><SUP>2</SUP>&psgr;)<UP>cos</UP><SUP>2</SUP>&thgr;, (8)
where cos theta  = 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 sin2psi , for which average values for narrow ranges of D are given by
⟨<UP>sin</UP><SUP>2</SUP>&psgr;<SUB><UP>n</UP></SUB>(D)⟩≡<LIM><OP>∫</OP></LIM><UP>sin</UP><SUP>2</SUP>&psgr;<SUB><UP>n</UP></SUB>(D)p<SUB><UP>n</UP></SUB>(D, &psgr;)<UP>d</UP>&psgr;. (9)
Fig. 5 shows values of < sin2psi n(D)> for two values of n for the upper and lower monolayers separately. The fact that < sin2psi 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 < sin2psi n(D)> was less than 0.5. 



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FIGURE 5   Simulated < sin2psi n(D)> as a function of D for n = 6 (triangle , down-triangle) and n = 12 (black-triangle, black-down-triangle ) averaged over sn-1 and sn-2 chains. triangle , black-triangle, The upper monolayer; down-triangle, black-down-triangle , the lower monolayer.

After integration of Eq. 8 over psi , the average order parameter
⟨S<SUB><UP>n</UP></SUB>(D)⟩=<LIM><OP>∫</OP></LIM>S<SUB><UP>n</UP></SUB>(D, &psgr;)p<SUB><UP>n</UP></SUB>(D, &psgr;)<UP>d</UP>&psgr; (10)
becomes
⟨S<SUB><UP>n</UP></SUB>(D)⟩=½⟨<UP>sin</UP><SUP>2</SUP>&psgr;<SUB><UP>n</UP></SUB>(D)⟩−½(1+⟨<UP>sin</UP><SUP>2</SUP>&psgr;<SUB><UP>n</UP></SUB>(D)⟩)(D/D<SUB><UP>M</UP></SUB>)<SUP>2</SUP>. (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 < sin2psi n(D)> . Clearly, the curve using a random distribution < sin2psi 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 (open circle ) are compared to Eq. 11------, the result for < sin2psi (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 < sin2psi n(D)>  = 0.5. Then,
⟨S<SUB><UP>n</UP></SUB>(D)⟩=<FR><NU>1</NU><DE>4</DE></FR><FENCE>1−3<FENCE><FR><NU>D</NU><DE>D<SUB><UP>M</UP></SUB></DE></FR></FENCE><SUP>2</SUP></FENCE>. (12)
Further integration over D yields the usual average order parameters,
⟨S<SUB><UP>n</UP></SUB>⟩=<FR><NU>1</NU><DE>4</DE></FR> <FENCE>1−3<FENCE><FR><NU>&Dgr;<SUB><UP>n</UP></SUB></NU><DE>D<SUB><UP>M</UP></SUB></DE></FR></FENCE><SUP>2</SUP></FENCE>. (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 Delta n.



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FIGURE 7   Comparison of < Sn> obtained from Eq. 13 (+) with directly simulated < Sn> (open circle ).

Equation 12 emphasizes that < Sn(D)> is a quadratic function of D, so that < Sn> is a function of < Dn2>  = Delta 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 Delta n:
⟨D<SUB><UP>n</UP></SUB>⟩≈&Dgr;<SUB><UP>n</UP></SUB>=D<SUB><UP>M</UP></SUB><RAD><RCD><FR><NU>1−4⟨S<SUB><UP>n</UP></SUB>⟩</NU><DE>3</DE></FR></RCD></RAD>, (14)
where the equality comes from inverting Eq. 13. This is a poor approximation, as shown first by Fig. 4, which compares < Dn> and Delta n, and, more importantly, by the lower curved line in Fig. 1. The reason for this is that Delta n is generally greater than < Dn> because pn(D) has a nonzero width sigma n:
&sfgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>≡⟨(D<SUB><UP>n</UP></SUB>−⟨D<SUB><UP>n</UP></SUB>⟩)<SUP>2</SUP>⟩=&Dgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>−⟨D<SUB><UP>n</UP></SUB>⟩<SUP>2</SUP>. (15)
Because sigma 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 sigma n for larger n, as indicated by the increasing difference between Delta n and < Dn> in Fig. 4, but they are not the fundamental problem.

To calculate Dn from Delta n, we need a way to estimate the mean square deviation sigma 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:
p<SUB><UP>n</UP></SUB>(D)=𝒫<SUB><UP>n</UP></SUB>e<SUP><UP>D/&lgr;<SUB>n</SUB></UP></SUP>, <UP>for</UP> D≤D<SUB><UP>M</UP></SUB>. (16)
The relevant parameter is the decay length lambda n, and the parameter Pn is just a normalization factor. It may be noted that the decay length lambda 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
&Dgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>=𝒫<SUB><UP>n</UP></SUB><LIM><OP>∫</OP><LL><UP>−D</UP><SUB><UP>M</UP></SUB></LL><UL><UP>D<SUB>M</SUB></UP></UL></LIM>D<SUP>2</SUP>e<SUP><UP>D/&lgr;<SUB>n</SUB></UP></SUP><UP>d</UP>D (17)

=D<SUP><UP>2</UP></SUP><SUB><UP>M</UP></SUB>+2&lgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>−2&lgr;<SUB><UP>n</UP></SUB>D<SUB><UP>M</UP></SUB> <UP>tanh</UP> <FR><NU>D<SUB><UP>M</UP></SUB></NU><DE>&lgr;<SUB><UP>n</UP></SUB></DE></FR>

⟨D<SUB><UP>n</UP></SUB>⟩=𝒫<SUB><UP>n</UP></SUB><LIM><OP>∫</OP><LL><UP>−D</UP><SUB><UP>M</UP></SUB></LL><UL><UP>D<SUB>M</SUB></UP></UL></LIM>De<SUP><UP>D/&lgr;<SUB>n</SUB></UP></SUP><UP>d</UP>D=D<SUB><UP>M</UP></SUB><UP>tanh</UP><FR><NU>D<SUB><UP>M</UP></SUB></NU><DE>&lgr;<SUB><UP>n</UP></SUB></DE></FR>−&lgr;<SUB><UP>n</UP></SUB>. (18)
With no further approximation, Eq. 17 can be solved numerically to give lambda n. However, analytical expressions are more appealing, and for this reason we extend the above integrals from -DM to -infinity (valid for lambda n << DM). Then,
&Dgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>=D<SUP><UP>2</UP></SUP><SUB><UP>M</UP></SUB>+2&lgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>−2&lgr;<SUB><UP>n</UP></SUB>D<SUB><UP>M</UP></SUB> (19)

⟨D<SUB><UP>n</UP></SUB>⟩=D<SUB><UP>M</UP></SUB>−&lgr;<SUB><UP>n</UP></SUB> (20)

&sfgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>=&lgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>. (21)
Solving for lambda n in terms of Delta n yields
&sfgr;<SUB><UP>n</UP></SUB>=&lgr;<SUB><UP>n</UP></SUB>=½<FENCE>D<SUB><UP>M</UP></SUB>−<RAD><RCD>2&Dgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>−D<SUP><UP>2</UP></SUP><SUB><UP>M</UP></SUB></RCD></RAD></FENCE> (22)

⟨D<SUB><UP>n</UP></SUB>⟩=½<FENCE>D<SUB><UP>M</UP></SUB>+<RAD><RCD>2&Dgr;<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>−D<SUP><UP>2</UP></SUP><SUB><UP>M</UP></SUB></RCD></RAD></FENCE>. (23)
The square roots above are imaginary for Delta n2 < DM2/2, and this sets a limit to the applicability of Eq. 23. For such small values of Delta n2 most of our previous approximations are questionable. In this limit, lambda 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 Delta n2 = DM2/3; this is only a little less than the applicability limit, so the restriction Delta 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> :
<FR><NU>⟨D<SUB><UP>n</UP></SUB>⟩</NU><DE>D<SUB><UP>M</UP></SUB></DE></FR>=<FR><NU>1</NU><DE>2</DE></FR><FENCE>1+<RAD><RCD><FR><NU><UP>−</UP>8⟨S<SUB><UP>n</UP></SUB>⟩−1</NU><DE>3</DE></FR></RCD></RAD></FENCE>, (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 lambda 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
TOP
ABSTRACT
INTRODUCTION
METHYLENE TRAVEL
AVERAGE CHAIN LENGTH
HYDROCARBON THICKNESS
AREA PER MOLECULE
DISCUSSION
REFERENCES

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:
⟨L<SUP>*</SUP><SUB><UP>C</UP></SUB>⟩≡⟨z<SUB>2</SUB>⟩−⟨z<SUB>16</SUB>⟩. (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
⟨L<SUB><UP>C</UP></SUB>⟩=(1/2)<LIM><OP>∑</OP><LL><UP>n=2</UP></LL><UL><UP>15</UP></UL></LIM>⟨D<SUB><UP>n</UP></SUB>⟩+⟨D<SUB>15</SUB>⟩, (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%.


                              
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TABLE 1   Comparison of partial chain lengths from different simulations (direct) and estimates using Eqs. 24 and 1

    HYDROCARBON THICKNESS
TOP
ABSTRACT
INTRODUCTION
METHYLENE TRAVEL
AVERAGE CHAIN LENGTH
HYDROCARBON THICKNESS
AREA PER MOLECULE
DISCUSSION
REFERENCES

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
⟨D<SUB><UP>C</UP></SUB>⟩≡<FR><NU>V<SUB><UP>C</UP></SUB></NU><DE>⟨A⟩</DE></FR>, (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:
P<SUB><UP>HC</UP></SUB>(z)=<LIM><OP>∑</OP><LL><UP>n=2</UP></LL><UL><UP>16</UP></UL></LIM> V<SUB><UP>n</UP></SUB>p<SUB><UP>n</UP></SUB>(z), (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
TOP
ABSTRACT
INTRODUCTION
METHYLENE TRAVEL
AVERAGE CHAIN LENGTH
HYDROCARBON THICKNESS
AREA PER MOLECULE
DISCUSSION
REFERENCES

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
⟨A<SUB><UP>n</UP></SUB>⟩=4V<SUB><UP>CH</UP><SUB><UP>2</UP></SUB></SUB>/⟨D<SUB><UP>n</UP></SUB>⟩, (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 (open circle ) 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)
⟨A<SUB><UP>n</UP></SUB>⟩=4V<SUB><UP>CH</UP><SUB><UP>2</UP></SUB></SUB>⟨1/D<SUB><UP>n</UP></SUB>⟩. (30)
The relation
<FENCE><FR><NU>1</NU><DE>D<SUB><UP>n</UP></SUB></DE></FR></FENCE>=<FENCE><FR><NU>1</NU><DE>⟨D<SUB><UP>n</UP></SUB>⟩+(D<SUB><UP>n</UP></SUB>−⟨D<SUB><UP>n</UP></SUB>⟩)</DE></FR></FENCE> (31)

≈<FR><NU>1</NU><DE>⟨D<SUB><UP>n</UP></SUB>⟩</DE></FR>+<FR><NU>⟨(D<SUB><UP>n</UP></SUB>−⟨D<SUB><UP>n</UP></SUB>⟩)<SUP>2</SUP>⟩</NU><DE>⟨D<SUB><UP>n</UP></SUB>⟩<SUP>3</SUP></DE></FR>

=<FR><NU>1</NU><DE>⟨D<SUB><UP>n</UP></SUB>⟩</DE></FR> <FR><NU>⟨D<SUP><UP>2</UP></SUP><SUB><UP>n</UP></SUB>⟩</NU><DE>⟨D<SUB><UP>n</UP></SUB>⟩<SUP>2</SUP></DE></FR>
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
TOP
ABSTRACT
INTRODUCTION
METHYLENE TRAVEL
AVERAGE CHAIN LENGTH
HYDROCARBON THICKNESS
AREA PER MOLECULE
DISCUSSION
REFERENCES

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 psi  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