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Wero
ski * 

* Theoretical Division and Center for Nonlinear Studies, and
Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, New Mexico;
Institute of Catalysis and Surface Chemistry, Polish Academy of Sciences, Kraków, Poland; and
Santa Fe Institute, Santa Fe, New Mexico
Correspondence: Address reprint requests to Pawe
Wero
ski, Theoretical Division, Los Alamos National Laboratory, MS-B284, Los Alamos, NM 87545. Tel.: 505-667-9956; Fax: 505-665-2659; E-mail: pawel{at}lanl.gov.
| ABSTRACT |
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T ensemble, two similar PNA molecules (6-mers) with the same nucleic base sequence and different terminal groups are investigated at the interface between water and a 1-palmitoyl-2-oleoylphosphatidylcholine lipid bilayer. The results of our simulations suggest that at low ionic strength of the solution, both PNA molecules adsorb at the lipid-water interface. In the case where the PNA molecule has charged terminal groups, the main driving force of adsorption is the electrostatic attraction between the charged groups of PNA and the lipid heads. The main driving force of adsorption of the PNA molecule with neutral terminal groups is the hydrophobic interaction of the nonpolar groups. Our simulations suggest that the system free energy change associated with PNA adsorption at the lipid-water interface is on the order of several tens of kT per PNA molecule in both cases. | INTRODUCTION |
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Recently, due to PNA's neutral backbone, a new potential application emerged. PNA or backbone modified lipophilic PNA can act as the genetic material in a minimal self-replicating nanomachine or protocell design proposed by Rasmussen and Chen (3
,4
). According to this design, a minimal protocell able to utilize resources, grow, self-replicate, and evolve could be as simple as a small lipid aggregate (micelle) acting as a container by anchoring a PNA molecule to its exterior and a photosensitizer to its interior. In such a protocell, light-driven metabolic processes from the lipid aggregate interior could synthesize lipids and PNA, from appropriate precursor molecules with PNA acting as both an information carrier and as a catalyst, leading to a spontaneous growth of the protocell. Micellar lipid clusters in water are thermodynamically stable below some critical size only; therefore the growing containers would divide as soon as they become large enough, providing the next generation of the protocells.
To verify this scenario we need to answer a number of important questions. Unlike DNA or RNA, our knowledge of PNA is still relatively limited and a number of important issues have not been addressed so far. One of them is whether PNA molecules at high local concentrations are going to spontaneously gather at a lipid-water interface, and if not, how hydrophobic the PNA backbone has to be before such an attachment occurs. The PNA-lipid attachment is a sine qua non condition for the protocell replication process. Molecular dynamics (MD) computer simulation is a suitable method for addressing this problem. This technique has been exploited with a significant success in many areas of bioscience and bioengineering, including some recent PNA-related phenomena (5
,6
). MD simulation is also one of the main tools used in theoretical studies of membranes and lipid bilayers (7
). In this article we present results of our MD simulations on the affinity of a small PNA molecule to a lipid-water interface.
| METHODS |
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Topology and parameterization
Unfortunately, the topology and parameters for PNA residues are not directly available in the standard molecular dynamics packages such as CHARMM (11
) because PNA molecules are not natural or common. To the best of our knowledge, only two sets of parameters for PNA have been published in the literature (12
14
). Both parameter sets, however, seem to be a little inconsistent with each other. More importantly, some of the parameters in these sets are different than parameters found in CHARMM27 parameter file for similar chemical structures (compare, e.g., partial atomic charges for the peptide bond). Therefore, to be consistent with the other parameters used in our simulations, we have obtained the parameters in PNA residues by comparison with similar chemical groups found in the CHARMM27 parameter file (15
21
). We have also assigned the atom types of the atoms involved in PNA residues as reported in Sen and Nilsson (13
), to follow CHARMM atom type definitions (see Fig. 1). This effort makes most of the bond, angle, and dihedral and all of the nonbonded parameters directly available from the combined CHARMM all-hydrogen parameter set for nucleic acids, lipids, and proteins. These, which are not available directly, are listed in the Supplementary Material. Corresponding topology and parameters files for NAMD calculations are also available upon request. Our force-field parameters have been tested in ongoing simulations of PNA partition in water-octanol system and the experimentally verified results will be published elsewhere.
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4-ns-long simulation at constant temperature, constant pressure component normal to xy plane, and constant area of the unit cell in this plane. At this stage of the simulation, the dimensions of the unit cell in the directions x and y were fixed at 4.743 nm that allowed the bilayer to expand to this size, which corresponds to the molecular area 0.625 nm2 per lipid found in experiments (24
the molecular area was
which fitted best the experimental result. Therefore, all the further simulations involving the lipid bilayer were conducted at this specific value of the surface tension.
The coordinates of the atoms in the single-stranded 6-mer PNA with the base sequence C1G1TAC2G2 were extracted from the crystal structure of the corresponding PNA duplex (Protein Data Bank identifier 1PUP (25
)). The coordinates of the missing H-atoms of the PNA molecule were generated by the GUESSCOORD facility of VMD. We created two PNA molecules with the same base sequence and different terminal groups. One of them, hereafter referred to as s-PNA, has standard C- and N-terminus, i.e., the charged groups COO and
respectively. The second molecule that we will call a-PNA has two neutral termini: amidated C-terminus NH2 and acetylated N-terminus COCH3 (see Fig. 2). Each of the molecules was solvated in water and equilibrated for 40 ns at constant temperature, pressure, and cross-section area. The size of the simulation boxes in the directions x and y was fixed at the value corresponding to the size of the lipid bilayer, i.e., at 4.743 x 4.743 nm. The z dimension of the box fluctuated around 3.9 nm.
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It should be noted that our systems are different than experimental systems that have been studied so far, e.g., in the PNA vesicle encapsulation experiments (26
). First of all, there is no salt or electrolyte in our systems and the lipid-water interface in our simulations is electrostatically neutral. In contrary, the experimental systems have usually been studied at the buffer concentration on the order of at least several millimolar and the measured surface potential of the lipid-water interface is on the order of 102mV (26
). This large value of the interface surface potential suggests that strong ion adsorption or desorption can take place at the interface, which in turn can produce a compact hydration layer and influence the PNA molecule behavior at the interface. Indeed, preliminary results of our simulations of the lipid bilayer at ionic strength on the order of fraction of mol/dm3 suggest that this is the case. It should also be noted that because of the MD length-scale limitation the PNA and lipid concentrations in our systems are equal to
102 M and 0.7 M, respectively, and so they are very high compared to the experimental conditions.
Molecular dynamics protocols
We employed NAMD (version 2.6b1) with its standard empirical potential energy function (8
). We used periodic boundary conditions and the particle mesh Ewald (PME) approach (27
,28
) for evaluating long-range electrostatic effects. The distance between subsequent grid points on the mesh was
0.1 nm. A time step of 2 fs was used for the integration of Newton's equations, since all the bond lengths between each hydrogen atom and the atom to which it was covalently bonded were constrained to their equilibrium values using the SHAKE algorithm (29
). A cutoff at 1.2 nm was used for the Lennard-Jones interactions and for electrostatics with smoothing functions activated at a switching distance 1.0 nm. The nonbonded pair list was updated every 10 steps and the maximum distance between atoms for inclusion in the list was 1.35 nm. The long-range Coulombic forces were updated every two steps. For electrostatic calculations a relative dielectric constant of 1.0 was used; 1-2 and 1-3 nonbonded interactions were excluded; 1-4 electrostatic interactions were taken into account without any modification and 1-4 van der Waals parameters were modified according to the CHARMM27 parameter file.
Simulations were carried out in the ensemble NPn
T at the constant pressure component normal to the lipid-water interface
surface tension
and temperature
Constant temperature was maintained by using the Langevin dynamics method (30
). We applied the Langevin damping coefficient to nonhydrogen atoms only. Its value was setup to 5/ps for the first 4000 time steps, when our systems were far from equilibrium. Then the coefficient was fixed at 1/ps. A combination of the Nose-Hoover constant pressure method (31
) with piston fluctuation control implemented using Langevin dynamics (32
) was used to control the pressure along the z axis and the surface tension in the xy plane. The Langevin piston oscillation period and the oscillation decay time were equal to 100 fs and 50 fs, respectively. The constant ratio of the unit cell dimensions in the xy plane was kept during the simulations while allowing cell shape fluctuations along all axes. The pressure was calculated using the hydrogen-group-based pseudomolecular virial and kinetic energy (useGroupPressure option of NAMD) in conjunction with the SHAKE algorithm.
Calculation of the free energy
We calculated the free energy change in our systems using several different methods. The first method was based on the adaptive biasing force (ABF) approach (33
). This method, implemented as a suite of Tcl routines directly available from the main configuration file used to run molecular dynamics simulations with NAMD, efficiently calculates the potential of mean force
acting between two groups of atoms along a reaction coordinate
, and applies ABFs that are needed to overcome free energy barriers and provide uniform sampling. This potential of the mean force is a measure of the system's free-energy change
G corresponding to the change in the reaction coordinate of a system from
1 to
2:
![]() | (1) |

i is the width of the bin over which the force is averaged. As discussed in the section "Mean force and the free energy profile", however, results of our simulations suggest that any biasing force acting on a flexible molecule like PNA or molecular structure such as the lipid bilayer can disturb its conformation and thus cause additional change of the free energy of the system. Therefore, to avoid the effect of the biasing force on the free energy calculation, we conducted our simulations monitoring the system's free energy without introducing any bias (applyBias option of NAMD).
The second method is strictly applicable to a system at equilibrium. Using the simulation data we can calculate the time evolution of the reaction coordinate and find the density of the distribution of this coordinate:
![]() | (2) |
) is the number of the microstates of the system in which the value of the reaction coordinate is smaller than
, and
ni is the number of the force measurements in the bin 
i. The last equality is correct for large numbers
ni and small width of the bins 
i. If the system is near equilibrium we can use the distribution density of the reaction coordinate
to calculate the change of the system free energy associated with the change of this coordinate. According to the Boltzmann relationship
![]() | (3) |
is the change of the reaction coordinate and the free energy is expressed in kT units. The change of the system free energy
G corresponding to the change in the reaction coordinate of the system from
1 to
2 can be calculated from Eq. 3 as
![]() | (4) |
If the width of the bin 
i is constant, the change of the system free energy can be calculated from the formula
![]() | (5) |
ni1 and
ni2 are the numbers of force measurements collected in the bins corresponding to the reaction coordinates
1 and
2, respectively. Equation 5 is convenient because the numbers
ni are directly available in ABF calculations with NAMD. Note that if the free energy changes by more then few kT units in the whole reaction-coordinate interval of interest then the ABF simulation with no biasing force applied will take a very long time. To avoid this inconvenience the whole interval of reaction coordinate should be divided into smaller pieces, in which the free energy varies little, with a harmonic bias enforced at their borders (forceConst parameter of NAMD).
As the reaction coordinate we chose the distance along the axis z between a PNA molecule and one of the lipid-water interfaces. Specifically, we calculated the z coordinate of the PNA molecule by averaging the z coordinates of its selected 14 atoms. These were six atoms of the nucleic bases (O4, N4, N6, and O6 in the residues thymine, cytosine, adenine, and guanine, respectively), six atoms N2' of the backbone, and two atoms of the terminal groups: N1' and C1' of the s-PNA molecule, and NT and CAY of the a-PNA molecule. The z coordinate of the lipid-water interface was calculated by averaging the z coordinates of the 36 N atoms and the 36 P1 atoms in this interface. The mean force was calculated between the 14 atoms of the PNA molecule and the 72 atoms of the lipid bilayer. The width of the bins in which the forces are accumulated has to be small enough to ascertain that the free energy profile varies regularly in the
-interval. On the other hand, it should be large enough to ensure sufficient sampling and avoid large fluctuations in the average force. In our system we used the bin width equal to 10 pm, which allowed us to collect the number of force samples in most of the bins on the order of 105106. To decrease the force fluctuation we averaged the mean force over 20 pm (dSmooth parameter of NAMD).
As discussed in the next section, the molecule s-PNA adsorbs rapidly and forms hydrogen bonds with the charged groups of the lipid molecules that can be easily identified. In this system we can use yet another approach to estimate the PNA adsorption free energy. We can estimate the change of the system free energy by summing up the free energy of these bonds. When the s-PNA molecule adsorbs at the interface during the first nanosecond of the simulation and its distance from the interface does not evolve in a systematic way, we can assume that the system is at equilibrium after the first several nanoseconds and use Eq. 4 to calculate the free energy of each of the bonds. In these calculations we can assume that the lengths of the formed hydrogen bonds are uncorrelated and use the distance between the atoms forming a specific hydrogen bond as the reaction coordinate.
| SIMULATION RESULTS AND DISCUSSION |
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PNA distance from the lipid interface
The time evolution of the mean distance of the s-PNA molecule from the interface is presented in Fig. 3 a and in Fig. 3 b the final configuration is shown at
The distance fluctuates around the mean value
No systematic drift of the distance can be observed in the timescale of the conducted simulation. From the simple linear regression analysis conducted over the entire time of the simulation we find that the slope of the dashed regression line is very small and equal to 0.20 ± 0.02 mm/s. The molecule approaches the interface quickly (in the first nanosecond of the simulation) and does not leave its position at the interface. Dash-dot-dot lines denote the mean distances of the 14 individual atoms of the molecule from the interface. The values of the mean distance and its standard deviation are listed in Table 1. Based on these data we can conclude that the molecule s-PNA is attached to the interface with its positively charged N-terminus, whereas the negatively charged C-terminus is pushed away from the interface.
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The time evolution of the mean distance of the a-PNA molecule from the interface is presented in Fig. 4 a and the final configuration is shown in Fig. 4 b at
Unlike the s-PNA molecule, the a-PNA molecule approaches the interface relatively slowly. Between 100 and 120 ns the molecule is even detached from the interface. We note a systematic drift of the mean distance of the a-PNA molecule from the interface toward smaller values. Slope of the dashed regression line calculated from the linear regression analysis of the simulation results is equal to 2.433 ± 0.012 mm/s. This large and negative value of the slope suggests that the molecule slowly sinks into the interface. Therefore, to achieve the equilibrium conformation of the system, we continued this simulation for a longer time until we saw that the free energy profile did not change any more, as discussed below. The mean distance of the a-PNA molecule from the interface, calculated in the time interval between 250 and 350 ns, fluctuates around the value
Thus, the distance is smaller by
0.5 nm than that of the s-PNA molecule. Dash-dot-dot lines denote the mean values of the distance between the 14 individual atoms of the a-PNA molecule and the interface. The distances and their standard deviations are listed in Table 2. Based on these data we can conclude that the a-PNA molecule is attached to the interface with its hydrophobic groups, namely the acetylated N-terminus and amidated C-terminus. The smallest value of the z coordinate is that of the atom O4 of thymine. The collected frames of the simulation suggest that this is because there is a hydrogen bond between this atom and the N-terminus of the a-PNA molecule. Thus, the terminal groups of the molecule as well as the thymine base in the central part of the molecule sink into the interface. Therefore we can conclude that the main driving force of a-PNA adsorption is the hydrophobic interaction. Note that all values of the standard deviation listed in Table 2 are smaller than those in Table 1, which suggests that although the a-PNA adsorption process is slower than that of s-PNA, it eventually results in a stronger attachment of the molecule to the interface.
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3% than that for the system with s-PNA. This may result from sinking of the hydrophobic parts of the a-PNA molecule into the internal part of the bilayer, as discussed in the previous section. The difference between both molecular areas, however, is below the calculated standard deviation. Therefore longer simulations would be necessary to verify this hypothesis.
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2 kT units. Therefore, it is difficult to predict an exact depth of the free energy minimum based on the results obtained in our simulations.
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For a comparison, two free energy profiles calculated with Eq. 1 and nonzero biasing force are presented in Fig. 6 b as well. The profiles correspond to adsorption and desorption of a-PNA molecule. Both profiles are quite different from the profiles obtained with no biasing force applied. The adsorption free energy profile calculated with the biasing force is shifted toward the larger distance z by
0.5 nm. This shift is a direct consequence of pushing a-PNA molecule toward the interface, which does not allow a sufficient equilibration of the lipid bilayer. Therefore, the rapid increase of the adsorption free energy below
represents mainly the change of the system free energy corresponding to the deformation of the lipid bilayer under nonequilibrium conditions. The desorption free energy, on the other hand, increases monotonically with the distance z. This change of the system free energy results from a stretching of a-PNA molecule mainly and is not a good estimate of the PNA adsorption free energy as well.
The results obtained with the applied biasing force suggest therefore that the ABF method is not well suitable for calculating the system free energy change in the case of flexible molecules or molecular structures in general. In its classical formulation, the method can offer an accurate estimation of desorption energy only if there is a single, well-defined bond between the molecule and the interface, which can be chosen as the reaction coordinate. If there are a number of bonds between the molecule and the interface, however, calculating the free energy of a single bond will inevitably result in a deformation of the molecule and in an additional change of the system free energy. The applicability of the method can be improved through additional harmonic constraints applied to the flexible parts of the simulated system (P. Wero
ski and Y. Jiang, unpublished data).
As discussed above, the results presented in Fig. 3 a suggest that the main driving force of s-PNA adsorption at the lipid-water interface is the electrostatic attraction between these atoms of the POPC molecules and s-PNA molecule, which bear high partial atomic charges and form hydrogen bonds. Therefore, to estimate the s-PNA adsorption free energy more accurately, we used the approach based on the summation of the free energy of the hydrogen bonds formed between the PNA molecule and the interface. We used this method to calculate the depth of the free energy primary minima for selected 14 atoms of the first two residues, C1 and G1, which approach the lipid-water interface the most. We chose the atoms identified as hydrogen bond donors or acceptors: N1' that is the N-terminus nitrogen atom, O1', O2, N3, N4, and O3' of the cytosine; and N2, O3', N3, O6, N7, O1', H1', and H1 of the guanine.
Note that in case of the atoms N4 of the cytosine and N2 of the guanine, which are covalently bonded to more than one hydrogen atom, we calculated the distribution density of the distances between the nitrogen atoms and the nearest oxygen atom of the phosphate groups. In case of atoms N1 and N1' of guanine, which are covalently bonded to single hydrogen atoms, we calculated the distribution density of the distances between these hydrogen atoms, H1 and H1', and the nearest oxygen atom O3 or O4 instead. The other nine of the chosen 14 atoms, namely O2, N3, O1', and O3' of the cytosine; and N3, O6, N7, O1', and O3' of the guanine; formed hydrogen bonds with the hydrogen atoms of the lipid amine groups. For these atoms, the distribution density of the distance between them and the nearest hydrogen atom of the POPC amine groups was calculated.
The time evolution of the distance rN1'C1 between the nitrogen atom N1' of the cytosine C1, to which the terminal hydrogen atoms HT1 through HT3 are bonded, and the nearest of the oxygen atoms O3 and O4 of the POPC molecules is presented in Fig. 7 a. The distribution density
(rN1'C1) calculated with Eq. 2 for our system at
is presented in Fig. 7 b. We chose the intervals of the distance rN1'C1 in such a way to keep the number of the microstates constant and equal to
except the last interval, where
The values of the distance rN1'C1 reported in Fig. 7 b represent the average values calculated for each of the intervals.
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as the reference value. Fig. 7 c shows that the depth of the primary minimum at the distance
when the N-terminus nitrogen atom is separated from the nearest oxygen atom with a single hydrogen atom of the N-terminus, is equal to about 7 kT. Fig. 7 c also shows that, in addition to the primary well, the free energy profile exhibits three successive minima of decreasing values, located at the distance rN1'C1 equal to 0.46 nm, 0.70 nm, and 0.91 nm. These minima correspond to the system configurations in which the N-terminus is separated from the lipid-water interface with one, two, and three water molecules. The results of our calculations are listed in Table 3. The deepest energy minimum of the value 7 kT is related to the hydrogen bonds formed by the terminal hydrogen atoms HT1 through HT3, bonded to the atom N1' of the residue C1. The adsorption energy of the s-PNA molecule estimated as a sum of the contributions originating from the individual atoms is equal to about 64 kT units, which is one order of magnitude larger than the values calculated from the free energy profiles in Fig. 6 a. We believe that this value is a better approximation of the actual PNA adsorption energy.
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The mean force and energy profiles changed during the simulations. In the case of the a-PNA molecule the change was caused by slow sinking of the molecule into the bilayer, as discussed above. Therefore, one can see that the free energy profile calculated for the a-PNA molecule extends to smaller values of the molecule-interface distance.
| CONCLUSIONS |
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The PNA membrane association for low ionic strength and high concentration of the lipid and PNA is an interesting and perhaps even an unexpected prediction because PNA is known to solvate easily in water. Preliminary results of our simulations of the lipid bilayer at ionic strength and pH corresponding to the physiological conditions, however, suggest that strong adsorption of ions at the lipid-water interface takes place. Therefore, we conjecture that at higher ionic strength a compact hydration layer associated with the interface can effectively prohibit PNA adsorption, in agreement with the experimental results. At these conditions, due to the only weak adsorption of the standard PNA, we conjecture a backbone modified PNA could be more suited as a simple gene for the proposed protocell. Exactly how the backbone modifications need to be done has to be calculated and ultimately tested experimentally, where the presented results can be used as benchmarks. It should also be noted that the predicted PNA-lipid adsorption could play a role for the investigations based on PNA for gene therapy utilizing liposome delivery systems.
| SUPPLEMENTARY MATERIAL |
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| ACKNOWLEDGEMENTS |
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This work was carried out under the auspices of the National Nuclear Security Administration of the U.S. Department of Energy at Los Alamos National Laboratory under contract No. DE-AC52-06NA25396.
Submitted on September 12, 2006; accepted for publication December 27, 2006.
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