Nucleic Acids Research Advance Access originally published online on January 18, 2008
Nucleic Acids Research 2008 36(5):1508-1516; doi:10.1093/nar/gkm1182
Nucleic Acids Research, 2008, Vol. 36, No. 5 1508-1516
© 2008 The Author(s)
This is an Open Access article distributed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/by-nc/2.0/uk/) which permits unrestricted non-commercial use, distribution, and reproduction in any medium, provided the original work is properly cited.
Insights into structure, dynamics and hydration of locked nucleic acid (LNA) strand-based duplexes from molecular dynamics simulations
Vineet Pande and
Lennart Nilsson*
Department of Biosciences and Nutrition, Karolinska Institutet, Huddinge SE-14157, Sweden
*To whom correspondence should be addressed. Tel: +46 8 6089228; Fax: +46 8 6089290; Email: lennart.nilsson{at}biosci.ki.se
Received November 5, 2007. Revised December 21, 2007. Accepted December 27, 2007.
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ABSTRACT
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Locked nucleic acid (LNA) is a chemically modified nucleic acid
with its sugar ring locked in an RNA-like (C3'-endo) conformation.
LNAs show extraordinary thermal stabilities when hybridized
with DNA, RNA or LNA itself. We performed molecular dynamics
simulations on five isosequential duplexes (LNA–DNA, LNA–LNA,
LNA–RNA, RNA–DNA and RNA–RNA) in order to
characterize their structure, dynamics and hydration. Structurally,
the LNA–DNA and LNA–RNA duplexes are found to be
similar to regular RNA–DNA and RNA–RNA duplexes,
whereas the LNA–LNA duplex is found to have its helix
partly unwound and does not resemble RNA–RNA duplex in
a number of properties. Duplexes with an LNA strand have on
average longer interstrand phosphate distances compared to RNA–DNA
and RNA–RNA duplexes. Furthermore, intrastrand phosphate
distances in LNA strands are found to be shorter than in DNA
and slightly shorter than in RNA. In case of induced sugar puckering,
LNA is found to tune the sugar puckers in partner DNA strand
toward C3'-endo conformations more efficiently than RNA. The
LNA–LNA duplex has lesser backbone flexibility compared
to the RNA–RNA duplex. Finally, LNA is less hydrated compared
to DNA or RNA but is found to have a well-organized water structure.
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INTRODUCTION
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Nucleic acids are central to transmission, expression and conservation
of genetic information. Consequently, high-affinity binding
of complementary nucleic acids has a plethora of applications
in biotechnology and medicine. Pragmatic in this context is
the development of nucleic acids with chemical modifications
rendering them high affinity and stability, since unmodified
DNA or RNA oligonucleotides have moderate affinities for complementary
targets and low stability in biological fluids (
1). One such
modification results in a Locked Nucleic Acid (LNA) molecule,
where the furanose conformation is chemically locked in an RNA
like (C3'-endo) conformation by introduction of a 2'-O, 4'-C
methylene linkage (
Figure 1A). LNAs show extraordinary thermal
affinities when hybridized with either DNA (
Tm = 1–8°C
per modification), RNA (
Tm = 2–10°C per modification)
or LNA itself (
Tm > 5°C per modification) (
2–4).
Eventually, LNA–LNA duplex formation constitutes the most
stable Watson–Crick base pairing system yet developed.
LNA has therefore found applications in several areas of therapeutics
and diagnostics, recently. For instance, LNAs have been employed
as aptamers for transcription factor NF-

B (
5), incorporated
into DNAzymes (
6), used as molecular beacons (
7), used as probes
to improve RNA
in situ hybridization (
8,
9) and applied to improve
siRNA stability and functionality (
10).

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Figure 1. (A) Structural differences in the ribonucleotide units forming RNA and LNA. (B) Sequence of the bases present in nucleic acid strands A and B. In case of RNA, Thymine (T) bases are changed to Uracil (U) bases. The numbering starts from 1 to 9 beginning with the first base in the 5' to 3' direction in both the strands.
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With such immense potential, it is of fundamental importance
to understand the structural nature of complexes formed by LNA
with RNA or DNA. There have been some studies in this direction,
mainly with NMR spectroscopy and X-ray crystallography, where
in most cases only selected nucleotides have been replaced by
LNA nucleotides in a regular RNA or DNA-based duplex (
11–13),
and in one recent study, NMR structure of a fully modified LNA
strand hybridized with an RNA strand was reported (
14). These
studies have given useful information on the nature of duplex
structure, with the introduction of LNA. For instance, these
studies show that with incorporation of an increasing number
of LNA nucleotides, duplexes achieve an increasing A-like character
(
14) and the duplexes containing LNA nucleotides show an increase
in the values of NMR order parameters compared to unmodified
duplexes (
15).
We undertook the present computational study of duplexes containing a fully modified LNA strand to be able to find answers to some questions of broad interest: (a) what are the characteristics of LNA–DNA and LNA–LNA duplexes, which are rather new to the structural arsenal of LNA based duplexes, (b) what are the differences and similarities amongst the LNA–RNA, LNA–DNA and LNA–LNA duplexes, (c) how do the structure and dynamics of LNA-based duplexes differ from the regular, unmodified RNA–DNA and RNA–RNA duplexes, (d) how does the aqueous solvent behave in each of the five different (LNA–DNA, LNA–LNA, LNA–RNA, RNA–DNA and RNA–RNA) duplexes and (e) to what extent the LNA strand induces its characteristics (in terms of flexibility, dynamics, sugar conformation, etc.) onto partner strands, compared to unmodified duplexes. An understanding of these fundamental properties will not only be instrumental in more efficient applications of LNA in biotechnology and medicine, but also provide a paradigm platform to plan future nucleic acid modifications effectively.
Molecular dynamics (MD) simulations in explicit solvent have been regularly used in order to address the kind of questions posed above in both regular (16–18) and modified (19–21) nucleic acids. These simulations have given excellent agreement with experimental results, besides providing a very detailed picture of the conformational space and thermodynamics of these molecules along with a clear representation of the behavior of solvent. Here we report the results of a total of 50 ns of MD simulations in aqueous solvent with periodic boundary conditions of three nucleic acid duplexes including a fully modified LNA strand (LNA–DNA, LNA–LNA and LNA–RNA) and two regular duplexes (RNA–DNA and RNA–RNA), for comparison.
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COMPUTATIONAL METHODS
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Duplex modeling and simulation setup
The 20 NMR structures of the 9-mer LNA–RNA duplex (
Figure 1B,
PDB ID 1h0q) were reported to have an average pairwise RMSD
of 1.06 Å (
14). The first structure out of these 20 was
used as a starting structure and four new duplexes (LNA–LNA,
LNA–RNA, RNA–DNA and RNA–RNA) were modeled
using this structure as a template with the introduction of
appropriate modifications in bases and ribose units (
Figure 1B).
All LNA-containing duplexes have their LNA strand fully modified
and all five duplexes are isosequential. Initial modeling of
new duplexes was performed using the Insight II (Accelrys Inc.,
San Diego, CA) molecular modeling package and CHARMM (version
c33a1) (
22) was used for force-field-based calculations. Parameters
for bonds, angles, dihedrals and impropers for LNA were derived
based on existing parameters for DNA or RNA within the CHARMM27
force-field (
23) for nucleic acids. Point charges for LNA were
based on the RESP charges derived by Nielsen
et al. (
14). The
new topology and parameters relevant to LNA are provided in
the Supplementary Data of this article. Each duplex was immersed
in a rhombic dodecahedron shaped box containing

3500 pre-equilibrated
TIP3P (
24) water molecules. Each side of the box extended at
least 10 Å away from any solute atom and water molecules
within a distance of 2.2 Å of any solute atom were deleted.
Sixteen sodium ions were randomly added to the water box in
each case to neutralize the net charge.
Molecular dynamics simulation protocol
To avoid the duplex ends from fraying apart during the simulation, weak harmonic distance restraints were imposed on the Watson–Crick hydrogen bonds present in the terminal base steps with a force constant of 4 kcal/mol/Å2. The system was subjected to an equilibration protocol first involving solvent minimization using 2500 steps of steepest descent and 5000 steps of Adopted Basis Newton Raphson (ABNR) algorithms, while holding the solute atoms restrained to their initial positions by means of a harmonic force constant of 50 kcal/mol/Å2. Following this, while still keeping the positional restraints on the solute, the solvent was heated from 100 to 300 K in a 4 ps phase while maintaining a constant pressure of 1 atm. Solvent dynamics was performed for 25 ps in this stage followed by a gradual release of positional restraints from the solute in decrements of 5 kcal/mol/Å2 mediated by series of minimization steps and dynamics. This equilibrated system was then subject to an unrestrained (except the hydrogen bonding restraints on the terminal base pairs) simulation at a constant temperature of 300 K and a constant pressure of 1 atm for 10 ns in each case.
The SHAKE algorithm (25) was used to constrain all covalent bonds involving a hydrogen atom, allowing a time step of 2 fs and the leapfrog algorithm was used to integrate the equations of motion. Constant pressure was maintained using the Langevin piston method (26) with a piston of mass 400 amu and a collision frequency of 20 ps–1, coupled to a temperature bath of 300 K. The system was maintained at 300 ± 10 K, once heated, by scaling the velocities accordingly. Furthermore, a dielectric constant of 1 was used, and atom-based non-bonded interactions were truncated beyond 12 Å using a force shift approach (27), which has been proven to accurately represent the long-range electrostatic effects in nucleic acids (28). The non-bonded lists were maintained for pairs within a distance of 14 Å and updated heuristically whenever an atom had moved more than 1 Å since last update. Periodic boundary conditions were applied and coordinates were saved every picosecond for further analysis.
Analysis of trajectories
Rotational and translational motion was removed from the trajectories by superimposing the solute (nucleic acid duplex) onto the starting structure, and the solvent was recentered around the solute atoms. All properties were calculated for the last 8 ns of the 10 ns trajectories. RMSD was calculated for all heavy atoms in each case, with respect to starting structure. The interstrand phosphate distance was calculated as the distance between the phosphorus atom of a nucleotide in one strand and the phosphorus atom of the nucleotide in partner strand. Since phosphate groups are not present in one of the strands of both terminal steps, these distances were calculated for all base pair steps, except the terminals, in each case. The intrastrand phosphate distance was calculated as the distance between the phosphorous atoms of two successive nucleotides within a strand. The helicoidal and step parameters were calculated with the program CURVES version 5.1 (29).
Hydration numbers were calculated for sets of major groove (O6, N7, O4, H61 and H62), minor groove (N3, O2, H21 and H22) and phosphate oxygen (O1P, O2P, O3' and O5') atoms in each case, representing the number of water molecules present at a distance of <3.0 Å of the solute atoms. Additionally, the radial distribution, g(r) of water protons was calculated for the set of phosphate oxygen atoms in each case. Next, solvent occupancy analysis of intrastrand hydrogen bond bridging water molecules was performed. A hydrogen bond was considered to be present when the distance between hydrogen atom and the hydrogen bond acceptor atom was <2.4 Å, which has been shown as a sufficient criterion (30). The solvent occupancy was interpreted by counting the number of solute atoms that formed a bridged hydrogen bond via any water molecule (water molecule donating and hence bridging two hydrogen bonds, simultaneously) resulting in a net occupancy of more than 100%.
Root mean square fluctuations (RMSFs) were calculated around average structures for the heavy atoms composing backbone atoms (P, O1P, O2P, O3', C5' and O5') of each nucleotide. Additionally, entropy calculations for all nucleic acid duplexes and their structural components (base, ribose and backbone atoms of each strand) were performed with the quasiharmonic analyses facility implemented in CHARMM. The configurational entropy estimator used is based on the use of the quasiharmonic analysis with the covariance (covariance matrix of atomic positional fluctuations accumulated during MD) related to the quantum-mechanical harmonic oscillator expression for the entropy (31). The entropies and their contribution to the free energy (TS) were calculated at 300 K.
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RESULTS AND DISCUSSION
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Overall structure and dynamics
All the simulated structures depict an ensemble of conformations
with stable 2–3Å RMSDs from the starting structure
(
Figure 2). The simulation of the LNA–RNA duplex was able
to very closely reproduce the NMR-derived structure (final,
energy minimized snapshot shows an RMSD of 1.2 Å when
superimposed with starting experimental structure; whereas average
pairwise RMSD for the set of NMR structures is 1.06 Å,
see Supplementary Data).
Figure 3 shows energy minimized, final
snapshots from the MD simulations of the five duplexes. All
the structures adopt typical A-type duplex geometries. The general
structure of LNA–DNA and LNA–RNA duplexes resemble
the RNA–DNA and RNA–RNA duplexes. However, the LNA–LNA
duplex exhibits a slight unwinding of the helix (see twist angles
in section on base stacking), resulting in relatively shallower
grooves, compared to other duplexes.

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Figure 2. Time evolution during the entire simulation of the root mean square deviation (rmsd) from the starting structures for all the heavy atoms of (a) LNA–DNA, (b) LNA–LNA, (c) LNA–RNA, (d) RNA–DNA and (e) RNA–RNA duplexes.
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Figure 3. Energy minimized structures of the last snapshots of duplexes studied with MD simulations in explicit solvent for 10 ns. Hydrogen atoms are omitted for clarity. Carbon atoms of Strand A are in cyan and that of Strand B in green for each duplex.
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To further characterize the general structural and dynamic features,
we calculated interstrand phosphate and intrastrand phosphate
distances during the simulation in each case.
Figure 4 shows
the interstrand phosphate distances, which describe a duplex
structure in its girth. LNA strand containing duplexes have
on average longer distances (upto 20 Å for LNA–LNA
duplex) compared to RNA–DNA and RNA–RNA duplexes.
Furthermore, intrastrand phosphate distances (
Figure 5) show
that LNA strands have around 5.7 Å intrastrand phosphate
distance, whereas DNA strands have a longer distance of around
6.4 Å. RNA strands are closer to LNA strands in their
intrastrand phosphate lengths (around 5.9 Å), however
at several base steps RNA strands have their average intrastrand
phosphate distances exceeding 6 Å.
Sugar puckering
Previous NMR studies (
14,
32) have determined that, in general,
the locked C3'-endo conformation of LNA drives the conformation
of the base paired strand into larger populations of
north sugar
puckers, in an attempt to achieve an overall A-type geometry.
This behavior is indeed expected, as RNA is also known to influence
DNA sugar puckering in DNA–RNA duplexes (
18). However,
the relative extent of such a conformational coupling between
sugar puckers in case of LNA is not known. Here we focused on
this sugar pucker conformation, and calculated the extent to
which LNA induces its C3'-endo pucker [pucker phase (
33) values
between 0° and 36°] on to a partner strand.
Table 1 depicts the frequency of occurrence of C3'-endo pucker in all
the strands during the simulation. We also report the frequency
of
north (0° ± 90°) conformation in all strands.
Sugars in all LNA strands stay locked in a C3'-endo pucker (and
north conformation). Sugars in all the RNA strands show greater
than 90% instances of C3'-endo pucker (and almost 100%
north conformations). The DNA strand in the LNA–DNA duplex shows
around 36% instances of C3'-endo pucker and 44% instances of
north conformation of its sugars. On the other hand, sugars
of the DNA strand in the RNA–DNA duplex show only around
9% of C3'-endo pucker and around 15% of
north conformation.
These results show that LNA tunes the sugar puckering in partner
DNA strand towards C3'-endo pucker or
north conformations more
efficiently than does RNA.
Backbone flexibility
In order to probe the influence of rigid sugar conformation
of LNA on nucleic acid backbone flexibility, we calculated the
RMSF values for backbone atoms of each nucleotide (
Figure 6).
It is clear that DNA backbone is slightly more flexible than
LNA/RNA backbone and that LNA does not impose its low backbone
flexibility onto partner strands. Also, the LNA–LNA duplex
has lesser backbone flexibility compared to the RNA–RNA
duplex. To further understand the nature of conformational flexibility,
we calculated absolute conformational entropies for all the
structural elements (backbone, sugar and bases) in the five
duplexes (see Supplementary Data). For backbone atoms, we do
not find any apparent influence of LNA in lowering the entropy
of partner strands and the LNA–LNA duplex is calculated
to have the lowest backbone entropy. Hence LNA tunes the sugar
pucker of DNA to a significant extent; it does not influence
the backbone flexibility of DNA or RNA.

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Figure 6. Root mean square fluctuations of the backbone atoms (P, O1P, O2P, O3', C5' and O5') of (a) LNA(A)–DNA(B), (b) LNA(A)–LNA(B), (c) LNA(A)–RNA(B), (d) RNA(A)–DNA(B) and (e) RNA(A)–RNA(B) duplexes. All A strands are plotted in black and all B strands in red.
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Water structure and dynamics
The aqueous solvent has a crucial role in nucleic acid structure,
stability and dynamics and has been a subject of study for a
long time (
34–37). We calculated the hydration numbers
in the first solvation shell of duplex groove and phosphodiester
backbone atoms (
Table 2). Minor groove hydration in RNA–RNA
duplex is the highest (average 17.4 water molecules) and in
the LNA–LNA duplex it is the lowest (average 15.6 water
molecules). The partially unwound helix of the LNA–LNA
duplex, resulting in a shallower minor groove, may lead to its
low minor groove hydration. Major groove hydration in the RNA–RNA
is also the highest compared to other duplexes. LNA–DNA
and RNA–DNA duplexes have similar major groove hydration
(hydration numbers

14.5), which is lower than the RNA–RNA
duplex (hydration number

18.5). Next, the hydration numbers
for backbone oxygen atoms (
Table 2) reveal that RNA and LNA
are lesser hydrated (hydration numbers

41) than DNA (hydration
numbers

46). Yet, the LNA strand in LNA–RNA duplex is
slightly lesser hydrated than the RNA strand. To further characterize
the backbone hydration, we calculated the radial distribution
function (RDF), which describes how on average, the water molecules
are radially packed around the various nucleic acid atoms. RDF
plots show that the backbone of DNA is more hydrated than RNA
or LNA and LNA is the least hydrated, even after the first shell
of solvation (Figure S2, Supplementary Data). This result is
in agreement with a recent experimental finding where it is
proposed that introduction of LNA nucleotides into DNA duplexes
results in a net lower uptake of water molecules (
38).
In order to probe the structure of water at an atomic level,
we studied the hydrogen bonding pattern in nucleic acid backbone.
We calculated the occupancy of water-mediated hydrogen bonding
bridges in the backbone of each strand during the simulation
(
Table 4). Phosphate oxygen atoms (O1P and O2P) are capable
of accepting multiple hydrogen bonds from water molecules and
they can also participate as one of the members in water-mediated
hydrogen bonding bridge involving other backbone oxygen atoms.
Interestingly, we find that whereas DNA and RNA only form very
infrequent multiple hydrogen bonding bridges during the course
of the simulation, LNA strands have the most frequent (resulting
in high occupancy) hydrogen-bonding bridges.
Table 3 shows the
number of atoms (eventually O1P and O2P atoms) in a strand involved
in multiple, water-mediated hydrogen bonding interactions that
result in a net occupancy of 100% or more (see Supplementary
Data for a complete list of all specific fractions of occupancy).
Figure 7 depicts a snapshot from the simulation of the LNA–LNA
duplex where the O1P atom of T5 is shown forming four water-bridged
hydrogen bonds with other backbone oxygen atoms, although not
all possible simultaneously, but distributed over the course
of simulation resulting in a net occupancy of more than 100%.
The water molecules bridging hydrogen bonds were exchanged by
other water molecules from the bulk solvent and the average
residence time for such a bridge ranged from 5 to 15 ps, quite
similar to what has been reported for double-stranded DNA(
39).

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Figure 7. A snapshot from the MD trajectory of LNA–LNA duplex depicting water-mediated hydrogen-bonding bridges formed by O1P of T5 in Strand A (carbon atoms in cyan) with other backbone oxygen atoms during the course of simulation resulting in a net occupancy of more than 100%. Similar hydrogen-bonding bridges have lower occupancies in both DNA and RNA strands. Hydrogen atoms are omitted and water oxygen atoms are shown as spheres. The water molecules were exchanged by other water molecules during the simulation.
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Table 3. Occupancy analyses for water-mediated hydrogen bonding bridges (number of solute atoms involved) in the nucleic acid duplexes
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It is an interesting finding that LNA is less hydrated compared
to DNA or RNA but has a well-organized water structure, in context
of the backbone. DNA may be more hydrated than RNA or LNA around
the backbone oxygen atoms because the intrastrand phosphate
distances in DNA are longer than in RNA or LNA (
Figure 5), which
may allow for more space and hence increase in the number of
water molecules in the first shell of hydration (owing to individual
shell of hydration for each phosphate oxygen atom). LNA may
also be less hydrated because of the apolar nature of the methylene
linkage in the sugar. Furthermore, the overall backbone conformation
and chemical environment of LNA, in addition to its shorter
intrastrand phosphate distances and lower backbone flexibility
allow for the formation of simultaneous water-mediated hydrogen
bonding bridges with greater occupancy than DNA or RNA. The
multiple water bridges in LNA may provide it with an extra stability
compared to DNA or RNA.
Base stacking
Stacking of bases plays a prominent role in the structural stability of nucleic acid duplexes. The stacking mode can be specified by helicoidal and step parameters. Helicoidal parameters demonstrate the orientation of a base pair relative to the global helical axis, and step parameters are required to describe the position and orientation of one base pair relative to another (29). Here, in order to characterize the structure of nucleic acid duplexes further, we present values of four parameters—x-displacement of base pairs from helix axis (defined as the perpendicular distance from the long axis of the base pair to the helix axis), propeller twist angles of base pairs (formed between two base planes that form a base pair), roll angles and twist angles of stacking base pairs, calculated directly from the simulation snapshots (Tables 4–7

). For comparison, we also calculated the values of these parameters for the 20 NMR structures of the LNA–RNA duplex, and found them to be in good agreement with those of the experimental structures (see Supplementary Data).
The x-displacement is positive if the helix axis passes by the major groove of the base pair and negative if it passes by the minor groove. On average, the LNA–LNA duplex is calculated to have the lowest x-displacement and the RNA–RNA duplex the highest (Table 4). The propeller twist angle is found to have a similar pattern along the length of the duplex for LNA–DNA and RNA–DNA duplexes, but in the RNA–RNA duple the otherwise negative propeller twist has positive values for base pairs 5–5 and 7–3 (Table 5). The roll angles (angles between two successive base pair planes) show similar trends in all the duplexes (Table 6). Finally, the twist angles (defined as the angle by which one base pair has to rotate to match with the next base pair around the helical axis), vary from one base pair to the next and these variations are probably influenced at least in part, by the attempt to maximize the base stacking overlap as one base pair encounters the next base pair. For the LNA–LNA duplex, the values for twist angles are generally lower compared to other duplexes (Table 7). This reflects the slight unwinding of the helix that the LNA–LNA duplex undergoes. This may also explain why a fully modified LNA strand is unable to form a triplex with a DNA duplex as found in a recent study (40). It is possible that a fully modified LNA strand does not have the ability to twine enough as a helix so as to form a stable triplex with the helical DNA duplex in a network of non Watson–Crick hydrogen bonds.
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CONCLUSIONS
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In the present computational study we have used state-of-the-art
MD simulations to understand in detail the structure, dynamics
and hydration of nucleic acid duplexes formed by a fully modified
LNA strand. We also performed two simulations on regular, unmodified
duplexes for comparison. Although LNA is an RNA mimic we have
found that the RNA–RNA duplex differs from the LNA–LNA
duplex in a number of properties. A fully modified LNA strand,
according to our calculations, has only subtle differences from
an equivalent RNA strand but these subtle differences altogether
impart to LNA certain unique physical properties. In conclusion,
this study has deepened our understanding of LNA-based nucleic
acid duplexes in the following specific aspects:
- The overall structure of LNA–DNA and LNA–RNA duplexes resemble the RNA–DNA and RNA–RNA duplexes. However, the LNA–LNA duplex exhibits a slight unwinding of the helix.
- Duplexes with an LNA strand have on average longer interstrand phosphate distances compared to RNA–DNA and RNA–RNA duplexes. Intrastrand phosphate distances in LNA strands are however shorter than DNA and slightly shorter than RNA.
- LNA tunes the sugar puckering in partner DNA strand towards C3'-endo pucker or North conformations more efficiently than RNA.
- The DNA backbone is slightly more flexible than LNA or RNA backbones and LNA does not show any conformational coupling of its reduced backbone flexibility onto partner strands. Also, the LNA–LNA duplex has lesser backbone flexibility compared to the RNA–RNA duplex.
- LNA is less hydrated compared to DNA or RNA but has a well-organized water structure, in context of the backbone. DNA and RNA only form very infrequent multiple hydrogen-bonding bridges via water molecules during the course of the simulation, however LNA strands have the most frequent hydrogen-bonding bridges, resulting in a net higher occupancy of water bridged backbone.
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SUPPLEMENTARY DATA
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Supplementary Data are available at NAR Online.
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ACKNOWLEDGEMENT
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This work was supported by the Swedish Research Council and
the Swedish Foundation for Strategic Research through the BioX
program.
Conflict of interest statement. None declared.
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