Weiming
Zheng‡
and
Lin
He
*
Department of Chemistry, North Carolina State University, Raleigh, NC 27695, USA. E-mail: Lin_He@ncsu.edu; Fax: +1-919-515-8920; Tel: +1-919-515-2993
First published on 14th July 2014
Cationic polythiophene derivatives have been used as unique optical probes for various biosensing applications with great success, because their optical responses are sensitive to the conformational changes from binding to single-stranded DNA (ssDNA) to binding to double-stranded DNA (dsDNA). It has long been suggested that the binding of cationic polymers to DNA has a major impact on the thermodynamics and kinetics of DNA hybridization; yet a quantitative assessment is lacking. We report here a systematic study to quantitatively measure the thermodynamic binding constants and hybridization rates of DNA duplexes in the presence/absence of cationic polythiophene. Our results show that the dissociation constant of dsDNA in the presence of polythiophene is three orders of magnitude smaller than that in the absence of polymers. The formation of the DNA/polymer triplex is also much slower than double helical DNA formation, suggesting a rate-limiting polymer–ssDNA dissociation step prior to DNA hybridization. The hybridization rate constant is further slowed down when polymer/DNA hybridization occurs on a solid surface due to steric hindrance. Having a means to quantitatively assess the DNA hybridization efficiency in the presence of cationic polymers, we were able to improve the DNA sensing performance through a combined tuning of reaction temperature and time.
Electrostatic repulsion plays an important role in DNA duplex formation. Electrostatic attraction, on the other hand, is the primary binding force between cationic polythiophene derivatives and negatively charged DNA molecules. It is reasonable to suspect, and has since been observed, that thermodynamic and kinetic behaviors of DNA duplexes would change significantly in the presence of positively charged polymers. A systematic study of thermodynamics and hybridization kinetic properties of cationic conjugated polymer–DNA complexes is therefore essential to understand and control the interaction between cationic polymers and DNA at the molecular level for effective assay optimization subsequently. Despite its importance, however, such a study is rather limited in the literature.4,8
In this report we describe quantitative measurements of thermodynamic stability of cationic polythiophene derivative–DNA complexes and hybridization kinetics of polymer–dsDNA formation. The thermodynamic properties of conjugated polymer–DNA complexes were studied by monitoring the melting parameters of the complexes in which the thermodynamic constants were directly derived. Hybridization kinetics of polymer bound-DNA was studied by in situ measuring of fluorescence intensity changes during DNA hybridization in the presence of polythiophene. Hybridization rate constants of polymer-present DNA hybridization in solution and on a solid carrier were compared side by side.
:
1 stoichiometric ratio to DNA X1 or X1′). This reaction ratio ensured an equivalent opposite charge in the mixture (i.e. 1
:
1 positive-to-negative charge ratio in polymer–ssDNA complex formation). The total reaction volume was adjusted to 100 μL with 10 mM phosphate buffer (PB, pH 7.2) and the mixture was kept at room temperature for 30 min to form conjugated polymer–ssDNA duplexes.
To form conjugated polymer–dsDNA triplexes, the pre-formed polymer–ssDNA duplex solution was added to 10 μL of 100 μM target DNA (5′-GAG GGA TTA TTG TTA, Y1) and the mixture was incubated at 37 °C for 30 min to allow hybridization to occur (the resulting triplex complex has a positive-to-negative charge ratio of 1
:
2 in the complex). Note that in the thermodynamic and kinetic studies, the concentration of polymer–ssDNA or polymer–dsDNA complexes refers to the theoretical concentration of complexes, which equals to that of DNA X1 or X1′, because both polythiophene and target DNA Y1 were added to the reaction mixture in stoichiometric ratios.
To form dsDNA duplexes without polymers, 10 μL of 100 μM X1 or X1′ was mixed with 10 μL of 100 μM Y1 in 80 μL PB buffer first. The mixture was then hybridized at room temperature overnight to form stable dsDNA duplexes.5,10
:
1 stoichiometric ratio) for 30 min to form the duplexes. The solution of polymer–ssDNA duplexes was then added into the particle solution and incubated overnight. After incubation, the particles were washed three times with PB buffer, and finally resuspended in 500 μL of PB buffer. UV absorbance at 260 nm of the supernatant showed little residual DNA in solution, suggesting that most polymer–ssDNA duplexes were immobilized on the particles. The concentration of immobilized polymer–ssDNA duplexes was calculated to be ∼3.2 μM. The surface density of immobilized duplexes was estimated to be ∼3 pmol cm−2 (for detailed calculation see ESI†).
For hybridization on particle surfaces, 20 μL of as prepared polymer–ssDNA duplex bound silica nanoparticle solution was mixed with 10 μL of 5 μM target DNA (Y1) for 0–2 h, as specified in the text, prior to washes.
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| Scheme 1 Illustration of binding of cationic polythiophene to ssDNA and subsequently complementary DNA during hybridization. | ||
Various techniques have been used to quantify polymer–DNA complexes, free polymers, and free nucleic acids in situ. Absorbance spectroscopy, for example, has been used to measure system hypochromicity. Circular dichroic spectrometry (CD), calorimetry, and nuclear magnetic resonance (NMR) are other techniques that have been successfully employed.13–17 In addition, because cationic polythiophene derivatives exhibit the unique optical emission signatures during the formation of polymer–DNA complexes, fluorescence has been a powerful technique to directly monitor the formation of polymer–DNA complexes. In this study, absorbance, fluorescence, and CD are the primary techniques used to study the thermodynamic and kinetic behaviors of polymer–DNA complexes.
It is known that some ions induce the Hofmeister effect on cationic polythiophene derivatives and cause aggregation at high concentrations.8 Selection of a phosphate-based buffer and a low operating ionic strength allowed us to introduce minimal arbitrary interference on polymer conformation changes. In addition, while high salt conditions are often used during DNA hybridization to reduce electrostatic repulsion of DNA strands, we found that DNA hybridization occurred without any problem in 10 mM PB because positively charged polythiophene in our system acts as the counter “ions” to neutralize the negative charges of ssDNA it binds to. A high salt concentration (>0.1 M) actually reduces fluorescence emission of polymer–dsDNA triplexes and adversely affects detection sensitivity of the system (data not shown). Consequently, all measurements were conducted in the same 10 mM PB buffer solution throughout our study to mitigate buffer interference and render the results more comparable across the board.
Similar to conventional DNA melting studies, the thermodynamic stability of polymer–DNA complexes is defined by the melting temperature, Tm, the temperature at which a dissociation fractional value, α, equals 0.5:
![]() | (1) |
Fig. 2A shows the plots of α against solution temperatures for dsDNA duplexes, polymer–ssDNA duplexes and polymer–dsDNA triplexes in the 10 mM PB buffer. Direct comparison of the melting experiments of polymer–ssDNA duplexes and dsDNA duplexes reveals that polymer–ssDNA duplexes are, as expected, more stable, dissociating at approximately 9 °C higher than dsDNA duplexes. It is interesting to note a change of slope in the polymer–ssDNA melting curve, probably caused by the additional conformational change of PT from a more rigid, planar state to a random, coil form, which is unique to PT–ssDNA complexes. The speculation is supported by the perfect two-state sigmoidal fitting of the melting curve and above 50 °C the overlap of the melting curve of 500 nm where PT is the only absorbing species (ESI Fig. 2†). While it is clear that multiple processes may be ongoing during PT–ssDNA dissociation, it is a challenging task to isolate each conformational reorganization process because of their intertwined nature. As such, a simple sigmoid fitting of the PT–ssDNA melting curve is used to roughly estimate the overall melting temperature of PT–ssDNA complexes.
Polymer–dsDNA triplexes are found to be the most stable among the three with a Tm of approx. 70 °C. The qualitative observation that positively charged polymers stabilize DNA duplexes is supported by the literature report where polyLysine is also found to improve the stability of dsDNAs.13,14 It is interesting to note that there is only one inflection point in the melting curve of polythiophene–dsDNA triplexes, suggesting that unwrapping of polymers from dsDNA is the rate-limiting step where dehybridization of dsDNA and any additional polymer conformational rearrangement are overshadowed by the initial dissociation of PT–dsDNA.
CD spectra of polymer–dsDNA triplexes at different temperatures also support the notion for a single transition temperature during polymer–dsDNA dissociation. As shown in Fig. 2B, at 45 °C, the triplexes were stable with both CD spectra features in the 190–300 nm and 450 nm regions, corresponding to the signature α-helix of dsDNA duplexes and the loose helical structure of polythiophene wrapping around DNA duplexes. At 75 °C, however, the intensities of both features dropped simultaneously, consistent with the expected dissociation of polymers and dsDNA. Continuous heating of the solution to 90 °C resulted in disappearance of both features, indicating full dissociation of triplexes.
Advancing beyond simple qualitative characterization, the thermodynamic parameters of conjugated polymer–DNA complexes can be derived from the concentration-dependent melting study.18,19 Specifically, multiple melting curves were obtained by varying the concentrations of the complexes to be studied, i.e. dsDNA, polymer–ssDNA (rough estimation from single sigmoid fitting) or polymer–dsDNA. 1/Tm was calculated for each melting curve and the results were plotted as a function of the complex concentration. The obtained plot was then fit to the following equation:
![]() | (2) |
| ΔG° = ΔH° − TΔS° | (3) |
![]() | (4) |
Plots of 1/Tm as a function of concentration (ln(Ct)) for dsDNA duplexes, polymer–ssDNA duplexes and polymer–dsDNA triplexes are shown in Fig. 3. Based on eqn (3) and (4), the thermodynamic data for each DNA complexes were calculated and summarized in Table 1. It is clear that both the enthalpies and the entropies of the polymer bound-DNA complexes changed significantly from those of pure dsDNA complexes, a result of change in binding forces and increased system chaos upon dissociation. Direct comparison of the ΔG°298 values shows that the presence of cationic polythiophene stabilizes dsDNA by ∼4 kcal mol−1, corresponding to >2 orders of magnitude lower in the dissociation constant than that of polymer–ssDNA duplexes, and 3 orders of magnitude more stable than that of dsDNA duplexes alone. It is this difference in thermodynamic stability between polymer–ssDNA duplexes and polymer–dsDNA triplexes that allows effective reduction of non-specific binding from non-complementary annealing on the sensor surface by increasing the incubation temperature.
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| Fig. 3 Thermodynamic analysis of concentration-dependent melting data for dsDNAs, polymer–ssDNA duplexes, and polymer–dsDNA triplexes. | ||
| Cdup. + Ct = Ctri. | (5) |
Fig. 4A shows the representative hybridization kinetic curve of conjugated polymer-bound DNA in the solution phase where fluorescence intensities of the hybridized mixture are plotted against reaction time. During the first 30 min reaction, the fluorescence intensity of the solution increased rapidly, indicating positive formation of polymer–dsDNA triplexes via hybridization. The curve slowly leveled off with little change in signal over the next 60 min until the hybridization reaction reached the equilibrium. A fractional value, f, is calculated based on the measured fluorescence intensity (I), the initial fluorescence intensity of solution at time zero (I0), and the fluorescence intensity at equilibrium (I∧) to quantify the hybridization kinetic data. Given the fact that polymer–ssDNA had little fluorescence and the fluorescence increase was linear to the concentration of hybridized triplexes in the range measured, the value of f represents the ratio of the concentration of triplexes at a given time (Ctri) to the concentration of triplexes at equilibrium (C∧tri):
![]() | (6) |
Therefore, the value f defines the extent of formation of polymer–dsDNA by hybridization reaction at any time. At time zero, f = 0, whereas at the equilibrium, f = 1. For hybridization in the solution phase, a bimolecular reaction mechanism to determine the association constant, ka, is the following equation where f was fit as a function of time according to the literature procedures:11
![]() | (7) |
Fig. 4B shows experimental results obtained for three different solution-based reaction conditions as well as the fits of these results with the bimolecular kinetic model according to eqn (7). Based on the fitting equation, an average ka value of 1.9 × 103 M−1 s−1 was obtained for 15-mer DNA hybridization in the presence of polythiophene in 10 mM PB buffer. This value is more than 2 orders of magnitude lower than the reported hybridization constant of 6.4 × 105 M−1 s−1 for a 16-mer DNA,20 suggesting that the steric hindrance induced by the presence of conjugated polythiophene around the single strand DNA is more pronounced than its charge shielding effect, resulting in an overall slower and less effective DNA hybridization when ssDNA is pre-bound with cationic conjugated polymers.
DNA hybridization was further impeded when the DNA probes were immobilized on a solid surface. Similarly, fluorescence curves were collected from the hybridization of target DNA to 100 nm silica nanoparticles coated with conjugated polymer-bound 15-mer DNA (Fig. 5A). The initial fitting of data using the same bimolecular kinetic model was unsuccessful because the presence of a solid surface introduced high steric constraints on the binding reactions by limiting (i) the suitable orientation of the binding reagent as it approaches towards the particle surface, (ii) the accessibility of the binding sites due to lateral interactions of neighboring molecules (i.e. crowding), and/or (iii) the necessary conformational change of surface bound molecules prior to binding.21,22 Due to such steric effects introduced by the particle surface, a biexponential kinetic model has been employed in the literature and is used here to describe the kinetics of solid-phase binding reactions:11
| f = 1 − a1e−b1t − (1 − a1)e−b2t | (8) |
![]() | (9) |
The experimental data from the conjugated polymer-bound DNA hybridization on a particle surface fit well with this biexponential model in which an initial fast reaction was followed by a secondary slow reaction (Fig. 5B). The ka0 values determined from four different particle-based reaction conditions show an averaged ka0 value of only 264 M−1 s−1. When compared to the solution-based association rate constant (1.9 × 103 M−1 s−1), the hybridization rate of polymer bound-DNA on the particles is ∼7 folds slower. The level of decrease quantified in this case is in agreement with the reported decrease for those observed from traditional DNA hybridization on latex microparticles,11 regardless a long poly-A spacer used to extend the capture probes into the solution. Note that although the particle-based system used DNA probes with an extra 20-base spacer to extend the probes away from the surface, this extra spacer played little role in stabilizing/destabilizing the dsDNA complexes studied (ESI Fig. 3†).
For the solid phased reaction, where one binding partner is immobilized on a solid surface and the other molecule is in solution, the association rate constants are often heavily influenced by mass transport rates (or diffusion rates). To determine whether the polymer-bound DNA hybridization on the silica nanoparticles was binding limited or diffusion limited, the Damköhler number (Da) was calculated according to the following equation:23
![]() | (10) |
The obtained ka values allowed us to further compare the energetic barriers of polymer-bound DNA hybridization in the solution with that of hybridization in the particle phase using the Arrhenius equation:
![]() | (11) |
The temperature dependencies of polymer bound 15-mer DNA hybridization reaction were examined by recording the association curves at a number of different temperatures both in solution and on silica nanoparticles. Fitting of the plots of the resulting ln (ka) versus 1/T data (ESI Fig. 4†) led to the derived activation energies, Eact., of 11.31 kcal mol−1 for the solution phase and 13.14 kcal mol−1 for the particle phase, respectively (Table 2).
| T (°C) | Solution, ka (M−1 s−1) | Particle surface, ka0 (M−1 s−1) |
|---|---|---|
| 37 | 1900 | 264 |
| 45 | 2969 | 389 |
| 50 | 4158 | 531 |
| E act. (kcal mol−1) | 11.3 ± 0.9 | 13.1 ± 1.2 |
Together with an understanding that the polymer–dsDNA exhibits significantly improved thermostability but higher activation energy is needed for polymer-bound DNA hybridization to occur, we were able to improve the DNA sensing performance by simply increasing the incubation temperature (50 °C) and extending the incubation time (>30 min) for maximum hybridization efficiency (Fig. 6).
Footnotes |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/C4BM00210E |
| ‡ Current address: Clinical Diagnostic Group, Bio-Rad Laboratories, Benicia, CA 94510. |
| This journal is © The Royal Society of Chemistry 2014 |