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. Author manuscript; available in PMC: 2021 Aug 26.
Published in final edited form as: Soft Matter. 2020 Aug 26;16(33):7715–7726. doi: 10.1039/d0sm00521e

Statistical mechanics of a double-stranded rod model for DNA melting and elasticity

Jaspreet Singh *,†, Prashant K Purohit *
PMCID: PMC7484343  NIHMSID: NIHMS1617982  PMID: 32734998

Abstract

The double-helical topology of DNA molecules observed at room temperature in the absence of any external loads can be disrupted by increasing the bath temperature or by applying tensile forces, leading to spontaneous strand separation known as DNA melting. Here, continuum mechanics of a 2D birod is combined with statistical mechanics to formulate a unified framework for studying both thermal melting and tensile force induced melting of double-stranded molecules: it predicts the variation of melting temperature with tensile load, provides a mechanics-based understanding of the cooperativity observed in melting transitions, and reveals an interplay between solution electrostatics and micromechanical deformations of DNA which manifests itself as an increase in the melting temperature with increasing ion concentration. This novel predictive framework sheds light on the micromechanical aspects of DNA melting and predicts trends that were observed experimentally or extracted phenomenologically using the Clayperon equation.

Graphical Abstract

graphic file with name nihms-1617982-f0001.jpg

1. Introduction

Double-stranded DNA (dsDNA) consists of two helical sugar-phosphate backbones held together by complementary base pairing. DNA melting or DNA denaturation is the separation of dsDNA into two single strands (ssDNA). The transition can be triggered by increasing the bath temperature or by applying tensile loads on the molecule. DNA melting is important in various biological processes such as DNA replication and DNA transcription, and ultimately impacts gene-expression. The first step in gene expression is the transcription of DNA to mRNA—it initiates via localized DNA melting caused by the protein RNA polymerase1. DNA replication and repair also initiate via localized melting caused by DNA helicases2,3. Several experimental techniques4–6 such as fluorescence microscopy, optical tweezers and calorimetry provide evidence for in-vitro DNA melting–both thermal and force-induced7,8. The transition of a single base pair from bound to melted state is impacted by neighbouring base pairs; if the neighbouring base pairs are melted, it has higher probability of melting–this property is known as cooperativity. Experiments suggest that the dsDNA→ssDNA transition is strongly cooperative9,10. This property manifests itself as a sudden melting transition resembling a first-order phase transition; the increase in inter-strand distance with temperature is sudden as opposed to a mere incremental linear thermal expansion. We illustrate this point in the appendix by a simple model which embodies the basic concept and outcomes of cooperativity.

Here, a double-stranded elastic rod model11 is combined with statistical mechanics12 to capture various characteristics of the melting transition. Although thermal melting of DNA has been studied extensively for some decades now13,14, a mechanics-based model which simultaneously captures both temperature-driven and tensile force-driven melting is yet to be explored. The novelty in the model proposed here is three fold: i) it goes beyond the existing Clausius-Clayperon based phenomenological description and provides a unified statistical-mechanics based framework to explain both temperature-driven and force-driven strand separation, ii) the model provides a mechanical basis for cooperativity in the melting transition by relating it to the bending resistance of the base pairs, and iii) the model accounts for the dependence of the electrostatic energy on the mircromechanical deformation of the birod which ultimately leads to familiar trends in melting temperature versus ion concentration and melting force versus ion concentration.

The sharp transition characterizing cooperative DNA melting depends on various factors4 such as i) the internal base pair sequence: DNA fragments with higher GC content have higher melting temperatures, ii) the tensile force: experimental evidence suggests that the melting temperature decreases as the tensile load increases, and iii) the ion concentration: the melting force and melting temperature both increase with an increase in ion concentration. Most attempts to model the melting transition rely on using the Clausius-Clayperon equation to get empirical relations between the various quantities of interest such as melting temperature versus tensile force or over-stretching force versus the ion concentration et cetera8,15. Since these empirical models interface directly with the experimental data, they have superior predictive capabilities and produce experimentally verifiable predictions. However, this approach abstracts out the underlying mechanics and biochemistry driving the process. To circumvent this drawback to some extent, several statistical mechanics based models16,17 have been proposed which begin by positing an energy functional that reproduces the characteristics of the cooperative melting transition observed experimentally. The detailed description sheds light on the underlying mechanism–cooperative H-bond disruption–and enables one to clearly discern the effect of various parameters such as, the cooperativity parameter and asymmetric interactions, on the melting transition. However, the inherent analytical intractability involved in evaluating the path integrals central to these approaches limits their application to relatively simple energy functionals. Molecular dynamics simulations have also been used to study several problems related to the melting transition, unzipping of DNA, and other structural transformations in DNA18,19. The interaction potentials are available for various chemical bonds in DNA thereby permitting a very detailed description of the structure, shape, and chemistry crucial to the problem. The results from the simulations agree well with the experimental data, but they entail a large computational burden.

Here, DNA is modelled as a 2D elastic birod. The elastic birod model has previously been used to study phenomenon such as allosteric interactions in DNA20,21 where the double-helical geometry and micromechanical deformations of base pairs are important. In this paper, DNA is assumed to be a straight ladder-like birod for analytical tractability. We import ideas from statistical mechanics to show that the average distance between the two strands in a birod increases steeply in an unbounded fashion as the temperature reaches the melting point. A similar effect can be achieved by increasing the tensile load while keeping the temperature constant. A non-quadratic interaction between the strands is essential to achieve this effect. For a quadratic interaction, the equipartition theorem implies that the average change in the distance between the two strands is zero even as the temperature increases. Despite simplifying assumptions, the model presented here captures the key mechanical characteristics of DNA such as the entropic elasticity of long oligomers, the cooperative melting transition, and the effect of tensile force and ion concentration on melting.

The paper is organised as follows:

  1. Kinematics and energetics: The section discusses the development of the model by highlighting key kinematic variables and their respective elastic constitutive relations.

  2. Force-extension curve: The force-extension curve for a birod is computed and the key features of the entropic elasticity exhibited by the birod are demonstrated.

  3. Melting transition: Temperature-driven and tensile force-driven melting transitions are discussed in detail. The focus is to quantitatively describe these transitions within the presented framework, and examine the interplay between the tensile force and the melting temperature.

  4. Effect of cooperativity: The bending resistance of the base pairs is identified to be the cause of cooperativity observed in the melting transition. By varying only one parameter in the model, we are able to capture the experimental trends in both force- and temperature-driven melting transitions.

  5. Effect of ion concentration The section uses the Poisson-Boltzmann formalism to compute the electrostatic energy for the birod. By accounting for the dependence of the electrostatic energy on the outer-radius of DNA in the birod model, it can be shown that both the melting temperature and melting force increase with ion concentration.

The model improves upon the existing statistical mechanics approaches16,17 by computing (as opposed to positing) the energy functional from the kinematic description of the birod, so that the key features – temperature-induced melting, force-induced melting and the cooperativity – emerge naturally.

2. Kinematics and energetics

We closely follow the birod framework presented in Moakher and Maddocks11. We envision a straight ladder-like birod acted upon by an external force F as shown in fig.1. We assume small displacements throughout and confine ourselves to deformations in a plane. The two outer strands and the web connecting them are elastic. The birod lies in e1 −e2 plane as shown in fig.1. The axial coordinate x is along e1: x ∈ [0,L] where L is the contour length. The reference configuration of the ± outer strands denoted by r0± is

r0±=xe1±ae2. (1)

For a general 2-D deformation in the e1 − e2 plane, the deformed configuration of the strands is:

r±=∫0x(1+ζ)d1dx±(a+v)d2±ud1, (2)

where, d1 = cosθe1 + sinθe2, and d2 = −sinθe1 + cosθe2. Note that r=r++r−2=∫0x(1+ζ)d1 dx denotes the deformed centerline (global/macro displacement), while u and v denote the displacements of the ± strands relative to the centerline (micro-displacements). They are related to the shearing and stretching of the base pairs, respectively. In the entire paper, we use a small strain assumption22 together with a moderate rotation approximation23,24 which means: θ2,v,θx ~ O(ε), which implies cos θ~1−θ22 and sin θ ~ θ. Any terms higher than O(ε) such as vθx, θθx, and uθx are neglected. The moderate rotation hypothesis is applicable when the applied force is large, which is indeed the case for DNA melting.

Fig. 1.

Fig. 1

(a) Cartoon of a straight birod acted upon by identical forces on both the strands. The two strands are referred to as ± strands. (b) Attachment of base pairs to the outer-strands. The short web representing the base pairs is welded to the outer strands.

Heretofore, ()x denotes derivative w.r.t x. Hence, d1x = θxd2 and d2x = −θxd1. Now, rx±=(1+ζ±ux∓aθx)d1±vxd2. We assume that the outer strands are inextensible which implies |rx±|=1. Hence, ζ ±ux ∓ aθx = 0, which gives ζ = 0, and ux = aθx. Or, u = aθ. For the ± strands, the tangent is t± = d1 ± vxd2, so the curvature is κ±=|tx±|=θx±vxx, respectively.

We now focus on the stretching, shearing and bending of the base pairs. Here we assume that the small rods–representing the base pairs–are welded to the outer long strands–representing the phosphate backbones (fig.1(b)). Such an arrangement permits the base pairs to exert both force and bending moment on the strands. For DNA, the base pairs are stacked on top of each other in a regular fashion, the space constraints and repulsion from neighbouring bases in this crowded environment prevents the bases from moving freely. A simplistic approach is to penalize the relative motions of the bases via elastic bending and stretching potentials, as done in this paper. This approach is similar to several previous studies25–28 where elasticity of base pairs has been shown to play an important role. A detailed study regarding the actual nature of the bonds is beyond the scope of the current work.

As mentioned, the tangent vectors to the ± strands are t± = d1 ± vxd2, hence the respective normal vectors are n± = ∓vxd1 + d2. The rotation matrices Q± = [t±,n±] can be decomposed as,

Q±=[cos θ−sin θsin θcos θ][1∓vx±vx1]. (3)

Z=[cos θ−sin θsin θcos θ] depends on the deformation of the center-line, while [1∓vx±vx1] depends only on the displacements of the strands about the center-line. Q± can be used to compute the micro-rotation tensor P and macro-rotation tensor Q (for details see11).

P2=Q+Q−T=Z(I2×2+[0−2vx2vx0])ZT, (4)

where I2×2 is the identity tensor. Hence,

P=[1−vxvx1], (5)

and

Q=PQ−=Z=d1⊗e1+d2⊗e2. (6)

The stretching and shearing of the base pairs are proportional to ξ = QT w − w011, where, w=r+−r−2, w0=r0+−r0−2 and ξ = aθe1 + ve2.

Just like the stretching and shearing of the base pairs can be computed from the difference in the displacements of the outer-strands, the bending of the base pairs can be computed from the rotations on the + and − strand. In fact, the moment transferred by the web is proportional to the Gibbs vector of the micro-rotation tensor P11. In a 2D-setting, this moment can be easily computed; since the directions of the rotations are fixed, there is no twisting, and bending is proportional to vx (see fig.1(b) for details).

We now discuss the energy associated with each kinematic deviation from the reference configuration. The bending energy per unit length for the outer ± strands is Es=EI2(κ+2+κ−2)=EI(θx2+vxx2) where EI is the bending resistance of the outer strands. The energy associated with shearing the base pairs is Esh = L1a2θ2, where L1 is the associated elastic constant. For the stretching of the base pairs, we use an assymetric energy profile of the form f (x) = (e−λx − 1)2– known as the Morse potential. This approach is meant to penalize the steric hindrance between the two strands and has been previously used in literature16,17. Hence, the energy per unit length required to stretch the base pairs Est = L2(e−λv −1)2. The energy associated with the bending of the base pairs is Ebb=H1vx2. Altogether, the energy of the birod is,

Ee=∫0Ldx(Eb+Esh+Est+Ebb)=∫0Ldx(EI(θx2+vxx2)+L1a2θ2+L2(e−λv−1)2+H1vx2), (7)

where both v and θ are functions of x. This energy will enter the statistical mechanical model for the birod. We use the following values of elastic constants: EI = 0.15 pNnm2, L1 = 80 pN/nm2, L2 = 1280 pN/nm2, H1 = 0.33 pN, a = 1 nm, and λ = 0.5Å−1. The values of the constants were chosen in a way that melting temperature of DNA at zero tensile force is approximately 75°C (fig. 3 of the main text). Also, the constants were tweaked to get the variation of the melting temperature with tensile force in the right region (fig.5(c) of the main text). One could use other criteria as well, such as the persistence length of B-DNA at room temperature and stretch moduli of B-DNA et cetera. However, the experimental values are for a 3D helical DNA which might not give the correct melting temperature in our model. Since, the focus here is on the melting of DNA, we chose to stick to the former.

Fig. 3.

Fig. 3

(a) 〈v〉 vs T curve. Each green × marker is 〈v〉 computed from an individual MC simulation at that temperature, while the solid green line is a smoothed univariate spline curve plotted to indicate the trend. The inset shows the corresponding data for the melted fraction fm, which is fit using a logistic function to compute the melting temperature (Tm = 360 K). (b) vi and I(vi > 5Å) vs i (1 ≤ i ≤ n) at T = 425 K. Red ∘ and blue ∘ markers denote the melted (vi > 5Å) and unmelted (vi < 5Å) discrete units at T = 250 K. The corresponding vi are also shown; here the solid black line shows vi = 5Å for reference. (c) vi and I(vi > 5Å) at T = 425 K. The data in (b) and (c) are computed at the end of N = 1000000 MC steps. We observe contiguous strands of unmelted DNA below the melting temperature and melted DNA above the melting temperature, indicating cooperative interactions. Further details on MC simulations are given in appendix A3.

Fig. 5.

Fig. 5

(a) Average inter-strand distance 〈v〉 vs temperature T curves for different values of tensile force F. Here each marker × denotes one MC simulation and the solid lines are smooth splines being fit to the MC simulation data to indicate the trend. (b) Fraction of melted DNA fm vs temperature T for different tensile loads. The MC simulation data is fitted using a logistic function to compute the melting temperature. (c) Melting temperature Tm vs tensile force F as computed from fig. (b). The experimental data is from4. (d) Average inter-strand distance 〈v〉 vs tensile force F (×) at 300 K fitted using a smooth spline (solid line). The inset shows the corresponding melted fraction fm (×) fitted using a logistic function (solid line). F ≈ 40 pN when fm = 0.5.

3. Force-extension curve for a thermally fluctuating birod

In this section, we discuss the force-displacement curve for the ladder-like birod. We already have the elastic energy of the birod given by eqn. 7. Next we need to compute the work done by external force F distributed equally on both strands. For + strand, the displacement at the free end is,

Δ+=∫0L(t+.e1−1)dx=∫0L(cos θ−sin θ vx−1)dx=∫0L(−θ22−θvx)dx. (8)

Similarly, for − strand, Δ−=∫0Lt−.e1 dx−L, which upon simplification yields Δ−=∫0L(−θ22+θvx)dx. Summing up the individual contributions from the strands yields,

We=F2(Δ++Δ−)=F∫0L−θ22dx. (9)

Hence, the potential energy functional of the birod is,

E=Ee−We=E(θ(x),v(x))=∫0Ldx(EI(θx2+vxx2)+L1a2θ2+L2(e−λv−1)2+H1vx2+F2θ2). (10)

The average end-to-end extension is,

y=∫0Lcos θ dx≈∫0L(1−θ22)dx, (11)

where we assumed that θ is a moderate rotation. The average end-to-end distance 〈y〉 is,

〈y〉=L−〈∫0Lθ22dx〉, (12)

where 〈〉 denotes the ensemble average. We need to evaluate the partition function to compute the above average. The partition function of the birod is a path-integral given as follows,

Z=∫Dθ(x)∫Dv(x)exp(−E(θ(x),v(x))kBT). (13)

The above partition function Z can be multiplicatively decomposed: Z = ZvZθ, where Zv comprises the path-integral over the function v(x), while Zθ over θ(x).

Zθ=∫Dθ(x)exp(−EθkBT), and Zv=∫Dv(x)exp(−EvkBT), (14)

where,

Eθ=∫0Ldx(EIθx2+(L1a2+F2)θ2), and Ev=∫0Ldx(EIvxx2+L2(e−λv−1)2+H1vx2). (15)

Now,

〈∫0Lθ22dx〉=1Z∫Dθ(x)∫Dv(x)(∫0Lθ22dx)exp(−E(θ(x),v(x))kBT). (16)

Summing over all the admissible functions v(x) and canceling the common factor Zv yields,

〈∫0Lθ22dx〉=1Zθ∫Dθ(x)(∫0Lθ22dx)exp(−Eθ(θ(x))kBT), (17)

The above expression can be evaluated by differentiating the logarithm of the partition function.

〈∫0Lθ22dx〉=−kBT∂ ln Zθ∂F, (18)

which gives,

〈y〉=L+kBT∂ ln Zθ∂F. (19)

Notice that the remaining functional is only a function of θ(x). Following Su and Purohit29, we discretize the domain x ∈ [0,L] into n−segments (xi,xi+1], where 0 ≤ i ≤ n, such that θx=θi−θi−1δ where δ=Ln. For the energy functional Eθ, the integral over the domain can be expressed as a quadratic expression in terms of θi’s:

Eθn=∑i=0nδ[EI(θi−θi−1δ)2+L1a2θi2+F2θi2]=θ.[EIδA+δ(L1a2+F2I)]θ=θ.Kθθ, (20)

where θ = [θ0,θ2,…θn]T, I is an identity matrix, and A is another matrix as follows:

An×n=[1−1000…0−12−100…00−12−10…0⋮⋱⋮00…0−12−100…00−11].

Notice that Kθ is a constant depending only on the elastic properties of the birod. This enables us to transform the path integral Zθ into a n−dimensional integral as follows:

Zθn=∫Dθ(x)exp(−EθkBT)=∏i=0n(∫−ππdθi)exp(−EθnkBT)=∫dθ exp(−θ.KθθkBT). (21)

To evaluate the above integral conveniently, we change the limits from −π,π to −∞,∞, which transforms the above expression into a n–dimensional Gaussian integral which can be computed analytically as follows,

Zθn=∫(−∞,∞)n+1dθ exp(−θ.KθθkBT)=πn/2(kBT)n/2det Kθ. (22)

Substituting it in eqn. 19 gives,

〈y〉=L+kBT∂ ln Zθ∂F=L−kBT2∂ log det Kθ∂F. (23)

An analytical derivation based on Fourier integral techniques30,31 is presented in appendix A2. The plot for the force-extension relation for the birod is shown in fig.2(a). At large forces (F > 20 pN), it can be approximated by a WLC model32 with persistence length 100 nm. As shown in fig. 2 (b), the end-to-end distance decreases with an increase in temperature–a typical entropic elasticity characteristic. The decrease in the variance of the transverse displacement (w(x)=∫0xsin θ dx) with an increase in tensile force shown in fig. 2 (c) is yet another signature of entropic elasticity31 (For analytical expression of 〈w2〉 see Purohit et al.31).

Fig. 2.

Fig. 2

(a) For large force, force-extension curve of the birod is similar to a WLC model with a persistence length of lp = 100 nm. (b) Effect of increase in temperature on the force-extension curve is in agreement with expectations of entropic elasticity. (c) 〈w2〉 vs x for various values of tensile force F. The boundary conditions for (a) and (b) are fixed-free while for (c) it is hinged-hinged. The values of parameters in the energy functional are EI = 0.15 pNnm2, L1 = 80 pN/nm2, L2 = 1280 pN/nm2, H1 = 0.33 pN, a = 1 nm, and λ = 0.5Å−1. For these calculations L = 200 nm and n = 300.

4. Thermal melting

At room temperature under zero tensile loads, the DNA molecule exhibits a double-helical structure. However, as the temperature increases and reaches the melting temperature, the complementary base pairing is disrupted and the two strands spontaneously disintegrate into two single strands. This melting transition is highly cooperative33, and the temperature at which it occurs is referred to as the melting temperature. Aside from the sequence dependence, the melting temperature is also highly sensitive to the tensile loads and the ionic concentration of the solution8,15. Experimental evidence suggests that the melting temperature increases with the increase in ionic concentration and drops with the increase in tensile loads on the molecule. Thermodynamics based studies relying on Clausius-Clayperon equation have led to various empirical relations among these quantities8,15,33. To provide a rough idea about the melting temperature, for the Na+ concentration of 0.075 M, the melting temperature is approximately 75°C34 (see reference for the exact bp-sequence). Using the birod model, we seek a relation between the average inter-strand distance 〈v〉 and the temperature T. In this section, we assume no tensile forces on the molecule, hence the elastic potential energy functional E is,

E=∫0Ldx(EI(θx2+vxx2)+L1a2θ2+L2(e−λv−1)2+H1vx2). (24)

The average distance between the strands can be computed as follows:

〈v〉=1Z∫Dθ(x)∫Dv(x)(1L∫0Lv(x)dx)exp(−E(θ(x),v(x))kBT), (25)

where the expression for the energy E and the partition function Z can be found in eqn. 7 and eqn.13, respectively. As done in the previous section, we discretize the domain into n-elements which transforms the integrals into sums and the path integrals into n-dimensional integrals:

En=∑i=0nδ[EI((θi−θi−1)2δ2+(vi+1−2vi+vi−1)2δ4)+L1a2θi2+L2(e−λvi−1)2+H1(vi−vi−1)2δ2],Zn=∏i=0n(∫(−∞,∞)2dθidvi)exp(−EnkBT),〈v〉=1Zn∏i=0n(∫(−∞,∞)2dθidvi)(1n∑vi)exp(−EnkBT). (26)

In contrast to the last section where the discretization together with quadratic energy functional enabled us to analytically evaluate the partition function, the partition function above can not be evaluated analytically because of the non-quadratic term (e−λvi − 1)2. Hence, we use Monte-Carlo simulations to compute 〈v〉 as a function of the bath temperature T. We use the Metropolis algorithm35 to perform the MC simulations (for more details see appendix A3). The results are recorded in fig. 3. Each individual marker × is one simulation. We find that as the temperature increases the average inter-strand distance increases strongly in a nonlinear fashion, hence can not be alluded to as mere thermal expansion. The asymmetry in the nonlinear interaction term ((e−λv − 1)2) is crucial for achieving this effect; if quadratic interaction is used the average inter-strand distance is zero even as the temperature increases.

We fit a continuous spline to 〈v〉 vs T data to indicate the trend. In reference configuration, the average inter-strand distance is 10 Å. We assume that the melting of a single discrete unit as shown in fig.3 occurs at 50% strain, i.e. when the unit is stretched to 15Å or when vi = 5Å. The oligomer is considered melted when more than 50% of the units are melted. We plot the fraction of melted DNA fm=1n∑i=1nI(vi>5Å), where I(vi>5Å)=1 if vi>5Å and 0 otherwise, as a function of temperature T in the inset. The data for fm vs T is fit using a logistic function g(x)=11+e−a0(x−a1) to read off the melting temperature from the plot: Tm ≈ 360K, which is quite close to the results for dsDNA documented in literature8,15,34. The melted (vi > 5Å) and unmelted (vi < 5Å) units and the corresponding vi are shown for T = 250K and T = 425K. The contiguous strands of unmelted DNA and melted DNA observed below and above the melting temperature, respectively, indicate cooperative interactions. Although the melting criterion vi = 5Å was deliberately chosen so that the results from the model agree with the experimental data, our main message is that the birod model has the essential ingredients to account for the cooperative melting transition and these crucial factors emerge naturally from the kinematic description of the birod.

5. Tensile force-induced melting

In this section, the effect of tensile force on the melting temperature is explored. We consider the birod shown in fig.4. Here, we apply the force on one strand as previous studies36 have indicated. As before, we need to compute the potential energy of the birod in this configuration. The elastic energy of the birod is available in eqn.7. The work done by external force F is,

We=F∫0Ldx(t−.e1−1). (27)

Now, t− = d1 −vxd2, hence t−.e1 = cosθ +v xsinθ ≈ 1−θ2/2+vxθ. This implies,

We=F∫0Ldx(−θ22+vxθ). (28)

The elastic potential energy E is,

E=Ee−We=∫0Ldx(EI(θx2+vxx2)+(L1a2+F2)θ2+L2(e−λv−1)2+H1vx2−Fvxθ). (29)

The term Fvxθ is responsible for coupling the force F and the inter-strand distance v. Now for a given θ(x), the probability of observing a configuration with interstand distance v(x) at force F is eFvxθ/kBT times the probability of observing the same configuration at F = 0. Granted, as the force F increases the birod straightens out and θ decreases as can be inferred from fig.2(b). However, for high forces (> 15 pN), the DNA molecule with a persistence length 50 nm is mostly straight. In other words, the θ(x) does not change much as the force increases from 15 pN to 40 pN, however this makes the higher values of v(x) much more likely. Based upon this qualitative argument we expect that the melting temperature should decrease with an increase in tensile load F.

Fig. 4.

Fig. 4

The birod cartoon for studying DNA melting. Note that the force is applied only on one strand.

The 〈v〉 vs T curves are presented in fig.5(a) for various tensile forces F, and we indeed observe that for a given temperature, the inter-strand separation increases with increasing tensile loads. We use the same criteria for computing the melting temperature Tm as in the previous section: the temperature at which the fraction of melted DNA fm exceeds 0.5. We fit the fm vs T data using a logistic function g(x)=11+e−a0(x−a1) as done previously to get the melting temperature Tm for various values of external load F. We find that Tm decreases with an increase in F as shown in fig.5(c). We use the experimental data from Zhang et al4 to conclude that the trend is correct. The slope of the line depends on the elastic constants of the birod and for the values chosen here a quantitative match is also achieved.

fig.5(d) shows that at a constant temperature (T = 300 K), the average inter-strand distance 〈v〉 increases with an increase in tensile load F indicating force-induced melting. We fit the simulation data using a smooth spline to highlight the trend. The corresponding melted fraction fm vs tensile load F is plotted in the inset. The logistic function fitted to the data reveals that at F = 40 pN fm = 0.5 i.e. DNA has melted. The critical force at which the DNA melts is sometimes referred to as overstretching force15. Experimental data shows that this force driven melting transition occurs at F = 60 pN7,37 (for exact details regarding the pH, sequence dependence and salt concentration see references), hence the value predicted by our model is in the correct region. Note that we modelled DNA using a straight ladder-like birod instead of a helical one, and we restricted the formulation to planar deformations–these assumptions could be causing this deviation.

6. Effect of cooperativity parameter

The structural transition from dsDNA→ssDNA is known to be highly cooperative33. The cooperativity exerts a strong influence on the mechanical behavior such as determining the sharpness of the force-extension curves and influences the melting temperature and overstretching force. One phenomenological approach accounting for cooperativity comes from authors’ previous work38 in which interfacial energy among various phases of DNA makes the transition among them cooperative. Yet, another approach is to postulate an energy functional which includes terms proportional to the gradient of the inter-strand distance16,17. The motivation for such approaches comes from Cahn–Hilliard formulation39 widely used to study nucleation and spoinodal decompositions in phase field modelling, where the phase boundaries are energetically penalized using a term proportional to the square of the gradient of the order parameter (~ (∇ϕ)2). A similar idea for penalizing the gradients is also used in the Landau-Ginzburg approach12 to study superfluidity and superconductivity transitions. In the birod formulation presented here, the gradient terms proportional to vx2 emerge from the bending rigidity of the base pairs which imparts cooperativity to the model. We demonstrate the effects and outcomes of cooperativity using a simple model in appendix A1.

We plot the fraction of melted DNA fm versus the temperature T and tensile load F in fig. 6(a) and (b), respectively. As the bending resistance of base pairs (cooperativity parameter) H1 increases, the melting temperature and overstretching force both increase. Experimental evidence documented in Zhang et al4 shows that as the GC content of the molecule increases, so does the overstretching force and melting temperature. Higher values of H1 represent higher GC content since GC base pairs consist of 3 hydrogen bonds compared to 2 hydrogen bonds in AT base pairs and are consequently stiffer. Higher GC content can have other effects such as increasing the constants L1 and L2 as well; we deal with this issue in appendix A4. In case of force-driven melting, the transition becomes sharper too. This is demonstrated by fitting the logistic function g(x)=11+e−a0(x−a1) to fm vs F transitions and observing that the parameter a0 which quantifies the width of the transition increases monotonically with H1. The phenomenological evidence for the sharpening can be found in authors’ previous work38 in which higher interfacial energies representing higher cooperativity parameters (therefore higher H1) correspond to sharper transitions.

Fig. 6.

Fig. 6

(a) Effect of the cooperativity parameter H1 on temperature driven transition. Here H0 = 0.33pN (b) Effect of the cooperativity parameter H1 on force driven transition. The simulation data represented by marker × is fit using the logistic function g(x)=11+e−a0(x−a1). Increasing the bending resistance of the base pairs leads to an increase in melting temperature and increases in the overstretching force. It also sharpens the force-driven transitions shown by the increasing values of a0 as H1 increases. The units of a0 are K−1 in (a) and pN−1 in (b).

7. Effect of ion concentration

Both force-induced and temperature-induced melting transitions are sensitive to the ion concentration of the solution. Here, the effect of changes of ion concentration on these melting transitions is explored. The phosphate backbone of DNA is negatively charged, hence the positive ions in the solution cluster around it. This stabilizes the double-stranded form of DNA. Therefore, the melting temperature and melting force should increase with an increase in ion concentration, as suggested by experimental evidence4. Empirical relations based on the Clausius-Clayperon equation connecting the melting force and melting temperature to the ion concentration have been proposed8,40. In this section we account for the effect of electrostatic interactions on the melting temperature and melting force by means of a Poisson-Boltzmanm equation based polyelectrolyte model of DNA41.

We use a highly simplified 1D Poisson-Boltzman equation to describe the electrostatics. For a detailed description refer Frank-Kamenetskii et al.41. The purpose of what follows is to compute the electrostatic energy of the rod in a configuration described by θ(x), v(x) and clearly highlight the underlying assumptions. To compute the electrostatic energy, we assume that the DNA molecule is almost straight i.e. the effect of θ(x) is negligible–a complete description of electrostatics for bent DNA is beyond the scope of the current study. Secondly, we assume that the radius of the DNA molecule in a configuration described by v(x) is a+va, where va=1L∫0Lv(x)dx. This assumption transforms the 2D PDE into a 1D ODE. We consider only monovalent ions such as K+ and Na+. Within the scope of these assumptions, the boundary value problem for the electrostatic potential U(y) can be written as,

d2wdy2=χ2 sinh(w),w′(a+va)=2qa+va, w(R)→0 as R→∞. (30)

Here, y is the coordinate perpendicular to x in fig.1, w=eUkBT is the nondimensional potential, e is the electronic charge, and a + va is the average radius of the DNA helix. The dimensionless charge q=lBb, where lB=e2DkBT is the Bjerrum’s length, b is the length of the cylinder containing negative charge e, ε0 is vacuum permittivity, and D is the dielectric constant of the solvent. c0 is the concentration of monovalent ions, and χ2=2c0e2Dε0kBT. The associated electrostatic energy Eel per unit length is obtained by incrementally charging the backbone from 0 to q41:

eel(c0,a+va)=−2kBT∫01dt w(tq). (31)

Note that the boundary condition on the average radius of the DNA backbone couples the electrostatic energy to the mechanical deformation of the birod. Hence, total energy per unit length e(θ(x),v(x)) is the sum of the elastic (eqn.29) and electrostatic energy (eqn.31):

e(θ(x),v(x))=EI(θx2+vxx2)+(L1a2+F2)θ2+L2(e−λv−1)2+H1vx2−Fvxθ+eel (32)

Having set this up, we wish to compute effect of the ion concentration on the melting temperature and melting force. There is only one parameter in the entire electrostatic formulation: q. We choose q = 0.05 for the computations. We start by examining the effect of ion concentration on thermal melting. The fraction of melted DNA fm versus the temperature T is computed for various concentrations c0 = 0.018mol/L to 0.15 mol/L. The simulation results (×) plotted in fig.7 (a) are fitted using a logistic function f(x)=11+e−a0(x−a1). The melting temperature is reached when fm ≥ 0.5. The simulations indicate that melting temperature Tm increases as the concentration c0 increases as shown in fig.7(b). Next, we consider force-induced melting. The simulation data × and the respective logistic fits are shown in fig.7(c). We find that the melting force increases as the concentration increases, see fig.7(d). Previous works such as8,40 have used thermodynamic analysis based on the Clausius-Clayperon equation together with experimental data to analyse the effect of concentration on thermal and force-induced melting and have reported similar results–the melting force and temperature increase with increasing ion concentration. In the analysis presented here the effect of ion concentration emerges from the coupling between the micromechanical deformations of the birod v(x) and the Poisson-Boltzman electrostatic model of DNA. Although, we were able to account for the effect of electrostatics using an elementary Poisson-Boltzmann model, there are several drawbacks: i) the assumption that the rod is straight can not be true at force F = 0, ii) the Poisson-Boltzmann model works only for weak ionic concentrations at T << Tm, iii) eqn.30 assumes that the positive ions are a non-interacting Boltzmann gas which is not true in the vicinity of DNA helix where ion-ion correlations must be considered and iv) eqn.30 neglects the effect of divalent ions such as Mg+2 and Ca+2. For a detailed discussion, we refer the reader to the existing literature on solution electrostatics41,42.

Fig. 7.

Fig. 7

Effect of ion concentration (a) Fraction of melted DNA fm versus the temperature T for various ion concentration, F = 0 (b) Monotonically increase in melting temperature Tm with the ion concentration c0. (c) Fraction of melted DNA fmversus the applied tensile load F, T = 300K. (d) Monotonically increasing melting force Fm with the ion concentration c0.

8. Conclusion

The theory of elastic birods is deployed to study temperature driven and tensile force driven melting transitions in DNA. The paper begins by discussing how the birod model embodies typical characteristics of entropic elasticity. Next, the model is used to study temperature induced DNA melting. The average inter-strand distance is found to increase monotonically with temperature in a nonlinear unbounded fashion. The nonlinear asymmetric interaction between the strands is crucial to correctly model the melting transition; for a linear-elastic interaction, leading to a quadratic energy functional, the average increase in the inter-strand distance is zero–independent of changes in temperature. Next, the model is used to study the effect of tensile force on the melting temperature. The model predicts that the melting temperature decreases with increasing tensile force and by appropriately choosing the elastic parameters the prediction can be shown to even match quantitatively with experimental data. The model shows that at a fixed temperature an increase in tensile load also leads to a melting transition and the critical force corresponding to this transition predicted by the model is 40 pN whereas the experimentally observed value is 60 pN. Various assumptions such as using a straight birod to model double-helical DNA and restricting to deformations on a plane could be responsible for the deviations. Furthermore, the birod model predicts that an increase in GC content causes an increase in cooperativity leading to higher melting temperature and melting forces. Finally, the interplay between the statistical mechanics of the birod model together with electrostatics from a Poisson-Boltzmann formulation accounts for the increase in melting temperatures and melting force with ion concentration.

This work demonstrates the ability of the elastic birod model to accurately describe the mechanics of the DNA melting transition in three ways: i) cooperativity in the melting transition, well documented in literature4,8,16,17, emerges naturally from the elasticity of the base pairs, ii) the birod model can successfully account for the intertwined effect of temperature and tensile force on the melting transition, and iii) the model can be coupled to the Poisson-Boltzmann formulation to account for the effect of ion concentration. However, using a straight ladder-like birod to model double-helical DNA is at best a first order approximation. Such a model is unable to account for the 1.7 times stretching during the melting transition accomplished by unwinding the DNA helix. The derivation of the energy functional assumes that the change in inter-strand distance is small, however this is not true during the melting transition. Further study is required to examine the effect of nonlinear coupling terms in the model. In our formulation, the asymmetry in the applied force is responsible for coupling the stretch (θ) with the interstrand distance (v). As such, if equal force is applied on both ends the stretch and inter-strand distance are decoupled. However, this is because the DNA is modeled using a straight non-helical birod. The authors’ previous work (see sec. 4 in supplementary materials20) on double-helical birods shows how the stretch is coupled to the inter-strand distance. Other crucial features of DNA arising out of double-helical topology, such as twist-stretch coupling, are absent in the straight ladder. Although, such a model can explain the melting transition, it can not explain other well documented4,43 transitions among various DNA phases such B-DNA → S-DNA and B-DNA → P-DNA. Hence, a natural extension of this work is to study the statistical mechanics of a double-helical birod.

Fig. 8.

Fig. 8

An elastic bar undergoing a cooperative phase transition. Here v(x) is the strain variable.

Fig. 13.

Fig. 13

Fraction of melted DNA fm vs temperature T. Here, instead of changing only H1, we change all the parameters L1,L2 and H1. As the stiffness of the base pairs increases, the melting temperature Tm increases.

Acknowledgement

JS and PKP acknowledge support for this work from grants NSF CMMI 1662101 and NIH R01 HL 135254. We thank the anonymous reviewers for pointing out several key points that helped us improve the manuscript.

Appendix

A1: A simple model illustrating cooperativity

The concept and effects of cooperativity are demonstrated using an elastic bar under a tensile load. The understanding derived from this exercise helps us rationalize the observations reported in the main text. Let the strain variable be v(x), hence the energy functional of the bar under a tensile load is E=∫0Ldxv22−FΔ, where L is the contour length and Δ is the displacement at the free end which can be expressed an an integral over the strain- Δ=∫0Lvdx. Now, we add a cooperativity term proportional to vx2. This is analogous to the surface energy term in the Allen-Cahn energy functional44 and gradient term in Landau-Ginzburg energy functional12. In view of the above discussion, the energy functional is,

E=∫0Ldx(kvx22+v22−Fv). (33)

To get the 〈v〉 vs F curve for the bar, we have:

〈v〉=1Z∫Dv(x)(1L∫0Lv(x)dx)exp(−E(v(x))kBT) (34)

where Z=∫Dv(x)exp(−E(v(x))kBT) is the partition function. Similarly, 〈v〉 vs T curves can also be obtained.

For simplicity, assume v(x) can either be relaxed or stretched: v ∈ {0,1}. Using the assumption, together with techniques used in the main text to numerically evaluate the partition function, we can compute the 〈v〉 vs F and 〈v〉 vs T curves. We focus on the effect of the cooperativity parameter k on the curves. The results are shown in fig.9. fig.9 (a) shows that for a fixed temperature T, 〈v〉 decreases with an increase in the cooperativity parameter k, a similar trend is observed by increasing H1 as shown in fig. 6(a) of the main text. Regarding the force driven stretching, fig. 9(b) shows that the width of the transition decreases with increasing k: 〈v〉 vs F curve is almost linear for k = 0 while for k = 3.0 it is sigmoidal. This happens because for large cooperativity coefficient k = 3.0, the units stretch simultaneously. To illustrate this point, we present the stretched and unstretched units in fig.10 for values of F below and above the melting force (F = 0.8,1.2) using cooperativity parameters k = 0 and k = 3.0. Similar sharpening of transition is also observed by increasing H1 in fig. 6(b) of the main text. While in this simple model, the sharpening effect of cooperativity can be clearly seen as shown in fig.9(b), and fig.10, in sec.6, we need to fit logistic curves to the MC simulation data to quantify the sharpness. One point of departure between the two models, is that the melting force increases with H1 in fig. 6(b), on the other hand it remains constant with increasing k in fig.9(b). This is because in the main text, the work done by the external force F is proportional to Fvxθ and θ decreases as F increases, consequently a larger force is required to melt the DNA. Based upon these two similarities, we claim that H1 is the cooperativity parameter in the birod model in the main text.

Fig. 9.

Fig. 9

Here × are the MC simulations while the solid lines are the smoothed spline being fit to the MC simulation data. (a) 〈v〉 vs T curves at F = 0, (b) 〈v〉 vs F curves at kBT = 0.5.

Fig. 10.

Fig. 10

Here ∘ denotes melted (= 1) or unmelted (= 0) state of ith unit at the end of the simulation (N = 100000 steps). We see a sudden transition from F = 0.8 to F = 1.2 when the cooperativity parameter is large (k = 3) in (c) and (d), respectively. On the other hand, we see smooth cross over when cooperativity parameter is low (k = 0). The values of k and F are given in the figure titles and kBT = 0.5.

A2: Analytical derivation of the force-extension curve

Here, we use Fourier integral techniques* to get an analytical expression for the force-extension curve30,31. The energy functional in sec.3 is,

E=∫xdx(EIθx2+(F2+L1a2)θ2). (35)

Define,

θ˜(q)=12π∫xdxe−iqxθ(x) and θ(x)=∫qdqeiqxθ(q). (36)

Noting that θ(x)2=∫q∫qdq1dq2eiq1xe−iq2xθ˜(q1)θ˜(q2) and ∫xdxei(q1−q2)x=δq1−q2 into eqn.35, we get,

E=∫qdq(EIq2+(F2+L1a2))θ˜2. (37)

The above expression is quadratic in θ˜(q), hence, using equipartition one can evaluate

〈θ˜(q)2〉=kBTEIq2+(F2+L1a2). (38)

Parseval’s identity–∫xθ(x)2dx=12π∫qθ˜(q)2dq–together with the above equation yield the following expression for the average end-to-end distance:

<y>=L(1−kBT8EI(F/2+L1a2)). (39)

In the limit F >> L1a2, the persistence length lp can be obtained by comparing the above expression to the WLC formula (〈y〉=L−L2kBTFlp):lp=8EIkBT. We verify this assumption by performing a simple calculation shown in fig.11. We can not do this calculation in sec. 3 to obtain the persistence length because the assumption F >> L1a2does not hold true, instead F ~ L1a2. For a similar calculation of 〈w2(x)〉, we direct the reader to Purohit et al.31.

Fig. 11.

Fig. 11

Using kBT = 5, L1 = 1, EI = 1, and L = 10. Here × data is obtained by discretizing the birod into n = 100 elements.

A3: Details of MC simulations

The Monte Carlo simulations were performed using the Metropolis-Hastings algorithm35. The DNA oligomer was modeled using a 2D birod fixed on one end and free on the other as shown in fig.1 of the main text. The length of oligomers was L = 40 nm and was discretized into n = 50 elements which gives m = 100 dof: (θi,vi) 0 ≤ i < n. The total number of MC moves was N = 1000000. At each move, a random degree of freedom was chosen and the magnitude of perturbation was normally distributed with mean 0 and standard deviation σv if the chosen dof is vi and σθ if the chosen dof is θi. The perturbed state is accepted if e−ΔEkBT>α, where ΔE is the energy difference between the initial state and perturbed (ΔE = Eperturbed − Einitial) and α is a random floating point number uniformly distributed between 0 and 1 (α ~ U(0,1)). We checked for the saturation of the energy to ensure steady-state. The averages were computed on the last N/2 states to discount the effects of burn-in process. The values of σv (≈ 0.25 nm) and σθ (≈ 0.2) were chosen such that the accepted fraction of states lies between 20 − 40%. The melted fraction fm=1n∑i=1nI(vi>5Å), where I(vi>5Å)=1 if vi>5Å and 0 otherwise. The DNA oligomer is considered melted when fm > 0.5. For fm = 0.5, we will always have 〈v〉 > 5Å, since there will be melted links where vi > 10Å, while for unmelted units 0 < vi < 5Å.

To access the impact of concentration, we need to compute the electrostatic free energy per unit length Eel(a + va) as a function of the average birod radius a+va. Note that va changes with each MC move, and solving the ODE at each move is computationally expensive. To circumvent the issue, Eel(a + va) was computed for various values of a + va and an exponential curve was fit to the data. The fitted exponential curve was then used to compute Eel in the MC simulations. For reference, we show Eel vs a + va and the fitted exponential curve for solution concentration c0 = 0.1M and T = 300K in fig.12.

Fig. 12.

Fig. 12

Plot of Eel vs a + va. The fitted exponential curve is used to compute Eel in MC simulations.

A4: Effect of increasing GC content

In sec.6, the effect of the cooperativity parameter H1 is discussed. It was observed that the melting temperature increases with increase in the value of H1, which in turn, is due to higher GC content. Higher GC content can have many other effects as well, such as higher stretch moduli L1 and shear moduli L2, and the combined inter-play could be much more complex and beyond the scope of the paper. Since, the section focusses on the effect of cooperativity, we increased only H1 and left L1 and L2 unchanged. Here we change all the parameters H1, L1 and L2 and show similar trends.

Footnotes

Conflicts of interest

There are no conflicts to declare.

*

We thank a reviewer for this suggestion.

References

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