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arXiv:1612.01737v1 [cond-mat.stat-mech] 06 Dec 2016

Dynamical scaling for underdamped strain order parameters
quenched below first-order phase transitions

N. Shankaraiah, Awadhesh K. Dubey, Sanjay Puri and Subodh R. Shenoy Affiliation: School of Physical Sciences, Jawaharlal Nehru University, New Delhi 110067, India;
TIFR Centre for Interdisciplinary Sciences, TIFR Hyderabad 500075, India.
Abstract

In the conceptual framework of phase ordering after temperature quenches below transition, we consider the underdamped Bales-Gooding-type ’momentum conserving’ dynamics of a 2D martensitic structural transition from a square-to-rectangle unit cell. The one-component or NOP=1N_{\rm OP}=1 order parameter is one of the physical strains, and the Landau free energy has a triple well, describing a first-order transition. We numerically study the evolution of the strain-strain correlation, and find that it exhibits dynamical scaling, with a coarsening length L(t)tαL(t)\sim t^{\alpha}. We find at intermediate and long times that the coarsening exponent sequentially takes on respective values close to α=2/3\alpha=2/3 and α=1/2\alpha=1/2. For deep quenches, the coarsening can be arrested at long times, with α0\alpha\simeq 0. These exponents are also found in 3D. To understand such behaviour, we insert a dynamical-scaling ansatz into the correlation function dynamics to give, at a dominant scaled separation, a nonlinear kinetics of the curvature g(t)1/L(t)g(t)\equiv 1/L(t). The curvature solutions have time windows of power-law decays g1/tαg\sim 1/t^{\alpha}, with exponent values α\alpha matching simulations, and manifestly independent of spatial dimension. Applying this curvature-kinetics method to mass-conserving Cahn-Hilliard dynamics for a double-well Landau potential in a scalar NOP=1N_{\rm OP}=1 order parameter yields exponents α=1/4\alpha=1/4 and 1/31/3 for intermediate and long times. For vector order parameters with NOP2N_{\rm OP}\geq 2, the exponents are α=1/4\alpha=1/4 only, consistent with previous work. The curvature kinetics method could be useful in extracting coarsening exponents for other phase-ordering dynamics.

I Introduction

Interacting systems such as magnets, binary fluids, liquid crystals, and quantum spin models can be probed by the dynamical evolutions of order parameters, after temperature or coupling-constant quenches below transition [1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13]. Such phase ordering can be quantitatively described by a time-dependent, two-point, order-parameter correlation C(R,t)C(\vec{R},t), that can exhibit dynamical scaling, dependent on space and time through a single scaled variable[1, 5, 6, 7, 8, 9, 10, 11, 12, 13] R¯|R|/L(t){\bar{R}}\equiv|\vec{R}|/L(t), with consequent data collapse onto a single scaled curve G(R¯)G(\bar{R}). The coarsening length L(t)L(t) is a measure of the typical spacing between domain walls separating competing order parameter (OP) phases. It can increase as L(t)tαL(t)\sim t^{\alpha}, where the exponent α\alpha is independent of material parameter values, but could depend on the nature of the OP dynamics, the number of components of the order parameter NOPN_{\rm OP}, the number of competing low-temperature variants NVN_{V}, and the spatial dimension dd. There can be a sequential appearance of different exponents, during coarsening [1].

In various dynamic models, the exponents α\alpha have been estimated by heuristic arguments, energy dissipation matchings, Gaussian fluctuations of domain wall profiles, self-consistent correlation function dynamics, and through numerical simulations [1, 5, 6, 7, 8, 9, 10, 11, 12]. The Allen-Cahn relaxation equation [1] for a nonconserved OP and the Cahn-Hilliard equation [1, 4] for a locally conserved OP are familiar models, both with a single time derivative, and typically use a double-well Landau free energy describing a second-order transition. It is of much interest to explore other phase-ordering dynamics; and to develop systematic methods of estimating coarsening-length exponents.

Solid-solid structural transitions have NOPN_{\rm OP} strain-tensor components as the order parameters [14, 15, 16, 17, 18, 19, 20, 21], with Landau free energies having NVN_{V} competing minima, for the NVN_{V} different unit cells, or ’variants’. The high-temperature, high-symmetry crystal structure is “austenite,” and the low-temperature, low-symmetry structures are “martensite.” Martensitic transitions can be described by a Bales-Gooding or BG-type strain dynamics [19] that has several features [19, 20], which differ from the more familiar magnetism-inspired phase orderings. Firstly, the Landau free energy [16] can have triple wells in the OP, describing a first-order phase transition, with a minimum also at zero values of the OP. Secondly, the dynamics is underdamped, with a Newtonian inertial term or double time derivative, describing acceleration of the order parameter. Thirdly, there is global momentum conservation, with the single time derivative damping term, suppressed at long wavelengths[19, 20]. Fourthly, with a 2D dynamics [20] generalized from [19] 1D, the order parameters have an additional power-law anisotropic interaction, coming from an elastic St-Venant compatibility constraint [15, 16], as used in several contexts [21].

Monte Carlo simulations in 2D of a discretized strain-pseudospin martensitic model Hamiltonian with power-law anisotropic (PLA) interactions show interesting evolutions under a temperature quench. For example, for successive quenches approaching the transition from below, the conversion time from seeded austenite evolving to martensite domains rises sharply, with these time delays caused by entropy barriers [18]. Clearly, martensites with continuous-strain dynamics [19, 20] are worth examining, in the framework of phase ordering ideas [1]. We here focus on effects of the triple well Landau term in the underdamped dynamics, and suppress the power-law anisotropic interaction, which will be considered in a subsequent publication.

In the first part of this paper, we apply phase-ordering ideas to the BG strain dynamics, with d=2d=2, NOP=1N_{\rm OP}=1, and NV=2N_{V}=2, in a sixth-order Landau polynomial in the scalar OP strain. We consider only Landau and Ginzburg terms in the OP dynamics to numerically determine the dynamic structure factor or OP-OP correlation, finding dynamical scaling in a coarsening length L(t)tαL(t)\sim t^{\alpha}. The exponent takes on sequential values such as α=2/3,1/2\alpha=2/3,1/2 over time windows, whose widths depend on the quench temperature TT. For deep quenches, there is an exponent α=1/3\alpha=1/3, and a final α0\alpha\simeq 0 flattening to a constant, analogous to ’coarsening arrest’ [22]. These 2D results are found to persist, for 3D.

In the second part of the paper, we use a scaled form of the underdamped OP dynamics, to obtain a dynamics for the OP-OP correlation C(R,t)C(R,t). Inserting the dynamic scaling form, C=G(R/L(t))C=G(R/L(t)), yields a nonlinear, underdamped kinetics for the curvature or inverse coarsening length g(t)1/L(t)g(t)\equiv 1/L(t), with coefficients evaluated at dominant coarsening-front separation. Here, to close what would otherwise be an infinite hierarchy, a spatial average of internal domain-wall factors is made, reducing the correlation between the chemical potential and order parameter, to the OP-OP correlation G(gR)G(gR). The curvature kinetics solutions from balancing kinematic and force terms are simple power-law decays g(t)1/tαg(t)\sim 1/t^{\alpha} in sequential time windows, showing exponents α=2/3,1/2\alpha=2/3,1/2 values, independent of dd, in agreement with simulations. For deep quenches, a toy model including higher powers of the curvature, explains the α=0\alpha=0 coarsening arrest, as a metastable trapping of curvature to a nonzero value.

As a check, the curvature kinetics method is applied to Cahn-Hilliard dynamics, yielding the well-known [1, 8, 9] values of α=1/3\alpha=1/3 for a scalar order parameter NOP=1N_{\rm OP}=1, and α=1/4\alpha=1/4 for vector order parameters with NOP2N_{\rm OP}\geq 2, all independent of dd.

The plan of the paper is as follows. In Sec. II, we state the Cahn-Hilliard and Bales-Gooding types of OP dynamics, and scale to absorb all, or most, of the OP temperature dependencies. Section III defines the OP-OP correlation functions and their dynamical scaling. Section IV shows the coarsening textures, numerically demonstrates dynamical scaling of the two-point correlation function, and states the obtained exponents. The second part of the paper, starting in Sec. V, obtains the correlation function dynamics, and inserts a dynamical-scaling ansatz. Section VI extracts the curvature kinetics, and predicts power-law exponents α\alpha that match the numerics. Finally, Sec. VII contains a discussion and comments on future work. Details are given, in Appendix A, of the closure approximation; in Appendix B, of coefficient signs in the curvature kinetics; in Appendix C, of estimation of coarsening exponents.

II Different order parameter dynamics

II.1 Cahn-Hilliard type dynamics

The simplest order parameter dynamics is the purely relaxational or over-damped Allen-Cahn equation [1] for a nonconserved order parameter that says the damping force balances the chemical-potential driving force from the free energy, e˙F/e\dot{e}\sim-\partial F/\partial e. Another dynamics is the Cahn-Hilliard equation [4] describing the evolution of a conserved order parameter e(r,t)e(\vec{r},t) that could be a mass-concentration density or a magnetization,

γe˙(r,t)=(2)[F(e)e(r,t)].(2.1)\gamma{\dot{e}}(\vec{r},t)=(-\vec{\nabla}^{2})\left[-\frac{\partial F(e)}{\partial e(\vec{r},t)}\right].~~(2.1)

This can be written as a continuity equation

e(r,t)/t+j(r,t),(2.2a)\partial e(\vec{r},t)/\partial t+\vec{\nabla}\cdot{\vec{j}}(\vec{r},t),~~~(2.2a)

where the diffusion current density is driven by spatial gradients of the chemical potential

j=Dμ(r,t),μF(e)e(r,t).(2.2b){\vec{j}}=-D\vec{\nabla}\mu(\vec{r},t),~~\mu\equiv\frac{\partial F(e)}{\partial e(\vec{r},t)}.~~(2.2b)

The diffusion constant is the inverse friction coefficient, D=γ1D=\gamma^{-1}. Since e˙(k,t)k2μ(k,t){\dot{e}}(\vec{k},t)\sim-k^{2}\mu(\vec{k},t), the uniform order parameter k0k\rightarrow 0 is independent of time, i.e., the spatial average of the order parameter is conserved.

The free energy in terms of the OP is typically taken as a Ginzburg or gradient term, plus a Landau term for a second-order transition, F=FG+FLF=F_{G}+F_{L}, where FG=E0rξ02(e)2F_{G}=E_{0}\sum_{\vec{r}}\xi_{0}^{2}(\vec{\nabla}e)^{2}, FL=E0r[ϵe2+e4/2]F_{L}=E_{0}\sum_{\vec{r}}[\epsilon e^{2}+e^{4}/2]. Here, ξ0\xi_{0} is a bending length, ϵ(TTc)/Tc\epsilon\equiv(T-T_{c})/T_{c}, and E0E_{0} is an energy density.

Re-defining space and time variables to make them dimensionless, in units of a numerical grid length a0a_{0}, and a chosen time unit, ra0r;t(γ/2E0)t,r\rightarrow a_{0}r;~~~t\rightarrow(\gamma/2E_{0})t, the Cahn-Hilliard equation of (2.2) becomes

e(r,t)t=r2μ(r,t),(2.3a)\frac{\partial e(\vec{r},t)}{\partial t}={\vec{\nabla}}_{\vec{r}}^{2}~\mu(\vec{r},t),~~~(2.3a)

where the chemical potential has Landau and Ginzburg terms,

μ=μLξ022e(2.3b),\mu=\mu_{L}-\xi_{0}^{2}{\vec{\nabla}^{2}}e~~(2.3b),

where μL(1/2)fL/e=(|ϵ|e2)e\mu_{L}\equiv(1/2)\partial f_{L}/\partial e=-(|\epsilon|-e^{2})e.

II.2 Bales-Gooding type dynamics

Refer to caption
Figure 1: (Color online) BG case temperature dependent parameters: (a) Landau free energy density fLf_{L} vs order parameter ee, for various temperatures τ\tau. There are well-minima at ε¯\bar{\varepsilon}, and barrier-maxima at ε¯b{\bar{\varepsilon}}_{b}. (b) Mean-field order parameter ε¯\bar{\varepsilon} and barrier ε¯b{\bar{\varepsilon}}_{b}, vs τ\tau. (c) Scaling length ξsc\xi_{\rm sc}, scaling time tsct_{\rm sc}, and residual TT-dependence of ηsc(τ)\eta_{\rm sc}(\tau), vs τ\tau.

Bales and Gooding (BG) have used a Lagrangian formalism to obtain [19] a continuous-strain, underdamped, momentum-conserving dynamics in 1D, for a one-component order parameter, or NOP=1N_{\rm OP}=1. For 1D, there is only one type of strain e=u(x)/xe=\partial u(x)/\partial x or gradient of displacement u(x)u(x), that is, the OP. The free energy F=E0xfF=E_{0}\sum_{x}f where the free energy density f=fL+fGf=f_{L}+f_{G} is a sum of a triple-well Landau term fL=e62e4+τe2f_{L}=e^{6}-2e^{4}+\tau e^{2}, and a Ginzburg term fGξ02(e/x)2f_{G}\sim\xi_{0}^{2}(\partial e/\partial x)^{2}.

The Lagrangian density is ρ0e˙2f\rho_{0}\dot{e}^{2}-f where in the “kinetic-energy” term, ρ0\rho_{0} is the mass of the unit cell of volume a0d{a_{0}}^{d}, and the “potential-energy” is ff. With a Lagrangian minimization, and adding a Rayleigh dissipation term γe˙\sim-\gamma\dot{e}, one gets [19]

ρ0e¨(x,t)=(2x2)[Fe(x,t)γe˙(x,t)].(2.4)\rho_{0}\ddot{e}(x,t)=\left(\frac{-\partial^{2}}{\partial x^{2}}\right)\left[\frac{-\partial F}{\partial e(x,t)}-\gamma\dot{e}(x,t)\right].~~(2.4)

Note that the long-wavelength k0k\rightarrow 0 limit enforces global conservation of the total system momentum, with nonzero damping only for k0\vec{k}\neq 0 internal momenta.

For higher spatial dimensions d=2d=2 and 33, there are multiple strain components, describing the physical shear, compression and “deviatoric” or rectangular, distortions of the unit cell. A subset of the physical strains are the NOPN_{\rm OP} order parameter components that enter the nonlinear Landau free energy. The remaining non-OP physical strains are linked to the OP strains by [15, 16] “compatibility constraints” that ensure the distorted unit cells fit together in a smoothly compatible way, without dislocations. A constrained minimization yields an OP-OP effective interaction with an elastic constant prefactor A1A_{1}, that is, power-law and anisotropic, inducing preferred diagonal domain-wall orientations [15, 16]. We will throughout, set A1=0A_{1}=0, and consider these compatibility-induced interactions, elsewhere.

For a square-to-rectangle transition, the OP is the deviatoric strain written as ee, and as before, the free energy F=E0[fL+fG]F=E_{0}\sum[f_{L}+f_{G}]. The triple-well Landau term as shown in Fig 1(a), has minima at e=0e=0, e=±ε¯(τ)e=\pm{\bar{\varepsilon}}(\tau),

fL=[(τ1)e2+e2(e21)2],(2.5)f_{L}=[(\tau-1)e^{2}+e^{2}(e^{2}-1)^{2}],~~(2.5)

with a scaled temperature defined as

τ(T)TTcT0Tc.(2.6a)\tau(T)\equiv\frac{T-T_{c}}{T_{0}-T_{c}}.~~(2.6a)

The minima are at e=±ε¯(τ)e=\pm{\bar{\varepsilon}}(\tau), where

ε¯223[1+13τ/4],(2.6b){\bar{\varepsilon}}^{2}\equiv\frac{2}{3}[1+\sqrt{1-3\tau/4}],~~(2.6b)

while the barriers between the austenite and martensite wells are at ε¯b(τ)223[113τ/4]{\bar{\varepsilon}}_{b}(\tau)^{2}\equiv\frac{2}{3}[1-\sqrt{1-3\tau/4}]. Here, just below T=T0T=T_{0}, or τ(T0)=1\tau(T_{0})=1, when the triple wells are degenerate, the OP jumps from zero to unity ε¯(1)=1\bar{\varepsilon}(1)=1. Below the austenite spinodal T=TcT=T_{c} or τ(Tc)=0\tau(T_{c})=0, the barriers vanish, ε¯b(τ=0)=0{\bar{\varepsilon}}_{b}(\tau=0)=0, and the metastable austenite minimum at e=0e=0 disappears, (when the martensite minima are at ε¯(0)=±4/3\bar{\varepsilon}(0)=\pm\sqrt{4/3}). At zero temperature, τ(0)=Tc/(T0Tc)\tau(0)=-T_{c}/(T_{0}-T_{c}) (see Fig 1).

The Ginzburg term is

FG=E0ξ02(e)2,(2.7)F_{G}=E_{0}\sum\xi^{2}_{0}(\vec{\nabla}e)^{2},~~(2.7)

where ξ0\xi_{0} is an OP bending length scale.

The underdamped dynamics is [20],

ρ0e¨(r,t)=c022[Fe+γe˙],(2.8)\rho_{0}\ddot{e}(\vec{r},t)=c_{0}^{2}\vec{\nabla}^{2}\left[\frac{\partial F}{\partial e}+\gamma\dot{e}\right],~~(2.8)

where c0=12c_{0}=\frac{1}{2} is a normalization. Here with a compatibility term fCA1=0f_{C}\sim A_{1}=0 suppressed, f=fL+fGf=f_{L}+f_{G}, and

fe(r,t)=fLe2ξ022e.(2.9)\frac{\partial f}{\partial e({\vec{r}},t)}=\frac{\partial f_{L}}{\partial e}-2\xi_{0}^{2}{\vec{\nabla}}^{2}e.~~(2.9)

Re-defining space and time variables as before, ra0r;t(γ/2E0)tr\rightarrow a_{0}r;~~~t\rightarrow(\gamma/2E_{0})t, (2.8) becomes

Λ2e(r,t)t2=r2[μ(r,t)+e(r,t)t],(2.10)\Lambda\frac{\partial^{2}e(\vec{r},t)}{\partial t^{2}}={{\vec{\nabla}}_{\vec{r}}}^{2}\left[\mu(\vec{r},t)+\frac{\partial e(\vec{r},t)}{\partial t}\right],~~(2.10)

where the dimensionless Λγ2\Lambda\sim\gamma^{-2} is an inverse-damping squared and, with the unit-cell length a0=1a_{0}=1, is

Λ[2E0ρ0c02]1γ2.(2.11)\Lambda\equiv\left[\frac{2E_{0}\rho_{0}}{c_{0}^{2}}\right]\frac{1}{\gamma^{2}}.~~~(2.11)

The chemical potential is

μ(r,t)=μLξ02r2e(r,t),(2.12)\mu(\vec{r},t)=\mu_{L}-{\xi_{0}}^{2}{\vec{\nabla}}_{\vec{r}}^{2}e(\vec{r},t),~~(2.12)

where μL(1/2)fL/e=e[τ4e2+3e4]\mu_{L}\equiv(1/2)\partial f_{L}/\partial e=e[\tau-4e^{2}+3e^{4}].

II.3 Scaling out the OP TT-dependence

As is well-known [1, 2, 4], the CH dynamics can be cast in TT-independent form, by scaling the OP by its Landau-minimum value, and introducing TT-dependent length and time scales, as

eε¯e;rrξsc(T);tttsc(T),(2.13)e\rightarrow{\bar{\varepsilon}}~e~;r\rightarrow r~\xi_{\rm sc}(T);~t\rightarrow t~t_{\rm sc}(T),~~(2.13)

where ε¯=|ϵ|1/2{\bar{\varepsilon}}=|\epsilon|^{1/2}. The kinetic term on the left side of (2.3) then has a factor ξsc4/tsc\xi_{\rm sc}^{4}/t_{\rm sc}, while the Landau term on right side has a factor ξsc2ε¯2\xi_{\rm sc}^{2}{\bar{\varepsilon}}^{2}. Setting both equal to unity, the scaling length is seen to be the Ginzburg-Landau correlation length ξsc=1/ε¯=1/|ϵ|1/2=ξGL(T)\xi_{\rm sc}=1/{\bar{\varepsilon}}=1/|\epsilon|^{1/2}=\xi_{GL}(T), while the scaling time is tsc=1/ε¯4=1/|ϵ|2t_{\rm sc}=1/{\bar{\varepsilon}}^{4}=1/|\epsilon|^{2}. The OP-scaled CH dynamics is then in the TT-independent form,

e/t=2μLξ024e,(2.14)\partial e/\partial t={\vec{\nabla}^{2}}\mu_{L}-\xi_{0}^{2}{\vec{\nabla}^{4}}e,~~(2.14)

where μL=ef0(e)\mu_{L}=-ef_{0}(e), with a scaled factor f0=(1e2)f_{0}=(1-e^{2}), that vanishes in the bulk.

For the BG case, the OP-scaling of (2.13) yields factors of the same type (ξsc2/tsc)2(\xi_{\rm sc}^{2}/t_{\rm sc})^{2}, and ξsc2/tsc\xi_{\rm sc}^{2}/t_{\rm sc}, for the inertial and damping terms, respectively, while the Landau term has a factor ξsc2ε¯4\xi_{\rm sc}^{2}{\bar{\varepsilon}}^{4}. Setting these to unity, ξsc=1/ε¯2(τ),tsc=1/ε¯4(τ)\xi_{\rm sc}=1/{\bar{\varepsilon}}^{2}(\tau),~t_{\rm sc}=1/{\bar{\varepsilon}}^{4}(\tau). The OP-scaled BG dynamics without compatibility interactions is

Λ2e/t2=2[μL+e/t]ξ024e,(2.15)\Lambda\partial^{2}e/\partial t^{2}={\vec{\nabla}^{2}}[\mu_{L}+\partial e/\partial t]-\xi_{0}^{2}{\vec{\nabla}^{4}}e,~~(2.15)

where μL=ef0(e)\mu_{L}=-ef_{0}(e) with f0=3(1e2)(e2ηsc(T))f_{0}=3(1-e^{2})(e^{2}-\eta_{\rm sc}(T)). Thus for a first-order transition, scaling the OP by its Landau value still leaves behind a residual temperature-dependence, through

ηsc(T)τ/3ε¯4,(2.16)\eta_{\rm sc}(T)\equiv\tau/3{\bar{\varepsilon}}^{4},~~(2.16)

that is negative for τ<0\tau<0 below the spinodal, and for τ>0\tau>0 is essentially the (positive) ratio of barrier height to well depth, ηsc=[ε¯b(τ)/ε¯(τ)]2\eta_{\rm sc}=[{\bar{\varepsilon}}_{b}(\tau)/~{\bar{\varepsilon}}(\tau)]^{2} [see Fig 1(c)].

For the numerical simulations of Sec. IV, we will use the unscaled or TT-dependent forms (2.3), (2.10), and only later multiply the curvature-evolution data by the scaling lengths and times. For the theoretical analysis of Sec. V, we will use the “OP-scaled” forms (2.14), and (2.15).

III Strain correlations and dynamical scaling

In this section, we define the OP-OP and related correlations, and their dynamical scaling forms.

For a one-component martensitic-strain order parameter e(r,t)e(\vec{r},t), we consider a two-point correlation between OP’s at r=R+r0\vec{r}=\vec{R}+\vec{r}_{0}, and r=r0\vec{r^{\prime}}=\vec{r}_{0} on a dd-dimensional lattice, and at equal times tt. With an average over all origins r0{\vec{r}_{0}} and over many runs, OP-OP correlations are dependent only on the separation R=rr\vec{R}=\vec{r}-\vec{r^{\prime}},

C(R,t)=e(r,t)e(r,t),(3.1a)C(\vec{R},t)=\langle e(\vec{r},t)e(\vec{r^{\prime}},t)\rangle,~~(3.1a)
=1Nr0<e(R+r0,t)e(r0,t)>.(3.1b)=\frac{1}{N}\sum_{r_{0}}<e({\vec{R}}+{\vec{r}}_{0},t)e({\vec{r}}_{0},t)>.~~(3.1b)

With a Fourier expansion e(r,t)=1Nkeikre(k,t)e(\vec{r},t)=\frac{1}{\sqrt{N}}\sum_{\vec{k}}e^{i\vec{k}\cdot\vec{r}}e(\vec{k},t), we get

C(R,t)=kS(k,t)eikR,(3.2a)C(\vec{R},t)=\sum_{\vec{k}}S(\vec{k},t)e^{i\vec{k}\cdot\vec{R}},~~(3.2a)

where the time-dependent structure factor is

S(k,t)=|e(k,t)|2.(3.2b)S(\vec{k},t)=\langle|e(k,t)|^{2}\rangle.~~(3.2b)

Since the OP is real, its Fourier coefficients e(k,t)=e(k,t)e(\vec{k},t)^{*}=e(-\vec{k},t) and so S(k,t)=S(k,t)S(\vec{k},t)=S(-\vec{k},t).

Another correlation that enters is the chemical potential-order parameter or μ\mu-OP correlation:

C(μ)(R,t)=μ(r,t)e(r,t)(3.3a)C^{(\mu)}(\vec{R},t)=\langle\mu(\vec{r},t)e(\vec{r^{\prime}},t)\rangle~~(3.3a)
=1Nr0μ(R+r0,t)e(r0,t).(3.3b)=\left\langle\frac{1}{N}\sum_{r_{0}}\mu({\vec{R}}+{\vec{r}}_{0},t)e({\vec{r}}_{0},t)\right\rangle.~~~(3.3b)

With a Fourier expansion μ(r,t)=1Nkeikrμ(k,t)\mu(\vec{r},t)=\frac{1}{\sqrt{N}}\sum_{\vec{k}}e^{i\vec{k}\cdot\vec{r}}\mu(\vec{k},t), we get

C(μ)(R,t)=kS(μ)(k,t)eikR,(3.4a)C^{(\mu)}(\vec{R},t)=\sum_{\vec{k}}S^{(\mu)}(\vec{k},t)e^{i\vec{k}\cdot\vec{R}},~~~~(3.4a)

where only the symmetric part survives, and the μ\mu-OP Fourier correlation is the real part,

S(μ)(k,t)=Reμ(k,t)e(k,t).(3.4b)S^{(\mu)}(\vec{k},t)=Re\langle\mu(\vec{k},t)e(\vec{k},t)^{\ast}\rangle.~~(3.4b)

Since the anisotropic compatibility interaction is switched off, the system is isotropic, and we can work throughout with averages <><...> that now include angular averages, so correlations become C(R,t)C(R,t)C(\vec{R},t)\rightarrow C(R,t) and S(k,t)S(k,t)S(\vec{k},t)\rightarrow S(k,t),S(μ)(k,t)S(μ)(k,t)S^{(\mu)}(\vec{k},t)\rightarrow S^{(\mu)}(k,t) where R|R|R\equiv|\vec{R}|, and k|k|k\equiv|\vec{k}|.

The OP-OP correlation C(R,t)C(R,t) for a given time tt will show a fall-off in separation RR; while at a given separation RR, it will increase with time. Since L(t)\sim L(t) is the scale of the OP-correlation region, it will also increase with tt. As L(t)L(t) is also the separation of the OP-dips at domain walls, these strain patterns must coarsen with time.

Dynamical scaling says that [1, 13] (i) the time tt enters only through the length L(t)L(t); (ii) the separation RR appears only in scaled form as R¯R/L(t)\bar{R}\equiv R/L(t), [and in Fourier space, the wave vector kk appears only as k¯kL(t)\bar{k}\equiv kL(t)]. Further, in a common assumption, (iii) the coarsening length scale grows as a power law LtαL\sim t^{\alpha}, which is plausible [1], but here is justified. The OP-OP correlation is then

C(R,t)/C(0,t)=G(R/L(t))G(R¯).(3.5)C(R,t)/C(0,t)=G(R/L(t))\equiv G(\bar{R}).~~~(3.5)

We find later that the zero-separation values, in a few hundred time steps, on the onset of dynamical scaling, are insensitive to time, C(0,t)C(0,tonset)C(0,t)\simeq C(0,t_{\rm onset}), so we henceforth suppress the constant denominator.

In Fourier space, the scaling behaviour is

S(k,t)=Ldχ(kL(t))Ldχ(k¯).(3.6)S(k,t)=L^{d}\chi(kL(t))\equiv L^{d}\chi(\bar{k}).~~~(3.6)

For sharp domain walls, of widths small compared to L(t)L(t), Porod’s law holds for the Fourier space structure factor [1, 7]

χ(k¯)1/[k¯]d+NOP.(3.7)\chi(\bar{k})\simeq 1/[\bar{k}]^{d+N_{\rm OP}}.~~~(3.7)

For NOP=1N_{\rm OP}=1, we have χ1/(kL)d+1\chi\simeq 1/(kL)^{d+1}, and a log-log plot of S(k,t)S(k,t) versus kk will be a straight line with slope (d+1)-(d+1), with the length L(t)L(t) extracted from the intercepts lnχ=(d+1)lnklnL(t)\ln\chi=-(d+1)\ln k-\ln L(t). Then with this scaling length, replots of lnχ\ln\chi versus ln(k¯)\ln(\bar{k}), as well as G(R¯)G(\bar{R}) versus R¯\bar{R}, will show data collapse of different-time curves.

The coarsening curvature is defined [1] as (d1)/L(t)(d-1)/L(t), but we will simply work with an inverse length, or

g(t)1/L(t),(3.8)g(t)\equiv 1/L(t),~~~(3.8)

and call this the “curvature,” as it indeed is, for d=2d=2. Thus the scaled variables are

R¯g(t)R;k¯k/g(t).(3.9)\bar{R}\equiv g(t)R~;\bar{k}\equiv k/g(t).~~~(3.9)

We later show that the correlation dynamics results in a nonlinear kinetics for the curvature g(t)g(t), that has power-law solutions g1/tαg\sim 1/t^{\alpha}, explaining the observed coarsening-length behaviour LtαL\sim t^{\alpha}.

IV Numerical results on dynamical scaling

In this section, we present numerical work, showing domain-wall (DW) textures, demonstrating dynamical scaling, and extracting exponent behaviour of coarsening curvatures. In an actual experimental quench, the physical temperature is changed suddenly, and the coarsening probe is followed in physical time. Any universal curve independent of quench temperatures TT, is obtained only by later scaling the measured physical values, by factors dependent on TT. As mentioned, we mimic this experimental procedure in simulations by using the unscaled forms of both the CH and BG dynamics in (2.3)and (2.10); only then doing scaling on the numerical data obtained.

Refer to caption
Figure 2: (Color online) Ordered-fraction evolutions: (a) BG case martensitic-ordered fraction nmn_{m} versus scaled time tε¯(τ)4t{\bar{\varepsilon}}(\tau)^{4}, for quenches τ=0.1,0.2,0.6\tau=-0.1,0.2,0.6. (b) CH case ordered fraction nmn_{m} versus scaled time tε¯4=tϵ(T)2t{\bar{\varepsilon}}^{4}=t~\epsilon(T)^{2}, for quenches to ϵ(T/Tc1)=0.5,0.1,0.02\epsilon\equiv(T/T_{c}-1)=-0.5,-0.1,-0.02. Critical slowing down is seen close to TcT_{c}, with ordered-fractions rising only slowly, within the holding-time t<tht<t_{h}.

The initial high-temperature state for both the CH and BG cases, corresponds to a single well, with a minimum at e(r,t=0)=0e(\vec{r},t=0)=0, plus a few local fluctuations of the ordered variants. A numerical “quench” then corresponds to evolving at some suddenly lower temperature TT. There will be an early-time regime where the ordered phases expand, to crowd out the initially dominant e=0e=0 background as a DW vapour phase; while at intermediate and long times, there will be only competing variants, separated by domain walls, as a DW liquid phase.

Refer to caption
Figure 3: (Color online) Relief plot of coarsening: Snapshots for various times, showing coarsening of the OP strain e(r,t)e({\vec{r}},t) after a quench, for system size 5122512^{2}.Positive/negative/zero strains are red/blue/green. See cross-sectional slices.The top of the relief plot shows positive (red) regions, plunging down through valleys, to reach complementary negative (blue) values, passing through domain walls regions, where order parameters go through zero (green).

We thus start with a dilute set of initial seeds of both martensite variants equally, in a sea of e=0e=0 austenite. The martensite conversion fraction nm(t)1Nre2(r,t)/|ε¯|n_{m}(t)\equiv\frac{1}{N}\sum_{\vec{r}}e^{2}(\vec{r},t)/|\bar{\varepsilon}| is initially nonzero only at 2%2\% random sites surrounded by 2×22\times 2 unit cells where e=±ε¯e=\pm{\bar{\varepsilon}}, with e=0e=0 elsewhere, and so nm(0)=0.08n_{m}(0)=0.08.

Refer to caption
Figure 4: (Color online) Contour-plots of strain evolutions: Snapshots of e(r,t)e(\vec{r},t) textures, held at fixed quench temperatures, up to a holding time th=20,000t_{h}=20,000 for system size 819228192^{2}; the pictures are zoomed in to an area of 409624096^{2}. (a) First row: shallow quench to τ=0.6\tau=0.6, or Δτ=0.1\Delta\tau=-0.1; (b) Second row: moderate quench to τ=0.2\tau=0.2, or Δτ=0.5\Delta\tau=-0.5; (c) Third row: deep quench to τ=0.1\tau=-0.1, or Δτ=0.8\Delta\tau=-0.8, when coarsening seems to slow, suggesting a glassy state.

We use an Euler-discretized dynamics of (2.3), (2.10) to find the OP evolution of e(r,t)e(\vec{r},t), focusing on Λ=1\Lambda=1. We take time steps Δt=0.05\Delta t=0.05; and spatial derivatives ν\nabla_{\nu} as finite-difference operators (a0)1Δν(a_{0})^{-1}\Delta_{\nu} on a square unit lattice. For wave vectors k\vec{k} in the Brillouin zone, Δν2sin(kνa0/2)\Delta_{\nu}\rightarrow 2\sin(k_{\nu}a_{0}/2) , with the grid scale set to a0=1a_{0}=1. A fast Fourier transform yields the Fourier coefficient e(k,t)e(\vec{k},t); and hence the angularly averaged dynamic structure factor S(k,t)=<|e(k,t)|2>S(k,t)=<|e(\vec{k},t)|^{2}> of (3.2). (To focus on DW time scales, a “strain-hardening” procedure is used [9].) Run averages are taken, over Nrun=5N_{run}=5. A reverse FFT yields the OP-OP correlations C(R,t)C(R,t) of (3.1). The quench temperature TT is held fixed, for a holding time th=20,000t_{h}=20,000 steps. The 2D system is of size Lsys2=81922L_{\rm sys}^{2}=8192^{2}.

Figure 2(a) shows the BG case single-run martensite or ordered-fraction nm(t)n_{m}(t) versus scaled time tε¯4(τ)t\bar{\varepsilon}^{4}(\tau). For temperatures just below T=T4T=T_{4} or τ=τ(T4)=0.74\tau=\tau(T_{4})=0.74 the martensite fraction rises slowly towards unity, with larger delays, closer to T4T_{4}. Above T4T_{4} there is no conversion at all, as the initial martensite seeds dissolve back into the four-fold symmetry austenite. We will quench to temperatures sufficiently below T4T_{4} so conversion delays are small.

Refer to caption
Figure 5: (Color online) Cahn-Hilliard OP correlations for various quenches : (a) For ϵ=0.5\epsilon=-0.5, data for C(R,t)C(R,t) vs RR for various times tt; (b) Porod’s Law behaviour in scaled structure factor χ(kL)\chi(kL) vs scaled wave-vector kL(t)kL(t), showing data collapse in Fourier space, for all times and temperatures; (c) Dynamical scaling in G(R¯)G(\bar{R}) vs scaled separation R¯R/L\bar{R}\equiv R/L, showing data collapse in coordinate space, for all times, and temperatures; (d) Log-log plot of unscaled curvature g(t)1/L(t)g(t)\equiv 1/L(t) vs time tt, showing “guide to the eye” indicated exponents α=1/4,1/3\alpha=1/4,1/3, seen within the holding time tht_{h}.
Refer to caption
Figure 6: (Color online) CH curvature coarsening and scaled variables: Plot of previous CH data of Fig. 5(d), in scaled variables, showing g/ε¯=g/|ϵ|1/2g/{\bar{\varepsilon}}=g/|\epsilon|^{1/2} vs tε¯4=t|ϵ|2t~{\bar{\varepsilon}}^{4}=t~|\epsilon|^{2}. There is data collapse for all temperatures, and guide to the eye lines indicate exponents of α=1/4\alpha=1/4 for intermediate times, crossing over to α=1/3\alpha=1/3 for long times.
Refer to caption
Figure 7: (Color online) Phase diagram: Inverse damping Λ\Lambda versus scaled quench temperature τ\tau, with austenite above the transition-temperature curve, and martensite, below it.
Refer to caption
Figure 8: (Color online) Bales-Gooding OP correlations for shallow quenches: (a) For τ=0.6\tau=0.6, data for C(R,t)C(R,t) versus RR for various times; (b) Porod’s Law behaviour in scaled structure factor χ(kL)\chi(kL) versus scaled wave-vector kL(t)kL(t) showing data collapse in Fourier space, for all times ; (c) Dynamical scaling in G(R¯)G(\bar{R}) versus scaled separation R¯R/L\bar{R}\equiv R/L showing data collapse in coordinate space, for all times. The scaled curves actually have slightly different shapes, for different temperatures, due to residual τ\tau dependence, and the τ=0.6\tau=0.6 curve is shifted downwards by 0.10.1, to highlight this.For decreasing temperatures τ=0.5,0.4\tau=0.5,0.4 the curves are closer in shape and values, so the data are not relatively shifted. (d) Log-Log plot of scaled coarsening curvature g(t)/ε¯(τ)2g(t)/{\bar{\varepsilon}}(\tau)^{2}, vs tε¯(τ)4t~{\bar{\varepsilon}}(\tau)^{4}, with indicated exponents α=2/3\alpha=2/3 seen, within tht_{h}.
Refer to caption
Figure 9: (Color online) Bales-Gooding OP correlations for moderate quenches: (a) For τ=0.3\tau=0.3, data for C(R,t)C(R,t) versus RR for various times; (b) Porod’s Law behaviour in scaled structure factor χ(kL)\chi(kL) versus scaled wave-vector kL(t)kL(t), showing data collapse in Fourier space for all times; (c) Dynamical scaling in G(R¯)G(\bar{R}) versus scaled separation R¯R/L\bar{R}\equiv R/L, showing data collapse in coordinate space, for all times, and approximately for all temperatures; (d) Log-Log plot of scaled coarsening curvature g(t)/ε¯(τ)2g(t)/{\bar{\varepsilon}}(\tau)^{2} versus scaled time tε¯(τ)4t~{\bar{\varepsilon}}(\tau)^{4}, with indicated exponentsα=2/3,1/2\alpha=2/3,1/2 seen within the tht_{h}.
Refer to caption
Figure 10: (Color online) Bales-Gooding OP correlations for deep quenches, including below the τ=0\tau=0 spinodal: (a) For τ=0.05\tau=0.05, data for C(R,t)C(R,t) versus RR for various times tt; (b) Porod’s Law behaviour in χ(kL)\chi(kL) versus scaled wave-vector kL(t)kL(t) showing data collapse in Fourier space, for all times, and temperatures ; (c) Dynamical scaling in G(R¯)G(\bar{R}) versus R¯R/L\bar{R}\equiv R/L showing data collapse for all times, and approximately for all temperatures; (d) Log-Log plot of scaled coarsening curvature g(t)/ε¯(τ)2g(t)/{\bar{\varepsilon}}(\tau)^{2} versus scaled time tε¯(τ)4t~{\bar{\varepsilon}}(\tau)^{4} with indicated exponents α=1/2,1/3,0\alpha=1/2,1/3,0, seen within the tht_{h}.

Figure 2(b) shows the CH case ordered-fraction nm(t)n_{m}(t) versus scaled time t/tsc=tϵ2t/t_{\rm sc}=t\epsilon^{2}, where its slow rise for TT close to TcT_{c} is due to critical slowing down near a second-order transition. As will be seen, these intermediate times can nonetheless show exponent behaviour.

Figure 3 shows snapshots of evolving relief plots of the OP e(r,t)e(\vec{r},t) versus position (x,y)(x,y), for early time evolutions for t=100,250,1500t=100,250,1500, and deep quenches. The strain textures or DW patterns, clearly coarsen with time.

Figure 4 again shows snapshots of coarsening, but now as evolving contour plots, for shallow, moderate and deep quenches. We will later consider several such quenches just below τ=+0.6,+0.3,+0.05\tau=+0.6,+0.3,+0.05, corresponding to Δτ(T)τ(T)τ(T4)=0.1,0.5,0.8\Delta\tau(T)\equiv\tau(T)-\tau(T_{4})=-0.1,-0.5,-0.8. The first row is for a shallow quench, to τ=0.6\tau=0.6, and shows, in a background of e=0e=0 austenite, many whorl-texture droplets at early times, like a DW vapour. The second and third rows are for moderate and deep quenches around τ=0.2,0.1\tau=0.2,-0.1, with wandering martensite-martensite interfaces, like a DW liquid. For deep quenches, the coarsening seems to slow, or be arrested to form a DW Glass, as discussed later.

As a benchmark, we start with the familiar CH case, in 2D and with a scalar NOP=1N_{OP}=1 order parameter. Fig 5 shows the well-known results of dynamical scaling.

Figure 5(a) shows C(R,t)C(R,t) versus RR curves at different times for a given quench, with ϵ(T)=0.5\epsilon(T)=-0.5 shown. Extracting the coarsening length and re-plotting, we find (i) data collapse of different- time curves on to a common scaling curve C(R,t)=G(g(t)R)C(R,t)=G(g(t)R), for that quench; further, (ii) data collapse of different-quench scaling curves G(R¯)G(\bar{R}) onto a single TT-independent curve. This is consistent with (2.14), which predicted a OP-scaled CH dynamics would be independent of temperature. The curvature exponents are consistent with the literature, with a long-time exponent [1] of α=1/3\alpha=1/3 and, for temperatures close to TcT_{c}, an intermediate-time exponent [5] α=1/4\alpha=1/4. Simulations in d=3d=3, show [8] the same asymptotic α=1/3\alpha=1/3 exponent, that is, thus independent of spatial dimension.

Figure 6 shows CH case log–log plots of the scaled curvature g/ε¯=g/|ϵ|1/2g/{\bar{\varepsilon}}=g/|\epsilon|^{1/2} versus scaled time tε¯4=t|ϵ|2t{\bar{\varepsilon}}^{4}=t|\epsilon|^{2}, showing data collapse, not only for all times, but also for all temperatures, as expected from the OP-scaled form of (2.14). Existing results [1, 8, 9] have temperature-independent exponents at intermediate-times where g(t)ξGL(T)>1g(t)\xi_{\rm GL}(T)>1 as α=1/4\alpha=1/4; and a long times where gξGL(T)<1g\xi_{\rm GL}(T)<1 as the Lifshitz-Slyozov exponent of α=1/3\alpha=1/3. Extracting exponent values from data (as for BG case of Appendix C), we find averaged exponents and standard deviations as

α=0.27±0.02;α=0.34±0.02,(4.1)~~~\alpha=0.27\pm 0.02~;~~\alpha=0.34\pm 0.02,~~~~~~~(4.1)

close to 1/41/4 and 1/31/3, as in previous work.

Turning to the BG case quenches, Bales and Gooding in 1D find a backward-bending phase boundary of inverse damping versus temperature. Figure 7 shows that in the 2D case, the phase diagram of inverse-damping Λ1/γ\sqrt{\Lambda}\sim 1/\gamma versus temperature τ(T)\tau(T) also has the transition occurring at lower τ\tau, for decreasing damping. Below the boundary, the dilute initial seeds with small nmn_{m}, evolve to nm1n_{m}\rightarrow 1 (martensite), while above it, nm0n_{m}\rightarrow 0 (austenite). All quenches are to below the phase boundary.

For d=2d=2 in previous Monte Carlo simulations of a related model, a complex textural energy was parametrized by a surrogate-droplet energy that was a universal inverted parabola versus a scaled evolving textural parameter [18]. As a check, our BG case dynamical evolutions were benchmarked against this energy parametrization [23].

The BG case plots of Figs. 8-10 show numerical results analogous to the CH case, demonstrating dynamical scaling, for the three quench regimes each, just below τ=0.6,0.3,0.05\tau=0.6,0.3,0.05, as mentioned. More in detail, all the Figures show the following: (a) correlations C(R,t)C(R,t) versus RR curves at different times, for quench to a given τ(T)\tau(T); (b) scaled structure factor χ(kL){\chi}(kL), using the extracted L(t)L(t), versus k¯=kL\bar{k}=kL showing Porod’s tail behaviour of exponent -3 and Fourier data collapse; (c) dynamical scaling with data collapse of different-time curves on to a common scaling curve C(R,t)=G(g(t)R)C(R,t)=G(g(t)R), for that τ\tau quench. However, the scaling curves G(R¯)G(\bar{R}), are different for different τ\tau, especially for the shallow quenches of Fig. 8; while for deeper quenches of Figs. 9 and 10, the curves are closer. This is consistent with the OP-scaled result of (2.15), that shows a residual TT-dependence of the BG dynamics, through ηsc(T)=τ(T)/3ε¯(T)4\eta_{sc}(T)=\tau(T)/3{\bar{\varepsilon}}(T)^{4}, that is, insensitive to τ\tau at low temperatures. Also they show (d) log-log plots of the coarsening curvature versus time, showing different indicated exponents in different time windows, within the holding time tht_{h}.

Figure 8 shows α=2/3\alpha=2/3; Fig. 9 shows α=2/3\alpha=2/3 followed by 1/21/2; Fig. 10 shows α=1/2\alpha=1/2 followed by α=1/3\alpha=1/3, and a peculiar flattening to ‘α=0\alpha=0’ at low temperatures. The trapped curvature g0=0.1g_{0}=0.1 is not just a finite-size effect, as for our system sizes, g01/Lsys104g_{0}\gg 1/L_{\rm sys}\sim 10^{-4} .

The exponent mean values and standard deviations, with simple arithmetic average over all temperatures, are

α=0.66±0.02and0.53±0.02,(4.2)~~~~~\alpha=0.66\pm 0.02~~~{\text{a}nd}~~~~0.53\pm 0.02,~~~~~~~~~~~~~~~~~~~~~~(4.2)

that are close to α=2/3\alpha=2/3 and α=1/2\alpha=1/2. See Appendix C for a time-window procedure for extracting exponents.

Refer to caption
Figure 11: (Color online) Contour plots of 3D strain evolutions: Snapshots for various times show the OP strain e(r,t)e({\vec{r}},t) evolving after a quench, in a system of size 5123512^{3}.
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Figure 12: (Color online) Bales-Gooding OP correlations in 3D for τ=0.01\tau=0.01 : (a) Dynamical scaling in G(R¯)G(\bar{R}) versus R¯R/L\bar{R}\equiv R/L for various times tt, showing data collapse in coordinate space; (b) Porod’s Law behaviour in χ(kL)\chi(kL) versus kLkL showing data collapse in Fourier space, with slope (d+NOP)=4-(d+N_{\rm OP})=-4; (c) Log-Log plot of scaled coarsening curvature g(t)/ε¯2g(t)/{\bar{\varepsilon}}^{2} versus scaled time tε¯4t\bar{\varepsilon}^{4} showing various indicated exponents; (d) Fitted exponent values α\alpha versus quench temperature τ\tau, showing that the 3D values close to 2/3,1/2,1/3,02/3,1/2,1/3,0 are the same as in 2D.

All this is for 2D. We have also considered 3D coarsening textures, as shown in surface contour plots of Fig. 11. The 3D case also shows dynamical scaling as shown in Fig. 12, with the Porod’s law exponent now (d+1)=4-(d+1)=-4, and data collapse as before. For successively deeper quenches, the exponents are found to be again close to α=2/3,1/2,1/3,0\alpha=2/3,1/2,1/3,0, so the coarsening exponents are independent of spatial dimension.

V Correlation-function Dynamics and Dynamical Scaling

The exponent behaviour has been extracted from various OP dynamics by many authors [1, 5, 6, 11], including Siggia through insightful heuristic arguments; Bray and Rutenberg through matching global and local dissipation; Ohta, Jasnow, and Kawasaki; Bray, and Puri, and Mazenko, through a fluctuating domain wall approach; and Langer et al. through a self-consistent truncation of correlation function dynamics. We suggest a complementary, and systematic curvature kinetics approach, to extract exponent behaviour.

In our theoretical analysis, we will use throughout, the OP-scaled form of the CH and BG dynamics, that fully or mostly, scales out the OP temperature dependence. We first obtain the dynamics of the two-point OP-OP correlation as done previously, elsewhere [5].

V.1 Evolution of correlation function

The correlation function dynamics can be derived [5, 24]. from a given order parameter dynamics, such as the OP-scaled dynamics of (2.14) and (2.15). From (2.14), the “mass-conserving” Cahn-Hilliard correlation function dynamics is

tC(R,t)=R2C(μ)(R,t).(5.1)\frac{\partial}{\partial t}C(R,t)={\vec{\nabla}_{\vec{R}}}^{2}C^{(\mu)}(R,t).~~~(5.1)

From (2.15) we similarly get a “momentum-conserving” Bales-Gooding correlation dynamics,

Λ2t2C(R,t)=R2[C(μ)(R,t)+C(R,t)t].(5.2)\Lambda\frac{\partial^{2}}{\partial t^{2}}C(R,t)={\vec{\nabla}_{\vec{R}}}^{2}\left[~C^{(\mu)}(R,t)+\frac{\partial C(R,t)}{\partial t}\right].~~~(5.2)

The chemical potential-order parameter correlation or μOP\mu-{\text{O}P} correlation of (3.3), has separate Landau and Ginzburg contributions,

C(μ)(R,t)C(μL)(R,t)+C(μG)(R,t),(5.3)C^{(\mu)}(R,t)\equiv{C}^{(\mu_{L})}(R,t)+{C}^{(\mu_{G})}(R,t),~~~(5.3)

where the Ginzburg term depends directly on the OP-OP correlation,

C(μG)(R,t)[12fGe(r,t)]e(r,t){C}^{(\mu_{G})}(R,t)\equiv\left\langle\left[\frac{1}{2}\frac{\partial f_{G}}{\partial e(\vec{r},t)}\right]e(\vec{r^{\prime}},t)\right\rangle
=R2C(R,t),(5.4a)=-{\vec{\nabla}_{\vec{R}}}^{2}C(R,t),~~~(5.4a)

while the Landau contribution carries the higher powers of the strain

C(μL)(R,t)[12fLe(r,t)]e(r,t){C}^{(\mu_{L})}(R,t)\equiv\left\langle\left[\frac{1}{2}\frac{\partial f_{L}}{\partial e(\vec{r},t)}\right]e(\vec{r^{\prime}},t)\right\rangle
f0(e(r,t))e(r,t)e(r,t),(5.4b)\equiv-\left\langle f_{0}(e(\vec{r},t))e(\vec{r},t)e(\vec{r^{\prime}},t)\right\rangle,~~~(5.4b)

where the BG-case scaled polynomial factors f0(e)f_{0}(e) have been given earlier.

V.2 Dynamic scaling ansatz

We assume the correlation functions have a dynamic scaling form, and insert this as an ansatz or trial solution,

C(R,t)=G(R¯),(5.5a)C(R,t)=G(\bar{R}),~~(5.5a)

where the argument of the scaling function is henceforth

R¯g(t)R.(5.5b){\bar{R}}\equiv g(t)R.~~(5.5b)

For the Landau part of μ\mu-OP correlation function with three lengths ξ0,R,L\xi_{0},R,L,we can similarly assume a general scaling form in ratios R/L(t),ξ0/L(t)R/L(t),\xi_{0}/L(t):

C(μL)(R,t)=(gξ0)δLG(μL)(R¯,gξ0),(5.6){C}^{(\mu_{L})}(R,t)=(g\xi_{0})^{\delta_{L}}G^{(\mu_{L})}(\bar{R},g\xi_{0}),~(5.6)

where G(μL)G^{(\mu_{L})} is some scaling function, and δL\delta_{L} some universal exponent.

The model dynamics can be written in terms of R¯{\bar{R}} derivatives of the scaling functions, and time-derivatives of the curvature g(t)g(t).

The Laplacians are derivatives in R¯\bar{R}, with no angular derivative surviving, when acting on isotropic functions

R2=g2D^;D^[2R¯2+(d1)R¯R¯].(5.7)\vec{\nabla}_{\vec{R}}^{2}=g^{2}{\hat{D}}~;{\hat{D}}\equiv\left[\frac{\partial^{2}}{\partial{\bar{R}}^{2}}+\frac{(d-1)}{\bar{R}}\frac{\partial}{\partial{\bar{R}}}\right].~(5.7)

The time derivatives are

G(gR)t={g˙g}R¯G(R¯);(5.8a)\frac{\partial G(gR)}{\partial t}=\left\{\frac{\dot{g}}{g}\right\}{\bar{R}}G^{\prime}({\bar{R}});~~~(5.8a)
2G(gR)t2={g¨g}R¯G(R¯)+{g˙g}2R¯2G′′(R¯),(5.8b)\frac{\partial^{2}G(gR)}{\partial t^{2}}=\left\{\frac{\ddot{g}}{g}\right\}{\bar{R}}G^{\prime}(\bar{R})+\left\{\frac{\dot{g}}{g}\right\}^{2}{\bar{R}}^{2}G^{\prime\prime}(\bar{R}),~~(5.8b)

where primes denote derivatives GdG/dR¯,G′′d2G/dR¯2G^{\prime}\equiv dG/d{\bar{R}},G^{\prime\prime}\equiv d^{2}G/d{\bar{R}}^{2} and so on. Note the prefactors of the curvature time-derivatives contain G(R¯)G^{\prime}(\bar{R}), which is slowly varying at its turning points G′′(R¯=R¯0)=0G^{\prime\prime}(\bar{R}=\bar{R}_{0})=0.

The Cahn-Hilliard (CH) dynamics is, setting ξ0=1\xi_{0}=1,

{g˙g}R¯G(R¯)=gδL[g2D^G(μL)(R¯,g)]g4[D^]2G.(5.9a)\left\{\frac{\dot{g}}{g}\right\}{\bar{R}}G^{\prime}({\bar{R}})=g^{\delta_{L}}\left[g^{2}{\hat{D}}{G}^{(\mu_{L})}({\bar{R}},g)\right]-g^{4}\left[{\hat{D}}\right]^{2}G~.~~(5.9a)

The Bales-Gooding (BG) dynamics is

Λ[{g¨g}R¯G(R¯)+{g˙g}2R¯2G′′(R¯)]=\Lambda\left[\left\{\frac{\ddot{g}}{g}\right\}{\bar{R}}G^{\prime}(\bar{R})+\left\{\frac{\dot{g}}{g}\right\}^{2}{\bar{R}}^{2}G^{\prime\prime}(\bar{R})\right]=
g2+δL[D^G(μL)(R¯)]g4[D^2G]+g2{g˙g}D^(R¯G).(5.9b)g^{2+\delta_{L}}\left[{\hat{D}}G^{(\mu_{L})}({\bar{R}})\right]-g^{4}\left[{\hat{D}}^{2}G\right]+g^{2}\left\{\frac{\dot{g}}{g}\right\}{\hat{D}}({\bar{R}}G^{\prime}).~~(5.9b)

The derivative operators of (5.7) yield

D^G(μL)=1R¯2[(d1)R¯G(μL)+R¯2G(μL)′′];(5.10a){\hat{D}}G^{(\mu_{L})}=\frac{1}{{\bar{R}}^{2}}\left[(d-1){\bar{R}}{G^{(\mu_{L})}}^{\prime}+{\bar{R}}^{2}{G^{(\mu_{L})}}^{\prime\prime}\right]~;~~(5.10a)
D^2G=1R¯4[(3d)(d1)(R¯GR¯2G′′){\hat{D}}^{2}G=\frac{1}{{\bar{R}}^{4}}[(3-d)(d-1)({\bar{R}}G^{\prime}-{\bar{R}}^{2}G^{\prime\prime})
+2(d1)R¯3G+R¯4G];(5.10b)+2(d-1){{\bar{R}}^{3}}G^{\prime\prime\prime}+{\bar{R}}^{4}G^{\prime\prime\prime\prime}]~;~~~~~~(5.10b)
D^[R¯G]=1R¯2[(d1)R¯G+(d+1)R¯2G′′+R¯3G′′′].(5.10c){\hat{D}}\left[{\bar{R}}G^{\prime}\right]=\frac{1}{{\bar{R}}^{2}}\left[(d-1){\bar{R}}G^{\prime}+(d+1){\bar{R}}^{2}G^{\prime\prime}+{\bar{R}}^{3}G^{\prime\prime\prime}\right].~(5.10c)

Collecting terms above, and dividing through by R¯G(R¯){\bar{R}}G^{{}^{\prime}}({\bar{R}})~, we have for the CH case,

g˙g=J3(R¯)g2+δL+J4(R¯)g4;(5.11a)\frac{-\dot{g}}{g}=J_{3}(\bar{R})g^{2+\delta_{L}}+J_{4}(\bar{R})g^{4};~~(5.11a)

and for the BG case,

Λ[g¨g+I2(R¯){g˙g}2]+K1(R¯){g˙g}g2-\Lambda\left[\frac{\ddot{g}}{g}+I_{2}(\bar{R})\left\{\frac{\dot{g}}{g}\right\}^{2}\right]+K_{1}(\bar{R})\left\{\frac{-\dot{g}}{g}\right\}g^{2}
=J3(R¯)g2+δL+J4(R¯)g4.(5.11b)=J_{3}(\bar{R})g^{2+\delta_{L}}+J_{4}(\bar{R})g^{4}.~~(5.11b)

Here JnJ_{n} are R¯\bar{R}-dependent coefficients of powers gng^{n} of the force terms, while K1(R¯)K_{1}(\bar{R}) is a coefficient of the kinetic damping term. (The Landau term coefficient is called J3(R¯)J_{3}(\bar{R}), as δL=1\delta_{L}=1, later.)

The coefficients in (5.11) are

K1(R¯)[1R¯2][(d1)+(d+1)I2+I3];(5.12a)K_{1}(\bar{R})\equiv\left[\frac{-1}{{{\bar{R}}}^{2}}\right]\left[(d-1)+(d+1)I_{2}+I_{3}\right]~;~~(5.12a)
J3(R¯,T)[1R¯2][(d1)R¯G(μL)+R¯2G(μL)′′]/R¯G;(5.12b)J_{3}(\bar{R},T)\equiv\left[\frac{-1}{{\bar{R}}^{2}}\right][(d-1){\bar{R}}{G^{(\mu_{L})}}^{\prime}+{\bar{R}}^{2}{G^{(\mu_{L})}}^{\prime\prime}]/{\bar{R}}G^{\prime}~;(5.12b)
J4(R¯)[1R¯4][(3d)(d1)(1I2)+2(d1)I3+I4],(5.12c)J_{4}(\bar{R})\equiv\left[\frac{1}{{\bar{R}}^{4}}\right]\left[(3-d)(d-1)(1-I_{2})+2(d-1)I_{3}+I_{4}\right],~(5.12c)

with all in terms of the derivative ratios of G(R¯)G(\bar{R}),

I2R¯2G(μL)′′(R¯)R¯G(R¯);I_{2}\equiv\frac{{{\bar{R}}}^{2}{G^{(\mu_{L})}}^{\prime\prime}({\bar{R}})}{{{\bar{R}}}G^{\prime}({\bar{R}})}~;
I3(R¯)R¯3G′′′(R¯)R¯G(R¯);I4(R¯)R¯4G′′′′(R¯)R¯G(R¯).(5.13)~I_{3}(\bar{R})\equiv\frac{{{\bar{R}}}^{3}G^{\prime\prime\prime}({\bar{R}})}{{{\bar{R}}}G^{\prime}({\bar{R}})}~;I_{4}(\bar{R})\equiv\frac{{{\bar{R}}}^{4}G^{\prime\prime\prime\prime}({\bar{R}})}{{{\bar{R}}}G^{\prime}({\bar{R}})}~.~~(5.13)

So far, this is formally exact, with the only input being a dynamical-scaling trial solution. The coefficient J3J_{3} contains the yet unspecified G(μL)G^{(\mu_{L})}, that carries the higher-order correlations in the OP. Its further evolution equations would induce a dynamically coupled, infinite hierarchy [5] . A closure approximation is needed, and there must be a coefficient evaluation at some physically motivated, expanding-front value of R¯\bar{R}.

V.3 Approximations

a) Closure Approximation:

The correlation between the Landau chemical potential and the OP is

C(μL)=f0(e(r,t))e(r,t)e(r,t).(5.14a)C^{(\mu_{L})}=-\left\langle f_{0}(e(\vec{r},t))~e(\vec{r},t)e(\vec{r^{\prime}},t)\right\rangle.~~(5.14a)

and the factor f0(e)f_{0}(e) carries higher order powers of ee, that induce the correlation hierarchy. For a uniform or bulk order parameter e=±1e=\pm 1, the Landau part of the chemical potential vanishes, μLfL/e=ef0(e)=0\mu_{L}\sim\partial f_{L}/\partial e=-ef_{0}(e)=0. The correlation C(μL)(R,t){C}^{(\mu_{L})}(R,t) has contributions only from the non-uniform OP regions around domain walls, where f0(e)0f_{0}(e)\neq 0 over a thickness ξ0\xi_{0} between the competing bulk values. Thus C(μL){C}^{(\mu_{L})} is a correlation between an OP and many possible DW. It decreases for decreasing DW thickness ξ0\xi_{0}, and C(gξ0)δLC\sim(g\xi_{0})^{\delta_{L}} as in (5.6). Interpreting the scaling function G(μL)G^{(\mu_{L})} as a correlation between the OP and a single DW the prefactor is then the probability of finding a DW, enabling an estimate of δL\delta_{L}.

In a coarsening volume L(t)2L(t)^{2}, the probability of finding a scalar-OP DW is roughly (ξ0L)/L2=ξ0/L=ξ0g(\xi_{0}L)/L^{2}=\xi_{0}/L=\xi_{0}g. The exponent in (5.6) for NOP=1N_{\rm OP}=1 is then δL=1\delta_{L}=1.

As Bray [1] has noted, for general number of OP components, and in dd spatial dimensions, the vanishing at a DW of all the NOPN_{\rm OP} components, corresponds to a ‘surface’ of reduced dimension dNOP>0d-N_{\rm OP}>0. Thus more generally, in a coarsening volume LdL^{d}, the probability of finding a DW is roughly (ξ0NOPLdNOP)/Ld=(ξ0/L)NOP=(ξ0g)NOP(\xi_{0}^{N_{\rm OP}}L^{d-N_{\rm OP}})/L^{d}=(\xi_{0}/L)^{N_{\rm OP}}=(\xi_{0}g)^{N_{\rm OP}}. The exponent for general NOPN_{\rm OP} is then δL=NOP\delta_{L}=N_{\rm OP}, and (5.6) is taken as

C(μL)(R,t)=(gξ0)NOPG(μL)(R¯,gξ0).(5.14b){C}^{(\mu_{L})}(R,t)=(g\xi_{0})^{N_{\rm OP}}G^{(\mu_{L})}(\bar{R},g\xi_{0}).~~~(5.14b)

We make a simple closure approximation for the domain-wall scaling function G(μL)(R¯,gξ0)G^{(\mu_{L})}(\bar{R},g\xi_{0}). To leading order in gξ0g\xi_{0}, we take G(μL)(R¯,gξ0)G(μL)(R¯,0)G^{(\mu_{L})}(\bar{R},g\xi_{0})\simeq G^{(\mu_{L})}(\bar{R},0). (However in Section VI, we will consider possible higher curvature corrections in gξ0g\xi_{0} from G(μL)(R¯,gξ0)G^{(\mu_{L})}(\bar{R},g\xi_{0}), in a toy model for coarsening arrest.) We then replace the DW factor f0(e)f_{0}(e) by its spatial average f¯0(T)=f0(e(r)){\bar{f}}_{0}(T)=\langle f_{0}(e(\vec{r}))\rangle. This yields, as in Appendix A,

G(μL)(R¯,gξ0)G(μL)(R¯,0)=f¯0(T)G(R¯).(5.14c)G^{(\mu_{L})}(\bar{R},g\xi_{0})\simeq G^{(\mu_{L})}(\bar{R},0)=-{\bar{f}}_{0}(T)G(\bar{R}).~~(5.14c)

Thus reasonably, G(μL)G^{(\mu_{L})} has the same R¯\bar{R} dependence as GG, as also holds in other approximations [5].

Inserting this closure approximation into the Landau term coefficient of (5.12b),

J3(R¯)f¯0(T)R¯2[(d1)+I2(R¯)].(5.15)~J_{3}(\bar{R})\simeq\frac{{\bar{f}}_{0}(T)}{{\bar{R}}^{2}}\left[(d-1)+I_{2}(\bar{R})\right]~.~(5.15)

b) Coefficient evaluations

The correlation-function dynamics of (5.11) is now closed, but has a peculiar form, of an equation nonlinear in the curvature g(t)g(t) and its time derivatives; with coefficients linear in G(R¯)G(\bar{R}) and its scaled space derivatives.

The coefficients are evaluated at some constant separation R¯\bar{R}. As the slope G(R¯)G^{\prime}(\bar{R}) is a prefactor in the kinetic terms, it is natural to focus on where it is slowly varying, at its own turning point, G′′(R¯0)=0G^{\prime\prime}({\bar{R}}_{0})=0. This defines a dominant curvature front R=R¯0L(t)R={\bar{R}}_{0}L(t). For both CH and BG dynamics, G(R¯)G(\bar{R}) first has a minimum (G′′>0G^{\prime\prime}>0), and then a maximum (G′′<0G^{\prime\prime}<0), so this point where G′′=0G^{\prime\prime}=0 is somewhere in between. We evaluate all coefficients at the first turning point R¯=R¯0\bar{R}={\bar{R}}_{0} of G(R¯)G^{\prime}(\bar{R}), that is also a non-stationary inflection point of the scaled correlation G(R¯)G(\bar{R}).

With G′′(R¯0)=0G^{\prime\prime}({\bar{R}}_{0})=0 and hence I2(R¯0)=0I_{2}({\bar{R}}_{0})=0, the coefficients are

K10K1(R¯0)=[1R¯02][I3(R¯0)+(d1)];(5.16a)K_{10}\equiv K_{1}({\bar{R}}_{0})=\left[\frac{-1}{{{\bar{R}}_{0}}^{2}}\right]\left[I_{3}(\bar{R}_{0})+(d-1)\right]~;~~(5.16a)
J30J3(R¯0)=f¯0(T)(d1)R¯02;(5.16b)J_{30}\equiv J_{3}({\bar{R}}_{0})=\frac{{\bar{f}}_{0}(T)~(d-1)}{{\bar{R}_{0}}^{2}}~;~~~(5.16b)
J40J4(R¯0)J_{40}\equiv J_{4}({\bar{R}}_{0})
=[1R¯04][I4(R¯0)+2(d1)I3(R¯0)+(3d)(d1)].(5.16c)=\left[\frac{1}{{\bar{R}_{0}}^{4}}\right]\left[I_{4}(\bar{R}_{0})+2(d-1)I_{3}(\bar{R}_{0})+(3-d)(d-1)\right].~(5.16c)

Note that I2=0I_{2}=0 in the inertial term of (5.8b), suppresses nonlinearities, leaving just a curvature acceleration, Λg¨/g\sim\Lambda\ddot{g}/g. Fits to G(R¯)G(\bar{R}) in Appendix B yield R¯0>1{\bar{R}}_{0}>1.

An alternative, and equivalent choice for coefficient evaluation is where the OP gradient-gradient correlation, or effective DW-DW correlation

Γ(R¯)g2re(r,t).re(r,t)(5.17)\Gamma(\bar{R})\equiv g^{-2}\langle\nabla_{\vec{r}}~e(\vec{r},t).\nabla_{\vec{r^{\prime}}}~e(\vec{r^{\prime}},t)\rangle~(5.17)

flattens to zero. Fig 15d of Appendix B shows that this flattening occurs near the previous choice, of the first inflection point R¯/R¯0=1{\bar{R}}/{\bar{R}}_{0}=1. This gives a physical justification to our evaluation choice.

The simple approximations made here are solely for the limited purpose of determining the now-constant coefficients, of a curvature kinetics.

VI Curvature Kinetics

The dynamics is now in terms of g(t)g(t) only, and can yield exponent behaviour for appropriate coefficient signs; with possible crossovers in time between these exponents.

The curvature kinetics, derived from a given order parameter dynamics, yields five main results.
i) There are time regimes where the curvatures decay as single power laws in time g1/tαg\sim 1/t^{\alpha}.
ii) The exponents α\alpha are ratios of integers, induced directly from the integer powers of the curvatures, in each derived kinetics.
iii) In addition to the long-time exponents, there can also be different exponent behaviour at intermediate times, from two different force terms sequentially balancing the kinetic term.
iv) The exponents are manifestly independent of spatial dimension dd that can be scaled out, but can depend on the number of order parameter components NOPN_{\rm OP}.
v) The scaled kinetics can be solved analytically in some cases, providing a universal scaling function of curvature versus time.

The curvature kinetics for the CH case is

g˙g=J30g2+NOP+J40g4.(6.1)\frac{-\dot{g}}{g}=J_{30}g^{2+N_{\rm OP}}+J_{40}g^{4}.~~(6.1)

The curvature kinetics for the BG case is,

Λ[g¨g]+K10{g˙g}g2-\Lambda\left[\frac{\ddot{g}}{g}\right]+K_{10}\left\{\frac{-\dot{g}}{g}\right\}g^{2}
=J30g2+NOP+J40g4.(6.2)=J_{30}g^{2+N_{\rm OP}}+J_{40}g^{4}.~~(6.2)

We now scale times and curvatures in crossover values tcr,gcrt_{\rm cr},g_{\rm cr}, and define

t¯t/tcr;g¯g/gcr.(6.3)\bar{t}\equiv t/t_{\rm cr}~;~~\bar{g}\equiv g/g_{\rm cr}.~~(6.3)

The ’dot’ notation henceforth is X˙dX/dt¯\dot{X}\equiv dX/d{\bar{t}}, and we pull out the coefficient signs σn\sigma_{n} through Jn0=σn|Jn0|J_{n0}=\sigma_{n}|J_{n0}|.

The curvature kinetics for the CH case is

g¯˙/g¯=σ3{tcrgcr2+NOP|J30|}g¯2+NOP+σ4{tcrgcr4|J40|}g¯4.(6.4a)-{\dot{\bar{g}}}/{\bar{g}}=\sigma_{3}\left\{t_{\rm cr}g_{\rm cr}^{2+N_{\rm OP}}|J_{30}|\right\}{\bar{g}}^{2+N_{\rm OP}}+\sigma_{4}\left\{t_{\rm cr}g_{\rm cr}^{4}|J_{40}|\right\}{\bar{g}}^{4}.~(6.4a)

Choosing both the curly brackets to be unity,

gcr=[|J30||J40|]1/λ;tcr=[|J40|2+NOP|J30|4]1/λ(6.4b).g_{\rm cr}=\left[\frac{|J_{30}|}{|J_{40}|}\right]^{1/\lambda};~~t_{\rm cr}=\left[\frac{|J_{40}|^{2+N_{\rm OP}}}{~|J_{30}|^{4}}\right]^{1/\lambda}~~(6.4b).

where λ=2NOP\lambda=2-N_{\rm OP}. For the special case NOP=2N_{\rm OP}=2, there is a line of possible scalings, tcrg¯cr4=1/(|J30|+|J40|)t_{\rm cr}{{\bar{g}}_{\rm cr}}^{4}=1/(|J_{30}|+|J_{40}|).

As discussed in Appendix B, we find from the CH case fits to the data, that R¯04.4\bar{R}_{0}\sim 4.4, independent of τ\tau, and J30,J40J_{30},J_{40} are positive, or σ3=σ4=1\sigma_{3}=\sigma_{4}=1. The CH scaled curvature kinetics is then

g¯˙/g¯=g¯3+g¯4.(6.4c)-{\dot{\bar{g}}}/{\bar{g}}={\bar{g}}^{3}+{\bar{g}}^{4}.~(6.4c)\

The curvature kinetics for the Bales-Gooding case is

{Λ/tcr2}g¯¨/g¯+σ1{|K10|gcr2/tcr}g¯2(g¯˙/g¯)-\left\{\Lambda/t_{\rm cr}^{2}\right\}{\ddot{\bar{g}}}/{\bar{g}}+\sigma_{1}\left\{|K_{10}|g_{\rm cr}^{2}/t_{\rm cr}\right\}{\bar{g}}^{2}(-{\dot{\bar{g}}}/{\bar{g}})
=σ3{|J30|gcr2+NOP}g¯2+NOP+σ4{|J40|gcr4}g¯4.(6.5a)=\sigma_{3}\left\{|J_{30}|g_{\rm cr}^{2+N_{\rm OP}}\right\}{\bar{g}}^{2+N_{\rm OP}}+\sigma_{4}\left\{|J_{40}|g_{\rm cr}^{4}\right\}{\bar{g}}^{4}.~~(6.5a)

Dividing through by {|K10|gcr2/tcr}\{|K_{10}|g_{\rm cr}^{2}/t_{\rm cr}\}, and choosing the crossover scales such that the resultant prefactors are unity as before,

gcr=[|J30||J40|]1/λ;tcr=|K10|[|J40|NOP|J30|2]1/λ;g_{\rm cr}=\left[\frac{|J_{30}|}{|J_{40}|}\right]^{1/\lambda};~~t_{\rm cr}=|K_{10}|~\left[\frac{|J_{40}|^{N_{\rm OP}}}{~|J_{30}|^{2}}\right]^{1/\lambda};
ΛΛ|K10|gcr2tcr=Λ|J40||K10|2.(6.5b)~{\Lambda}^{\prime}\equiv\frac{\Lambda}{|K_{10}|g_{\rm cr}^{2}t_{\rm cr}}=\frac{\Lambda|J_{40}|}{|K_{10}|^{2}}.~(6.5b)

where Λ\Lambda^{\prime} is independent of NOPN_{\rm OP}.

For the BG case, R¯0\bar{R}_{0} and hence the coefficients, depend on τ\tau, as in Fig 15c of Appendix B. While K10,J40K_{10},J_{40} are positive, or σ1=σ4=+1\sigma_{1}=\sigma_{4}=+1, the sign σ3\sigma_{3} of J30J_{30} is that of f¯0(1τ/τf)\bar{f}_{0}\sim(1-\tau/\tau_{f}), as in Appendix B. The BG scaled curvature kinetics is then

Λg¯¨/g¯+g¯2(g¯˙/g¯)=σ3g¯3+g¯4.(6.5c)-{\Lambda}^{\prime}{\ddot{\bar{g}}}/{\bar{g}}+{\bar{g}}^{2}(-{\dot{\bar{g}}}/{\bar{g}})=\sigma_{3}{\bar{g}}^{3}+{\bar{g}}^{4}.~~(6.5c)

Note that in both the CH and BG cases, dd only enters the coefficients, and can be scaled out. The exponents are then predicted to be independent of spatial dimension, as is indeed found in simulations, for the CH case [1, 9], and in the BG case of Fig 12.

We now turn to power-law solutions and their regimes.

VI.1 Exponent regimes for CH equation

For a pure power-law decay, g¯(t)=g¯α/t¯α\bar{g}(t)={\bar{g}}_{\alpha}/\bar{t}^{\alpha}, the time derivative terms in (5.11) are independent of the prefactor g¯α\bar{g}_{\alpha}; and the time powers are independent of α\alpha:

g¯˙g¯=αt¯;g¯¨g¯=α(1+α)t¯2.(6.6)\frac{\dot{\bar{g}}}{\bar{g}}=\frac{-\alpha}{\bar{t}};~~\frac{\ddot{\bar{g}}}{\bar{g}}=\frac{\alpha(1+\alpha)}{{\bar{t}}^{2}}.~(6.6)

For asymptotic vanishing of the curvature g¯(t)0\bar{g}(t)\rightarrow 0, the balancing of kinetic terms with the lowest power of g<1g<1 determines the long-time behaviour; while a balancing with higher powers of curvature determines the intermediate-time behaviour.

With σ3=σ4=+1\sigma_{3}=\sigma_{4}=+1, as in Appendix B, the CH curvature kinetics is (g¯˙/g¯)=g¯3+g¯4(-{\dot{\bar{g}}}/{\bar{g}})={\bar{g}}^{3}+{\bar{g}}^{4}. The kinetic term can balance the two forces sequentially, resulting in two exponents: (g¯˙/g¯)=g¯n(-\dot{\bar{g}}/{\bar{g}})={\bar{g}}^{n}, with n=3,4n=3,4, with power-law solutions g¯=g¯α/t¯α{\bar{g}}={\bar{g}}_{\alpha}/{\bar{t}}^{\alpha}, with α=1/n\alpha=1/n and g¯α=(1/n)1/n\bar{g}_{\alpha}=(1/n)^{1/n}.

In previous results [9], from heuristic arguments, the t¯1/4{\bar{t}}^{1/4}-regime is associated with diffusion of material along interfaces, while the t¯1/3{\bar{t}}^{1/3}-regime is associated with bulk diffusion. In the curvature kinetics approach, these physical results are derived directly, yielding the 1/41/4 exponent from the Ginzburg term, and the 1/31/3 exponent from the Landau term.

We go back to the scaled CH dynamics of (6.4c) and note it can be integrated exactly to yield a theoretical scaling function. For NOP=1N_{\rm OP}=1,

t¯=I(1/g¯)(6.7a){\bar{t}}=I(1/{\bar{g}})~~~~~~~~~~~~~~(6.7a)

where

I(Y)=[=1,2,3{(1)+1Y/}ln|1+Y|](6.7b)I(Y)=[\sum_{\ell=1,2,3}\{(-1)^{\ell+1}Y^{\ell}/\ell\}-\ln|1+Y|]~~(6.7b)

where the sum is the first three terms of an expansion of the logarithm ln(1+(1/g¯))\ln(1+(1/{\bar{g}})). For Y1Y\ll 1, the leading term is Y4Y^{4}, yielding g¯1/t¯1/4\bar{g}\sim 1/{\bar{t}}^{1/4}, while for Y1Y\gg 1 the leading term is Y3Y^{3}, yielding g¯1/t¯1/3\bar{g}\sim 1/{\bar{t}}^{1/3}.

For multicomponent [1, 10] or ’vector’ OP with NOP2N_{\rm OP}\geq 2, the Landau term g¯2+NOP{\bar{g}}^{2+N_{\rm OP}} is comparable to the Ginzburg term g¯4{\bar{g}}^{4} for NOP=2N_{\rm OP}=2; and smaller than it, for NOP>2N_{\rm OP}>2. Hence the long-time exponent is predicted to be α=1/4\alpha=1/4 for vector order parameters. This is again consistent with known 2D simulation results [1], that yield a long-time falloff of g¯1/(tlnt)1/4{\bar{g}}\sim 1/(t\ln t)^{1/4} for NOP=2N_{\rm OP}=2, and of 1/t1/4\sim 1/t^{1/4} for NOP>2N_{\rm OP}>2. The intermediate time exponents are predicted to be α=1/(2+NOP)\alpha=1/(2+N_{\rm OP}), or 1/5,1/6..1/5,1/6.. for NOP=3,4..N_{\rm OP}=3,4.. .

VI.2 Exponent regimes for BG equation

From Appendix B, the coefficient J30f¯0(T)(1τ/τf)J_{30}\sim\bar{f}_{0}(T)\sim-(1-\tau/\tau_{f}) goes from negative to positive on cooling through τ=τf+0.3\tau=\tau_{f}\sim+0.3. Simulations further show there is a possible flattening of the curvature for quenches below some τg0.3\tau_{g}\sim-0.3. Hence we consider three temperature quench ranges, with characteristic exponents.

VI.2.1 τ>τf>τg\tau>\tau_{f}>\tau_{g} quench range

Here σ3=1\sigma_{3}=-1, and the scaled curvature kinetics is

Λg¯¨/g¯+g¯2(g¯˙/g¯)=g¯2+NOP+g¯4.(6.8)-{\Lambda}^{\prime}~{\ddot{\bar{g}}}/{\bar{g}}+{\bar{g}}^{2}(-{\dot{\bar{g}}}/{\bar{g}})=-{\bar{g}}^{2+N_{\rm OP}}+{\bar{g}}^{4}.~~(6.8)

For scalar order parameters NOP=1N_{\rm OP}=1, a balance between the Landau term g¯3{\bar{g}}^{3} and the acceleration term Λ/t¯2\Lambda/{\bar{t}}^{2} yields g¯1/t¯2/3\bar{g}\sim 1/{\bar{t}}^{2/3}. A balance between the Ginzburg term g¯4{\bar{g}}^{4} and the damping term g¯2/t¯{\bar{g}}^{2}/{\bar{t}} supports g¯1/t¯1/2\bar{g}\sim 1/{\bar{t}}^{1/2}. Since damping should dominate acceleration at late times, the kinetics predicts α=2/3\alpha=2/3 in the acceleration-dominated or inertial regime at intermediate times; and α=1/2\alpha=1/2 in the damping-dominated regime at long times. This explains the behaviour of Figs. 8-10. Simulations in other models with inertial terms, [10], can show other exponent sequences of α=1,1/2\alpha=1,1/2.

For vector order parameters with NOP>2N_{\rm OP}>2, the acceleration dominated intermediate-time regime shows exponents α=2/(2+NOP)=2/5,1/3..\alpha=2/(2+N_{\rm OP})=2/5,1/3.. for NOP=3,4..N_{\rm OP}=3,4..; while the damping dominated late-time regime shows exponent α=1/2\alpha=1/2 as before. For the special case NOP=2N_{\rm OP}=2, one needs higher order curvature terms, similar to the toy model as given below, that could yield α=2/5\alpha=2/5, in this quench range.

VI.2.2 τfτ>τg\tau_{f}\geq\tau>\tau_{g} quench range

Here σ3=+1\sigma_{3}=+1, and the Landau term is the wrong sign to balance the acceleration. In fact, going back to the unscaled kinetics if τ=τf\tau=\tau_{f}, then J3=0J_{3}=0, and only the Ginzburg term survives, to balance both the acceleration and damping. Inserting a pure power-law solution g¯=g¯α/t¯α{\bar{g}}={\bar{g}}_{\alpha}/{\bar{t}}^{\alpha},

g¯α4/t¯4α(g¯α2/t¯1+2α)+(Λα(α+1)/t¯2)0,(6.9){{\bar{g}}_{\alpha}}^{4}/{\bar{t}}^{4\alpha}-({{\bar{g}}_{\alpha}}^{2}/{\bar{t}}^{1+2\alpha})+({\Lambda}^{\prime}\alpha(\alpha+1)/{\bar{t}}^{2})\simeq 0,~~(6.9)

This gives α=1/2\alpha=1/2, with a prefactor from solving the quadratic as g¯1/22=(1/4)(1+112Λ){\bar{g}}_{1/2}^{2}=(1/4)(1+\sqrt{1-12\Lambda^{\prime}}).

There is also the possibility of the damping and Landau terms balancing, to give in a narrow τ\tau region, a small final tail g¯1/t<<1{\bar{g}}\sim 1/t<<1 with α=1\alpha=1, but after inaccessibly long crossover times [25].

VI.2.3 τ<τg<0\tau<\tau_{g}<0 quench range

For deep quenches well below the τ=0\tau=0 spinodal, simulations show a peculiar curvature flattening g(t)g0g(t)\rightarrow g_{0}, or the exponent α=0\alpha=0 of Fig 10, corresponding to the possible DW glass [26] of Fig. 4(c) . A similar “coarsening arrest” has been considered elsewhere [22]. We here suggest a toy model, to provide some understanding.

VI.3 Coarsening arrest: a toy model

The closure approximation (5.14c) had kept only the leading term in gξ0g\xi_{0}, approximating G(μL)(R¯,gξ0)G(μL)(R¯,0)=f¯0G(R¯){G^{(\mu_{L})}}(\bar{R},g\xi_{0})\simeq G^{(\mu_{L})}(\bar{R},0)=-{\bar{f}}_{0}~G(\bar{R}), as is reasonable for an asymptotically vanishing curvature. However, if for deep quenches the curvature is constant, then with higher terms, G(μL)(R¯,gξ0)[f¯0+f¯1(gξ0)f¯2(gξ0)2]GG^{(\mu_{L})}(\bar{R},g\xi_{0})\simeq\left[-{\bar{f}}_{0}+{\bar{f}}_{1}~(g\xi_{0})-{\bar{f}}_{2}~(g\xi_{0})^{2}\right]~G, where f¯n{\bar{f}}_{n} are constants. For (6.2) in the damping-dominated regime,

K10{g˙g}g2=[J30X40g+X50g2]g3+J40(τ)g4K_{10}\left\{\frac{-\dot{g}}{g}\right\}g^{2}=\left[J_{30}-X_{40}g+X_{50}g^{2}\right]g^{3}+J_{40}(\tau)g^{4}
=J30g3+{J40(τ)X40}g4+X50g5(6.10)=J_{30}g^{3}+\left\{J_{40}(\tau)-X_{40}\right\}g^{4}+X_{50}g^{5}~~(6.10)

where X40f¯1,X50f¯2X_{40}\sim{\bar{f}}_{1},X_{50}\sim{\bar{f}}_{2} are the extra coefficients, assumed for simplicity to be positive, τ\tau-independent constants.

Refer to caption
Figure 13: (Color online) Curvature Potential: (a) Schematic plot of parameter θ(τ)=1J(τ0)/J(τ)\theta(\tau)=1-J(\tau_{0})/J(\tau) versus τ\tau, showing linear approximation and special temperatures τ=τ0,0,τg\tau=\tau_{0},0,\tau_{g}. (b) Plot of curvature potential V(ρ)V(\rho) versus scaled curvature ρ\rho, for various decreasing values of the scaled variable θ¯(τ){\bar{\theta}}(\tau). Note onset of a metastable minimum in curvature, below θ¯=1\bar{\theta}=-1, at a coarsening arrest onset temperature τg\tau_{g}.

Figure 15(c) of Appendix B shows J40(τ)J_{40}(\tau) has a dip near τ=0\tau=0. Just above this, the falling J40(τ)J_{40}(\tau) could cross the constant at some positive τ=τ0>0\tau=\tau_{0}>0 where J40(τ0)=X40J_{40}(\tau_{0})=X_{40}. Then doing scaling as before to absorb |J30|,|J40(τ)||J_{30}|,|J_{40}(\tau)|, and with the scaled version of the coefficient X50X_{50} factor written without subscripts, as X¯{\bar{X}},

g¯2(g¯˙/g¯)=g¯3+θ(τ)g¯4+X¯g¯5.(6.11){\bar{g}}^{2}(-{\dot{\bar{g}}}/{\bar{g}})={\bar{g}}^{3}+\theta(\tau){\bar{g}}^{4}+{\bar{X}}{\bar{g}}^{5}.~~(6.11)

where

θ(τ)1J40(τ0)/J40(τ)b(τ/τ01)(6.12)\theta(\tau)\equiv 1-J_{40}(\tau_{0})/J_{40}(\tau)\simeq b(\tau/\tau_{0}-1)~(6.12)

and θ(τ0)=0\theta(\tau_{0})=0.

Drawing on the J40(τ)J_{40}(\tau) behaviour of Fig. 15(c), we assume a θ\theta versus τ\tau curve as in the schematic of Fig. 13(a), and for ease of discussion, assume linearity around τ0\tau_{0}, as in (6.12), followed by a low-temperature levelling (dashed curve). The slope bb, in terms of the J40(τ)J_{40}(\tau) values at τ=τ0,0\tau=\tau_{0},0, is b=(J(τ0)/J(0))1>0b=(J(\tau_{0})/J(0))-1>0.

Forces in (6.11) vanish at the usual zero-curvature g¯=0{\bar{g}}=0 final value. However, for τ/τ0<1\tau/\tau_{0}<1, i.e., for θ<0\theta<0, the net forces can also vanish at a nonzero, metastable curvature g¯0{\bar{g}}_{0}. Absorbing X¯\bar{X} by defining scaled curvatures and temperature deviations,

ρgX¯;θ¯(τ)=θ(τ)/2X¯,(6.13)\rho\equiv g\sqrt{\bar{X}};~{\bar{\theta}}(\tau)=\theta(\tau)/2\sqrt{\bar{X}},~(6.13)

we find (6.11) becomes

ρ˙=ρ2X¯[1+2θ¯ρ+ρ2]1X¯Vρ,(6.14)\dot{\rho}=\frac{-\rho^{2}}{\sqrt{\bar{X}}}\left[1+2{\bar{\theta}}\rho+{\rho^{2}}\right]\equiv\frac{-1}{\sqrt{\bar{X}}}\frac{\partial V}{\partial\rho},~(6.14)

where VV is an effective curvature potential

V(ρ,θ¯)=ρ33+θ¯ρ42+ρ55(6.15)V(\rho,{\bar{\theta}})=\frac{\rho^{3}}{3}+\frac{{\bar{\theta}}\rho^{4}}{2}+\frac{\rho^{5}}{5}~~(6.15)

with maxima/ minima at roots

ρ±(τ)=θ¯(τ)±θ¯(τ)21(6.16)\rho_{\pm}(\tau)=-{\bar{\theta}(\tau)}\pm\sqrt{{\bar{\theta}(\tau)}^{2}-1}~~(6.16)

provided θ¯<0{\bar{\theta}}<0 and θ¯2>1{\bar{\theta}}^{2}>1. The roots are real only for (sub-spinodal) deep quenches τ<τg\tau<\tau_{g}, below the glassy or ‘coarsening-arrest’ temperature τg<0\tau_{g}<0, defined by θ¯(τg)1{\bar{\theta}}(\tau_{g})\equiv-1. Here,

τg/τ0=[(4X¯/b)1]<0,(6.17)\tau_{g}/\tau_{0}=-\left[(\sqrt{4{\bar{X}}}/b)-1\right]<0,~~(6.17)

and ρ(τg)=1\rho(\tau_{g})=1. See Fig. 13(a).

The curvature potential VV is plotted in Fig. 13(b), showing manifestly metastable minima. To check that parameters are reasonable and obey required constraints, we draw on Fig. 15(c) to estimate values as τ0+0.025,J(τ0)10,J(0)1\tau_{0}\simeq+0.025,J(\tau_{0})\simeq 10,J(0)\simeq 1 so that b10>0b\simeq 10>0. Taking X¯=100{\bar{X}}=100, one has τg0.025<0\tau_{g}\simeq-0.025<0; and θ(τg)20\theta(\tau_{g})\simeq-20. The trapped curvature is then g0(τg)0.1g_{0}(\tau_{g})\simeq 0.1, comparable to the flat value of Fig. 10.

The intermediate-time curvature decay towards the metastable value g0g_{0}, is dominated by the highest power, g¯˙X¯g¯4\dot{\bar{g}}\simeq-{\bar{X}}{\bar{g}}^{4}, that yields g¯1/t¯1/3{\bar{g}}\sim 1/{\bar{t}}^{1/3}, or α=1/3\alpha=1/3, preceding the curvature flattening, as is indeed the case in Fig. 10. The (dd-independent) toy model thus explains the relevant coarsening-arrest features seen in Fig. 10 for 2D, and in Fig. 12 for 3D.

VII Discussion and Future Work

Dynamical scaling is found in numerical simulations for martensitic models with first-order transitions and Bales-Gooding dynamics. The coarsening exponent values include α=2/3,1/2\alpha=2/3,1/2 for intermediate and long times. For deep quenches there is some indication α=1/3\alpha=1/3 can occur, before an α=0\alpha=0 value of coarsening arrest.

The simulation exponents are theoretically understood through a curvature kinetics, can be generally derived as follows. i) Derive the dynamics of the two-point OP-OP correlation function, from a given OP-dynamics. ii) Insert a dynamical scaling form, as an ansatz solution, with partial time derivatives now yielding total time derivatives of the curvature, multiplying space derivatives of the scaled correlation function. iii) Make approximations that (a) treat the chemical potential-OP correlation as a DW-OP correlation and (b) spatially average the internal DW profile to yield a two-point OP-OP correlation, providing closure of the hierarchy. iv) Evaluate coefficients at a dominant curvature front, yielding a characteristic curvature kinetics for the given OP-dynamics. v) Balance kinetic and force terms, to find powerlaw contributions, and their exponents.

We will elsewhere study the effects of compatibility-induced power-law anisotropic interactions. Since the Fourier kernels are scale-independent, dynamic scaling could again hold. Further work could study multicomponent martensitic order-parameter dynamics with NOP=2,3N_{\rm OP}=2,3 and NV=3,4,6N_{V}=3,4,6; and for both 2D and 3D.

More generally, the curvature kinetics method could be tried out on other models such as binary fluids, where different sequential exponents α=1/3,1,2/3\alpha=1/3,1,2/3 also occur [1]. Of course, in the case of fluids, we have to deal with two coupled equations for the composition and velocity fields.

Acknowledgements: It is a pleasure to thank Prasad Perlekar and Surajit Sengupta for useful conversations. NS acknowledges support from the University Grants Commission, India for a Dr. D. S. Kothari Postdoctoral Fellowship.

Appendix A: Closure approximation for Correlation Dynamics

The DW-OP correlation of (5.14a) is

C(μL)=<f0(e)e(r,t)e(r,t)>,(A1)C^{(\mu_{L})}=-<f_{0}(e)~e(\vec{r},t)~e(\vec{r^{\prime}},t)>~,~~~~(A1)

where the factor f0(e)f_{0}(e) vanishes for the equilibrium, uniform OP, f0(ε¯)=0f_{0}(\bar{\varepsilon})=0, and is nonzero only in a region of order ξ0\xi_{0} around the domain walls, i.e., in a relative volume (ξ0/L)(\xi_{0}/L). In a closure approximation, we spatially average at each domain wall, the factor as <f0(e(x))>f¯0(T)<f_{0}(e(x))>\equiv{\bar{f}}_{0}(T) so

C(μL)(R,t)(ξ0/L)f¯0(T)G(R/L).(A2){C}^{(\mu_{L})}(R,t)\simeq-(\xi_{0}/L){\bar{f}}_{0}(T)G(R/L).~~~(A2)

Note that [1] the total chemical potential around a spherical domain wall is a constant μ<0\mu<0 inside, and μσ/R=σ/R¯L\mu\sim-\sigma/R=-\sigma/{\bar{R}}L outside, where σ\sigma is the surface tension. Hence for fixed R¯{\bar{R}}, one also has effectively, μ1/L\mu\sim 1/L.

Now we estimate the average f¯0{\bar{f}}_{0} for a domain wall. For the CH case and a double-well scaled Landau potential, fL=e2+e4/2f_{L}=-e^{2}+e^{4}/2, so f0(e)=1e2,f_{0}(e)=1-e^{2},~~ as plotted versus ee in Fig. 14(a). In a direction perpendicular to the domain wall and a thickness ξ0\sim\xi_{0}, we take a linear profile e=x{e}=x for |x|<1|x|<1; and flat at e(x)=±1{e}(x)=\pm 1 for |x|>1|x|>1. Then spatially averaging, <x¯2>=1/3<\bar{x}^{2}>=1/3 and

f¯0=(2/3)(A3){\bar{f}}_{0}=(2/3)~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~(A3)

is constant, as in Fig. 14(b). Thus, for the CH case, J3f¯0>0J_{3}\sim{\bar{f}}_{0}>0 is always positive, or σ3=+1\sigma_{3}=+1 as used in the text.

Refer to caption
Figure 14: (Color online) Evaluation of prefactor f¯0{\bar{f}}_{0}: First row: (a) Plot of CH case f0(e)f_{0}(e) versus ee, showing it has a maximum at e=0e=0, at the centre of a domain wall, and is zero in the bulk on either side. (b) CH case average f¯0(T){\bar{f}}_{0}(T) versus ϵ\epsilon showing constant positive value. Second row: (c) Plot of BG case f0(e)f_{0}(e) versus ee for τ=0,0.6\tau=0,0.6, showing a double peak, with a minimum at e=0e=0, that can give a negative f0(e)f_{0}(e); (d) BG case average f¯0(T){\bar{f}}_{0}(T) versus τ\tau showing change of sign from negative to positive, on cooling through τ=τf\tau={\tau}_{f}. The approximation gives τf=0.7\tau_{f}=0.7, while the simulation suggests from exponent-change, that τf0.3\tau_{f}\simeq 0.3.

For BG dynamics, and a triple-well scaled Landau potential, f0(e)=3[1e2)(e2ηsc(τ))]f_{0}(e)=3[1-e^{2})(e^{2}-\eta_{\rm sc}(\tau))] as plotted versus ee in Fig. 14(c), where ηscτ/3ε¯4\eta_{\rm sc}\equiv\tau/3{\bar{\varepsilon}}^{4}. We take linear profiles e=xe=x as before, for simplicity (although the martensitic profiles actually are different [14]), to obtain

f¯0=3[(1+ηsc)<x2><x4>ηsc],(A4){\bar{f}}_{0}=3[(1+\eta_{\rm sc})<x^{2}>-<x^{4}>-\eta_{\rm sc}],~(A4)

or

f¯0(τ)=(2/5)[15ηsc(τ)].(A5){\bar{f}}_{0}(\tau)=(2/5)[1-5\eta_{\rm sc}(\tau)].~~(A5)

From Fig. 14(d), f¯0(τ){\bar{f}}_{0}(\tau) changes sign from negative to positive on cooling through some τ=τf\tau=\tau_{f}. The temperature dependence of f0(T)f_{0}(T) comes from the first-order nature of the Landau free energy fL(e)f_{L}(e). A linear form is

f¯0(τ)=(2/5)[1τ/τf].(A6){\bar{f}}_{0}(\tau)=(2/5)[1-\tau/\tau_{f}].~~(A6)

The exponent α=2/3\alpha=2/3 is supported for τ>τf\tau>\tau_{f} when f¯0<0{\bar{f}}_{0}<0, and simulations find this exponent for τ<τf+0.3\tau<\tau_{f}\simeq+0.3. However, the above mean-field-like approximation yields a higher value, τf+0.7\tau_{f}\simeq+0.7.




Appendix B: Coefficients of curvature kinetics

The coefficients J3(R¯),J4(R¯),K1(R¯)J_{3}(\bar{R}),J_{4}(\bar{R}),K_{1}(\bar{R}) are evaluated at some dominant scale R¯0{\bar{R}}_{0}. The scaled function G(R¯)G(\bar{R}) is fitted to a hexic-exponential function

G(R¯)=[1+=16bR¯]eλR¯(B1)G(\bar{R})=\left[1+{\sum_{\ell=1}}^{6}b_{\ell}{\bar{R}}^{\ell}\right]e^{-\lambda{\bar{R}}}~~(B1)

from the origin at R¯=0\bar{R}=0 to R¯=10\bar{R}=10. We choose R¯0{\bar{R}}_{0} as the non-stationary inflection point where G′′(R¯0)=0G^{\prime\prime}({\bar{R}}_{0})=0, while G(R¯0)0G^{\prime}({\bar{R}}_{0})\neq 0.

The CH value is R¯0=4.4{\bar{R}}_{0}=4.4, independent of temperature, as expected from the OP-scaled CH dynamics with a second-order transition. The coefficients are positive, J30=+0.03;J40=+0.25J_{30}=+0.03;J_{40}=+0.25, so the signs are σ3=σ4=+1\sigma_{3}=\sigma_{4}=+1.

The BG value R¯0(τ){\bar{R}}_{0}(\tau) is temperature- dependent through the residual ηsc(τ)\eta_{\rm sc}(\tau) of (2.16) in the OP-scaled BG dynamics with a first-order transition. Figure 15(a) shows the values of R¯0{\bar{R}}_{0} versus τ\tau, and Fig. 15(c) shows the coefficients evaluated at this R¯0(τ){\bar{R}}_{0}(\tau). Since K10>0,J40>0K_{10}>0,J_{40}>0, the signs are σ1=σ4=+1\sigma_{1}=\sigma_{4}=+1 always. From Fig 15b, the sign of J30f0(T)/R¯0(τ)J_{30}\sim f_{0}(T)/{\bar{R}}_{0}(\tau) is negative for τ>τf\tau>\tau_{f} (supporting an exponent α=2/3\alpha=2/3), but changes sign to positive on cooling through τf\tau_{f}. These results are used in the curvature kinetics of the text.

The text also has a toy model for coarsening arrest [22] with the g4g^{4} effective-coefficient dependent on J40(τ)X¯J_{40}(\tau)-\bar{X} where X¯\bar{X} is a constant. Note the Fig 15a local maxima in R¯0{\bar{R}}_{0} at τ=0\tau=0 and 0.30.3, show up in the Fig 15c curves of J40(τ)1/R¯0(τ)J_{40}(\tau)\sim 1/{\bar{R}}_{0}(\tau), as local minima. Thus the fall of J40(τ)J_{40}(\tau) for temperatures just below the τ=0\tau=0 spinodal, can make the effective g4g^{4} coefficient J40(τ)X¯J_{40}(\tau)-\bar{X} go negative at low temperatures, supporting a metastable glassy state of trapped curvature.

Refer to caption
Figure 15: (Color online) Signs of BG case curvature-dynamics coefficients: a) Plot of coefficient-evaluation choice R¯0(τ){\bar{R}}_{0}(\tau) versus τ\tau from data, with dashed lines as guides to the eye. Arrows mark local maxima near τ=0\tau=0 and τ=τf=0.3\tau=\tau_{f}=0.3. b) Plot of J30f¯0(T)/R¯0(τ)J_{30}\sim{\bar{f}}_{0}(T)/{\bar{R}}_{0}(\tau) versus τ\tau, showing the change in sign at τf0.3\tau_{f}\simeq 0.3; c)Log-linear plot of (positive) coefficients log10(J40)\log_{10}(J_{40}), log10(K10)\log_{10}(K_{10}) versus τ\tau. Arrows mark local minima near τ=0,0.3\tau=0,0.3. d) Plot of domain-wall correlation Γ(R¯)\Gamma(\bar{R}) versus R¯/R¯0(τ)\bar{R}/{\bar{R}}_{0}(\tau), showing that it flattens to zero, close to our inflection-point choice of R¯/R¯0(τ){\bar{R}}/{\bar{R}}_{0}(\tau).

An alternate choice of R¯\bar{R} for coefficient evaluation, is where the domain-wall correlations fall to zero. As domain walls carry nonzero OP gradients, we define the gradient-gradient OP correlations scaled in the curvature as

Γ(R¯)g2re(r,t).re(r,t)=g2r.rG(R¯)\Gamma(\bar{R})\equiv g^{-2}\langle\nabla_{\vec{r}}~e(\vec{r},t).\nabla_{\vec{r^{\prime}}}~e(\vec{r^{\prime}},t)\rangle=g^{-2}\nabla_{\vec{r}}.\nabla_{\vec{r^{\prime}}}G(\bar{R})
=D^G(R¯)=[G′′+(d1)G/R¯].(B2)=-{\hat{D}}G(\bar{R})=-[G^{\prime\prime}+(d-1)G^{\prime}/{\bar{R}}].~(B2)

This is a measure of DW correlations during coarsening, and also appears in the correlation dynamics of (5.9a), (5.9b). Fig 15d shows that Γ(R¯)\Gamma(\bar{R}) flattens to zero close to R¯/R¯0=1{\bar{R}}/{{\bar{R}}_{0}}=1, so this alternative choice gives the same coefficient signs, as our GG-inflection choice.

Appendix C: Coarsening exponents

We here outline the procedure for numerically extracting, from curvature falloffs, the exponent values given in the text.

A possible diagnostic for whether g(t)g(t) has a powerlaw decay component 1/tα\sim 1/t^{\alpha} is to plot tαg(t)t^{\alpha}g(t) versus tt. It will flatten, where α\alpha is the most prominent contribution, and fall (or rise) as tαβt^{\alpha-\beta}, where another exponent β\beta contributes more substantially. Fig 16a shows the variable

Yα=(tε¯4)α(g/ε¯2),(C1)Y_{\alpha}=(t{\bar{\varepsilon}}^{4})^{\alpha}(g/{\bar{\varepsilon}}^{2}),~~~(C1)

plotted versus (tε¯4)(t{\bar{\varepsilon}}^{4}) for the test or trial values α=2/3,1/2\alpha=2/3,1/2. This shows clear signatures of single powerlaw decay contributions, with actual exponents close to these trial values. A supporting width-diagnostic for the time windows, is dlogg/dlogtd\log g/d\log t versus tt (not shown): although the data is noisy, it also shows flat regions as in Fig 16a. Fig 16b shows linear fits in log-log plots within these single-powerlaw, dominance windows, that yield the actual, numerically fitted exponents.

Refer to caption
Figure 16: (Color online) Intermediate and late time BG exponents for τ=0.2\tau=0.2 : (a) Plot of data for YαY_{\alpha} defined in the text vs tε¯4t{\bar{\varepsilon}}^{4}, for test values α=2/3,1/2\alpha=2/3,1/2. Flat regions are from dominance of single power-laws, with exponents close to these test values. Horizontal bars denote the time windows taken, for numerical fits. (b) Plot of log10g/ε¯2\log_{10}g/{\bar{\varepsilon}}^{2} vs log10tε¯4\log_{10}t{\bar{\varepsilon}}^{4} showing lines numerically fitted, within the time windows (see text).

With this procedure, in the dominance time-windows, the exponent mean values and standard deviations, for τ=0.6,0.5,0.4,0.3,0.2,0.1,0.05\tau=0.6,~0.5,~0.4,~0.3,~0.2,~0.1,~0.05 are found to be respectively α=0.619±0.012;0.680±0.018;0.688±0.014;0.683±;0.662±0.015;0.636±0.013;0.649±0.026\alpha=0.619\pm 0.012;~~0.680\pm 0.018;~~0.688\pm 0.014;~~0.683\pm;~~0.662\pm 0.015;~~0.636\pm 0.013;~~0.649\pm 0.026, which are all close to 2/32/3. For τ=0.3,0.2,0.1,0.05\tau=0.3,~0.2,~0.1,~0.05 the exponents are found to be α=0.555±0.03;0.534±0.02;0.543±0.01;0.497±0.01\alpha=0.555\pm 0.03;~~0.534\pm 0.02;~~0.543\pm 0.01;~~0.497\pm 0.01, which are all close to 1/21/2. The exponents are expected to be τ\tau-independent, and a simple arithmetic average yields α=0.661±0.017;α=0.531±0.016\alpha=0.661\pm 0.017;~~\alpha=0.531\pm 0.016. Keeping two significant figures for consistency,

α=0.66±0.02,and0.53±0.02.(C2)\alpha=0.66\pm 0.02,~~~{\text{a}nd}~~~0.53\pm 0.02.~~~~(C2)

For deep quenches of Fig 10, the other exponents seen are α=0.35±0.03;α=0.001±0.002\alpha=0.35\pm 0.03;~~\alpha=0.001\pm 0.002, which are close to 1/31/3 and 00. See Sec. VI on coarsening arrest.

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