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Time-Fractional Cahn–Hilliard Equation

Updated 9 July 2026
  • Time-fractional Cahn–Hilliard equation is a phase-field model that replaces the standard time derivative with a Caputo derivative to capture nonlocal memory and anomalous diffusion effects.
  • It preserves the mass-conserving gradient flow structure while introducing modified energy dissipation laws and sharp-interface asymptotics that affect coarsening dynamics.
  • Recent studies focus on structure-preserving discretization techniques that ensure energy stability and accurate convergence on both uniform and nonuniform time grids.

The time-fractional Cahn–Hilliard equation is a phase-field model for phase separation in which the classical first-order time derivative is replaced by a Caputo derivative of order α(0,1)\alpha\in(0,1). In the literature summarized here, this replacement is used to encode nonlocal memory effects, anomalous diffusion, and subdiffusive coarsening, while preserving the Cahn–Hilliard structure of mass-conserving gradient flow. A representative form is

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,

with constant-mobility reductions such as

tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).

For this class of models, the main research themes are derivation from constitutive laws with memory, continuous and discrete energy dissipation, weak solution theory under degenerate mobility and singular free energies, sharp-interface asymptotics, and structure-preserving numerical schemes on uniform and nonuniform time grids (Fritz et al., 2021, Quan et al., 2022, Tang et al., 2021).

1. Governing formulation and constitutive origin

In the time-fractional Cahn–Hilliard model derived from continuum mixture theory, conservation of mass is combined with a memory-modified Fick law. Writing ϕ\phi for the phase variable and μ\mu for the chemical potential, the constitutive relation is

J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},

which leads to

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.

The Caputo derivative is

tαφ(t)=1Γ(1α)0t(ts)αddsφ(s)ds.\partial_t^\alpha \varphi(t)=\frac{1}{\Gamma(1-\alpha)}\int_0^t (t-s)^{-\alpha}\frac{d}{ds}\varphi(s)\,ds.

This model was derived to describe phase separation with nonlocal memory effects, and the analytical framework was developed for positive and degenerating mobility functions together with Landau, Flory–Huggins, and double-obstacle free energies (Fritz et al., 2021).

For constant mobility, the equation is frequently written as

tαu=γΔ ⁣(ε2Δu+F(u)),\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right),

with free energy

E(u)=Ω(ε22u2+F(u))dx.E(u)=\int_\Omega\left(\frac{\varepsilon^2}{2}|\nabla u|^2+F(u)\right)\,dx.

The same free-energy density appears in several numerical studies, often with tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,0 and periodic or homogeneous Neumann boundary conditions (Quan et al., 2022, Yu et al., 13 Jun 2025, Zhang et al., 2020).

A recurring point in the time-fractional literature is that the adjective “fractional” refers specifically to the time derivative. This distinguishes the Caputo-based model from space-fractional Cahn–Hilliard systems involving fractional Laplacians or fractional powers of elliptic operators, which form a separate branch of the literature (Akagi et al., 2015, Colli et al., 2019).

2. Energy structure and modified dissipation laws

A central departure from the classical Cahn–Hilliard equation is that the standard energy dissipation law

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,1

is generally not satisfied for time-fractional phase-field models because of the nonlocal-in-time memory effect. The continuous theory therefore replaces direct monotonicity of tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,2 by monotonicity of a modified, nonlocal-in-time energy that augments the original Ginzburg–Landau functional by a memory accumulation term (Quan et al., 2022).

For the time-fractional Cahn–Hilliard equation, let tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,3 with suitable boundary and mean constraints. The modified energy is

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,4

where

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,5

The key monotonicity statement is

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,6

together with

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,7

Moreover, tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,8, tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ,\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi,9 as tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).0 under convergence to steady state, and tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).1 for fixed tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).2 as tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).3 (Quan et al., 2022).

A related variational formulation introduces

tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).4

for which the continuous inequality

tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).5

serves as the template for variable-step discrete energy laws. This framework is asymptotically compatible with the classical Cahn–Hilliard dissipation law as tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).6 (Ji et al., 2022).

These results clarify a common misconception. For time-fractional Cahn–Hilliard dynamics, monotonic decay of the original energy is not the fundamental structure. The fundamental structure is monotonic decay of a modified energy that includes memory. Numerical studies nevertheless report that the original energy can decay, and in the continuous theory it is shown to decay with respect to time in a small neighborhood at tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).7 (Quan et al., 2022, Yu et al., 13 Jun 2025).

3. Weak solutions, degeneracy, and analytical difficulties

The analytical theory for the Caputo-time model includes existence, uniqueness, and regularity of weak solutions. In the derivation-and-analysis framework based on continuum mixture theory, weak solutions are obtained by the Faedo–Galerkin method, energy estimates, and compactness theorems, with explicit treatment of degenerating mobility and free energies of Landau, Flory–Huggins, and double-obstacle type (Fritz et al., 2021).

A major obstacle is the missing chain rule for fractional derivatives: tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).8 in general. To compensate for this, a fractional chain inequality for semiconvex functions is proved and used to derive the energy-type estimates needed for well-posedness. For positive mobility and Landau potential, existence of weak solutions is established, and uniqueness holds for constant mobility. For degenerate mobility and general potentials, the analysis uses regularized problems for tαu=γΔ ⁣(ε2Δu+F(u)).\partial_t^\alpha u=\gamma \Delta\!\left(-\varepsilon^2\Delta u+F'(u)\right).9 and ϕ\phi0, uniform energy estimates, and entropy-type estimates based on an entropy function ϕ\phi1 with ϕ\phi2; the resulting weak solutions satisfy ϕ\phi3 almost everywhere (Fritz et al., 2021).

This analytical picture suggests that the memory term alters the standard gradient-flow toolkit at a structural level rather than merely perturbing coefficients. A plausible implication is that the main technical novelty of the time-fractional theory lies not in the elliptic part of the equation, but in recovering energy control without the usual local-in-time differential identities.

4. Sharp-interface asymptotics and coarsening laws

Matched asymptotic expansions yield sharp-interface limits that differ from the classical Cahn–Hilliard equation both in kinetics and in timescale separation. For constant mobility, the time-fractional Cahn–Hilliard equation

ϕ\phi4

has two distinguished asymptotic regimes (Tang et al., 2021).

At the timescale ϕ\phi5, the sharp-interface limit is a fractional Stefan problem. The interface law takes the form

ϕ\phi6

At the longer timescale ϕ\phi7, the sharp-interface limit becomes a fractional Mullins–Sekerka problem: ϕ\phi8

ϕ\phi9

μ\mu0

For one-sided degenerate mobility μ\mu1, analogous one-sided fractional Stefan and Mullins–Sekerka limits arise, together with an even slower regime at μ\mu2 (Tang et al., 2021).

The scaling properties of the sharp-interface models imply coarsening laws that are slower than in the classical case. For constant mobility, the predicted rate is

μ\mu3

For one-sided degenerate mobility, a crossover from μ\mu4 to μ\mu5 is obtained at late times (Tang et al., 2021).

This asymptotic picture should be read together with computational observations on transient behavior. One numerical study reports that smaller μ\mu6 can produce faster early coarsening, while another reports that for very small μ\mu7 the initial evolution can be sharper but reaching the steady state takes longer (Zhang et al., 2020, Fritz et al., 2021). These statements concern early-time and long-time regimes, respectively, and are therefore not mutually inconsistent.

5. Structure-preserving discretization

Because time-fractional solutions are singular at the initial time and because the energy law is intrinsically nonlocal, the numerical literature is dominated by nonuniform temporal meshes and modified discrete energies. Several families of schemes have been designed to preserve mass, energy decay, and asymptotic compatibility with the classical μ\mu8 limit (Zhang et al., 2020, Ji et al., 2022, Liao et al., 2022, Yu et al., 13 Jun 2025, Li et al., 24 Aug 2025).

Scheme Temporal approximation Stated properties
Convex-splitting scheme (Zhang et al., 2020) μ\mu9 on non-uniform meshes second-order in time, spectrally accurate in space, uniquely solvable, mass preserving, unconditionally energy stable
Variable-step L1-type schemes (Ji et al., 2022) L1, half-grid L1, averaged L1 L1 and L1J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},0 energy stable; adaptive time stepping; asymptotically compatible as J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},1
Variable-step FBDF2 (Liao et al., 2022) fractional BDF2 discrete energy dissipation law; asymptotically compatible energy; adaptive stepping
Linear relaxation (Yu et al., 13 Jun 2025) L1J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},2-CN linear, second-order accurate in time, unconditionally energy stable
Refined L2-type scheme (Li et al., 24 Aug 2025) variable-step L2-type unique solvability, exact discrete volume conservation, proper energy dissipation laws, optimal convergence rates

In the variable-step L1 analysis, the decisive discrete tools are the discrete orthogonal convolution kernels and discrete complementary convolution kernels. They are used to prove positive definiteness of the discrete fractional derivative and to derive discrete cumulative energies of the form

J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},3

The same work reports that L1J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},4 can lose energy stability if time-step ratios are not controlled (Ji et al., 2022).

For second-order variable-step methods, two developments are especially notable. The FBDF2 scheme introduces a local-nonlocal splitting of the fractional BDF2 formula and proves a discrete energy dissipation law under the weak step-ratio constraint

J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},5

Its modified discrete energy and dissipation law converge, as J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},6, to those of the variable-step BDF2 scheme for the classical Cahn–Hilliard equation (Liao et al., 2022). The refined L2-type analysis further relaxes mesh restrictions to the upper bound

J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},7

eliminating the lower bound used in earlier variable-step L2 theory. The same paper couples this time discretization with a fourth-order compact difference scheme in space and proves exact discrete volume conservation, proper energy dissipation laws, and optimal convergence rates (Li et al., 24 Aug 2025).

A complementary line of work addresses the memory cost directly. By approximating the Laplace spectrum J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},8 of the fractional kernel with a rational function using the adaptive Antoulas–Anderson algorithm, the history integral is replaced by a small system of ODEs. Applied to the time-fractional Cahn–Hilliard problem, this yields a method with J(t)=0tk(ts)m(ϕ(s))μ(s)ds,k(t)=tα1Γ(α),J(t)=-\int_0^t k(t-s)\,m(\phi(s))\nabla\mu(s)\,ds, \qquad k(t)=\frac{t^{\alpha-1}}{\Gamma(\alpha)},9 time and tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.0 memory, together with error bounds and long-time 2D simulations (Khristenko et al., 2021).

6. Stochastic extensions and neighboring fractional models

A stochastic extension of the time-fractional Cahn–Hilliard equation replaces the deterministic right-hand side by a fractionally integrated additive Gaussian noise: tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.1 For this model, a piecewise linear finite element method in space is combined with convolution quadrature in time for both time-fractional operators and an tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.2-projection for the noise. Strong convergence rates are proved for both the spatially semidiscrete and fully discrete schemes, and the temporal Hölder continuity of the solution is identified as a key ingredient in the error analysis. The paper emphasizes that, unlike the stochastic Allen–Cahn equation, the presence of the unbounded elliptic operator in front of the cubic nonlinearity adds substantial complexity (Al-Maskari et al., 2024).

The broader fractional Cahn–Hilliard literature also includes models that are not time-fractional in the Caputo sense. One branch studies space-fractional systems such as

tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.3

with homogeneous Dirichlet boundary conditions of solid type (Akagi et al., 2015), while another treats generalized systems with fractional powers tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.4 and tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.5 and characterizes their omega-limit sets in terms of the first eigenvalue of tαϕ=div(m(ϕ)μ),μ=Ψ(ϕ)ε2Δϕ.\partial_t^\alpha \phi=\operatorname{div}(m(\phi)\nabla\mu),\qquad \mu=\Psi'(\phi)-\varepsilon^2\Delta\phi.6 (Colli et al., 2019). A separate space-fractional Cauchy–Dirichlet theory proves global existence of weak solutions, parabolic smoothing effects, and convergence of each solution to a single equilibrium via a variant of the Łojasiewicz–Simon inequality for the fractional Dirichlet Laplacian (Akagi et al., 2018). This suggests that the phrase “fractional Cahn–Hilliard equation” is not uniform across the literature; in current usage, the time-fractional equation is the Caputo-memory model, whereas fractional Laplacian models belong to a distinct class.

The time-fractional Cahn–Hilliard equation therefore occupies a specific position within the broader fractional phase-field landscape: it retains the mass-conserving Cahn–Hilliard transport structure, but replaces local time evolution by hereditary dynamics. The resulting theory is organized around nonlocal energy functionals, initial-layer-aware time discretizations, and interface laws in which memory persists even in the sharp-interface limit.

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