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Heat Flow of Harmonic Mappings

Updated 2 February 2026
  • Heat flow of harmonic mappings is the L²-gradient flow of Dirichlet energy that deforms maps to become harmonic, ensuring optimality in energy reduction.
  • The methodology leverages the Caffarelli–Silvestre–Stinga extension to handle fractional operators and employs Ginzburg–Landau penalization to manage boundary constraints.
  • Key results demonstrate partial regularity, monotonicity formulas, and asymptotic smoothing, leading to global convergence to stationary states.

The heat flow of harmonic mappings is the evolution equation describing the negative L2L^2-gradient flow of the Dirichlet energy for maps between manifolds, providing a canonical deformation from general maps to harmonic maps (critical points of the energy). The subject encompasses the intricate regularity, compactness, uniqueness, and long-time behavior of weak and strong solutions, and extends to fractional, conformal, and free boundary analogues. This field also connects closely to integrability by compensation, monotonicity formulas, and parabolic partial differential equations with nonlocal operators.

1. Half-Harmonic Maps, Free Boundary Harmonic Maps, and Their Energies

Let NRN \subset \mathbb{R}^\ell be a compact Riemannian manifold. In one spatial dimension, a half-harmonic map u:RNu: \mathbb{R} \to N is a critical point of the H˙1/2\dot{H}^{1/2}-energy,

E1/2(u)=12R(Δ)1/4u(x)2dx.E_{1/2}(u) = \frac{1}{2} \int_{\mathbb{R}} |(-\Delta)^{1/4}u(x)|^2\,dx.

In the conformal case m=1m=1, Da Lio and Rivière demonstrated that critical points satisfy (Δ)1/2u(x)Tu(x)N(-\Delta)^{1/2}u(x) \perp T_{u(x)}N distributionally. Millot and Sire established that the harmonic extension U(x,y)U(x,y) of such uu from R\mathbb{R} into the upper half-plane R×[0,)\mathbb{R} \times [0,\infty) yields a classical harmonic map into NN with free boundary, creating a direct correspondence between half-harmonic maps on R\mathbb{R} and harmonic maps on the disk with free boundary on NN. This integrability by compensation is crucial in the one-dimensional setting.

2. The Fractional Heat Flow: Definition and Extension Problem

The half-harmonic heat flow involves the fractional parabolic operator

(tΔ)1/2=F(x,t)(ξ,σ)1((ξ2+iσ)1/2),(\partial_t - \Delta)^{1/2} = \mathcal{F}^{-1}_{(x,t)\to(\xi,\sigma)}\left((|\xi|^2 + i\sigma)^{1/2}\right),

yielding the flow equation

(tΔ)1/2u(x,t)Tu(x,t)N,xRm,t>0,(\partial_t - \Delta)^{1/2}u(x,t) \perp T_{u(x,t)}N, \qquad x \in \mathbb{R}^m,\, t > 0,

with u(x,t)=u0(x)u(x,t) = u_0(x) for t0t \le 0. The equation can be recast via the Caffarelli–Silvestre–Stinga extension: introduce U(x,y,t)U(x,y,t) on R+m+1×R\mathbb{R}^{m+1}_+ \times \mathbb{R} solving

y12stU=divX(y12sXU)y^{1-2s}\,\partial_t U = \operatorname{div}_X(y^{1-2s} \nabla_X U)

with U(x,0,t)=u(x,t)U(x,0,t)=u(x,t) and boundary condition limy0+y12syU(x,y,t)Tu(x,t)N\lim_{y \to 0^+} y^{1-2s} \partial_y U(x,y,t) \perp T_{u(x,t)}N. For s=1/2s=1/2, this reduces to a standard heat equation in the half-space paired with a nonlinear Neumann boundary condition, localizing the fractional operator.

3. Weak Formulation and the Ginzburg–Landau Approximation

Weak solutions are constructed in the weighted Sobolev space H1(R+m+1;y12sdX)H^1(\mathbb{R}_+^{m+1}; y^{1-2s} dX). For the pair (U,u)(U,u), the weak formulation requires:

  • tULt2LX2(y12s)\partial_t U \in L^2_t L^2_X(y^{1-2s}), ULtHX1(y12s)U \in L_{t}^{\infty} H^1_X(y^{1-2s}),
  • U(x,0,t)=u(x,t)U(x,0,t) = u(x,t) for t0t \leq 0,
  • for every test field Φ\Phi with Φ(x,0,t)Tu(x,t)N\Phi(x,0,t) \in T_{u(x,t)}N, the identity

0R+m+1tU,Φ+XU,XΦy12sdXdt=0\int_0^{\infty} \int_{\mathbb{R}_+^{m+1}} \langle \partial_t U, \Phi \rangle + \langle \nabla_X U, \nabla_X \Phi \rangle\, y^{1-2s} dX dt = 0

must hold.

To manage the constraint uNu \in N, a Ginzburg–Landau penalization is introduced on the boundary: limy0+y12syUε=csε2(1uε2)uε.\lim_{y \to 0^+} y^{1-2s} \partial_y U^\varepsilon = -\frac{c_s}{\varepsilon^2} (1 - |u^\varepsilon|^2) u^\varepsilon. The corresponding penalized energy is

Eε(Uε)=12y12sXUε2+cs4ε2(1uε2)2,\mathscr{E}_\varepsilon(U^\varepsilon) = \frac{1}{2} \int y^{1-2s} |\nabla_X U^\varepsilon|^2 + \frac{c_s}{4\varepsilon^2} \int (1 - |u^\varepsilon|^2)^2,

and the time-discretized (Rothe) scheme produces approximate solutions converging to a weak solution of the half-harmonic heat flow.

4. Partial Regularity, Monotonicity, and Energy Quantization

The fundamental existence theorem asserts: for u0H˙1/2(Rm,N)u_0 \in \dot{H}^{1/2}(\mathbb{R}^m,N), there exists a global weak solution u(x,t)u(x,t) with u(,t)=u0u(\cdot,t) = u_0 for t0t \leq 0, and uL(R+;H˙1/2(Rm))u \in L^\infty(\mathbb{R}_+; \dot{H}^{1/2}(\mathbb{R}^m)). There is a closed singular set ΣRm×(0,)\Sigma \subset \mathbb{R}^m \times (0,\infty) of locally finite parabolic mm-Hausdorff measure such that uu is CC^\infty away from Σ\Sigma. Each time slice Σt\Sigma_t has finite (m1)(m-1)-Hausdorff measure.

The monotonicity formula is central: defining

Dε(Z0,R)=R2[12R+m+1XUε2GZ0(X,t0R2)+cs4ε2Rm(1uε2)2GZ0]\mathcal{D}_\varepsilon(Z_0, R) = R^2 \left[ \frac{1}{2} \int_{\mathbb{R}_+^{m+1}} |\nabla_X U^\varepsilon|^2 G_{Z_0}(X, t_0 - R^2) + \frac{c_s}{4\varepsilon^2} \int_{\mathbb{R}^m} (1 - |u^\varepsilon|^2)^2 G_{Z_0} \right]

and analogous Eε(Z0,R)E_\varepsilon(Z_0,R), both are nondecreasing in RR. The local energy inequality and ε\varepsilon-regularity lemma state that sufficiently small energy in a parabolic cylinder implicates regularity in a smaller subcylinder, yielding C1+αC^{1+\alpha} bounds.

5. Long-Time Behavior and Asymptotic Smoothing

For sufficiently large T0T_0 (depending on u0H˙1/2\|u_0\|_{\dot{H}^{1/2}}), Σ[Rm×[T0,))=\Sigma \cap [\mathbb{R}^m \times [T_0, \infty)) = \emptyset and

u(,t)LCt1/2.\|\nabla u(\cdot, t)\|_{L^\infty} \leq C t^{-1/2}.

As tt \to \infty, u(,t)u(\cdot, t) converges in Cloc2C^2_{\mathrm{loc}} to a constant pNp \in N. This demonstrates global smoothing after finite time and convergence to a stationary (constant) state.

6. Comparison to Classical and Boundary Value Heat Flows

The half-harmonic flow is dual to Struwe's classical harmonic map heat flow with free boundary: in the Struwe program, the interior constraint uNu \in N is penalized and the boundary condition remains exact, whereas in the half-harmonic setting, the penalization occurs only at the boundary, and the flow is governed in the bulk by a fractional parabolic operator. Both frameworks rely on monotonicity formulas and ε\varepsilon-regularity arguments, but the half-harmonic case employs parabolic extensions and nonlocal operators, exploiting the Caffarelli–Silvestre–Stinga extension to localize the nonlocal evolution.

7. Key Analytical Tools and Implications

Principal formulas and energy identities include:

  • Energy dissipation for the penalized flows:

ddtEε(Uε(t))+y12stUε2=0.\frac{d}{dt} \mathscr{E}_\varepsilon(U^\varepsilon(t)) + \int y^{1-2s} |\partial_t U^\varepsilon|^2 = 0.

  • Monotonicity in RR for Eε(Z0,R)E_\varepsilon(Z_0, R) and Dε(Z0,R)\mathcal{D}_\varepsilon(Z_0, R).
  • ε\varepsilon-regularity: small energy in a parabolic cylinder controls higher regularity.

The framework demonstrates that partial regularity, energy dissipation, and global smoothing arise from a combination of compensatory integrability (in m=1m=1), penalization methods adapted to fractional operators, and parabolic ε\varepsilon-regularity.

A plausible implication is that this variational–parabolic–extension method generalizes to fractional harmonic flows in higher dimensions and to more general geometric flows subject to nonlocal constraints, subject to analogous monotonicity and compactness principles.

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