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Marchaud-Type Singular Integral Representation

Updated 31 January 2026
  • Marchaud-type singular integrals are nonlocal operators defined via weighted difference quotients, essential for extending classical derivatives to fractional orders.
  • The approach underpins the spectral time-fractional KdV equation by employing a bilinear Hirota method to preserve soliton structures while altering temporal dispersion.
  • Explicit one- and two-soliton solutions are derived with a precise fractional dispersion law, demonstrating the method’s practical impact on integrable systems.

The spectral time-fractional Korteweg–de Vries (KdV) equation generalizes the integrable KdV model by replacing the classical time derivative with a spectral (Fourier-multiplier) fractional derivative of order 0<α10<\alpha\leq 1. This construction, built via a fractional extension of the Hirota bilinear calculus, directly alters the temporal dispersive character of soliton solutions while preserving the spatial algebraic structure and soliton interaction properties. The approach exploits well-defined nonlocal operators—specifically, the spectral fractional derivative and its bilinear extension—to derive explicit one- and two-soliton τ\tau-functions and the corresponding dispersion relation ωα=k3\omega^\alpha = -k^3 (Ray, 24 Jan 2026).

1. Spectral Fractional Derivative: Definition and Properties

Let fS(R)f\in S(\mathbb{R}) and 0<α10<\alpha\leq 1. The spectral fractional derivative DξαD_\xi^\alpha is defined through its Fourier transform by

F[Dξαf](k)=(ik)αf^(k),\mathcal{F}[D_\xi^\alpha f](k) = (i k)^\alpha \hat{f}(k),

where the principal branch of (ik)α(i k)^\alpha is used. This operator extends by density to Dξα:HsHsαD_\xi^\alpha: H^s\to H^{s-\alpha} for any sRs\in\mathbb{R}.

For 0<α<10<\alpha<1, the Marchaud-type singular integral representation holds: Dξαf(ξ)=Cα0[f(ξ)f(ξy)]y1αdy,Cα=αΓ(1α)=1Γ(α).D_\xi^\alpha f(\xi) = C_\alpha \int_0^\infty [f(\xi) - f(\xi-y)] y^{-1-\alpha}\, dy, \qquad C_\alpha = \frac{\alpha}{\Gamma(1-\alpha)} = -\frac{1}{\Gamma(-\alpha)}.

Bilinear Operator

Defined for f,gS(R)f,g\in S(\mathbb{R}) as

Dξαfg:=(Dξαf)gf(Dξαg),D_\xi^\alpha f\cdot g := (D_\xi^\alpha f)g - f(D_\xi^\alpha g),

this operator is equivalently realized through a two-variable extension Dξ1αDξ2αD_{\xi_1}^\alpha - D_{\xi_2}^\alpha on f(ξ1)g(ξ2)f(\xi_1)g(\xi_2) with evaluation at ξ1=ξ2=ξ\xi_1 = \xi_2 = \xi. Its Fourier symbol is (ik1)α(ik2)α(i k_1)^\alpha - (i k_2)^\alpha, leading to the key form: Dξαfg(ξ)=(2π)2R2[(ik1)α(ik2)α]f^(k1)g^(k2)ei(k1+k2)ξdk1dk2.D_\xi^\alpha f\cdot g(\xi) = (2\pi)^{-2} \int_{\mathbb{R}^2} [(i k_1)^\alpha - (i k_2)^\alpha] \hat{f}(k_1)\hat{g}(k_2) e^{i(k_1+k_2)\xi}\, dk_1\, dk_2. For 0<α<10<\alpha<1, the Marchaud-kernel representation generalizes to

Dξαfg(ξ)=Cα0[f(ξ)g(ξy)f(ξy)g(ξ)]y1αdy.D_\xi^\alpha f\cdot g(\xi) = C_\alpha \int_0^\infty [f(\xi) g(\xi-y) - f(\xi-y) g(\xi)] y^{-1-\alpha} dy.

Algebraic and Sobolev Properties

  • Bilinear in (f,g)(f,g).
  • Skew-symmetric: Dξαfg=DξαgfD_\xi^\alpha f\cdot g = -D_\xi^\alpha g\cdot f.
  • Diagonal vanishing: Dξαff=0D_\xi^\alpha f\cdot f = 0.
  • Bounded: Dξα:Hs×HsHsαD_\xi^\alpha : H^s\times H^s\to H^{s-\alpha}, for s>1/2s > 1/2.
  • Classical limit: DξαfgDξfgD_\xi^\alpha f\cdot g \to D_\xi f\cdot g as α1\alpha \to 1^-.

2. Bilinear Formulation of the Spectral Time-Fractional KdV Equation

The spectral time-fractional KdV equation on Rx×Rt\mathbb{R}_x\times\mathbb{R}_t is

Dtαu+uxxx+6uux=0,0<α1,D_t^\alpha u + u_{xxx} + 6uu_x = 0, \quad 0<\alpha\leq 1,

where DtαD_t^\alpha is the spectral fractional derivative in tt. The Hirota τ\tau-function ansatz is applied: u(x,t)=2x2(logτ(x,t)),τ>0.u(x,t) = 2 \partial_x^2 (\log \tau(x,t)), \qquad \tau > 0. The equivalent bilinear equation is

[DxDtα+Dx4] ττ=0,[D_x D_t^\alpha + D_x^4]\ \tau\cdot\tau = 0,

where DxD_x and Dx4D_x^4 are Hirota operators in xx, and DtαD_t^\alpha is the fractional bilinear operator in tt. This reduction is justified by explicit calculation: the local terms are captured by

Dx2ττ=2τ2(logτ)xx,Dx4ττ=2τ2((logτ)xxxx+6((logτ)xx)2),D_x^2 \tau\cdot\tau = 2\tau^2(\log\tau)_{xx}, \qquad D_x^4 \tau\cdot\tau = 2\tau^2 \left((\log\tau)_{xxxx} + 6((\log\tau)_{xx})^2\right),

while the mixed term satisfies

DxDtαττ=2[τDtατxτxDtατ],D_x D_t^\alpha \tau\cdot\tau = 2[\tau D_t^\alpha \tau_x - \tau_x D_t^\alpha \tau],

which, under standard manipulations, reduces to 2Dtα(logτ)x2D_t^\alpha (\log\tau)_x. Normalizing by τ2\tau^2 yields the equation for uu.

3. Fractional Dispersion Relation

To determine the dispersion law, consider the single exponential ansatz: τ(x,t)=1+eθ,θ=kx+ωt+δ.\tau(x,t) = 1 + e^\theta, \quad \theta = k x + \omega t + \delta. Off-diagonal contributions give

Dxne0xekx=(k)nekx,Dtαe0teωt=ωαeωt.D_x^n e^{0\cdot x}\cdot e^{k x} = (-k)^n e^{k x}, \qquad D_t^\alpha e^{0\cdot t}\cdot e^{\omega t} = -\omega^\alpha e^{\omega t}.

Thus,

(DxDtα+Dx4)(1eθ)=kωαeθ+k4eθ.(D_x D_t^\alpha + D_x^4)(1\cdot e^\theta) = k\omega^\alpha e^\theta + k^4 e^\theta.

Symmetry yields the factor 2[kωα+k4]eθ2[k\omega^\alpha + k^4] e^\theta, leading to the fractional dispersion relation: ωα=k3.\omega^\alpha = -k^3. When α=1\alpha=1, the classical cubic ω=k3\omega=-k^3 is recovered. For 0<α<10<\alpha<1, the phase speed ω/k\omega/k is a nonlinear function of α\alpha, and wave packet dispersion corresponds to a time-rescaled fractional power: ωk3/α\omega\sim k^{3/\alpha}. This suggests that the fractional order parameter α\alpha directly modifies the temporal scaling of dispersive propagation while preserving the cubic dependence on kk structure.

4. Explicit Soliton Solutions

One-Soliton τ\tau-Function

With

τ(x,t)=1+ekx+ωt+δ,\tau(x,t) = 1 + e^{k x + \omega t + \delta},

and dispersion ωα=k3\omega^\alpha=-k^3, the associated solution is

u(x,t)=2x2log(1+ekx+ωt+δ)=2k2sech2(kx+ωt+δ2),u(x,t) = 2 \partial_x^2 \log (1 + e^{k x + \omega t + \delta}) = 2k^2 \,\operatorname{sech}^2 \left(\frac{k x + \omega t + \delta}{2}\right),

a localized pulse with speed determined by the fractional dispersion relation.

Two-Soliton τ\tau-Function

The Hirota ansatz leads to

τ(x,t)=1+eθ1+eθ2+A12eθ1+θ2,\tau(x,t) = 1 + e^{\theta_1} + e^{\theta_2} + A_{12} e^{\theta_1 + \theta_2},

with θj=kjx+ωjt+δj\theta_j = k_j x + \omega_j t + \delta_j and ωjα=kj3\omega_j^\alpha = -k_j^3 for j=1,2j=1,2. The interaction coefficient is

A12=(k1k2k1+k2)2,A_{12} = \left(\frac{k_1 - k_2}{k_1 + k_2}\right)^2,

exactly as in the classical KdV case. The formal two-soliton solution for uu is then u=2x2logτ(x,t)u=2\partial_x^2\log\tau(x,t). In the classical limit α1\alpha\to 1^-, this construction and coefficient reduce directly to the standard KdV soliton result.

5. Summary of Analytical Features

$\begin{array}{lcl} \text{Spectral Fractional Operator} & D_\xi^\alpha f & (i\,k)^\alpha \hat{f}(k) \ \text{Marchaud Integral (0<\alpha<1)} & D_\xi^\alpha f(\xi) & C_\alpha \int_0^\infty [f(\xi) - f(\xi-y)] y^{-1-\alpha} dy \ \text{Bilinear Hirota Operator} & D_\xi^\alpha f\cdot g & (D_\xi^\alpha f)g - f(D_\xi^\alpha g) \ \text{Bilinear KdV Form} & D_x D_t^\alpha \tau\cdot\tau + D_x^4 \tau\cdot\tau & = 0 \ \text{Dispersion Law} & \omega^\alpha & = -k^3 \ \end{array}$

These results demonstrate that the spectral time-fractional KdV equation retains the structure of soliton solutions, with explicit τ\tau-functions and interaction coefficients matching the classical case. A plausible implication is that soliton interaction properties are dictated by the spatial algebraic structure, while the temporal evolution is sensitive to the fractional order. The construction unifies nonlocal calculus and integrable systems while admitting limit transitions to standard models (Ray, 24 Jan 2026).

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