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Integrability of Nonlinear Systems

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<strong>Nonlinear</strong> Waves, Solitons, and IST 19<br />

where δ is a constant and Tu is the singular integral operator,<br />

(Tu)(x) = 1 ∫ ∞ ( π<br />

)<br />

2δ − cosh<br />

2δ (y − x) u(y)dy, (3.49)<br />

−∞<br />

∫ ∞<br />

and − denotes the principal value integral. (3.48) is referred to as the Intermediate<br />

Long Wave (ILW) equation. Indeed, it has two well known limits:<br />

−∞<br />

a) δ → 0 ILW reduces to the KdV equation,<br />

u t +2uu x + δ 3 u xxx =0, (3.50)<br />

b) δ →∞ ILW reduces to the Benjamin-Ono (BO) equation.<br />

u t +2uu x +Hu xx =0, (3.51)<br />

where Hu is the Hilbert transform,<br />

(Hu)(x) = 1 ∫ ∞<br />

π − u(y)<br />

dy. (3.52)<br />

−∞ y − x<br />

The BO equation was derived in the context <strong>of</strong> long internal gravity waves in<br />

a stratified fluid [14–16], whereas the ILW equation was derived in a similar<br />

context in [17,18]. In [7] the IST analysis associated with the ILW equation and<br />

BO equation is reviewed. The unusual aspect <strong>of</strong> the IST scheme is the fact that<br />

the scattering operator is a differential RHBVP. Related generalizations are also<br />

discussed in [7].<br />

4 IST for 2+1 Equations<br />

In Sect. 2 we discussed the relevance <strong>of</strong> the KP equation in two-dimensional water<br />

waves. The normalized KP equation is given by (1.14). In this section, a broad<br />

outline <strong>of</strong> the main results <strong>of</strong> IST for the KP equation will be outlined. Just as<br />

the KdV equation was the first 1+1 equation linearized by IST methods, the KP<br />

equation was the first nontrivial equation linearized by 2+1 IST methods. After<br />

the methods were established for the KP equation, they were quickly generalized<br />

to other equations such as the Davey-Stewartson equation and the 2+1 N wave<br />

equation (cf. [7]).<br />

The compatible linear system for KP is given by<br />

σv y + v xx + uv =0<br />

(4.1a)<br />

v t +4v xxx +6uv x +3u x v − 3σ(∂x −1 u y )v + γv =0, (4.1b)<br />

∫ x<br />

where ∂x −1 = dx ′ , and γ is an arbitrary constant. In the case when σ 2 = −1,<br />

−∞<br />

i.e., KPI, then (4.1a) is the nonstationary Schrödinger equation. When σ 2 = +1,

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