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5.7 The One-Variable Hirota Operator  221
          5.7   The One-Variable Hirota Operator


          5.7.1  Definition and Taylor Relations
          Several nonlinear equations of mathematical physics, including the Korteweg–
          de Vries, Kadomtsev–Petviashvili, Boussinesq, and Toda equations, can be
          expressed neatly in terms of multivariable Hirota operators. The ability of
          an equation to be expressible in Hirota form is an important factor in the
          investigation of its integrability.
            The one-variable Hirota operator, denoted here by H , is defined as
                                                            n
          follows: If f = f(x) and g = g(x), then
                              	         
 n
                                ∂     ∂

                   H (f, g)=      −        f(x)g(x )
                    n
                               ∂x    ∂x
                                                    x   =x

                              n
                                       n                       d
                           =    (−1) r    D  n−r (f)D (g),  D =  .   (5.7.1)
                                                   r
                                       r                      dx
                             r=0
          The factor (−1) distinguishes this sum from the Leibnitz formula for
                        r
          D (fg). The notation H x , H xx , etc., is convenient in some applications.
           n
          Examples.
                                   1
                        H x (f, g)= H (f, g)= f x g − fg x
                                         = −H x (g, f),
                                   2
                       H xx (f, g)= H (f, g)= f xx g − 2f x g x + fg xx
                                         = H xx (f, g).
          Lemma.
                             e zH (f, g)= f(x + z)g(x − z).
          Proof. Using the notation r = i (→ j) defined in Appendix A.1,
                         ∞
                           z n
             e zH (f, g)=     H (f, g)
                                n
                            n!
                        n=0
                              n(→∞)
                         ∞
                           z  n            n
                      =            (−1) r     D n−r (f)D (g)
                                                       r
                            n!             r
                        n=0    r=0
                        ∞                ∞
                               r
                                  r
                                              n
                           (−1) D (g)        z D n−r (f)
                      =                                  (put s = n − r)
                                r!             (n − r)!
                        r=0           n=0(→r)
                        ∞                ∞
                                            s
                                               s
                                    r
                               r r
                           (−1) z D (g)     z D (f)
                      =                            .
                                 r!           s!
                        r=0             s=0
          These sums are Taylor expansions of g(x − z) and f(x + z), respectively,
          which proves the lemma.
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