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Laplace Transform Method for Partial differential equations
                .



                   Example 5.16, Solve the integral equation

                                                              t
                                                           ∫
                                           κ(t) = e  −t  +     sin(t − τ)κ(τ)dτ.
                                                             0
                .
               . . . . .
                   Solution. We apply the Laplace transform to both sides of the equation so
                   that
                                                            −t
                                           L(κ(t)) = L(e ) + L(sin t)L(κ(t))
                   and
                                                   −t
                                                                 2
                                               L(e )            s + 1           2       1     1
                               L(κ(t)) =                   =              =         +      − .
                                                               2
                                            1 − L(sin t)      s (s + 1)      s + 1     s 2    s
                   Hence
                                                    κ(t) = 2e  −t  + t − 1.

               . . . .

                     Laplace Transform Method for Partial differential

                     equations



               Partial differential equations, like their one-variable counterpart, ordinary
               differential equations, are ubiquitous throughout the scientific spectrum.

               However, they are, in general, more difficult to solve. Yet here again, we may
               apply the Laplace transform method to solve PDE’s by reducing the initial
               problem to a simpler ODE.
                   Partial differential equations come in three types. For a function of two
               variables u = u(x, y), the general second-order linear PDE has the form


                                                  2
                                                            2
                                      2
                                    ∂ u         ∂ u       ∂ u       ∂u       ∂u
                                  a      + 2b         + c       + d     + e      + fu = g,                (5.8)
                                    ∂x 2       ∂x∂y       ∂y  2     ∂x       ∂y
               where a, b, c, d, e, f, g may depend on x and y only. We call (5.8)
                                  2
                   • elliptic if b − ac < 0,
                                       2
                   • hyperbolic if b − ac > 0,
                                      2
                .  • parabolic if b − ac = 0.



                   Example 5.17,
                    1. The heat equation

                                                                      2
                                                            ∂u       ∂ u
                                                                = c
                                                            ∂t       ∂x 2
                        is parabolic.
               . . . . .


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