Page 69 - INTRODUCTION TO THE CALCULUS OF VARIATIONS
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56                                                    Classical methods

                         3. Minimal surfaces of revolution.
                            This example will be treated in Chapter 5. Let us briefly present it here.
                                                                         p     2
                            The function under consideration is f (u, ξ)=2πu 1+ ξ and the min-
                            imization problem (which corresponds to minimization of the area of a
                            surface of revolution) is
                                                (                           )
                                                        Z
                                                          b
                                       (P)   inf  I (u)=   f (u (x) ,u (x)) dx  = m
                                                                    0
                                            u∈X
                                                         a
                                       ©      1                              ª
                            where X =   u ∈ C ([a, b]) : u (a)= α, u (b)= β, u > 0  and α, β > 0.
                            The Euler-Lagrange equation and its first integral are
                                         ∙        ¸ 0
                                            u u       p                       02
                                              0
                                                                     00
                                          √         =   1+ u 02  ⇔ u u =1 + u
                                            1+ u 02
                                                           0
                                           p              u u
                                                  02   0
                                          u 1+ u − u √          = λ = constant.
                                                         1+ u 02
                            This leads to
                                                            u 2
                                                       02
                                                      u =    2  − 1.
                                                            λ
                            The solutions, if they exist (this depends on a, b, α and β, see Exercise
                            5.2.3), are of the form (µ being a constant)
                                                              ³ x   ´
                                                  u (x)= λ cosh  + µ .
                                                               λ
                          We conclude this section with a generalization of a classical example.
                                                                                     p     2
                       Example 2.6 Fermat principle. The function is f (x, u, ξ)= g (x, u)  1+ ξ
                       and
                                            (                             )
                                                       b
                                                     Z
                                                                   0
                                   (P)   inf  I (u)=    f (x, u (x) ,u (x)) dx  = m
                                         u∈X
                                                      a
                                 ©                               ª
                                       1
                       where X = u ∈ C ([a, b]) : u (a)= α, u (b)= β . Therefore the Euler-Lagrange
                       equation is
                                          ∙              ¸
                                       d            u 0             p
                                                                           02
                                           g (x, u) √      = g u (x, u)  1+ u .
                                       dx          1+ u 02
                       Observing that
                                               ∙         ¸
                                             d      u 0         u 00
                                                 √        =
                                             dx   1+ u 02    (1 + u ) 3/2
                                                                  02
                       we get
                                                                   ¡     02  ¢
                                    g (x, u) u +[g x (x, u) u − g u (x, u)] 1+ u  =0.
                                            00
                                                        0
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