Page 79 - INTRODUCTION TO THE CALCULUS OF VARIATIONS
P. 79

66                                                    Classical methods

                                                 0
                       Moreover since v = f ξ (x, u, u ) and u satisfies (E), we have
                                           d       d
                                                              0
                                                                           0
                                       0
                                      v =    [v]=    [f ξ (x, u, u )] = f u (x, u, u ) .
                                           dx     dx
                       The second equation follows then from the combination of the above identity
                       and (2.8).
                       Example 2.12 The present example is motivated by classical mechanics. Let
                                                                 2
                                    1
                       m> 0, g ∈ C ([a, b]) and f (x, u, ξ)= (m/2) ξ − g (x) u. The integral under
                       consideration is
                                                  Z  b
                                            I (u)=   f (x, u (x) ,u (x)) dx
                                                                0
                                                   a
                       and the associated Euler-Lagrange equation is
                                                00
                                             mu (x)= −g (x) ,x ∈ (a, b) .
                       The Hamiltonian is then
                                                          v 2
                                              H (x, u, v)=   + g (x) u
                                                          2m
                       while the associated Hamiltonian system is

                                                ⎧
                                                ⎨ u (x)= v (x) /m
                                                    0
                                                   v (x)= −g (x) .
                                                ⎩
                                                    0
                       Example 2.13 We now generalize the preceding example. Let p> 1 and p =
                                                                                         0
                       p/ (p − 1),
                                         1  p                          1   p 0
                              f (x, u, ξ)=  |ξ| − g (x, u) and H (x, u, v)=  |v| + g (x, u) .
                                         p                            p 0

                       The Euler-Lagrange equation and the associated Hamiltonian system are
                                              d  h  0 p−2  i
                                                  |u |  u 0  = −g u (x, u)
                                              dx
                       and
                                                 ⎧         p −2
                                                            0
                                                      0
                                                 ⎨   u = |v|   v
                                                 ⎩
                                                   v = −g u (x, u) .
                                                    0
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