Page 58 - INTRODUCTION TO THE CALCULUS OF VARIATIONS
P. 58

Chapter 2



                Classical methods







                2.1    Introduction

                In this chapter we study the model problem
                                   ©           1                         ª
                           (P)  inf I (u): u ∈ C ([a, b]) ,u (a)= α, u (b)= β
                           2
                where f ∈ C ([a, b] × R × R) and
                                           Z  b
                                    I (u)=    f (x, u (x) ,u (x)) dx .
                                                         0
                                            a
                   Before describing the results that we will obtain, it might be useful to recall
                                                n
                the analogy with minimizations in R ,namely
                                                           n
                                       inf {F (x): x ∈ X ⊂ R } .
                                                                             0
                The methods that we call classical consist in finding x ∈ X satisfying F (x)= 0,
                and then analyze the higher derivatives of F so as to determine the nature of the
                critical point x: absolute minimizer or maximizer, local minimizer or maximizer
                or saddle point.
                                                                              0
                   In Section 2.2 we derive the Euler-Lagrange equation (analogous to F (x)= 0
                   n
                                            2
                in R )thatshouldsatisfy any C ([a, b]) minimizer, u,of(P),
                              d
                        (E)     [f ξ (x, u (x) , u (x))] = f u (x, u (x) , u (x)) ,x ∈ [a, b]
                                                               0
                                            0
                             dx
                where for f = f (x, u, ξ) we let f ξ = ∂f/∂ξ and f u = ∂f/∂u.
                                              n
                   In general (as in the case of R ), the solutions of (E) are not necessarily
                minima of (P); they are merely stationary points of I (cf. below for a more
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