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S.Ezzeroual, B.Sadik / IJOCTA, Vol.15, No.3, pp.396-406 (2025)
                                    P k   2
            If we add the condition      u ≤ 1, the system    A vector v is a symmetry of our system if it
                                      i=1  i
            given by equations Equations(2)-(4), becomes:     satisfies the following two conditions:
                           k             k                             L v (∆) ⊂ ∆  and L v (g) = 0.      (7)
                          X             X   2
                      ˙ x =  u i X i (x),  u ≤ 1,             where L denotes the Lie derivative.    In what
                                            i
                          i=1           i=1             (5)   follows, we outline the necessary steps for com-
                     x(0) = q 0 ,  x(t 1 ) = q 1 ,
                                                              puting the symmetry algebra of a system de-
                     t 1 → min .                              fined by Equations (2)-Eq.(4).    We consider
                                  1
            By Filipov’s theorem, the existence of optimal    ∆ = {∆ q ⊂ T q M | q ∈ M}, where
                                                              ∆ q = span{X 1 (q), . . . , X k (q)}. Additionally,
            solutions for the optimal control problem Equa-
                                                                   P  n
                                                              g =        a
            tion (5), is guaranteed.                                  i=1 i dq i ⊗ dq i , where a i are some con-
                                                  4
                The Pontryagin Maximum Principle provides     stants, represents a Riemannian metric such
                                                              that g(X i , X j ) = δ ij . Furtheremore, we suppose
            necessary conditions for the optimality of trajec-
                                                              that ∆ is a contact distribution, meaning that
            tory solutions of sub-Riemannian control prob-
                                                                                      1
                                                              ker(ω) = ∆, where ω ∈ Λ (M) is a 1-form in the
            lems. Following this principle, we first compute
            trajectories, called extremals, of a dynamic sys-  manifold M. In terms of the local coordinates
            tem in the cotangent bundle of the variety M.     q 1 , . . . , q n , the contact form can be written as
                                                                     n
                                                                   P
                                                                        e
            Then the projections of the extremals on the state  ω =  i=1 i dq i , where e i are scalar functions of
                                                              the coordinates q 1 , . . . , q n . An arbitrary vector
            space M constitute the optimal solutions and are
                                                              field v can be expressed as
            called geodesics. A point γ(t 1 ) is called a Maxwell
                                                              v = h 1 (q 1 , . . . , q n )X 1 +. . .+h n (q 1 , . . . , q n )X n and
            point along a geodesic γ if there exists another ge-
                                                              it is a symmetry vector if it satisfies the two pre-
            odesic eγ ̸≡ γ such that γ(t 1 ) = eγ(t 1 ). This means
                                                              ceding conditions Equation (7). We recall that in
            that there exists a geodesic bγ coming to the point
                                                              local coordinates, each X j is of the form
            q 1 = γ (t 1 ) earlier than γ.
                                                                    P n   j            j
                                                              X j =      g ∂q i , where g are some scalar func-
                                                                      i=1 i            i
                                                              tions defined on M.   Our approach begins by
            3. Computing infinitesimal symmetries
                                                              calculating L v (X 1 ), . . . , L v (X k ):
                of a sub-Riemannian problem
                                                              L v (X j ) = [v, X j ]
            Let (M, ∆, g) be a sub-Riemannian manifold,
                                                                     = [h 1 X 1 + . . . + h n X n , X j ]
            where M is endowed with a Lie group structure
            of dimension n that is left-invariant. This means        = −[X j , h 1 X 1 + . . . + h n X n ]
            that                                                     = −h 1 [X j , X 1 ] − (X j h 1 )X 1 − . . .
                      ∆ ab = L a∗ ∆ b ,
                                                                     − h j [X j , X j ]
                  g b (v, w) = g ab (L a∗ v, L a∗ w),  ∀a, b ∈ M.
                                                                     − (X j h j )X j  − . . . − h n [X j , X n ]
            where L a∗ denotes the differential of the left trans-
                                                                     − (X j h n )X n
            lation by a. We consider the sub-Riemannian sys-
                                                                             n            n       !   n
            tem Equations(2)-(4) on the Lie group (M, ∆, g)                 X     ∂      X    j  ∂h 1  X  1  ∂
                                                                     = −h 1     s i  −       g          g i
            and we assume it is controllable. Then Lie q ∆ =                     ∂q i         i  ∂q i     ∂q i
                                                                            i=1          i=1         i=1
            T q M for every q ∈ M. Therefore,

                                                                                  n       !  n
                                                                                 X   j  ∂h j  X  j  ∂
                     Lie q (∆) = span{X 1 (q), . . . , X k (q),        − . . . −    g i         g i
                                                         (6)                           ∂q i       ∂q i
                       X k+1 (q), . . . , X n (q)}                               i=1        i=1
                                                                                   n            n       !
            for all q ∈ M, where ∆ is given by the vector fields                  X     ∂     X    j  ∂h n
            X 1 , . . . , X k and X k+1 , . . . , X n ∈ Lie(∆). Further-  − . . . − h n  t i  ∂q i  −  g i  ∂q i
                                                                                  i=1          i=1
            more, suppose the problem admits optimal solu-
                                                                      n
            tions.                                                   X    n  ∂
                                                                         g i
            Definition 1. (Agrachev and Barilari.   16)  Let         i=1   ∂q i
            M be a 2m + 1 dimensional manifold. A sub-        where s i and t i are some scalar functions defined
            Riemannian structure on M is said to be contact   on M. Then, applying the condition
            if ∆ is a contact distribution, i.e. ∆ = ker ω,   ω(L v (X j )) = 0 yields an equation of the form:
                        1
            where ω ∈ Λ M satisfies ( V m  dω) ∧ ω ̸= 0.         n        n                n
                                                                X        X     ∂h 1       X     ∂h n
                                                                   b i h i +  c i  + . . . +  d i   = 0, (8)
                By reference to Olver, 17  which provides us                   ∂q i             ∂q i
                                                                i̸=j     i=1              i=1
            with an important result regarding the condi-
                                                              where b i , c i and d i are some scalar functions.
            tions that a symmetry vector must satisfy, we
                                                              Extending the procedure to the all vector fields
            have that:
                                                           398
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