In mathematics, a non-autonomous system of ordinary differential equations is defined to be a dynamic equation on a smooth fiber bundle                     Q        →                  R                         over                               R                        . For instance, this is the case of non-relativistic non-autonomous mechanics, but not relativistic mechanics. To describe relativistic mechanics, one should consider a system of ordinary differential equations on a smooth manifold                     Q                 whose fibration over                               R                         is not fixed. Such a system admits transformations of a coordinate                     t                 on                               R                         depending on other coordinates on                     Q                . Therefore, it is called the relativistic system. In particular, Special Relativity on the Minkowski space                     Q        =                              R                                4                                   is of this type.
Since a configuration space                     Q                 of a relativistic system has no preferable fibration over                               R                        , a velocity space of relativistic system is a first order jet manifold                               J                      1                                1                          Q                 of one-dimensional submanifolds of                     Q                . The notion of jets of submanifolds generalizes that of jets of sections of fiber bundles which are utilized in covariant classical field theory and non-autonomous mechanics. A first order jet bundle                               J                      1                                1                          Q        →        Q                 is projective and, following the terminology of Special Relativity, one can think of its fibers as being spaces of the absolute velocities of a relativistic system. Given coordinates                     (                  q                      0                          ,                  q                      i                          )                 on                     Q                , a first order jet manifold                               J                      1                                1                          Q                 is provided with the adapted coordinates                     (                  q                      0                          ,                  q                      i                          ,                  q                      0                                i                          )                 possessing transition functions
                              q                      ′                          0                                      =                  q                      ′                          0                                      (                  q                      0                          ,                  q                      k                          )        ,                          q                      ′                          i                                      =                  q                      ′                          i                                      (                  q                      0                          ,                  q                      k                          )        ,                                                    q              ′                                            0                                i                          =                  (                                                    ∂                                  q                                      ′                                          i                                                                                                  ∂                                  q                                      j                                                                                            q                          0                                      j                                +                                                    ∂                                  q                                      ′                                          i                                                                                                  ∂                                  q                                      0                                                                                )                                      (                                                            ∂                                      q                                          ′                                              0                                                                                                              ∂                                      q                                          j                                                                                                          q                              0                                            j                                      +                                                            ∂                                      q                                          ′                                              0                                                                                                              ∂                                      q                                          0                                                                                            )                                −            1                          .                The relativistic velocities of a relativistic system are represented by elements of a fibre bundle                               R                ×        T        Q                , coordinated by                     (        τ        ,                  q                      λ                          ,                  a                      τ                                λ                          )                , where                     T        Q                 is the tangent bundle of                     Q                . Then a generic equation of motion of a relativistic system in terms of relativistic velocities reads
                              (                                                                      ∂                                      λ                                                                    G                                      μ                                          α                                              2                                                              …                                          α                                              2                        N                                                                                                                        2                N                                              −                      ∂                          μ                                            G                          λ                              α                                  2                                            …                              α                                  2                  N                                                              )                          q                      τ                                μ                                    q                      τ                                              α                              2                                                    ⋯                  q                      τ                                              α                              2                N                                                    −        (        2        N        −        1        )                  G                      λ            μ                          α                              3                                      …                          α                              2                N                                                              q                      τ            τ                                μ                                    q                      τ                                              α                              3                                                    ⋯                  q                      τ                                              α                              2                N                                                    +                  F                      λ            μ                                    q                      τ                                μ                          =        0        ,                                              G                                    α                              1                                      …                          α                              2                N                                                              q                      τ                                              α                              1                                                    ⋯                  q                      τ                                              α                              2                N                                                    =        1.                For instance, if                     Q                 is the Minkowski space with a Minkowski metric                               G                      μ            ν                                  , this is an equation of a relativistic charge in the presence of an electromagnetic field.