In mathematics, an Abel equation of the first kind, named after Niels Henrik Abel, is any ordinary differential equation that is cubic in the unknown function. In other words, it is an equation of the form
                              y          ′                =                  f                      3                          (        x        )                  y                      3                          +                  f                      2                          (        x        )                  y                      2                          +                  f                      1                          (        x        )        y        +                  f                      0                          (        x        )                        where                               f                      3                          (        x        )        ≠        0                . If                               f                      3                          (        x        )        =        0                 and                               f                      0                          (        x        )        =        0                , or                               f                      2                          (        x        )        =        0                 and                               f                      0                          (        x        )        =        0                , the equation reduces to a Bernoulli equation, while if                               f                      3                          (        x        )        =        0                 the equation reduces to a Riccati equation.
The substitution                     y        =                                            1              u                                               brings the Abel equation of the first kind to the "Abel equation of the second kind" of the form
                    u                  u          ′                =        −                  f                      0                          (        x        )                  u                      3                          −                  f                      1                          (        x        )                  u                      2                          −                  f                      2                          (        x        )        u        −                  f                      3                          (        x        )        .                        The substitution
                                                                        ξ                                                            =                ∫                                  f                                      3                                                  (                x                )                                  E                                      2                                                                   d                x                ,                                                                    u                                                            =                                  (                  y                  +                                                                                                                                          f                                                          2                                                                                (                          x                          )                                                                          3                                                      f                                                          3                                                                                (                          x                          )                                                                                                      )                                                  E                                      −                    1                                                  ,                                                                    E                                                            =                exp                                                  (                  ∫                                      (                                          f                                              1                                                              (                    x                    )                    −                                                                                                                        f                                                          2                                                                                      2                                                                                (                          x                          )                                                                          3                                                      f                                                          3                                                                                (                          x                          )                                                                                      )                                                       d                  x                  )                                                                            brings the Abel equation of the first kind to the canonical form
                              u          ′                =                  u                      3                          +        ϕ        (        ξ        )        .                        Dimitrios E. Panayotounakos and Theodoros I. Zarmpoutis discovered an analytic method to solve the above equation generally.