We considered the phantom cosmology with the lagrangian L = 1 η [1 − 1 + ηg µν φ , µ φ , ν ] − u(φ), which is original from the nonlinear Born-Infeld type scalar field with the lagrangian L = 1 η [1 − 1 − ηg µν φ , µ φ , ν ] − u(φ). This cosmological model can explain the accelerated expansion of the universe with the equation of state parameter ω < −1. We find that the potential u(φ) should be...