The cubic Taylor expansion at the double-zero point isThere are no quadratic or quartic terms because the local vector field is odd under . Set , , and use . The linear transformation is invertible, and the positive time rescaling preserves orbit orientation. With primes denoting , the result isThis supplies the requested cubic functions, with a remainder stronger than .
There is an important normal form check. Setting , straightens the first equation, and differentiating givesIn particular the nilpotent cubic damping invariant is . A nonsingular cubic near-identity transformation and rescaling cannot change this vanishing invariant into the nonzero coefficient in the supplied later normal form. The conclusions for that assumed system are therefore given separately from the independently derived conclusions for the printed original equations.
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