Let . Expanding shows that the required flux isIndeed , cancelling the from the time derivative. Introduce a potential by , . Equality of its mixed derivatives is precisely the conservation law. With , these equations become the linear auxiliary systemThis is a Lax pair in the affine-potential form used for linear evolution equations. If a homogeneous matrix pair is preferred, set and use , . Its zero-curvature condition has upper-right entry and all other entries zero.
The Cole-Hopf transformation for the sign convention here is , with and . Indeed , soConversely a solution determines a locally nonzero through , ; their compatibility is this Burgers equation. A spatially constant term can be removed by rescaling in time.
Set in the heat-equation pair. Division by givesTheir compatibility can be checked without referring back to : writing , , we have , . The coefficient of in is , and the constant term is . Thus this linear auxiliary pair is compatible exactly for the required viscous Burgers equation. As in part (a), adjoining a constant component turns it into a homogeneous matrix Lax pair.
Balance the time derivative, cubic dispersion and quadratic transport using the cylindrical KdV equation similarity ansatz , on . For the same real cube-root convention can be used separately. Substitution and removal of the common factor giveEvery term is a total derivative: and . Integration therefore gives the requested second-order equationwhere is a constant determined by any additional boundary data. No condition in the question forces .
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