Abstract
We consider the lagrangian in classical (=non-quantized) two-dimensional fourth-order gravity and give new relations to Einstein's theory with a non-minimally coupled scalar field. We distinguish between scale-invariant lagrangians and scale-invariant field equations. is scale-invariant for $F = c_1 R\sp {k+1}$ and a divergence for . The field equation is scale-invariant not only for the sum of them, but also for . We prove this to be the only exception and show in which sense it is the limit of $\frac{1}{k} R\sp{k+1}$ as . More generally: Let be a divergence and a scale-invariant lagrangian, then has a scale-invariant field equation. Further, we comment on the known generalized Birkhoff theorem and exact solutions including black holes.
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