  Multiple methods for deriving the energy-momentum tensor for a physical
theory exist in the literature. The most common methods are to use Noether's
first theorem with the 4-parameter Poincar\'{e} translation, or to write the
action in a curved spacetime and perform variation with respect to the metric
tensor, then return to a Minkowski spacetime. These are referred to as the
Noether and Hilbert (metric/ curved space/ variational) energy-momentum
tensors, respectively. In electrodynamics and other simple models, the Noether
and Hilbert methods yield the same result. Due to this fact, it is often
asserted that these methods are generally equivalent for any theory considered,
and that this gives physicists a freedom in using either method to derive an
energy-momentum tensor depending on the problem at hand. $\dots$ For spin-2,
the ideal candidate to check this equivalence for a more complicated model,
there exist many energy-momentum tensors in the literature, none of which are
gauge invariant, so it is not clear which expression one hopes to obtain from
the Noether and Hilbert approaches unlike in the case of e.g. electrodynamics.
It has been shown, however, that the linearized Gauss-Bonnet gravity model
(second order derivatives, second rank tensor potential) has an energy-momentum
tensor that is unique, gauge invariant, symmetric, conserved, and trace-free
when derived from Noether's first theorem (all the same properties of the
physical energy-momentum tensor of electrodynamics). This makes it the ideal
candidate to check if the Noether and Hilbert methods coincide for a more
complicated model. It is proven here using this model as a counterexample, by
direct calculation, that the Noether and Hilbert energy-momentum tensors are
not, in general, equivalent.
