Abstract
Abstract We give a detailed canonical analysis of the n-dimensional f(Riemann)
gravity, correcting the earlier results in the literature. We also
write the field equations in the Fischer-Marsden form which is amenable
to identifying the non-stationary energy on a spacelike hypersurface.
We give pure R^2 and R_{\mu\nu}R^{\mu\nu} theories as examples.
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