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We study nonrelativistic gravity using the Hamiltonian formalism. For the dynamics of general relativity (relativistic gravity) the formalism is well known and called the Arnowitt-Deser-Misner (ADM) formalism. We show that if the lapse function is constrained correctly, then nonrelativistic gravity is described by a consistent Hamiltonian system. Surprisingly, nonrelativistic gravity can have solutions identical to relativistic gravity ones. In particular, (anti--)de Sitter black holes of Einstein gravity and IR limit of Ho {r} {r}{}ava gravity are locally identical.
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A. A. Kocharyan (2009) studied this question.
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