A Hamiltonian approach to the strong gravity limit.

Physics

Scientific paper

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General Relativity

Scientific paper

The Hamiltonian for general relativity is examined in the strong gravity (SG) limitG → ∞. In this limit a perfect fluid moves irrotationally along geodesics. An appropriate SG limit for the scalar field is developed such that the energy density has a limit. The solutions in this limit, which were previously known, are shown to come out simply and directly. A classification of the trace-free part of the momentum is given in the Appendix.

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