The next-to-leading order gravitational spin(1)-spin(2) dynamics in Hamiltonian form
arXiv:0712.1716 · doi:10.1103/PhysRevD.77.081501
Abstract
Based on recent developments by the authors a next-to-leading order spin(1)-spin(2) Hamiltonian is derived for the first time. The result is obtained within the canonical formalism of Arnowitt, Deser, and Misner (ADM) utilizing their generalized isotropic coordinates. A comparison with other methods is given.
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