The next-to-leading order gravitational spin(1)-spin(2) dynamics in Hamiltonian form
General Relativity and Quantum Cosmology
2010-02-16 v2 High Energy Astrophysical Phenomena
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.
Keywords
Cite
@article{arxiv.0712.1716,
title = {The next-to-leading order gravitational spin(1)-spin(2) dynamics in Hamiltonian form},
author = {Jan Steinhoff and Steven Hergt and Gerhard Schäfer},
journal= {arXiv preprint arXiv:0712.1716},
year = {2010}
}
Comments
REVTeX4, 5 pages, published version