Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
| dc.creator | Damour, Thibault | |
| dc.creator | Jaranowski, Piotr | |
| dc.creator | Schäfer, Gerhard | |
| dc.date | 2008-03-06 | |
| dc.date.accessioned | 2026-07-07T11:40:41Z | |
| dc.date.available | 2026-07-07T11:40:41Z | |
| dc.description | Using a recent, novel Hamiltonian formulation of the gravitational interaction of spinning binaries, we extend the Effective One Body (EOB) description of the dynamics of two spinning black holes to next-to-leading order (NLO) in the spin-orbit interaction. The spin-dependent EOB Hamiltonian is constructed from four main ingredients: (i) a transformation between the ``effective'' Hamiltonian and the ``real'' one, (ii) a generalized effective Hamilton-Jacobi equation involving higher powers of the momenta, (iii) a Kerr-type effective metric (with Padé-resummed coefficients) which depends on the choice of some basic ``effective spin vector'' $\bf{S}_{\rm eff}$, and which is deformed by comparable-mass effects, and (iv) an additional effective spin-orbit interaction term involving another spin vector $\bsigma$. As a first application of the new, NLO spin-dependent EOB Hamiltonian, we compute the binding energy of circular orbits (for parallel spins) as a function of the orbital frequency, and of the spin parameters. We also study the characteristics of the last stable circular orbit: binding energy, orbital frequency, and the corresponding dimensionless spin parameter $\hat{a}_{\rm LSO}\equiv c J_{\rm LSO}/\boldsymbol(G(H_{\rm LSO}/c^2)^2\boldsymbol)$. We find that the inclusion of NLO spin-orbit terms has a significant ``moderating'' effect on the dynamical characteristics of the circular orbits for large and parallel spins. | |
| dc.description | REVTeX, 22 pages, 7 figures | |
| dc.identifier | https://arxiv.org/abs/0803.0915 | |
| dc.identifier | http://arxiv.org/abs/0803.0915 | |
| dc.identifier | Phys.Rev.D78:024009,2008 | |
| dc.identifier | doi:10.1103/PhysRevD.78.024009 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/200327 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling | |
| dc.type | text |