The deterministic nature of conservative post-Newtonian accurate dynamics of compact binaries with leading order spin-orbit interaction
arXiv:gr-qc/0511009 · doi:10.1103/PhysRevD.72.121501
Abstract
We formally show that the conservative second post-Newtonian (PN) accurate dynamics of spinning compact binaries moving in eccentric orbits, when spin effects are restricted to the leading order spin-orbit interaction cannot be chaotic for the following two distinct cases: (i) the binary consists of compact objects of arbitrary mass, where only one of them is spinning with an arbitrary spin and (ii) the binary consists of equal mass compact objects, having two arbitrary spins. We rest our arguments on the recent determination of PN accurate Keplerian-type parametric solutions to the above cases, indicating that the PN accurate dynamics is integrable in these two situations. We compare predictions of our case (i) with those from a numerical investigation of an equivalent scenario that observed chaos in the associated dynamics. We also present possible reasons for the discrepancies.
arXiv comment5 pages; accepted by PRD
References in corpus (21)
- A Double-Pulsar System - A Rare Laboratory for Relativistic Gravity and Plasma Physics
- Coalescing binary systems of compact objects to (post)$^{5/2}-Newtonian order. V. Spin Effects
- Coalescence of Two Spinning Black Holes: An Effective One-Body Approach
- Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
- Constraining the Equation of State with Moment of Inertia Measurements
- Dimensional regularization of the gravitational interaction of point masses
- Dimensional regularization of the third post-Newtonian dynamics of point particles in harmonic coordinates
- Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits
- Phasing of gravitational waves from inspiralling eccentric binaries
- Poincaré invariance in the ADM Hamiltonian approach to the general relativistic two-body problem
- Third post-Newtonian dynamics of compact binaries: Equations of motion in the center-of-mass frame
- Dynamical invariants for general relativistic two-body systems at the third post-Newtonian approximation
- Gravity Waves, Chaos, and Spinning Compact Binaries
- Post-Newtonian accurate parametric solution to the dynamics of spinning compact binaries in eccentric orbits: The leading order spin-orbit interaction
- On Estimation of the Post-Newtonian Parameters in the Gravitational-Wave Emission of a Coalescing Binary
- Lyapunov timescales and black hole binaries
- The Moment of Inertia of the Binary Pulsar J0737-3039A: Constraining the Nuclear Equation of State
- Gravitomagnetic Effects
- The fate of chaotic binaries
- Ruling Out Chaos in Compact Binary Systems
- A timing formula for main-sequence star binary pulsars
Cited by in corpus (21)
- Phasing of gravitational waves from inspiralling eccentric binaries at the third-and-a-half post-Newtonian order
- Resurvey of order and chaos in spinning compact binaries
- Symplectic structure of post-Newtonian Hamiltonian for spinning compact binaries
- Dynamics of Black Hole Pairs I: Periodic Tables
- Chaos and Order in Models of Black Hole Pairs
- Symplectic Integration of Post-Newtonian Equations of Motion with Spin
- Dynamics of Black Hole Pairs II: Spherical Orbits and the Homoclinic Limit of Zoom-Whirliness
- Characterization of the gravitational wave emission of three black holes
- Chaos in two black holes with next-to-leading order spin-spin interactions
- Second post-Newtonian Lagrangian dynamics of spinning compact binaries
- Integrability of eccentric, spinning black hole binaries up to second post-Newtonian order
- The exact dynamical Chern Simons metric for a spinning black hole possesses a fourth constant of motion: A Dynamical-Systems-Based Conjecture
- Beyond-Newtonian dynamics of a planar circular restricted three-body problem with Kerr-like primaries
- Stability and chaos of hierarchical three black hole configurations
- Extended phase-space symplectic-like integrators for coherent post-Newtonian Euler-Lagrange equations
- A note on the equivalence of Lagrangian and Hamiltonian formulations at post-Newtonian approximations
- Parametric derivation of the observable relativistic periastron advance for binary pulsars
- Energy-conserving integrator for conservative Hamiltonian systems with ten-dimensional phase space
- Escape of photons from two fixed extreme Reissner-Nordström black holes
- Resonant Islands of Effective-One-Body Dynamics
- GPU accelerated manifold correction method for spinning compact binaries