Evolution of small-mass-ratio binaries with a spinning secondary
arXiv:1708.03720 · doi:10.1103/PhysRevD.96.084057
Abstract
We calculate the evolution and gravitational-wave emission of a spinning compact object inspiraling into a substantially more massive (non-rotating) black hole. We extend our previous model for a non-spinning binary [Phys. Rev. D 93, 064024] to include the Mathisson-Papapetrou-Dixon spin-curvature force. For spin-aligned binaries we calculate the dephasing of the inspiral and associated waveforms relative to models that do not include spin-curvature effects. We find this dephasing can be either positive or negative depending on the initial separation of the binary. For binaries in which the spin and orbital angular momentum are not parallel, the orbital plane precesses and we use a more general osculating element prescription to compute inspirals.
17 pages, 6 figures
References in corpus (30)
- Laser Interferometer Space Antenna
- Can environmental effects spoil precision gravitational-wave astrophysics?
- Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
- Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes
- Gravitational wave snapshots of generic extreme mass ratio inspirals
- Gravitational self-force correction to the innermost stable circular orbit of a Schwarzschild black hole
- Gravitational radiation reaction and inspiral waveforms in the adiabatic limit
- Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals
- Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism
- Gravitational waves from intermediate-mass-ratio inspirals for ground-based detectors
- Towards adiabatic waveforms for inspiral into Kerr black holes: II. Dynamical sources and generic orbits
- Computing inspirals in Kerr in the adiabatic regime. I. The scalar case
- An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole
- Gravitational Self-Force Correction to the Innermost Stable Circular Equatorial Orbit of a Kerr Black Hole
- Forced motion near black holes
- A practical, covariant puncture for second-order self-force calculations
- Two-body gravitational spin-orbit interaction at linear order in the mass ratio
- Self-force corrections to the periapsis advance around a spinning black hole
- Tidal invariants for compact binaries on quasi-circular orbits
- Gravitational perturbations and metric reconstruction: Method of extended homogeneous solutions applied to eccentric orbits on a Schwarzschild black hole
- Comparison Between Self-Force and Post-Newtonian Dynamics: Beyond Circular Orbits
- Investigating spinning test particles: spin supplementary conditions and the Hamiltonian formalism
- Second-order perturbation theory: the problem of infinite mode coupling
- Lorenz gauge gravitational self-force calculations of eccentric binaries using a frequency domain procedure
- Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
- Linear-in-mass-ratio contribution to spin precession and tidal invariants in Schwarzschild spacetime at very high post-Newtonian order
- A conservative effect of the second-order gravitational self-force on quasicircular orbits in Schwarzschild spacetime
- Intermediate-mass-ratio-inspirals in the Einstein Telescope: I. Signal-to-noise ratio calculations
- Metric perturbations from eccentric orbits on a Schwarzschild black hole: I. Odd-parity Regge-Wheeler to Lorenz gauge transformation and two new methods to circumvent the Gibbs phenomenon
- Self-force gravitational waveforms for extreme and intermediate mass ratio inspirals. III: Spin-orbit coupling revisited
Cited by in corpus (4)
- Bounds on spinning particles in their innermost stable circular orbits around rotating braneworld black hole
- Spin dynamics of a millisecond pulsar orbiting closely around a massive black hole
- Highly eccentric EMRI waveforms via fast self-forced inspirals
- Orbital spin dynamics of a millisecond pulsar around a massive black hole with an general mass quadrupole