Applying the effective-source approach to frequency-domain self-force calculations
arXiv:1311.3104 · doi:10.1103/PhysRevD.89.044046
Abstract
The equations of motion of a point particle interacting with its own field are defined in terms of a certain regularized self-field. Two of the leading methods for computing this regularized field are the mode-sum and effective-source approaches. In this work we unite these two distinct regularization schemes by generalizing traditional frequency-domain mode-sum calculations to incorporate effective-source techniques. For a toy scalar-field model we analytically compute an appropriate puncture field from which the regularized residual field can be calculated. To demonstrate the method, we compute the self-force for a scalar particle on a circular orbit in Schwarzschild spacetime. We also demonstrate the relation between the worldtube and window function approaches to localizing the puncture field to the neighborhood of the worldline and show how the method reduces to the well-known mode-sum regularization scheme in a certain limit. This new computational scheme can be applied to cases where traditional mode-sum regularization is inadequate, such as in calculations at second perturbative order.
13 pages, 1 figure. Correct minor typo and update references
References in corpus (14)
- Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
- Gravitational wave snapshots of generic extreme mass ratio inspirals
- Gravitational self-force correction to the innermost stable circular orbit of a Schwarzschild black hole
- High-Order Post-Newtonian Fit of the Gravitational Self-Force for Circular Orbits in the Schwarzschild Geometry
- A Rigorous Derivation of Electromagnetic Self-force
- An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole
- Conservative, gravitational self-force for a particle in circular orbit around a Schwarzschild black hole in a Radiation Gauge
- Scalar-field perturbations from a particle orbiting a black hole using numerical evolution in 2+1 dimensions
- Nonlinear gravitational self-force. I. Field outside a small body
- Self-Force Calculations with Matched Expansions and Quasinormal Mode Sums
- m-Mode Regularization Scheme for the Self Force in Kerr Spacetime
- Conservative self-force correction to the innermost stable circular orbit: comparison with multiple post-Newtonian-based methods
- Mode-sum regularization of the scalar self-force: Formulation in terms of a tetrad decomposition of the singular field
- Self-Force and Green Function in Schwarzschild spacetime via Quasinormal Modes and Branch Cut
Cited by in corpus (33)
- Black holes, gravitational waves and fundamental physics: a roadmap
- Self-force and radiation reaction in general relativity
- Gravitational waveforms for compact binaries from second-order self-force theory
- Second-order self-force calculation of the gravitational binding energy in compact binaries
- Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
- The Science of the Einstein Telescope
- Highly eccentric inspirals into a black hole
- A practical, covariant puncture for second-order self-force calculations
- Evolution of small-mass-ratio binaries with a spinning secondary
- Tidal invariants for compact binaries on quasi-circular orbits
- Applying the effective-source approach to frequency-domain self-force calculations: Lorenz-gauge gravitational perturbations
- Second-order perturbation theory: problems on large scales
- Dissipation in extreme-mass ratio binaries with a spinning secondary
- 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
- A conservative effect of the second-order gravitational self-force on quasicircular orbits in Schwarzschild spacetime
- Self force on a scalar charge in Kerr spacetime: inclined circular orbits
- Fast spectral source integration in black hole perturbation calculations
- Octupolar invariants for compact binaries on quasi-circular orbits
- Self-force correction to geodetic spin precession in Kerr spacetime
- Applying the effective-source approach to frequency-domain self-force calculations for eccentric orbits
- Accelerated motion and the self-force in Schwarzschild spacetime
- Implementation of a GHZ-Teukolsky puncture scheme for gravitational self-force calculations
- Radiation-Reaction Force on a Small Charged Body to Second Order
- Second-order gravitational self-force in a highly regular gauge: Covariant and coordinate punctures
- Gravitational radiation from a particle plunging into a Schwarzschild black hole: frequency-domain and semirelativistic analyses
- Post-adiabatic waveforms from extreme mass ratio inspirals in the presence of dark matter
- Toward Second-Order Self-Force for Eccentric Extreme-Mass Ratio Inspirals in Schwarzschild Spacetime
- Toward exponentially-convergent simulations of extreme-mass-ratio inspirals: A time-domain solver for the scalar Teukolsky equation with singular source terms
- Eternal binaries
- Generic effective sources for first-order in mass-ratio gravitational self-force calculations in Schwarzschild spacetime
- Hyperboloidal method for frequency-domain self-force calculations