Simple, efficient method of calculating the Detweiler-Whiting singular field to very high order
arXiv:2404.10082 · doi:10.1103/PhysRevD.110.084007
Abstract
Most self-force calculations rely, in one way or another, on representations of a particle's Detweiler- Whiting singular field. We present a simple method of calculating the singular field to high order in a local expansion in powers of distance from the particle. As a demonstration, we compute the singular field to 14th order in distance, 10 orders beyond the previous state of the art, in the simple case of a scalar charge in circular orbit around a Schwarzschild black hole. We provide the result in both a 4-dimensional form and a decomposed form suitable for use in an m-mode puncture scheme. Our method should have applications in overcoming bottlenecks in current self-force calculations at both first and second order in perturbation theory.
24 pages, 5 figures
References in corpus (46)
- The motion of point particles in curved spacetime
- Self-force and radiation reaction in general relativity
- Self-force via a Green's function decomposition
- Gravitational self force in extreme mass-ratio inspirals
- Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
- FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis
- Gravitational waveforms for compact binaries from second-order self-force theory
- Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
- Second-order gravitational self-force
- Second-order self-force calculation of the gravitational binding energy in compact binaries
- Hadamard Regularization
- Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency
- Gravitational self-force on generic bound geodesics in Kerr spacetime
- The self-consistent gravitational self-force
- Gravitational-wave energy flux for compact binaries through second order in the mass ratio
- Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
- Second Order Gravitational Self-Force
- Regularization of fields for self-force problems in curved spacetime: foundations and a time-domain application
- Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
- A practical, covariant puncture for second-order self-force calculations
- Nonlinear gravitational self-force. I. Field outside a small body
- Self-Force Calculations with a Spinning Secondary
- Frequency-domain calculation of the self force: the high-frequency problem and its resolution
- m-Mode Regularization Scheme for the Self Force in Kerr Spacetime
- Self-force via -mode regularization and 2+1D evolution: III. Gravitational field on Schwarzschild spacetime
- Motion of small objects in curved spacetimes: An introduction to gravitational self-force
- High-order expansions of the Detweiler-Whiting singular field in Schwarzschild spacetime
- Applying the effective-source approach to frequency-domain self-force calculations: Lorenz-gauge gravitational perturbations
- Spinning test body orbiting around a Kerr black hole: Eccentric equatorial orbits and their asymptotic gravitational-wave fluxes
- Second-order perturbation theory: the problem of infinite mode coupling
- Self force via -mode regularization and 2+1D evolution: II. Scalar-field implementation on Kerr spacetime
- Self-force correction to the deflection angle in black-hole scattering: a scalar charge toy model
- Modeling transient resonances in extreme-mass-ratio inspirals
- Transport Equation Approach to Calculations of Hadamard Green functions and non-coincident DeWitt coefficients
- High-order expansions of the Detweiler-Whiting singular field in Kerr spacetime
- Self force via m-mode regularization and 2+1D evolution: Foundations and a scalar-field implementation on Schwarzschild
- 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
- Scalar self-force for highly eccentric equatorial orbits in Kerr spacetime
- Self-force: Computational Strategies
- Metric perturbations of Kerr spacetime in Lorenz gauge: Circular equatorial orbits
- New self-force method via elliptic partial differential equations for Kerr inspiral models
- Applying the effective-source approach to frequency-domain self-force calculations for eccentric orbits
- Highly eccentric EMRI waveforms via fast self-forced inspirals
- Frequency-domain approach to self-force in hyperbolic scattering
- Implementation of a GHZ-Teukolsky puncture scheme for gravitational self-force calculations
- Multi-domain spectral method for self-force calculations
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- The Science of the Einstein Telescope
- Post-adiabatic waveform-generation framework for asymmetric precessing binaries
- Multi-domain spectral method for self-force calculations
- Constants of motion in gravitational self-force theory
- Generic effective sources for first-order in mass-ratio gravitational self-force calculations in Schwarzschild spacetime