Fourth order indirect integration method for black hole perturbations: even modes
arXiv:1102.2404 · doi:10.1088/0264-9381/28/13/134012
Abstract
On the basis of a recently proposed strategy of finite element integration in time domain for partial differential equations with a singular source term, we present a fourth order algorithm for non-rotating black hole perturbations in the Regge-Wheeler gauge. Herein, we address even perturbations induced by a particle plunging in. The forward time value at the upper node of the grid cell is obtained by an algebraic sum of i) the preceding node values of the same cell, ii) analytic expressions, related to the jump conditions on the wave function and its derivatives, iii) the values of the wave function at adjacent cells. In this approach, the numerical integration does not deal with the source and potential terms directly, for cells crossed by the particle world line. This scheme has also been applied to circular and eccentric orbits and it will be object of a forthcoming publication.
This series of papers deals with EMRI for LISA. With the respect to the v1 version, the algorithm has been improved; convergence tests and references have been added; v2 is composed by 23 pages, and 6 figures. Paper accepted by Class. Quantum Gravity for the special issue on Theory Meets Data Analysis at Comparable and Extreme Mass Ratios (Capra and NRDA) at Perimeier Institute in June 2010
References in corpus (18)
- Mass, inertia and gravitation
- Motion in alternative theories of gravity
- Binary black hole merger in the extreme mass ratio limit
- Perturbations of Schwarzschild black holes in the Lorenz gauge: Formulation and numerical implementation
- Binary black hole merger in the extreme-mass-ratio limit: a multipolar analysis
- Pragmatic approach to gravitational radiation reaction in binary black holes
- Understanding initial data for black hole collisions
- Scalar self-force on eccentric geodesics in Schwarzschild spacetime: a time-domain computation
- Gravitational perturbations and metric reconstruction: Method of extended homogeneous solutions applied to eccentric orbits on a Schwarzschild black hole
- A One-Parameter Family of Time-Symmetric Initial Data for the Radial Infall of a Particle into a Schwarzschild Black Hole
- A Finite Element Computation of the Gravitational Radiation emitted by a Point-like object orbiting a Non-rotating Black Hole
- Discontinuous Galerkin method for computing gravitational waveforms from extreme mass ratio binaries
- An Efficient Pseudospectral Method for the Computation of the Self-force on a Charged Particle: Circular Geodesics around a Schwarzschild Black Hole
- Finite Element, Discontinuous Galerkin, and Finite Difference Evolution Schemes in Spacetime
- A time-domain fourth-order-convergent numerical algorithm to integrate black hole perturbations in the extreme-mass-ratio limit
- A spectral collocation approximation for the radial-infall of a compact object into a Schwarzschild black hole
- Regular second order perturbations of binary black holes: The extreme mass ratio regime
- A source-free integration method for black hole perturbations and self-force computation: Radial fall