Computational Methods for the Self-Force in Black Hole Spacetimes
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Publication:2999505
DOI10.1007/978-90-481-3015-3_12zbMath1213.83032OpenAlexW1643535179MaRDI QIDQ2999505
Publication date: 13 May 2011
Published in: Mass and Motion in General Relativity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/978-90-481-3015-3_12
Black holes (83C57) Gravitational energy and conservation laws; groups of motions (83C40) Equations of motion in general relativity and gravitational theory (83C10) Computational methods for problems pertaining to relativity and gravitational theory (83-08)
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Cites Work
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- Radiation damping in a gravitational field
- The Gravitational Reaction Force on a Particle in the Schwarzschild Background
- Self-Force on a Scalar Charge in Circular Orbit around a Schwarzschild Black Hole
- Gravitational Self-Force on a Particle Orbiting a Kerr Black Hole
- A New Analytical Method for Self-Force Regularization. II: -- Testing the Efficiency for Circular Orbits --
- Quasilocal contribution to the scalar self-force: Nongeodesic motion
- Gravitational Field of a Particle Falling in a Schwarzschild Geometry Analyzed in Tensor Harmonics
- Stability of a Schwarzschild Singularity
- A toy model for testing finite element methods to simulate extreme-mass-ratio binary systems
- Discontinuous Galerkin method for computing gravitational waveforms from extreme mass ratio binaries
- Adiabatic Expansion for a Metric Perturbation and the Condition to Solve the Gauge Problem for the Gravitational Radiation Reaction Problem
- Adiabatic Evolution of Orbital Parameters in Kerr Spacetime
- A new method to integrate (2+1)-wave equations with Dirac's delta functions as sources
- Probing black holes at low redshift using LISA EMRI observations
- Perturbative evolution of particle orbits around Kerr black holes: time-domain calculation
- Event rate estimates for LISA extreme mass ratio capture sources
- Covariant Self-Force Regularization of a Particle Orbiting a Schwarzschild Black Hole: Mode Decomposition Regularization
- Self-force on static charges in Schwarzschild spacetime
- Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA
- Adiabatic Evolution of Three 'Constants' of Motion for Greatly Inclined Orbits in Kerr Spacetime
- A time-domain fourth-order-convergent numerical algorithm to integrate black hole perturbations in the extreme-mass-ratio limit
- Perspective on gravitational self-force analyses
- From the self-force problem to the radiation reaction formula
- Mass change and motion of a scalar charge in cosmological spacetimes
- A matched expansion approach to practical self-force calculations
- Computing inspirals in Kerr in the adiabatic regime: I. The scalar case
- Constraint damping in the Z4 formulation and harmonic gauge
- Adiabatic Radiation Reaction to Orbits in Kerr Spacetime
- General Relativity
- A rigorous derivation of gravitational self-force
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