The overlap of numerical relativity, perturbation theory and post-Newtonian theory in the binary black hole problem
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Publication:5176243
DOI10.1142/S0218271814300225zbMath1310.83020arXiv1408.5505WikidataQ114738589 ScholiaQ114738589MaRDI QIDQ5176243
Publication date: 3 March 2015
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1408.5505
Black holes (83C57) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Gravitational waves (83C35) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (10)
High-Order Post-Newtonian Contributions to Gravitational Self-force Effects in Black Hole Spacetimes ⋮ Hamiltonian formulation of the conservative self-force dynamics in the Kerr geometry ⋮ First law of compact binary mechanics with gravitational-wave tails ⋮ Spin and quadrupole couplings for high spin equatorial intermediate mass-ratio coalescences ⋮ The effective field theorist's approach to gravitational dynamics ⋮ Multipolar particles in helically symmetric spacetimes ⋮ Inspiral into Gargantua ⋮ Horizon surface gravity in corotating black hole binaries ⋮ Accelerated motion and the self-force in Schwarzschild spacetime ⋮ New metric reconstruction scheme for gravitational self-force calculations
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