Reducing orbital eccentricity in binary black hole simulations

DOI10.1088/0264-9381/24/12/S06zbMath1117.83075arXivgr-qc/0702106OpenAlexW2099824817WikidataQ59452806 ScholiaQ59452806MaRDI QIDQ5293846

Harald P. Pfeiffer, Geoffrey Lovelace, Lawrence E. Kidder, Duncan A. Brown, Mark A. Scheel, Lee Lindblom

Publication date: 4 July 2007

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0702106

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Equations of motion in general relativity and gravitational theory (83C10) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Related Items (12)

Extraction of gravitational waves in numerical relativity ⋮ Black-hole binaries, gravitational waves, and numerical relativity ⋮ Boundary conditions for coupled quasilinear wave equations with application to isolated systems ⋮ Methods for relativistic self-gravitating fluids: from binary neutron stars to black hole-disks and magnetized rotating neutron stars ⋮ Post-Newtonian quasicircular initial orbits for numerical relativity ⋮ The initial boundary value problem for free-evolution formulations of general relativity ⋮ Improvements to the construction of binary black hole initial data ⋮ Nature abhors a circle ⋮ The eccentric behavior of inspiralling compact binaries ⋮ Spectral methods for numerical relativity ⋮ Black-hole puncture initial data with realistic gravitational wave content ⋮ Continuum and discrete initial-boundary value problems and Einstein's field equations

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