Post-Newtonian quasicircular initial orbits for numerical relativity

DOI10.1088/1361-6382/aa7929zbMath1373.83057arXiv1702.00872OpenAlexW3100875815MaRDI QIDQ4592654

Yosef Zlochower, Hiroyuki Nakano, James Healy, C. O. Loustó

Publication date: 7 November 2017

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

Full work available at URL: https://arxiv.org/abs/1702.00872

zbMATH Keywords

post-Newtoniannumerical evolutionsbinary black hole evolutionsquasicircular initial orbits

Mathematics Subject Classification ID

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) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (1)

Initial data and eccentricity reduction toolkit for binary black hole numerical relativity waveforms

Uses Software

• Cactus

Cites Work

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• The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
• Black-hole puncture initial data with realistic gravitational wave content
• Binary black hole initial data for numerical general relativity based on post-Newtonian data
• Evolutions in 3D numerical relativity using fixed mesh refinement
• A fast apparent horizon finder for three-dimensional Cartesian grids in numerical relativity
• Reducing orbital eccentricity in binary black hole simulations
• Next‐to‐next‐to‐leading order post‐Newtonian linear‐in‐spin binary Hamiltonians

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