A new numerical method to construct binary neutron star initial data
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Publication:3183691
DOI10.1088/0264-9381/26/17/175018zbMath1176.83023arXiv0908.0620OpenAlexW2067153652MaRDI QIDQ3183691
Publication date: 20 October 2009
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0908.0620
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Galactic and stellar dynamics (85A05) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Gravitational waves (83C35)
Related Items (4)
Methods for relativistic self-gravitating fluids: from binary neutron stars to black hole-disks and magnetized rotating neutron stars ⋮ Source term method for binary neutron stars initial data ⋮ KADATH: a spectral solver for theoretical physics ⋮ Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections
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