AMR simulations of the low T/W bar-mode instability of neutron stars

DOI10.1016/j.cpc.2007.04.001zbMath1196.85006arXiv0704.0356OpenAlexW2083742555WikidataQ60735652 ScholiaQ60735652MaRDI QIDQ710184

Pablo Cerdá-Durán, Vicent Quilis, José A. Font

Publication date: 18 October 2010

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0704.0356

zbMATH Keywords

gravitational waveshydrodynamicsinstabilitiesstars: neutron stars: rotation

Mathematics Subject Classification ID

Computational methods for problems pertaining to astronomy and astrophysics (85-08) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (1)

Gravitational waves from gravitational collapse

Cites Work

• Local adaptive mesh refinement for shock hydrodynamics
• Rotating stars in relativity

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