Gravitational waves from the 3D collapse of a neutron star to a Kerr black hole

DOI10.1016/j.cpc.2005.03.083zbMath1196.83026OpenAlexW2081087171WikidataQ59830088 ScholiaQ59830088MaRDI QIDQ709779

Ian Hawke, Erik Schnetter, Luciano Rezzolla, Luca Baiotti

Publication date: 18 October 2010

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

Full work available at URL: http://hdl.handle.net/11858/00-001M-0000-0013-4F4E-5

zbMATH Keywords

black holeshydrodynamicsneutron starsnumerical relativity

Mathematics Subject Classification ID

Black holes (83C57)

Related Items (4)

Extraction of gravitational waves in numerical relativity ⋮ Black hole free energy during charged collapse: a numerical study ⋮ Gravitational waves from the 3D collapse of a neutron star to a Kerr black hole ⋮ Numerical hydrodynamics and magnetohydrodynamics in general relativity

Cites Work

• Gravitational waves from the 3D collapse of a neutron star to a Kerr black hole
• Adaptive mesh refinement for hyperbolic partial differential equations
• Evolutions in 3D numerical relativity using fixed mesh refinement
• Quasi-normal modes of stars and black holes

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