Phenomenological gravitational radiation from rotating stellar collapse to an intermediate mass Kerr black hole

DOI10.1007/S10714-010-1001-9zbMath1200.83047OpenAlexW2137304566MaRDI QIDQ711668

Jin Li, Matthew J. Benacquista

Publication date: 27 October 2010

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10714-010-1001-9

zbMATH Keywords

gravitational wavesoblate spheroidal coordinatesintermediate mass black holes

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (1)

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Cites Work

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• The gravitational-wave signature of core-collapse supernovae
• Theoretical Astrophysics

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