Phenomenological gravitational radiation from rotating stellar collapse to an intermediate mass Kerr black hole
type: Item
instance of: scholarly article
title: Phenomenological gravitational radiation from rotating stellar collapse to an intermediate mass Kerr black hole
zbMATH Open document ID: 1200.83047
author: Jin Li
author: M. J. Benacquista
published in: General Relativity and Gravitation
publication date: 2010-10-27T00:00:00Z
Mathematics Subject Classification ID: 83C35
Mathematics Subject Classification ID: 83C57
Mathematics Subject Classification ID: 85A15
Mathematics Subject Classification ID: 83C75
Mathematics Subject Classification ID: 83C10
Mathematics Subject Classification ID: 83C25
zbMATH DE Number: 5806802
zbMATH Keywords: intermediate mass black holes
zbMATH Keywords: oblate spheroidal coordinates
zbMATH Keywords: gravitational waves
MaRDI profile type: Publication
full work available at URL: s10714-010-1001-9
OpenAlex ID: W2137304566
cites work: The gravitational-wave signature of core-collapse supernovae
cites work: Q5447502
cites work: Theoretical astrophysics, Vol. 2. Stars and stellar systems
DOI: 10.1007/S10714-010-1001-9
description: scientific article; zbMATH DE number 5806802