On the gravitational radiation from the collapse of neutron stars to rotating black holes

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dc.creatorBaiotti, Luca
dc.creatorHawke, Ian
dc.creatorRezzolla, Luciano
dc.date2007-01-06
dc.date.accessioned2026-07-07T10:37:12Z
dc.date.available2026-07-07T10:37:12Z
dc.descriptionWe provide details and present additional results on the numerical study of the gravitational-wave emission from the collapse of neutron stars to rotating black holes in three dimensions. More specifically, we concentrate on the advantages and disadvantages of the use of the excision technique and on how alternative approaches to that of excision can be successfully employed. Furthermore, as a first step towards source-characterization, we present a systematic discussion of the influence that rotation and different perturbations have on the waveforms and hence on the energy emitted in gravitational waves.
dc.description21 pages, 10 figures; submitted to Classical and Quantum Gravity's special issue on numerical relativity, proceeding of the NFNR conference, Potsdam 2006
dc.identifierhttps://arxiv.org/abs/gr-qc/0701043
dc.identifierhttp://arxiv.org/abs/gr-qc/0701043
dc.identifierClass.Quant.Grav.24:S187-S206,2007
dc.identifierdoi:10.1088/0264-9381/24/12/S13
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180299
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn the gravitational radiation from the collapse of neutron stars to rotating black holes
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