A template bank to search for gravitational waves from inspiralling compact binaries: II. Phenomenological model

dc.creatorCokelaer, Thomas
dc.date2007-09-07
dc.date.accessioned2026-07-07T11:19:11Z
dc.date.available2026-07-07T11:19:11Z
dc.descriptionMatched filtering is used to search for gravitational waves emitted by inspiralling compact binaries in data from ground-based interferometers. One of the key aspects of the detection process is the deployment of a set of templates, also called a template bank, to cover the astrophysically interesting region of the parameter space. In a companion paper, we described the template-bank algorithm used in the analysis of LIGO data to search for signals from non-spinning binaries made of neutron star and/or stellar-mass black holes; this template bank is based upon physical template families. In this paper, we describe the phenomenological template bank that was used to search for gravitational waves from non-spinning black hole binaries (from stellar mass formation) in the second, third and fourth LIGO science runs. We briefly explain the design of the bank, whose templates are based on a phenomenological detection template family. We show that this template bank gives matches greater than 95% with the physical template families that are expected to be captured by the phenomenological templates.
dc.description10 pages, 9 figures
dc.identifierhttps://arxiv.org/abs/0709.1050
dc.identifierhttp://arxiv.org/abs/0709.1050
dc.identifierClass.Quant.Grav.24:6227-6242,2007
dc.identifierdoi:10.1088/0264-9381/24/24/006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193599
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA template bank to search for gravitational waves from inspiralling compact binaries: II. Phenomenological model
dc.typetext

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