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Analytical meets numerical relativity: status of complete gravitational waveform models for binary black holes

Ohme, Frank 2012. Analytical meets numerical relativity: status of complete gravitational waveform models for binary black holes. Classical and Quantum Gravity 29 (12) , 124002. 10.1088/0264-9381/29/12/124002

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Abstract

Models of gravitational waveforms from coalescing black-hole binaries play a crucial role in the efforts to detect and interpret the signatures of those binaries in the data of large-scale interferometers. Here we summarize recent models that combine information both from analytical approximations and numerical relativity. We briefly lay out and compare the strategies employed to build such complete models and we recapitulate the errors associated with various aspects of the modelling process.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Additional Information: Special issue: Selected articles from the 9th Edoardo Amaldi Meeting and the 2011 Numerical Relativity and Data Analysis Meeting (AMALDI 9/NRDA 2011) (Cardiff, 10–15 July 2011)
Publisher: IOP Publishing
ISSN: 0264-9381
Last Modified: 04 Jun 2017 05:17
URI: http://orca.cf.ac.uk/id/eprint/50324

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