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  Analytical meets numerical relativity - status of complete gravitational waveform models

Ohme, F. (2012). Analytical meets numerical relativity - status of complete gravitational waveform models. Classical and quantum gravity, 29: 124002.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-3238-F Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-323B-9
Genre: Conference Paper

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1111.3737 (Preprint), 4KB
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 Creators:
Ohme, Frank1, Author              
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: Models of gravitational waveforms from coalescing black-hole binaries play a crucial role in the efforts to detect and interpret those signatures 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.

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 Dates: 2011-11-16201120122012
 Publication Status: Published in print
 Pages: 12 pages, 2 figures, 1 table, NRDA2011/Amaldi 9 proceedings
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1111.3737
DOI: 10.1088/0264-9381/29/12/124002
 Degree: -

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Title: 9th Edoardo Amaldi Meeting and the 2011 Numerical Relativity and Data Analysis Meeting (AMALDI 9/NRDA 2011)
Place of Event: Cardiff University
Start-/End Date: 2011-07-10 - 2011-07-15

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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics
Pages: - Volume / Issue: 29 Sequence Number: 124002 Start / End Page: - Identifier: ISSN: 0264-9381
CoNE: /journals/resource/954925513480_1