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Conference Paper

Analytical meets numerical relativity - status of complete gravitational waveform models

MPS-Authors
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Ohme,  Frank
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Fulltext (public)

1111.3737
(Preprint), 4KB

CQG29_12_124002.pdf
(Any fulltext), 737KB

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Citation

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


Cite as: http://hdl.handle.net/11858/00-001M-0000-0012-3238-F
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.