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

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

2011-11-16

arxiv.org/abs/1111.3737v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, 2 figures, 1 table, NRDA2011/Amaldi 9 proceedings; published version with extended discussion of accuracy requiremen

Scientific paper

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.

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