Matching post-Newtonian and numerical relativity waveforms: Systematic errors and a new phenomenological model for nonprecessing black hole binaries

Author(s)
Lucia Santamaria, Frank Ohme, Parameswaran Ajith, Bernd Brügmann, Nils Dorband, Mark Hannam, Sascha Husa, Philipp Mösta, Denis Pollney, Christian Reisswig, Emma L. Robinson, J. Seiler, Badri Krishnan
Abstract

We present a new phenomenological gravitational waveform model for the inspiral and coalescence of nonprecessing spinning black hole binaries. Our approach is based on a frequency-domain matching of post-Newtonian inspiral waveforms with numerical relativity based binary black hole coalescence waveforms. We quantify the various possible sources of systematic errors that arise in matching post-Newtonian and numerical relativity waveforms, and we use a matching criteria based on minimizing these errors; we find that the dominant source of errors are those in the post-Newtonian waveforms near the merger. An analytical formula for the dominant mode of the gravitational radiation of nonprecessing black hole binaries is presented that captures the phenomenology of the hybrid waveforms. Its implementation in the current searches for gravitational waves should allow cross-checks of other inspiral-merger-ringdown waveform families and improve the reach of gravitational-wave searches.

Organisation(s)
Gravitational Physics
External organisation(s)
Max-Planck-Institut für Gravitationsphysik (Albert Einstein Institut), California Institute of Technology (Caltech), Friedrich-Schiller-Universität Jena, University of the Balearic Islands, National Aeronautics & Space Administration (NASA)
Journal
Physical Review D
Volume
82
No. of pages
21
ISSN
1550-7998
DOI
https://doi.org/10.1103/PhysRevD.82.064016
Publication date
2010
Peer reviewed
Yes
Austrian Fields of Science 2012
103036 Theoretical physics
Portal url
https://ucrisportal.univie.ac.at/en/publications/matching-postnewtonian-and-numerical-relativity-waveforms-systematic-errors-and-a-new-phenomenological-model-for-nonprecessing-black-hole-binaries(d61fb023-6a60-4497-9b6c-5454d4057b70).html