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

Journal Article · · Physical Review. D, Particles Fields
; ; ; ; ;  [1];  [2];  [3];  [4]; ;  [5];  [6];  [7]
  1. Max-Planck-Institut fuer Gravitationsphysik (Albert-Einstein-Institut), Am Muehlenberg 1, D-14476 Golm (Germany)
  2. LIGO Laboratory, California Institute of Technology, Pasadena, California 91125 (United States)
  3. Theoretisch-Physikalisches Institut, Friedrich Schiller Universitaet Jena, Max-Wien-Platz 1, 07743 Jena (Germany)
  4. Faculty of Physics, University of Vienna, Boltzmanngasse 5, A-1090 Vienna (Austria)
  5. Departament de Fisica, Universitat de les Illes Balears, Carretera Valldemossa km 7.5, E-07122 Palma (Spain)
  6. Theoretical Astrophysics, California Institute of Technology, Pasadena, California 91125 (United States)
  7. NASA Goddard Space Flight Center, Greenbelt, Maryland 20771 (United States)

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.

OSTI ID:
21421158
Journal Information:
Physical Review. D, Particles Fields, Vol. 82, Issue 6; Other Information: DOI: 10.1103/PhysRevD.82.064016; (c) 2010 American Institute of Physics; ISSN 0556-2821
Country of Publication:
United States
Language:
English