The NINJA-2 catalog of hybrid post-Newtonian/numerical-relativity waveforms for non-precessing black-hole binaries
- Author(s)
- Parameswaran Ajith, Michael Boyle, Duncan A Brown, Bernd Brügmann, Luisa T Buchman, Laura Cadonati, Manuela Campanelli, Tony Chu, Zachariah B Etienne, Stephen Fairhurst, Mark Hannam, James Healy, Ian Hinder, Sascha Husa, Lawrence E Kidder, Badri Krishnan, Pablo Laguna, Yuk Tung Liu, Lionel London, Carlos O Lousto, Geoffrey Lovelace, Ilana MacDonald, Pedro Marronetti, Satya Mohapatra, Philipp Mösta, Doreen Müller, Bruno C Mundim, Hiroyuki Nakano, Frank Ohme, Vasileios Paschalidis, Larne Pekowsky, Denis Pollney, Harald P Pfeiffer, Marcelo Ponce, Michael Puerrer, George Reifenberger, Christian Reisswig, Lucia Santamaria, Mark A Scheel, Stuart L Shapiro, Deirdre Shoemaker, Carlos F Sopuerta, Ulrich Sperhake, Béla Szilágyi, Nicholas W Taylor, Wolfgang Tichy, Petr Tsatsin, Yosef Zlochower
- Abstract
The numerical injection analysis (NINJA) project is a collaborative effort between members of the numerical-relativity and gravitational wave data-analysis communities. The purpose of NINJA is to study the sensitivity of existing gravitational-wave search and parameter-estimation algorithms using numerically generated waveforms and to foster closer collaboration between the numerical-relativity and data-analysis communities. The first NINJA project used only a small number of injections of short numerical-relativity waveforms, which limited its ability to draw quantitative conclusions. The goal of the NINJA-2 project is to overcome these limitations with long post-Newtonian—numerical-relativity hybrid waveforms, large numbers of injections and the use of real detector data. We report on the submission requirements for the NINJA-2 project and the construction of the waveform catalog. Eight numerical-relativity groups have contributed 56 hybrid waveforms consisting of a numerical portion modeling the late inspiral, merger and ringdown stitched to a post-Newtonian portion modeling the early inspiral. We summarize the techniques used by each group in constructing their submissions. We also report on the procedures used to validate these submissions, including examination in the time and frequency domains and comparisons of waveforms from different groups against each other. These procedures have so far considered only the (ℓ, m) = (2, 2) mode. Based on these studies, we judge that the hybrid waveforms are suitable for NINJA-2 studies. We note some of the plans for these investigations.
- Organisation(s)
- Gravitational Physics
- External organisation(s)
- California Institute of Technology (Caltech), Cornell University, Syracuse University, Friedrich-Schiller-Universität Jena, University of Massachusetts, Amherst, Rochester Institute of Technology, University of Illinois at Urbana-Champaign, Cardiff University, Georgia Institute of Technology, Max-Planck-Institut für Gravitationsphysik (Albert Einstein Institut), University of the Balearic Islands, University of Toronto, Florida Atlantic University, Spanish National Research Council (CSIC)
- Journal
- Classical and Quantum Gravity
- Volume
- 29
- No. of pages
- 27
- ISSN
- 0264-9381
- DOI
- https://doi.org/10.1088/0264-9381/29/12/124001
- Publication date
- 2012
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103036 Theoretical physics, 103028 Theory of relativity
- Portal url
- https://ucris.univie.ac.at/portal/en/publications/the-ninja2-catalog-of-hybrid-postnewtoniannumericalrelativity-waveforms-for-nonprecessing-blackhole-binaries(a66e9039-e643-4004-9bfa-e45ae1456045).html