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The NINJA-2 catalog of hybrid post-Newtonian/numerical-relativity waveforms for non-precessing black-hole binaries

Authors :
Ajith, P.
Boyle, Michael
Brown, Duncan A.
Brügmann, Bernd
Buchman, Luisa T.
Cadonati, Laura
Campanelli, Manuela
Chu, Tony
Etienne, Zachariah B.
Fairhurst, Stephen
Hannam, Mark
Healy, James
Hinder, Ian
Husa, Sascha
Kidder, Lawrence E.
Krishnan, Badri
Laguna, Pablo
Liu, Yuk Tung
London, Lionel
Lousto, Carlos O.
Lovelace, Geoffrey
MacDonald, Ilana
Marronetti, Pedro
Mohapatra, Satya
Mösta, Philipp
Müller, Doreen
Mundim, Bruno C.
Nakano, Hiroyuki
Ohme, Frank
Paschalidis, Vasileios
Pekowsky, Larne
Pollney, Denis
Pfeiffer, Harald P.
Ponce, Marcelo
Pürrer, Michael
Reifenberger, George
Reisswig, Christian
Santamaría, Lucía
Scheel, Mark A.
Shapiro, Stuart L.
Shoemaker, Deirdre
Sopuerta, Carlos F.
Sperhake, Ulrich
Szilágyi, Béla
Taylor, Nicholas W.
Tichy, Wolfgang
Tsatsin, Petr
Zlochower, Yosef
Publication Year :
2012

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 63 hybrid waveforms consisting of a numerical portion modelling the late inspiral, merger, and ringdown stitched to a post-Newtonian portion modelling 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 $(\ell,m)=(2,2)$ 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.<br />Comment: Presented at Amaldi 9

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1201.5319
Document Type :
Working Paper
Full Text :
https://doi.org/10.1088/0264-9381/29/12/124001