Lindblom, Lee and Baker, John G. and Owen, Benjamin J. (2010) Improved time-domain accuracy standards for model gravitational waveforms. Physical Review D, 82 (8). 084020 . ISSN 0556-2821. http://resolver.caltech.edu/CaltechAUTHORS:20101102-093727097
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Model gravitational waveforms must be accurate enough to be useful for detection of signals and measurement of their parameters, so appropriate accuracy standards are needed. Yet these standards should not be unnecessarily restrictive, making them impractical for the numerical and analytical modelers to meet. The work of Lindblom, Owen, and Brown [Phys. Rev. D 78, 124020 (2008)] is extended by deriving new waveform accuracy standards which are significantly less restrictive while still ensuring the quality needed for gravitational-wave data analysis. These new standards are formulated as bounds on certain norms of the time-domain waveform errors, which makes it possible to enforce them in situations where frequency-domain errors may be difficult or impossible to estimate reliably. These standards are less restrictive by about a factor of 20 than the previously published time-domain standards for detection, and up to a factor of 60 for measurement. These new standards should therefore be much easier to use effectively.
|Additional Information:||© 2010 American Physical Society. Received 10 August 2010; published 12 October 2010. We thank Michael Holst for valuable discussions about rigorous mathematical error bounds, Sean McWilliams for other useful discussions, and Duncan Brown for helpful comments on an earlier draft of this paper. This research was supported in part by grants to Caltech from the Sherman Fairchild Foundation, NSF Grants No. DMS-0553302, No. PHY-0601459, and No. PHY-0652995, and NASA Grant No. NNX09AF97G; by NASA Grants No. 08-ATFP08-0126 and No. 09-ATP09-0136 to Goddard Space Flight Center; by NSF Grant No. PHY- 0855589 to Penn State; and by the LIGO Visitors Program. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under cooperative agreement PHY-0757058. This paper has LIGO Document No. LIGO-P1000078.|
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|Classification Code:||PACS: 07.05.Kf, 04.25.D-, 04.25.dg, 04.30.-w|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Jason Perez|
|Deposited On:||02 Nov 2010 20:43|
|Last Modified:||26 Dec 2012 12:35|
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