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Journal Article

Improved filters for gravitational waves from inspiralling compact binaries

MPS-Authors

Damour,  Thibault
Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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206286.pdf
(Publisher version), 463KB

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Citation

Damour, T., Iyer, B. R., & Sathyaprakash, B. S. (1998). Improved filters for gravitational waves from inspiralling compact binaries. Physical Review D, 57(2), 885-907.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0013-59B9-4
Abstract
The order of the post-Newtonian expansion needed to extract in a reliable and accurate manner the fully general relativistic gravitational wave signal from inspiraling compact binaries is explored. A class of approximate wave forms, called P-approximants, is constructed based on the following two inputs: (a) the introduction of two new energy-type and flux-type functions e(v) and f(v), respectively, (b) the systematic use of the Padé approximation for constructing successive approximants of e(v) and f(v). The new P-approximants are not only more effectual (larger overlaps) and more faithful (smaller biases) than the standard Taylor approximants, but also converge faster and monotonically. The presently available (v/c)5-accurate post-Newtonian results can be used to construct P-approximate wave forms that provide overlaps with the exact wave form larger than 96.5%, implying that more than 90% of potential events can be detected with the aid of P-approximants as opposed to a mere 10–15 % that would be detectable using standard post-Newtonian approximants.