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- W4285179754 endingPage "1277" @default.
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- W4285179754 abstract "To enable detection and maximize the physics output of gravitational wave observations from compact binary systems, the availability of accurate waveform models is crucial. The present work aims at giving an overview for non-experts of the (inspiral) waveforms used in the gravitational wave data analysis for compact binary coalescence. We first provide the essential elements of gravitational radiation physics within a simple Newtonian orbital dynamics and the linearized gravity theory, describing the adiabatic approximation applied to binary systems: the key element to construct the theoretical gravitational waveforms in practice. We next lay out the gravitational waveforms in the post-Newtonian approximation to general relativity and highlight the basic input for the inspiral waveform of the slowly evolving, spinning, nonprecessing, and quasicircular binary black holes, namely, post-Newtonian energy, fluxes, and the (absorption-corrected) balance equation. The post-Newtonian inspiral templates are then presented both in the time and frequency domain. Finally, including the merger and subsequent ringdown phase, we briefly survey the two families of the full waveform models of compact binary mergers currently implemented in LSC Algorithm Library Simulation: the effective-one-body approach and the phenomenological frequency-domain model." @default.
- W4285179754 created "2022-07-14" @default.
- W4285179754 creator A5017434183 @default.
- W4285179754 creator A5043200675 @default.
- W4285179754 creator A5055106955 @default.
- W4285179754 date "2022-01-01" @default.
- W4285179754 modified "2023-09-29" @default.
- W4285179754 title "Post-Newtonian Templates for Gravitational Waves from Compact Binary Inspirals" @default.
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