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• W2267134623 abstract "Inspiraling compact binaries with non-negligible orbital eccentricities are plausible gravitational wave (GW) sources for the upcoming network of GW observatories. In this paper, we present two prescriptions to compute post-Newtonian (PN) accurate inspiral templates for such binaries. First, we adapt and extend the post-circular scheme of Yunes {it et al.} [Phys. Rev. D 80, 084001 (2009)] to obtain a Fourier-domain inspiral approximant that incorporates the effects of PN-accurate orbital eccentricity evolution. This results in a fully analytic frequency-domain inspiral waveform with Newtonian amplitude and 2PN order Fourier phase while incorporating eccentricity effects up to sixth order at each PN order. The importance of incorporating eccentricity evolution contributions to the Fourier phase in a PN consistent manner is also demonstrated. Second, we present an accurate and efficient prescription to incorporate orbital eccentricity into the quasi-circular time-domain {texttt{TaylorT4}} approximant at 2PN order. New features include the use of rational functions in orbital eccentricity to implement the 1.5PN order tail contributions to the far-zone fluxes. This leads to closed form PN-accurate differential equations for evolving eccentric orbits and the resulting time-domain approximant is accurate and efficient to handle initial orbital eccentricities $leq 0.9$. Preliminary GW data analysis implications are probed using match estimates." @default.
• W2267134623 created "2016-06-24" @default.
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• W2267134623 date "2016-03-09" @default.
• W2267134623 modified "2023-10-18" @default.
• W2267134623 title "Frequency and time-domain inspiral templates for comparable mass compact binaries in eccentric orbits" @default.
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• W2267134623 doi "https://doi.org/10.1103/physrevd.93.064031" @default.
• W2267134623 hasPublicationYear "2016" @default.
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