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Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism

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dc.contributor.author Mukherjee, Sajal
dc.date.accessioned 2024-02-28T11:58:04Z
dc.date.available 2024-02-28T11:58:04Z
dc.date.issued 2024-02
dc.identifier.uri https://arxiv.org/abs/2402.08883
dc.identifier.uri http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14485
dc.description.abstract We develop a fully analytical waveform model for precessing binaries with arbitrary spin vectors using post-Newtonian theory in the extreme mass-ratio limit and a hierarchical multi-scale analysis. Although the post-Newtonian series poorly converges in this limit, our results can be used to estimate how precession affects the measurability of certain binary parameters, and to inform and compare with other waveform approximants, such as effective-one-body models, hybrid waveforms, and self-force calculations. en_US
dc.language.iso en en_US
dc.publisher ARXIV en_US
dc.subject Physics en_US
dc.subject General Relativity and Quantum Cosmology (gr-qc) en_US
dc.title Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism en_US
dc.type Article en_US


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