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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14485
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dc.contributor.authorMukherjee, Sajal-
dc.date.accessioned2024-02-28T11:58:04Z-
dc.date.available2024-02-28T11:58:04Z-
dc.date.issued2024-02-
dc.identifier.urihttps://arxiv.org/abs/2402.08883-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14485-
dc.description.abstractWe 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.isoenen_US
dc.publisherARXIVen_US
dc.subjectPhysicsen_US
dc.subjectGeneral Relativity and Quantum Cosmology (gr-qc)en_US
dc.titleAnalytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalismen_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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