Numerical Relativity for Inspiraling Binaries in Co-Rotating Coordinates: Test Bed for Lapse and Shift Equations

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dc.creatorThorne, Kip S.
dc.date1998-08-09
dc.date.accessioned2026-07-07T03:32:35Z
dc.date.available2026-07-07T03:32:35Z
dc.descriptionGravitational-wave data analysis requires a detailed understanding of the highly relativistic, late stages of inspiral of neutron-star and black-hole binaries. A promising method to compute the late inspiral and its emitted waves is numerical relativity in co-rotating coordinates. The coordinates must be kept co-rotating via an appropriate choice of numerical relativity's lapse and shift functions. This article proposes a model problem for testing the ability of various lapse and shift prescriptions to keep the coordinates co-rotating.
dc.description4 pages; submitted to Physical Review D15 as a regular article
dc.identifierhttps://arxiv.org/abs/gr-qc/9808024
dc.identifierhttp://arxiv.org/abs/gr-qc/9808024
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36289
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNumerical Relativity for Inspiraling Binaries in Co-Rotating Coordinates: Test Bed for Lapse and Shift Equations
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