A fast stroboscopic spectral method for rotating systems in numerical relativity

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dc.creatorBonazzola, Silvano
dc.creatorJaramillo, José-Luis
dc.creatorNovak, Jerome
dc.date2007-03-23
dc.date2007-08-17
dc.date.accessioned2026-07-07T10:37:16Z
dc.date.available2026-07-07T10:37:16Z
dc.descriptionWe present a numerical technique for solving evolution equations, as the wave equation, in the description of rotating astrophysical compact objects in comoving coordinates, which avoids the problems associated with the light cylinder. The technique implements a fast spectral matching between two domains in relative rotation: an inner spherical domain, comoving with the sources and lying strictly inside the light cylinder, and an outer inertial spherical shell. Even though the emphasis is placed on spectral techniques, the matching is independent of the specific manner in which equations are solved inside each domain, and can be adapted to different schemes. We illustrate the strategy with some simple but representative examples.
dc.description16 pages, 15 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0703118
dc.identifierhttp://arxiv.org/abs/gr-qc/0703118
dc.identifierClass.Quant.Grav.24:4037-4052,2007
dc.identifierdoi:10.1088/0264-9381/24/16/005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180325
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA fast stroboscopic spectral method for rotating systems in numerical relativity
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