Quasi-radial modes of rotating stars in general relativity

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dc.creatorYoshida, S'i.
dc.creatorEriguchi, Y.
dc.date1999-08-31
dc.date2000-09-18
dc.date.accessioned2026-07-07T11:34:13Z
dc.date.available2026-07-07T11:34:13Z
dc.descriptionBy using the Cowling approximation, quasi-radial modes of rotating general relativistic stars are computed along equilibrium sequences from non-rotating to maximally rotating models. The eigenfrequencies of these modes are decreasing functions of the rotational frequency. The eigenfrequency curve of each mode as a function of the rotational frequency has discontinuities, which arise from the avoided crossing with other curves of axisymmetric modes.
dc.description7 pages, 10 figures, submitted to MNRAS. (revisions: new results are presented)
dc.identifierhttps://arxiv.org/abs/astro-ph/9908359
dc.identifierhttp://arxiv.org/abs/astro-ph/9908359
dc.identifierMon.Not.Roy.Astron.Soc.322:389,2001
dc.identifierdoi:10.1046/j.1365-8711.2001.04115.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198168
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuasi-radial modes of rotating stars in general relativity
dc.typetext

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