Linear and Nonlinear Dynamics of Relativistic Tori

dc.creatorRezzolla, Luciano
dc.date2003-03-14
dc.date2003-03-21
dc.date.accessioned2026-07-07T03:27:43Z
dc.date.available2026-07-07T03:27:43Z
dc.descriptionI present results of two-dimensional general relativistic hydrodynamical simulations of constant specific angular momentum tori orbiting around a Schwarzschild black hole. After introducing axisymmetric perturbations, these objects either become unstable to the runaway instability or respond with regular oscillations. The latter, in particular, are responsible for quasi-periodic bursts of accretion onto the black hole as well as for the emission of intense gravitational radiation, with signal-to-noise ratios at the detector which are comparable or even larger than the typical ones expected in stellar-core collapse.
dc.descriptionInvited Talk at the 15th SIGRAV Conference, Frascati Sept. 2002; IOP Conference Series, one reference added
dc.identifierhttps://arxiv.org/abs/gr-qc/0303057
dc.identifierhttp://arxiv.org/abs/gr-qc/0303057
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34539
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleLinear and Nonlinear Dynamics of Relativistic Tori
dc.typetext

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