2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/33744A core-collapse supernova might produce large amplitude gravitational waves if, through the collapse process, the inner core can aquire enough rotational energy to become dynamically unstable. In this report I present the results of 3-D numerical simulations of core collapse supernovae. These simulations indicate that for some initial conditions the post-collapse inner core is indeed unstable. However, for the cases considered, the instability does not produce a large gravitational-wave signal.12 pages, 10 figures; prepared for the proceedings of the workshop on Astrophysical Sources of Gravitational RadiationGeneral Relativity and Quantum CosmologyAstrophysicstext