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- W1505371860 abstract "We present results of simulations in full General Relativity of the dynamical instability against barmode deformations of rapidly and differentially rotating neutron stars. Because of the high accuracy and long‐term stability of our code the instability can develop without the introduction of initial, ad‐hoc perturbations. This allows us to estimate accurately the threshold for the development of the instability that we determine to be βc = T/|W| ≃ 0.254 for polytropic models with Γ = 2. We also find that the dynamics of the instability sensitively depends on the quantity β − βc, with persistent bars being possible only for β ≳ βc and with strong nonlinear hydrodynamical effects emerging when β ≫ βc." @default.
- W1505371860 created "2016-06-24" @default.
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- W1505371860 date "2006-01-01" @default.
- W1505371860 modified "2023-09-23" @default.
- W1505371860 title "Accurate simulations of the barmode instability in General Relativity" @default.
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- W1505371860 doi "https://doi.org/10.1063/1.2218203" @default.
- W1505371860 hasPublicationYear "2006" @default.
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