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late-time instability

Similarly to the vacuum, electro-vacuum cases, our results show that the BSSN, CCZ0 formulations do not provide robust results in the long term, failing in this case to fully capture the formation of the scalarized black hole, with th · 2000

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Stable long-term evolution in numerical relativity

gr-qc · 2025-01-02 · conditional · novelty 6.0

Two modified CCZ4 schemes that propagate momentum constraint violations without damping suppress a late-time instability seen in long BSSN black hole simulations.

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  • Stable long-term evolution in numerical relativity gr-qc · 2025-01-02 · conditional · none · ref 4

    Two modified CCZ4 schemes that propagate momentum constraint violations without damping suppress a late-time instability seen in long BSSN black hole simulations.