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The Initial Spin Matters: The Impact of Rapid Rotation on Magnetic-field Amplification at Merger

  • Authors: Harry Ho-Yin Ng, Jin-Liang Jiang, Luciano Rezzolla

Harry Ho-Yin Ng et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure B1.

Time evolution of the maximum of the conserved rest-mass density from simulations using FIL (dashed lines) and BHAC+, either without GWRR terms (dotted lines) or with them included. Note the importance of the latter in reproducing the results of overall dynamics compared to the full numerical-relativity simulations. Unless otherwise stated, all simulations have a finest spatial resolution of 300 m. For the IR case only, the purple solid and dashed lines correspond to simulations with a higher resolution of 100 m.

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