Image Details

Choose export citation format:

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 1.

Top panel: evolution of the total EM for the four binaries considered, star symbols indicating when the KHI can be considered to be considerably reduced (t = tsh,1/2). Second panel: evolution of the EM energy in the poloidal (solid lines) and toroidal components (dashed lines). Third panel: evolution of the KHI growth rate ﹩\gamma := {\dot{E}}_{{}_{{\rm{EM}}}}/{E}_{{}_{{\rm{EM}}}}﹩. Bottom panel: evolution of the KHI growth rates in the poloidal (solid lines) and toroidal components (dashed lines). In all panels, the vertical dashed lines mark the merger time tmer for each binary.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse