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Poloidal-field Instability in Magnetized Relativistic Stars

  • Authors: Riccardo Ciolfi and Luciano Rezzolla

Ciolfi & Rezzolla 2012 The Astrophysical Journal 760 1.

  • Provider: AAS Journals

Caption: Figure 7.

Top: evolution of magnetic helicity normalized to (see the text), for different initial magnetic-field strengths: 6.5 (continuous black line), 3.5 (long-dashed blue line), and 1.5 × 10 16 G (dot-dashed magenta line). Bottom: evolution of magnetic helicity normalized to the initial value of , for the same set of simulations.

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