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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 8.

Gravitational-wave signal for different initial magnetic-field strength B p, in the range B p = B 1.0B 6.5. Top (bottom) panels refer to the amplitude in × (+) polarization; d is the source distance, which needs to be specified to obtain the amplitudes h ×, h +. Note that the y-scale changes with B p.

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