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Generalized, Energy-conserving Numerical Simulations of Particles in General Relativity. II. Test Particles in Electromagnetic Fields and GRMHD

  • Authors: F. Bacchini, B. Ripperda, O. Porth, and L. Sironi

2019 The Astrophysical Journal Supplement Series 240 40.

  • Provider: AAS Journals

Caption: Figure 9.

Representation in three-dimensional space of the unstable spherical orbits B (left panel) and D (right panel) from Table 2. The outer event horizon is shown as a colored sphere of radius ﹩{r}_{+}=M\pm \sqrt{{M}^{2}-{a}^{2}-{Q}^{2}-{P}^{2}}﹩. The equatorial red circle indicates the constant radius r0 characterizing each orbit. The starting point of the orbits is marked by a red dot.

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