Figure 2 from Generalized, Energy-conserving Numerical Simulations of Particles in General Relativity. II. Test Particles in Electromagnetic Fields and GRMHD

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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 2.

Simulation of orbit RKA3 as in Figure 1, projected onto the φ = 0 plane, obtained with the four integration methods. A spurious damping of the particle gyration is observed in the RK4 run, due to unbounded energy errors and lack of symplecticity.

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