Numerical chaos indicators applied to the Schwarzschild-Bertotti-Robinson-Bonnor-Melvin family show that chaos occurs without swirling and that electromagnetic field strengths and directions tightly restrict bound orbits.
Electromagnetic field and chaotic charged-particle motion around hairy black holes in Horndeski gravity,
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A Reissner-Nordström-like black hole in Kalb-Ramond gravity with external magnetic field reproduces observed twin-peak QPO frequencies from GRO J1655-40, XTE J1550-564 and M82 X-1 after MCMC fitting of the Lorentz-violating parameter ℓ, charge Q/M, particle charge ε and magnetic coupling β.
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Chaotic motion of particles around a Schwarzschild black hole in a swirling electromagnetic background
Numerical chaos indicators applied to the Schwarzschild-Bertotti-Robinson-Bonnor-Melvin family show that chaos occurs without swirling and that electromagnetic field strengths and directions tightly restrict bound orbits.
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Particle dynamics and quasi-periodic oscillations of a Reissner--Nordstr\"om-like black hole in Kalb--Ramond gravity under an external magnetic test field
A Reissner-Nordström-like black hole in Kalb-Ramond gravity with external magnetic field reproduces observed twin-peak QPO frequencies from GRO J1655-40, XTE J1550-564 and M82 X-1 after MCMC fitting of the Lorentz-violating parameter ℓ, charge Q/M, particle charge ε and magnetic coupling β.