Deflection angle of charged massive particles in slowly rotating Kerr-Newman spacetimes derived via Gauss-Bonnet theorem (via plasma correspondence) and Hamilton-Jacobi method, depending on M, a, Q, P, q, v.
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Negative tidal charge enlarges the shadow of rotating braneworld black holes while inhomogeneous plasma shrinks it and homogeneous plasma enlarges it; EHT data limits q to roughly -1.15 to 0.45 for M87* in the low-density limit.
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Deflection angle of charged massive particles in slowly rotating Kerr-Newman space-times via Gauss-Bonnet theorem and Hamilton-Jacobi method
Deflection angle of charged massive particles in slowly rotating Kerr-Newman spacetimes derived via Gauss-Bonnet theorem (via plasma correspondence) and Hamilton-Jacobi method, depending on M, a, Q, P, q, v.
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Investigating the interplay of the braneworld gravity and the plasma environment on the black hole shadow
Negative tidal charge enlarges the shadow of rotating braneworld black holes while inhomogeneous plasma shrinks it and homogeneous plasma enlarges it; EHT data limits q to roughly -1.15 to 0.45 for M87* in the low-density limit.