Increasing the global monopole parameter enlarges the black hole shadow and ISCO radius while slowing the damping of electromagnetic quasinormal modes.
Tsukamoto, Black hole shadow in an asymptotically flat, stationary, and axisymmetric spacetime: The Kerr- Newman and rotating regular black holes, Phy
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Strong Lensing and Quasinormal modes of black hole around global monopole
Increasing the global monopole parameter enlarges the black hole shadow and ISCO radius while slowing the damping of electromagnetic quasinormal modes.