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gr-qc2022
Revisiting the quasinormal modes of the Schwarzschild black hole: Numerical analysis
Luis A. H. Mamani, Angel D. D. Masa, Lucas Timotheo Sanches +1
We revisit the problem of calculating the quasinormal modes of spin , , , , , and spin fields in the asymptotically flat Schwarzschild black hole spacetime…
gr-qc2022★ 2 cited
Rotating regular black holes and other compact objects with a Tolman type potential as a regular interior for the Kerr metric
Angel D. Masa, Vilson T. Zanchin
We obtain a new class of stationary axisymmetric spacetimes by using the Gürses-Gürsey metric with an appropriate mass function in order to generate a rotating core of matter that…