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Arbitrarily deformed Kerr-Newman black hole in an external gravitational field of arbitrary real parameters and able to describe a deformed Kerr-Newman black hole in an external
Stationary double black hole without naked ring singularity attention as exact solutions suitable for visualization of ultra-compact objects beyond the Kerr paradigm
Zero mass limit of Kerr spacetime is a wormhole in the literature, the zero mass limit of Kerr spacetime is not flat Minkowski space but a spacetime whose geometry
Is the Kerr black hole a super accelerator? velocities. As of today the only such candidate mechanism in the case of the nonextreme Kerr black hole
Quasinormal modes of massive fermions in Kerr spacetime: Long-lived modes and the fine structure for the Kerr solution. Here we calculate quasinormal modes of a massive Dirac field in the Kerr background. We
Kerr-bolt spacetimes and KERR/CFT correspondenceKerr-bolt spacetimes and KERR/CFT correspondence
Generalizations of the Kerr-Newman and charged Tomimatsu-Sato metrics in the Jordan-Brans-Dicke theoryGeneralizations of the Kerr-Newman and charged Tomimatsu-Sato metrics in the Jordan
Completing characterization of photon orbits in Kerr and Kerr-Newman metrics of domains filling the entire Kerr-like spacetimes. This construction provides a novel optical description
Half-Dose Tenecteplase or Primary Percutaneous Coronary Intervention in Older Patients With ST-Elevation Myocardial Infarction: STREAM-2 1-Year Mortality Follow-Up
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