Constructive proof of the Kerr-Newman black hole uniqueness: derivation of the full solution from scratch
classification
🌀 gr-qc
astro-ph.HEhep-th
keywords
solutionblackholekerr-newmanasymptoticallyaxisymmetricboundaryconnected
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The Kerr-Newman black hole solution can be constructed straightforwardly as the unique solution to the boundary value problem of the Einstein-Maxwell equations corresponding to an asymptotically flat, stationary and axisymmetric electro-vacuum spacetime surrounding a connected Killing horizon.
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