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Corrections and Comments on the Multipole Moments of Axisymmetric Electrovacuum Spacetimes
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Following the method of Hoenselaers and Perj\'{e}s we present a new corrected and dimensionally consistent set of multipole gravitational and electromagnetic moments for stationary axisymmetric spacetimes. Furthermore, we use our results to compute the multipole moments, both gravitational and electromagnetic, of a Kerr-Newman black hole.
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Cited by 2 Pith papers
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Stationary generalizations for the vacuum ring wormhole
Numerical non-perturbative stationary vacuum ring wormhole solutions invariant under throat reflections, with slow-rotation M ~ J^2, fast-rotation J = M^2, and limits mimicking extremal Kerr.
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Leading Higher Derivative Corrections to Multipole Moments of Kerr-Newman Black Hole
The 4-derivative corrections to Kerr-Newman multipole moments depend only on field-redefinition-invariant couplings, and parity-odd terms turn on multipole moments that vanish in Einstein-Maxwell theory.
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