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We derive the multipole moments of the Kerr-NUT black hole spacetime using the Geroch-Hansen formalism, even though the spacetime is not asymptotically flat.
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G. Clément, D. Gal’tsov, and M. Guenouche, “Rehabilitating space-times with NUTs,” Phys. Lett. B
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B. Mukhopadhyay and N. Dadhich, “Scalar and spinor perturbation to the Kerr-NUT space-time,” Class. Quant. Grav
2004
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V. Manko and E. Ruiz, “Physical interpretation of NUT solution,” Class. Quant. Grav
2005
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M. H. Dehghani and R. B. Mann, “NUT-charged black holes in Gauss-Bonnet gravity,” Phys. Rev
2005
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T. Backdahl and M. Herberthson, “Explicit multipole moments of stationary axisymmetric spacetimes,” Class. Quant. Grav
2005
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V. Manko, J. Martin, and E. Ruiz, “Singular sources in the Demianski-Newman spacetimes,” Class. Quant. Grav
2006
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V. Cardoso and L. Gualtieri, “Testing the black hole ‘no-hair’ hypothesis,” Class. Quant. Grav
2016
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2016
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G. Clément, D. Gal’tsov, and M. Guenouche, “NUT wormholes,” Phys. Rev. D
2016
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G. Compère, R. Oliveri, and A. Seraj, “Gravitational multipole moments from Noether charges,” JHEP
2018
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P. Jefremov and V. Perlick, “Circular motion in NUT space-time,” Class. Quant. Grav
2018
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2019
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2019
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