2019
DOI: 10.1016/j.physletb.2019.134938
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Taub-NUT from the Dirac monopole

Abstract: Writing the metric of an asymptotically flat spacetime in Bondi coordinates provides an elegant way of formulating the Einstein equation as a characteristic value problem.In this setting, we find that a specific class of asymptotically flat spacetimes, including stationary solutions, contains a Maxwell gauge field as free data. Choosing this gauge field to correspond to the Dirac monopole, we derive the Taub-NUT solution in Bondi coordinates.

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Cited by 26 publications
(37 citation statements)
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“…This property was instrumental in interpreting the exact solution as the double copy of a point charge in [5], and this conclusion extends to many other cases, including the Kerr and Taub-NUT metrics -in fact, it extends to all vacuum type D spacetimes [15]. This double-copy interpretation is further supported by more recent arguments involving solution-generating techniques, computations with scattering amplitudes, duality considerations, and asymptotic symmetries [20,64,66,69,72]. Notice that, in terms of the 'fat graviton' (2.9), the Schwarzschild case (Y = 0) does not look particularly simple.…”
Section: Basicsmentioning
confidence: 75%
“…This property was instrumental in interpreting the exact solution as the double copy of a point charge in [5], and this conclusion extends to many other cases, including the Kerr and Taub-NUT metrics -in fact, it extends to all vacuum type D spacetimes [15]. This double-copy interpretation is further supported by more recent arguments involving solution-generating techniques, computations with scattering amplitudes, duality considerations, and asymptotic symmetries [20,64,66,69,72]. Notice that, in terms of the 'fat graviton' (2.9), the Schwarzschild case (Y = 0) does not look particularly simple.…”
Section: Basicsmentioning
confidence: 75%
“…In standard setups, this integral must vanish since the null normals provide a trivialization of the normal bundle. However, notable exceptions are given by configurations possessing nontrivial NUT charges, where C 1 is seen to be proportional to the NUT charge (see, for example, the analysis near null infinity in Bondi coordinates of [90]). In order for the surface S to be a regular embedded spacelike surface when the NUT charge is nonvanishing, there must be a physical Misner string penetrating the surface, which provides a compensating contribution to the outer curvature, to enforce that the normal bundle remains globally trivial [91][92][93][94].…”
Section: Nontrivial Bundles and Nut Chargesmentioning
confidence: 99%
“…In (31), the time evolution equation of A 1 involves the coupling constant a. Since A 1 is related to the electric dipole [39], the non-minimal coupling effect can be seen from the first radiating source in the multipole expansion.…”
Section: Solution Space In Series Expansionmentioning
confidence: 99%
“…The rest three supplementary equations determine the time evolution of the integration constants M, N and q. Since those integration constants are related to the conserved quantities, the supplementary equations are also called conservation equations [31].…”
Section: Conservation Laws and The Loss Of Massmentioning
confidence: 99%
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