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This paper explores the relationship between the Schwarzschild and Kerr black hole geometries through the lens of BMS supertranslations, demonstrating that the asymptotic structure of Kerr can be derived from Schwarzschild via two successive supertranslations. The authors identify two classes of supertranslation functions that correspond to center-of-mass displacements and the intrinsic mass multipole structure of Kerr spacetime. This work emphasizes the significance of infinite-dimensional asymptotic symme

Author

Enzo Ric

Language

EN