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From Schwarzschild to Kerr: Generating spinning Einstein-Maxwell fields from static fields

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

The Kerr solution is generated from the Schwarzschild solution by a simple combination of real global coordinate transformations and of invariance transformations acting on the space of stationary solutions of the Einstein-Maxwell equations. The same transformation can be used to generate a spinning field configuration from any static axisymmetric configuration. We illustrate this by generating from the continuous family of Voorhees--Zipoy vacuum solutions a family of solutions endowed with mass, angular momentum, dipole magnetic moment and quadrupole electric moment.

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hep-th 2

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2026 2

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UNVERDICTED 2

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representative citing papers

Generating Rotation in a Snap

hep-th · 2026-05-14 · unverdicted · novelty 7.0

An algebraic technique generates rotating black holes and multi-source solutions from static ones by transforming to AdS×S asymptotics, applying a rotating frame shift, and returning to flat asymptotics.

Monodromy-Matrix Description of Extremal Multi-centered Black Holes

hep-th · 2026-04-07 · unverdicted · novelty 6.0

The authors derive explicit monodromy matrices for Bena-Warner BPS solutions and almost-BPS configurations including two-center black rings, factorize them via nilpotent elements of so(4,4), and construct an SO(4,4) duality relating branches of the Rasheed-Larsen solution.

citing papers explorer

Showing 2 of 2 citing papers.

  • Generating Rotation in a Snap hep-th · 2026-05-14 · unverdicted · none · ref 17 · internal anchor

    An algebraic technique generates rotating black holes and multi-source solutions from static ones by transforming to AdS×S asymptotics, applying a rotating frame shift, and returning to flat asymptotics.

  • Monodromy-Matrix Description of Extremal Multi-centered Black Holes hep-th · 2026-04-07 · unverdicted · none · ref 48

    The authors derive explicit monodromy matrices for Bena-Warner BPS solutions and almost-BPS configurations including two-center black rings, factorize them via nilpotent elements of so(4,4), and construct an SO(4,4) duality relating branches of the Rasheed-Larsen solution.