Killing spinors as a characterisation of rotating black hole spacetimes

DOI10.1088/0264-9381/33/12/125019zbMath1342.83215arXiv1601.04666OpenAlexW2302861549MaRDI QIDQ2994614

Juan Antonio Valiente Kroon, Michael J. Cole

Publication date: 2 August 2016

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1601.04666

zbMATH Keywords

black holesKerr-Newman solutionKilling spinorsinvariant characterisationsspinorial methods

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (6)

The conformal Killing spinor initial data equations ⋮ A geometric invariant characterising initial data for the Kerr-Newman spacetime ⋮ On Local Characterization Results in Geometry and Gravitation ⋮ Algorithmic characterization results for the Kerr-NUT-(A)dS space-time. I. A space-time approach ⋮ Perturbations of the asymptotic region of the Schwarzschild-de Sitter spacetime ⋮ Killing spinor data on distorted black hole horizons and the uniqueness of stationary vacuum black holes

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