Characterization of (asymptotically) Kerr–de Sitter-like spacetimes at null infinity

DOI10.1088/0264-9381/33/15/155001zbMath1346.83016arXiv1603.05839OpenAlexW3102755292MaRDI QIDQ2820649

Walter Simon, José M. M. Senovilla, Marc Mars, Tim-Torben Paetz

Publication date: 9 September 2016

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

Full work available at URL: https://arxiv.org/abs/1603.05839

zbMATH Keywords

characterizationcosmological constantnull infinityMars-Simon tensorKerr-de Sitter-like

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (10)

Relative-observer definition of the Simon tensor ⋮ The conformal Killing spinor initial data equations ⋮ Asymptotic structure with a positive cosmological constant ⋮ On staticity of bifurcate Killing horizons* ⋮ An ideal conformally covariant characterization of the Kerr conformal structure ⋮ Analysis of a Bianchi-like equation satisfied by the Mars-Simon tensor ⋮ Algorithmic characterization results for the Kerr-NUT-(A)dS space-time. I. A space-time approach ⋮ Algorithmic characterization results for the Kerr-NUT-(A)dS space-time. II. KIDs for the Kerr-(A)(de Sitter) family ⋮ Non-singular Kerr-NUT-de Sitter spacetimes ⋮ Type D conformal initial data

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