A rotating pure radiation field of Kerr-Schild type

DOI10.1088/0264-9381/15/7/016zbMath0939.83010OpenAlexW1984107301MaRDI QIDQ4699672

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Publication date: 18 November 1999

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

Full work available at URL: https://doi.org/10.1088/0264-9381/15/7/016

zbMATH Keywords

gravitational energy

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Gravitational energy and conservation laws; groups of motions (83C40) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (3)

Symmetries of asymptotically flat axisymmetric space–times with null dust ⋮ Kerr-Schild metrics and gravitational radiation ⋮ Algebraically special, expanding and twisting gravitational fields with vanishing Newman–Unti–Tamburino parameter

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