The stationary axisymmetric two-body problem in general relativity

DOI10.1002/cpa.3160450907zbMath0782.53088OpenAlexW2139179641WikidataQ125359816 ScholiaQ125359816MaRDI QIDQ4036104

Gilbert Weinstein

Publication date: 16 May 1993

Published in: Communications on Pure and Applied Mathematics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1002/cpa.3160450907

zbMATH Keywords

prescribed singularitiesharmonic mapangle of deficiency of the conical singularityKerr-like solutions

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) PDEs in connection with relativity and gravitational theory (35Q75)

Related Items (10)

Hawking's local rigidity theorem without analyticity ⋮ Time-periodic Einstein-Klein-Gordon bifurcations of Kerr ⋮ The geometry and topology of stationary multiaxisymmetric vacuum black holes in higher dimensions ⋮ Singular harmonic maps and applications to general relativity ⋮ Non-existence of multiple-black-hole solutions close to Kerr-Newman ⋮ On the Dirichlet problem for harmonic maps with prescribed singularities ⋮ Existence and uniqueness of asymptotically flat toric gravitational instantons ⋮ N-Black hole stationary and axially symmetric solutions of the einstein/maxwell equations ⋮ The interaction force between rotating black holes at equilibrium ⋮ Equilibrium configuration of black holes and the inverse scattering method

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