Kerr–Schild gravitational fields in matter and the Kerr-interior problem in general relativity

DOI10.1063/1.531226zbMath0842.73017OpenAlexW2048495548MaRDI QIDQ4873470

Giulio Magli

Publication date: 1 August 1996

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.531226

zbMATH Keywords

Einstein field equationsKerr metricshell distribution of elastic stress energysources of Kerr space-time

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Elastic materials (74B99)

Related Items (5)

Unconstrained variational principle and canonical structure for relativistic elasticity ⋮ Physically valid black hole interior models ⋮ Kerr-Schild symmetries ⋮ A null-tetrad approach to Kerr–Schild gravitational fields in matter ⋮ The formation of non-Keplerian rings of matter about compact stars

Cites Work

• Some overdetermined boundary value problems for harmonic functions
• Relativistic elastomechanics as a Lagrangian field theory
• Ellipsoidal space-times, sources for the Kerr metric
• The dynamical structure of the Einstein equations for a non-rotating star
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• On the covariant equations of the relativistic electrodynamics of continua. III. Elastic solids
• Tuning the properties of matter to any chosen dynamical behavior in cosmological models with elastic media

This page was built for publication: Kerr–Schild gravitational fields in matter and the Kerr-interior problem in general relativity