Hamiltonian approach to relativistic star models

DOI10.1088/0264-9381/12/5/019zbMath0823.53079arXivgr-qc/9411047OpenAlexW2038755253MaRDI QIDQ4835564

Kjell Rosquist

Publication date: 17 October 1995

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9411047

zbMATH Keywords

polytope solutionrelativistic star configurations

Mathematics Subject Classification ID

Quantization of the gravitational field (83C45) Applications of differential geometry to physics (53Z05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (3)

Static perfect fluids with Pant-Sah equations of state ⋮ Third rank Killing tensors in general relativity. The \((1+1)\)-dimensional case ⋮ Superfluid quantum vortex in curved space

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