scientific article; zbMATH DE number 1515730
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Publication:4508102
DOI<368::AID-ANDP368>3.0.CO;2-Q 10.1002/(SICI)1521-3889(200005)9:3/5<368::AID-ANDP368>3.0.CO;2-QzbMath0972.83040arXivgr-qc/9911113MaRDI QIDQ4508102
Publication date: 10 October 2000
Full work available at URL: https://arxiv.org/abs/gr-qc/9911113
Title: zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)
Cites Work
- Stationary axisymmetric perfect fluid solutions in general relativity
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Perfect fluid spacetimes with a purely magnetic Weyl tensor
- Third rank Killing tensors in general relativity. The \((1+1)\)-dimensional case
- Perfect fluids with vanishing Simon tensor
- Symmetries of Einstein’s field equations with a perfect fluid source as examples of Lie–Bäcklund symmetries
- New family of stationary and axisymmetric perfect-fluid solutions
- Invariant construction of solutions to Einstein's field equations - LRS perfect fluids I
- Stationary rotating matter in general relativity
- A differential form approach for rotating perfect fluids in general relativity
- Axistationary perfect fluids - a tetrad approach
- An interior solution in general relativity
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