Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids. Perfect fluids
DOI10.1063/5.0156227zbMath1521.83055arXiv2305.11565OpenAlexW4379050783MaRDI QIDQ6080732
Publication date: 4 October 2023
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.11565
Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) 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 cylindrical anisotropic fluid
- A vacuum exterior to Maitra's cylindrical dust solution
- Exact Solutions of Einstein's Field Equations
- Axial symmetry and conformal Killing vectors
- Some special solutions of the equations of axially symmetric gravitational fields
- A Petrov type I cylindrically symmetric solution for perfect fluid in steady rigid body rotation
- Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. II. More about axial pressure
- Fully integrated interior solutions of GR for stationary rigidly rotating cylindrical perfect fluids
- Exact Space-Times in Einstein's General Relativity
- Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. III. Azimuthal pressure
- Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. IV. Radial pressure
This page was built for publication: Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids. Perfect fluids
