Charged sphere of shear-free fluids with \(\frac{\partial\rho}{\partial r} \leq 0\)
From MaRDI portal
Publication:2583261
DOI10.1007/s10714-005-0165-1zbMath1091.83009OpenAlexW2048479446MaRDI QIDQ2583261
Publication date: 13 January 2006
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-005-0165-1
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Einstein-Maxwell equations (83C22)
Related Items
EVOLVING SPHERES OF SHEAR-FREE ANISOTROPIC FLUID ⋮ Comment: On charged analogue of shear-free fluids
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- A class of spherically symmetric solutions with conformal Killing vectors
- Monodromy- and spectrum-preserving deformations. I
- On shear free normal flows of a perfect fluid
- Expanding spherically symmetric models without shear
- Solvable models of relativistic charged spherically symmetric fluids
- A new interior solution of Einstein's field equations for a spherically symmetric perfect fluid in shear-free motion
- On spherically symmetric shear-free perfect fluid configurations (neutral and charged). I
- Jeffery-Williams Lecture, 1976 Non-Static Radially Symmetric Distributions of Matter
- Non-static shear-free spherically symmetric charged perfect fluid distributions: a symmetry approach
- Shear-free relativistic fluids and the absence of movable branch points
- Spherically symmetric perfect fluids in shear-free motion - the symmetry approach
