Non-static shear-free spherically symmetric charged perfect fluid distributions: a symmetry approach

DOI10.1088/0264-9381/17/15/314zbMath0965.83015OpenAlexW2010572855MaRDI QIDQ4507979

F. M. Mahomed, C. Wafo Soh

Publication date: 29 July 2001

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

Full work available at URL: https://doi.org/10.1088/0264-9381/17/15/314

zbMATH Keywords

symmetry methodEinstein-Maxwell equationsspherically symmetricLie point symmetrycharged perfect fluidNoether point symmetry

Mathematics Subject Classification ID

Symmetries, invariants of ordinary differential equations (34C14) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Einstein-Maxwell equations (83C22)

Related Items (7)

Analytical models for gravitating radiating systems ⋮ Integrable cases of gravitating static isothermal fluid spheres ⋮ What makes a shear-free spherical perfect fluid be inhomogeneous with tidal effects? ⋮ Semi-analytical solution of a constrained fourth-order integro-differential equation of steady flow--structure interaction in a model collapsible tube ⋮ Some new static charged spheres ⋮ A fifth order differential equation for charged perfect fluids ⋮ Charged sphere of shear-free fluids with \(\frac{\partial\rho}{\partial r} \leq 0\)

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