Solvable models of relativistic charged spherically symmetric fluids
It is known that charged relativistic shear-free fluid spheres are described by the equation yxx = f(x)y2+g(x)y3, where f and g are arbitrary functions of x only and y is a function of x and an external parameter t.Necessary and sufficient conditions on f and g are obtained such that this equation p...
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| Format: | Default Preprint |
| Published: |
2000
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| Online Access: | https://hdl.handle.net/2134/755 |
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