Non conducting spherically symmetric fluids

Details Non conducting spherically symmetric fluids Non conducting spherically symmetric fluids

2002-09-18

arxiv.org/abs/gr-qc/0209063v3

Gen.Rel.Grav. 36 (2003) 193-197

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages revtex4. Added references

Scientific paper

10.1023/B:GERG.0000006965.74658.

A class of spherically symmetric spacetimes invariantly defined by a zero flux condition is examined first from a purely geometrical point of view and then physically by way of Einstein's equations for a general fluid decomposition of the energy-momentum tensor. The approach, which allows a formal inversion of Einstein's equations, explains, for example, why spherically symmetric perfect fluids with spatially homogeneous energy density must be shearfree.

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