Purely radiative irrotational dust spacetimes

Details Purely radiative irrotational dust spacetimes Purely radiative irrotational dust spacetimes

2006-11-14

arxiv.org/abs/gr-qc/0611079v2

J.Phys.Conf.Ser.66:012023,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, ERE 2006 conference, minor corrections

Scientific paper

10.1088/1742-6596/66/1/012023

We consider irrotational dust spacetimes in the full non-linear regime which
are "purely radiative" in the sense that the gravitational field satisfies the
covariant transverse conditions div(H) = div(E) = 0. Within this family we show
that the Bianchi class A spatially homogeneous dust models are uniquely
characterised by the condition that $H$ is diagonal in the shear-eigenframe.

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