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DYNAMICAL PROPERTIES OF COSMOLOGICAL SOLUTIONS

GEORGE F. R. ELLIS

Mathematics Department, University of Cape Town, Rondebosch 7701, Cape Town, South Africa

https://doi.org/10.1142/S0219891605000464Cited by:1 (Source: Crossref)

Abstract

I will consider how there are FOSH formulations and associated results in relativistic cosmology expressed in 1+3 tetrad form. The characteristics of scalar and vector perturbations are timelike, hence the real domains of dependence in cosmology are much smaller than implied by the light cone, associated with gravitational wave perturbations.

Keywords:

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