Detecting large-scale deviations from a FRW geometry with future CMB observations

Details Detecting large-scale deviations from a FRW geometry with future CMB observations Detecting large-scale deviations from a FRW geometry with future CMB observations

1999-06-04

arxiv.org/abs/astro-ph/9906094v1

Astronomy and Astrophysics

Astrophysics

6 pages, no figs

Scientific paper

We discuss the question to what degree the geometrical structure and the
matter content of the universe at scales exceeding the present Hubble horizon
is constrained by cosmological observations, in particular by measurements of
the cosmic microwave background radiation. For an answer, a simple formalism is
described, which goes back to a paper by Kristian and Sachs in 1966.

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