Realistic cosmological measurement of distances in the Friedmann universe
2016 ◽
Vol 31
(02n03)
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pp. 1641013
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Keyword(s):
We consider application of our development of Zeldovich’s ideas, presented in Ref. 1, for measurement of the cosmological angular diameter distance (ADD) in the Friedmann Universe. To make a comparison with [Formula: see text]CDM we analyze ADD measurement in [Formula: see text]CDM model responsible for the later inflation (present accelerated expansion of the Universe). We also analyze a small deviation from equality in the distance duality relation induced by the fullness (by matter) of the cone of light rays (CLR) which is used for the ADD measurement method.