Observational Tests of FRW World Models

dc.creatorLahav, Ofer
dc.date2001-12-21
dc.date.accessioned2026-07-07T11:46:00Z
dc.date.available2026-07-07T11:46:00Z
dc.descriptionObservational tests for the Cosmological Principle are reviewed. Assuming the FRW metric we then summarize estimates of cosmological parameters from various data sets, in particular the Cosmic Microwave Background and the 2dF galaxy redshift survey. These and other analyses suggest a best-fit Lambda-Cold Dark Matter model with Omega_m = 1 - Omega_lambda = 0.3 and H_0 = 70 km/sec/Mpc. It is remarkable that different measurements converge to this `concordance model', although it remains to be seen if the two main components of this model, the dark matter and the dark energy, are real entities or just `epicycles'. We point out some open questions related to this fashionable model.
dc.description11 pages with 3 figures included. Invited review at ``The Early Universe and Cosmological Observations: a Critical Review'', UCT, Cape Town, July 2001, to appear in "Classical and Quantum Gravity"
dc.identifierhttps://arxiv.org/abs/astro-ph/0112524
dc.identifierhttp://arxiv.org/abs/astro-ph/0112524
dc.identifierClass.Quant.Grav.19:3517-3526,2002
dc.identifierdoi:10.1088/0264-9381/19/13/309
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202072
dc.subjectAstrophysics
dc.titleObservational Tests of FRW World Models
dc.typetext

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