Deceleration without dark matter
Open Access
- 11 March 1997
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 285 (4) , 806-810
- https://doi.org/10.1093/mnras/285.4.806
Abstract
In homogeneous isotropic cosmological models the angular size θ of a standard measuring rod changes with redshift z in a manner that depends upon the parameters of the model. It has been argued that as a population ultracompact (milliarcsecond) radio sources measured by very long-baseline interferometry (VLBI) do not evolve with cosmic epoch, and thus comprise a set of standard objects, at least in a statistical sense. Here we examine the angular-size/redshift relation for 256 ultracompact sources with z in the range 0.5 to 3.8 for cosmological models with two degrees of freedom (Ω0 and Λ0,). The canonical inflationary cold dark matter model (Ω0 = 1, Λ0 = 0) appears to be ruled out by the observed relationship, whereas low-density models with a cosmological constant of either sign are favoured.Keywords
All Related Versions
This publication has 0 references indexed in Scilit: