The quasi-steady-state cosmology: a study of angular size against redshift

Details The quasi-steady-state cosmology: a study of angular size against redshift The quasi-steady-state cosmology: a study of angular size against redshift

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999mnras.307...73b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 307, Issue 1, pp. 73-78.

Astronomy and Astrophysics

Astronomy

10

Scientific paper

The data on angular sizes and redshifts of ultracompact radio sources used by Jackson & Dodgson in a recent paper have been applied to the various theoretical models in the framework of the quasi-steady-state cosmology proposed by Hoyle, Burbidge & Narlikar. It is found that although acceptable fits to the data are available for the flat models, those with a negative curvature of spatial sections provide a better fit. These latter models require low densities of matter and as such do not demand too high a proportion of dark matter. A comparison is made with the work of Jackson & Dodgson and theoretical implications of the test are discussed.

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