Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.207..231l&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 207, no. 2, p. 231-248
Astronomy and Astrophysics
Astrophysics
Astronomical Models, Big Bang Cosmology, Coordinate Transformations, Relativity, Space-Time Functions, Angular Velocity, Eigenvectors, Red Shift, Stellar Magnitude
Scientific paper
We present a non-general relativistic cosmological model with the following features. (1) All cosmological objects appear to be receding from each other. There are two mathematically distinct types of objects. (2) Type 1 objects have apparent magnitudes and apparent angular diameters comparable to those for standard FLRW models. Their redshifts are bounded; this bound is at least 3. (3) Type 2 objetcs can have unlimited redshifts. They appear significantly smaller than Type 1 objects with the same redshift, and (for redshifts greater than 1) appear brighter (and more so for larger redshifts). The model is an extension of classical de Sitter spacetime in which the location of infinity is allowed to be relative.
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