Inherent weaknesses of cosmology

Details Inherent weaknesses of cosmology Inherent weaknesses of cosmology

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986comap..11..193c&link_type=abstract

Comments on Modern Physics, Part C - Comments on Astrophysics (ISSN 0146-2970), vol. 11, July 1986, p. 193-199.

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Cosmology, Astronomical Spectroscopy, Hydrogen Recombinations, Time Measurement, Universe

Scientific paper

Sources of astrophysical evidence necessary to verify a cosmological model are reviewed. Cosmological history of the universe is divided into four epochs, each unique in its physical conditions related to observability at present. The current epoch, started after recombination of hydrogen in the universe, offers the most in observability. In earlier epochs, verifiable astrophysical evidence gradually disappeared. It seems that no astrophysical evidence has been left behind from the singularity epoch of the Universe. The gradual disappearance of astrophysical evidence ascertainable at present is the result of physical conditions structured within the cosmological models, hence indicating certain inherent weaknesses of cosmology as a verifiable physical theory.

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