Abstract
Most cosmological models are based on the ‘cosmological principle’ according to which the Universe is homogeneous and isotropic on a certain level, chosen such that the present mean density is of the order of 10−3O±1 g cm−3.
Article Note
The Original paper has been revised and considerably shortend because of information obtained after the symposium concerning recent calculations on the hydrogen-antihydrogen potential, which invalidate conclusions based on earlier computations.
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Elvius, A., Karlson, E.T., Laurent, B.E. (1974). The Low Density Symmetric Cosmology. In: Longair, M.S. (eds) Confrontation of Cosmological Theories with Observational Data. International Astronomical Union / Union Astronomique Internationale, vol 63. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2220-0_30
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DOI: https://doi.org/10.1007/978-94-010-2220-0_30
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