Abstract
Recent observational results (cf. Refs. [1, 2, 3, 4, 5, 6], in particular results of studies of distant supernovae as standard candles [2, 4, 6] and studies of anisotropy of cosmic microwave background [3], set forth a problem of the cosmological constant once again. The most probable values of ΩM and ΩV, i. e. the normalized ratios (with respect to the critical density) of matter density and cosmological-constant energy density, turned out to be most probably equal to 0.3–0.4 and 0.6–0.7 respectively. By usual definition, ΩM = P M/P cr , Ωv = P v/P cr , where P M is the density of matter, P M is the density of vacuum; the critical density p cr = 3H 2/8πG; H is the Hubble parameter, G is the gravitational constant. According to the observational tests, the sum of ΩM and ΩV seems to be greater than one; this implies that the Universe is closed.
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Shevchenko, I.I. (2003). Conformal Time in Cosmology. In: Buccheri, R., Saniga, M., Stuckey, W.M. (eds) The Nature of Time: Geometry, Physics and Perception. NATO Science Series, vol 95. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0155-7_28
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DOI: https://doi.org/10.1007/978-94-010-0155-7_28
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