Indeterministic Quantum Gravity IV. The Cosmic-length Universe and the Problem of the Missing Dark Matter

Details Indeterministic Quantum Gravity IV. The Cosmic-length Universe and the Problem of the Missing Dark Matter Indeterministic Quantum Gravity IV. The Cosmic-length Universe and the Problem of the Missing Dark Matter

1996-09-13

arxiv.org/abs/gr-qc/9609035v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, LATEX 2.09

Scientific paper

This paper is a sequel of the series of papers [gr-qc/9409010, gr-qc/9505034, gr-qc/9603022], being an immediate continuation and development of the latter of them. In the Friedmann universe, the equation $\Omega_0=2q_0$ holds ($\Omega$ is density parameter, $q$ is deceleration parameter, and subscript 0 indicates present-day values), which gives rise to the problem of the missing matter as observational data give $\Omega_0<2q_0$. In the cosmic-length universe, $\Omega_0=2q_0- L/R_0^3H_0^2$ ($R_0$ is the radius of the universe, $H_0$ is Hubble constant), which lifts the problem. The cosmic length, $L=const \approx 1/H_0$, is the infimum of the set of maximal radii of a closed universe.

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