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

Abstract

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, ${\Omega }_0=2q_0-L/R_0^3{H}_0^2$ ($R_0$ 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.

7 pages, LATEX 2.09