Universal relationship between the constituent masses of regular systems and their distances from the centerA. Dinculescu
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received 5 August 2008; accepted in final form 28 August 2008; published October 2008
published online 22 September 2008
One can describe all regular systems regardless of their size by a simple equation that relates the relative masses of their constituents with respect to the mass of the system, to their relative distances from the center with respect to a transition radius equally defined for all systems. Based on this equation one can estimate the value of the Hubble constant from the distribution of matter inside a large enough sample of atomic and/or gravitational systems.
04.40.-b - Self-gravitating systems; continuous media and classical fields in curved spacetime.
98.80.Es - Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc.).
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