Characteristic actions ħ(s) in the structure of the universe
1985
It is suggested that gravitationally bound systems in the Universe can be characterized by a set of actions ħ(s). The actions
$$\hbar ^{\left( s \right)} = \left( {{\hbar \mathord{\left/ {\vphantom {\hbar {\frac{1}{{2\pi }}\frac{{C^5 }}{{GH_0^2 }}}}} \right. \kern-\nulldelimiterspace} {\frac{1}{{2\pi }}\frac{{C^5 }}{{GH_0^2 }}}}} \right)^{s/6} \left( {\frac{1}{{2\pi }}\frac{{C^5 }}{{GH_0^2 }}} \right)$$
,derived from general theoretical consideration, are only determined by the fundamental physical constants (Planck's action ħ, the velocity of lightC, gravitational constantG, and Hubble's constantH0) and a scale parameters. It is shown thats=1, 2, and 3 correspond, respectively, to the scales of galaxies, stars, and larger asteroids.
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