Relativity and Cosmology

    

Is Fine Structure Ratio – an Index of Cosmic Expansion?

Authors: U.V.S. Seshavatharam, S. Lakshminarayana

Within the expanding cosmic Hubble volume, Hubble length can be considered as the gravitational or electromagnetic interaction range. Product of ‘Hubble volume’ and ‘cosmic critical density’ can be called as the ‘Hubble mass’. Based on this cosmic mass unit, authors noticed four peculiar semi empirical relations. With the observed relations it is possible to say that, in atomic and nuclear physics, there exists a cosmological physical variable. By observing its rate of change, the future cosmic acceleration can be verified. Fine structure ratio may be considered as the index of present cosmic expansion. By observing its cosmological rate of change, future cosmic acceleration can be verified.

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[v1] 2012-12-14 20:19:32

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