Authors: Bernard Riley
By application of the 10D/4D correspondence, the radii of nearby stars have been shown to map onto the masses of stable atomic nuclei. The correspondence is now used to calculate the mass m and radius r of the subatomic object that corresponds to a typical 1.4 solar mass neutron star. The mass m is found to be 4.0 TeV. Using natural units, r/m is precisely 2.
Comments: 8 Pages.
[v1] 2017-07-12 03:52:25
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