Determination of Upper Limit of Stars Mass Based on Model of Expansive Nondecelerative Universe
arXiv:gr-qc/0101027
Abstract
Incorporation of the Vaidya metric in the model of Expansive Nondecelerative Universe allows to localize the energy density of gravitational field that, subsequently, enables to determine the upper limit of stars mass. The upper limit decreases with cosmological time and at present is close to 30-fold of our Sun mass.
3 pages, LaTeX