Determination of Upper Limit of Stars Mass Based on Model of Expansive Nondecelerative Universe

Details Determination of Upper Limit of Stars Mass Based on Model of Expansive Nondecelerative Universe Determination of Upper Limit of Stars Mass Based on Model of Expansive Nondecelerative Universe

2001-01-08

arxiv.org/abs/gr-qc/0101027v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

3 pages, LaTeX

Scientific paper

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.

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