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

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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

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/33767

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0101027
 http://arxiv.org/abs/gr-qc/0101027

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arXiv