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

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dc.creatorSima, Jozef
dc.creatorSukenik, Miroslav
dc.date2001-01-08
dc.date.accessioned2026-07-07T03:25:35Z
dc.date.available2026-07-07T03:25:35Z
dc.descriptionIncorporation 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.
dc.description3 pages, LaTeX
dc.identifierhttps://arxiv.org/abs/gr-qc/0101027
dc.identifierhttp://arxiv.org/abs/gr-qc/0101027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33767
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDetermination of Upper Limit of Stars Mass Based on Model of Expansive Nondecelerative Universe
dc.typetext

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