Testing the Metric-Field Equations of Gravitation

dc.creatorVerozub, L. V.
dc.date2007-02-15
dc.date2007-03-21
dc.date.accessioned2026-07-07T07:52:47Z
dc.date.available2026-07-07T07:52:47Z
dc.descriptionPhysical consequences from gravitation equations based on Poincaré ideas of relativity of space and time in respect of measuring instruments are considered. The most interesting of them are the possibility of the existence of stable supermassive configurations $(10^{2} ÷10^{12} M_{\odot})$ which can exist in galactic centres, and an explanation of the acceleration of the Universe expansion as a manifestation of the gravitational force properties in the theory under consideration.
dc.descriptionLatex, 6 pages, 7 figures. Proc. of the EPS-13 Conference "Beyond Einstein - Physics for the 21st Century", 2005, Bern, Switzerland (ESA, SP-637)
dc.identifierhttps://arxiv.org/abs/gr-qc/0702088
dc.identifierhttp://arxiv.org/abs/gr-qc/0702088
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/126005
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleTesting the Metric-Field Equations of Gravitation
dc.typetext

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