Significance of tension for Kaluza-KIein models: critical remarks

dc.contributor.authorZhuk, Alexander
dc.contributor.authorEingorn, Maxim
dc.date.accessioned2013-11-22T12:00:28Z
dc.date.available2013-11-22T12:00:28Z
dc.date.issued2012
dc.description.abstractWe clarify the problematic aspects of gravitational interaction in the weak field limit of Kaluza-KIein models. We explain why some models meet the classical gravitational tests, while the others do not. We show that variation of the total volume of the internal spaces generates the fifth force. This is the main reason of the problem. It happens for all considered models (linear with respect to the scalar curvature and nonlinear f(R), with toroidal and spherical compactifications). We explicitly single out the contribution of the fifth force to nonrelativistic gravitational potentials.uk
dc.identifier.citation12-th Odessa International astronomical Gamow conference-school, "Astronomy and beyond: astrophysics, cosmology and gravitation, cosmomicrophysics, radio-astronomy and astrobiology" : program and abstracts, August 20-26, 2012 / "Astronomy and beyond: astrophysics, cosmology and gravitation, cosmomicrophysics, radio-astronomy and astrobiology", international astronomical Gamow conference-school (12;2012; Odessa) - ; chief I. N. Koval . – Odessa, 2012 . – 53 p.uk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/3940
dc.language.isoenuk
dc.publisherОдеський національний університет імені І. І. Мечниковаuk
dc.relation.ispartofseries12-th international astronomical Gamov conference-school
dc.subjectKaluza-KIein modelsuk
dc.subjectgravitational interactionuk
dc.titleSignificance of tension for Kaluza-KIein models: critical remarksuk
dc.typeArticleuk
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