dc.creatorMinotti, Fernando Oscar
dc.date.accessioned2019-10-22T15:49:02Z
dc.date.accessioned2022-10-15T00:10:15Z
dc.date.available2019-10-22T15:49:02Z
dc.date.available2022-10-15T00:10:15Z
dc.date.created2019-10-22T15:49:02Z
dc.date.issued2018-07
dc.identifierMinotti, Fernando Oscar; Possible Means of Electrostatic Propulsion According to the Mbelek–Lachièze-Rey Scalar-Tensor Theory of Gravitation; Springer; Gravitation & Cosmology; 24; 3; 7-2018; 285-288
dc.identifier0202-2893
dc.identifierhttp://hdl.handle.net/11336/86861
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4323179
dc.description.abstractAs was shown recently, the scalar-tensor theory of gravitation proposed by Mbelek and Lachièze-Rey allows for a possible explanation of the forces reported in asymmetric microwave cavities. We show here that the theory in its revised version predicts a much simpler way of producing thrust by electrostatic means. We here briefly present the equations and derivations indicating that a constant force is predicted for a spherical capacitor with an asymmetric mass distribution, kept at constant voltage. Apart form other practical implications, this particular prediction, and a complementary proposal in which the spherical capacitor takes the place of the large mass in a Cavendish-like experiment, provides an additional possibility of experimentally testing this particular scalar-tensor gravitational theory.
dc.languageeng
dc.publisherSpringer
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1134/S0202289318030106
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectSCALAR TENSOR GRAVITY
dc.subjectELECTRIC PROPULSION
dc.titlePossible Means of Electrostatic Propulsion According to the Mbelek–Lachièze-Rey Scalar-Tensor Theory of Gravitation
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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