CONSTRAINING SPACETIME TORSION WITH THE MOON, MERCURY AND LAGEOS

dc.contributor.author	March, Riccardo
dc.contributor.author	Bellettini, Giovanni
dc.contributor.author	Tauraso, Roberto
dc.contributor.author	Dell’Agnello, Simone
dc.date.accessioned	2021-12-01T13:27:30Z
dc.date.available	2021-12-01T13:27:30Z
dc.date.issued	2013
dc.identifier.citation	Acta Polytechnica. 2013, vol. 53, no. A, p. 817-820.
dc.identifier.issn	1210-2709 (print)
dc.identifier.issn	1805-2363 (online)
dc.identifier.uri	http://hdl.handle.net/10467/98695
dc.description.abstract	We consider an extension of Einstein General Relativity where, beside the Riemann curvature tensor, we suppose the presence of a torsion tensor. Using a parametrized theory based on symmetry arguments, we report on some results concerning the constraints that can be put on torsion parameters by studying the orbits of a test body in the solar system.	en
dc.format.mimetype	application/pdf
dc.language.iso	eng
dc.publisher	České vysoké učení technické v Praze	cs
dc.publisher	Czech Technical University in Prague	en
dc.relation.ispartofseries	Acta Polytechnica
dc.relation.uri	https://ojs.cvut.cz/ojs/index.php/ap/article/view/2002
dc.rights	Creative Commons Attribution 4.0 International License	en
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/
dc.title	CONSTRAINING SPACETIME TORSION WITH THE MOON, MERCURY AND LAGEOS
dc.type	article	en
dc.date.updated	2021-12-01T13:27:30Z
dc.identifier.doi	10.14311/AP.2013.53.0817
dc.rights.access	openAccess
dc.type.status	Peer-reviewed
dc.type.version	publishedVersion

Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License