On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory

The post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble or ECSK theory is developed. It is used to obtain a drastic reduction on the density of the source needed to detect the spin. It is also proved that if we know the structure of the source, up to order -v, the spin can be detected,...

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Autores principales: Castagnino, M., Levinas, M.L., Umerez, N.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00017701_v17_n7_p683_Castagnino
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
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spelling todo:paper_00017701_v17_n7_p683_Castagnino2023-10-03T13:51:57Z On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory Castagnino, M. Levinas, M.L. Umerez, N. The post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble or ECSK theory is developed. It is used to obtain a drastic reduction on the density of the source needed to detect the spin. It is also proved that if we know the structure of the source, up to order -v, the spin can be detected, and if we know it up to order -v2 the theory can be verified. © 1985 Plenum Publishing Corporation. Fil:Castagnino, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Levinas, M.L. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Umerez, N. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00017701_v17_n7_p683_Castagnino
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description The post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble or ECSK theory is developed. It is used to obtain a drastic reduction on the density of the source needed to detect the spin. It is also proved that if we know the structure of the source, up to order -v, the spin can be detected, and if we know it up to order -v2 the theory can be verified. © 1985 Plenum Publishing Corporation.
format JOUR
author Castagnino, M.
Levinas, M.L.
Umerez, N.
spellingShingle Castagnino, M.
Levinas, M.L.
Umerez, N.
On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory
author_facet Castagnino, M.
Levinas, M.L.
Umerez, N.
author_sort Castagnino, M.
title On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory
title_short On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory
title_full On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory
title_fullStr On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory
title_full_unstemmed On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory
title_sort on the post-newtonian approximation of the einstein-cartan-sciama-kibble theory
url http://hdl.handle.net/20.500.12110/paper_00017701_v17_n7_p683_Castagnino
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AT levinasml onthepostnewtonianapproximationoftheeinsteincartansciamakibbletheory
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