Energy-momentum and equivalence principle in non-Riemannian geometries
We introduce an energy-momentum density vector which is independent of the affine structure of the manifold and whose conservation is linked to observers. Integrating this quantity over time-like surfaces we can define Hamiltonian and momentum for the system which coincide with the corresponding ADM...
Guardado en:
Publicado: |
1997
|
---|---|
Materias: | |
Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v29_n6_p691_Castagnino http://hdl.handle.net/20.500.12110/paper_00017701_v29_n6_p691_Castagnino |
Aporte de: |
id |
paper:paper_00017701_v29_n6_p691_Castagnino |
---|---|
record_format |
dspace |
spelling |
paper:paper_00017701_v29_n6_p691_Castagnino2023-06-08T14:21:34Z Energy-momentum and equivalence principle in non-Riemannian geometries Conservation laws We introduce an energy-momentum density vector which is independent of the affine structure of the manifold and whose conservation is linked to observers. Integrating this quantity over time-like surfaces we can define Hamiltonian and momentum for the system which coincide with the corresponding ADM definitions for the case of irrotational Riemann-ian manifolds. As a consequence of our formalism, a Weak Equivalence Principle version for manifolds with torsion appears as the natural extension to non-Riemannian geometries from the Equivalence Principle of General Relativity. 1997 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v29_n6_p691_Castagnino http://hdl.handle.net/20.500.12110/paper_00017701_v29_n6_p691_Castagnino |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Conservation laws |
spellingShingle |
Conservation laws Energy-momentum and equivalence principle in non-Riemannian geometries |
topic_facet |
Conservation laws |
description |
We introduce an energy-momentum density vector which is independent of the affine structure of the manifold and whose conservation is linked to observers. Integrating this quantity over time-like surfaces we can define Hamiltonian and momentum for the system which coincide with the corresponding ADM definitions for the case of irrotational Riemann-ian manifolds. As a consequence of our formalism, a Weak Equivalence Principle version for manifolds with torsion appears as the natural extension to non-Riemannian geometries from the Equivalence Principle of General Relativity. |
title |
Energy-momentum and equivalence principle in non-Riemannian geometries |
title_short |
Energy-momentum and equivalence principle in non-Riemannian geometries |
title_full |
Energy-momentum and equivalence principle in non-Riemannian geometries |
title_fullStr |
Energy-momentum and equivalence principle in non-Riemannian geometries |
title_full_unstemmed |
Energy-momentum and equivalence principle in non-Riemannian geometries |
title_sort |
energy-momentum and equivalence principle in non-riemannian geometries |
publishDate |
1997 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v29_n6_p691_Castagnino http://hdl.handle.net/20.500.12110/paper_00017701_v29_n6_p691_Castagnino |
_version_ |
1768543872848232448 |