Non-Riemannian generalizations of the Born-Infeld model and the meaning of the cosmological term
Theory of gravitation based on a non-Riemannian geometry with dynamical torsion field is geometrically analyzed. To this end, the simplest Lagrangian density is introduced as a measure (reminiscent of a sigma model) and the dynamical equations are derived. Our goal is to rewrite this generalized aff...
Guardado en:
| Autor principal: | Cirilo, Diego Julio |
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| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02198878_v14_n7_p_CiriloLombardo http://hdl.handle.net/20.500.12110/paper_02198878_v14_n7_p_CiriloLombardo |
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