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| DOI | 10.1142/S0217732316501832 | ||||
| Año | 2016 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
We discuss the relation between Noether (point) symmetries and discrete symmetries for a class of minisuperspace cosmological models. We show that when a Noether symmetry exists for the gravitational Lagrangian, then there exists a coordinate system in which a reversal symmetry exists. Moreover, as far as concerns, the scale-factor duality symmetry of the dilaton field, we show that it is related to the existence of a Noether symmetry for the field equations, and the reversal symmetry in the normal coordinates of the symmetry vector becomes scale-factor duality symmetry in the original coordinates. In particular, the same point symmetry as also the same reversal symmetry exists for the Brans-Dicke scalar field with linear potential while now the discrete symmetry in the original coordinates of the system depends on the Brans-Dicke parameter and it is a scale-factor duality when omega(BD) = 1. Furthermore, in the context of the O'Hanlon theory for f(R)-gravity, it is possible to show how a duality transformation in the minisuperspace can be used to relate different gravitational models.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Paliathanasis, Andronikos | - |
Universidad Austral de Chile - Chile
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| 2 | Capozziello, Salvatore | Hombre |
Univ Naples Federico II - Italia
Ist Nazl Fis Nucl - Italia Gran Sasso Sci Inst INFN - Italia Università Degli Studi di Napoli Federico II - Italia Istituto Nazionale di Fisica Nucleare, Sezione di Napoli - Italia Gran Sasso Science Institute - Italia |
| Fuente |
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| FONDECYT |
| Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica |
| COST (European Cooperation in Science and Technology) |
| European Cooperation in Science and Technology |
| Istituto Nazionale di Fisica Nucleare |
| Fondo Nacional de Desarrollo CientÃfico, Tecnológico y de Innovación Tecnológica |
| Instituto Nazionale di Fisica Nucleare |
| INFN |
| Agradecimiento |
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| The authors would like to thank the anonymous referee for his/her careful reading and for his/her valuable comments which improved the quality and the presentation of this work. The research of AP was supported by FONDECYT postdoctoral Grant No. 3160121. S.C. acknowledges the support of INFN (iniziative specifiche QGSKY and TEONGRAV). This paper is based upon work from COST Action (CANTATA/CA15117), supported by COST (European Cooperation in Science and Technology). |
| The research of AP was supported by FONDECYT postdoctoral Grant No. 3160121. S.C. acknowledges the support of INFN (iniziative specifiche QGSKY and TEONGRAV). This paper is based upon work from COST Action (CANTATA/CA15117), supported by COST (European Cooperation in Science and Technology). |