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De sitter invariant special relativity and the dark energy problem

dc.contributor.authorAraujo, A. [UNESP]
dc.contributor.authorLópez, D. F. [UNESP]
dc.contributor.authorPereira, J. G. [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2021-06-25T10:34:09Z
dc.date.available2021-06-25T10:34:09Z
dc.date.issued2017-01-01
dc.description.abstractDue to the existence of an invariant length at the Planck scale, Einstein special relativity is believed to break down at the scale. A possible solution to this problem is to replace the Poincaré invariant special relativity by a de Sitter invariant special relativity. Such replacement produces concomitant changes in general relativity, the most relevant being the fact that both the background de Sitter curvature and the gravitational dynamical curvature are now included in the same curvature tensoren
dc.description.affiliationUniversidade Estadual Paulista (UNESP) Instituto de Física Teórica
dc.description.affiliationUnespUniversidade Estadual Paulista (UNESP) Instituto de Física Teórica
dc.format.extent293-294
dc.identifier.citationProceedings of the 52nd Rencontres de Moriond - 2017 Gravitation, p. 293-294.
dc.identifier.scopus2-s2.0-85091332897
dc.identifier.urihttp://hdl.handle.net/11449/206548
dc.language.isoeng
dc.relation.ispartofProceedings of the 52nd Rencontres de Moriond - 2017 Gravitation
dc.sourceScopus
dc.titleDe sitter invariant special relativity and the dark energy problemen
dc.typeTrabalho apresentado em evento
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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