De sitter invariant special relativity and the dark energy problem
| Autor(a) principal: | |
|---|---|
| Data de Publicação: | 2017 |
| Outros Autores: | , |
| Tipo de documento: | Artigo de conferência |
| Idioma: | eng |
| Título da fonte: | Repositório Institucional da UNESP |
| Texto Completo: | http://hdl.handle.net/11449/206548 |
Resumo: | Due 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 tensor |
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De sitter invariant special relativity and the dark energy problemDue 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 tensorUniversidade Estadual Paulista (UNESP) Instituto de Física TeóricaUniversidade Estadual Paulista (UNESP) Instituto de Física TeóricaUniversidade Estadual Paulista (Unesp)Araujo, A. [UNESP]López, D. F. [UNESP]Pereira, J. G. [UNESP]2021-06-25T10:34:09Z2021-06-25T10:34:09Z2017-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject293-294Proceedings of the 52nd Rencontres de Moriond - 2017 Gravitation, p. 293-294.http://hdl.handle.net/11449/2065482-s2.0-85091332897Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengProceedings of the 52nd Rencontres de Moriond - 2017 Gravitationinfo:eu-repo/semantics/openAccess2021-10-23T07:21:36Zoai:repositorio.unesp.br:11449/206548Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T19:35:14.546814Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
| dc.title.none.fl_str_mv |
De sitter invariant special relativity and the dark energy problem |
| title |
De sitter invariant special relativity and the dark energy problem |
| spellingShingle |
De sitter invariant special relativity and the dark energy problem Araujo, A. [UNESP] |
| title_short |
De sitter invariant special relativity and the dark energy problem |
| title_full |
De sitter invariant special relativity and the dark energy problem |
| title_fullStr |
De sitter invariant special relativity and the dark energy problem |
| title_full_unstemmed |
De sitter invariant special relativity and the dark energy problem |
| title_sort |
De sitter invariant special relativity and the dark energy problem |
| author |
Araujo, A. [UNESP] |
| author_facet |
Araujo, A. [UNESP] López, D. F. [UNESP] Pereira, J. G. [UNESP] |
| author_role |
author |
| author2 |
López, D. F. [UNESP] Pereira, J. G. [UNESP] |
| author2_role |
author author |
| dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
| dc.contributor.author.fl_str_mv |
Araujo, A. [UNESP] López, D. F. [UNESP] Pereira, J. G. [UNESP] |
| description |
Due 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 tensor |
| publishDate |
2017 |
| dc.date.none.fl_str_mv |
2017-01-01 2021-06-25T10:34:09Z 2021-06-25T10:34:09Z |
| dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
| dc.type.driver.fl_str_mv |
info:eu-repo/semantics/conferenceObject |
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conferenceObject |
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publishedVersion |
| dc.identifier.uri.fl_str_mv |
Proceedings of the 52nd Rencontres de Moriond - 2017 Gravitation, p. 293-294. http://hdl.handle.net/11449/206548 2-s2.0-85091332897 |
| identifier_str_mv |
Proceedings of the 52nd Rencontres de Moriond - 2017 Gravitation, p. 293-294. 2-s2.0-85091332897 |
| url |
http://hdl.handle.net/11449/206548 |
| dc.language.iso.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
Proceedings of the 52nd Rencontres de Moriond - 2017 Gravitation |
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info:eu-repo/semantics/openAccess |
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openAccess |
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293-294 |
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Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
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Universidade Estadual Paulista (UNESP) |
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UNESP |
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UNESP |
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Repositório Institucional da UNESP |
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Repositório Institucional da UNESP |
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Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
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1808129090783281152 |