Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state
We show that there is a correspondence between cosmology from non-extensive thermodynamics and cosmology with fluids of redefined and generalized equation of state. We first establish the correspondence in the case of basic non-extensive thermodynamics, and then we proceed by investigating the more...
| Autores: | , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2020 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/236777 |
| Acceso en línea: | http://hdl.handle.net/10261/236777 |
| Access Level: | acceso abierto |
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Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of stateNojiri, Shin'ichiOdintsov, Sergei D.Saridakis, EmmanuelMyrzakulov, RatbayWe show that there is a correspondence between cosmology from non-extensive thermodynamics and cosmology with fluids of redefined and generalized equation of state. We first establish the correspondence in the case of basic non-extensive thermodynamics, and then we proceed by investigating the more consistent case, from the quantum field theoretical point of view, of varying exponent, namely depending on the scale. The obtained duality provides a way of explaining the complicated phenomenological forms of the effective fluid equation-of-state parameters that are being broadly used in the literature, since their microphysical origin may indeed lie in the non-extensive thermodynamics of spacetime. Finally, concerning the cosmological behavior, we show that at late times the effective fluid may drive the universe acceleration even in the absence of an explicit cosmological constant, and even if the initial fluid is the standard dust matter one. Similarly, at early times we obtain an effective cosmological constant which is enhanced through screening, and hence it can drive a successful inflation without spoiling the correct late-time acceleration.This work is partly supported by MEXT KAKENHI Grant-in-Aid for Scientific Research on Innovative Areas g Cosmic Acceleration h No. 15H05890 (S.N.) and the JSPS Grant-in-Aid for Scientific Research (C) No. 18K03615 (S.N.), and by MINECO (Spain), FIS2016-76363-P, and by project 2017 SGR247 (AGAUR, Catalonia) (S.D.O). The work was carried out with the financial support of the Ministry of Education and Science of the Republic of Kazakhstan, Grant No 0118RK00935.Peer reviewedElsevierMinistry of Education, Culture, Sports, Science and Technology (Japan)Japan Society for the Promotion of ScienceMinisterio de Economía y Competitividad (España)Generalitat de CatalunyaMinistry of Education and Science (Kazakhstan)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202120212020info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/236777reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/FIS2016-76363-Phttps://doi.org/10.1016/j.nuclphysb.2019.114850Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/2367772026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state |
| title |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state |
| spellingShingle |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state Nojiri, Shin'ichi |
| title_short |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state |
| title_full |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state |
| title_fullStr |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state |
| title_full_unstemmed |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state |
| title_sort |
Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state |
| dc.creator.none.fl_str_mv |
Nojiri, Shin'ichi Odintsov, Sergei D. Saridakis, Emmanuel Myrzakulov, Ratbay |
| author |
Nojiri, Shin'ichi |
| author_facet |
Nojiri, Shin'ichi Odintsov, Sergei D. Saridakis, Emmanuel Myrzakulov, Ratbay |
| author_role |
author |
| author2 |
Odintsov, Sergei D. Saridakis, Emmanuel Myrzakulov, Ratbay |
| author2_role |
author author author |
| dc.contributor.none.fl_str_mv |
Ministry of Education, Culture, Sports, Science and Technology (Japan) Japan Society for the Promotion of Science Ministerio de Economía y Competitividad (España) Generalitat de Catalunya Ministry of Education and Science (Kazakhstan) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| description |
We show that there is a correspondence between cosmology from non-extensive thermodynamics and cosmology with fluids of redefined and generalized equation of state. We first establish the correspondence in the case of basic non-extensive thermodynamics, and then we proceed by investigating the more consistent case, from the quantum field theoretical point of view, of varying exponent, namely depending on the scale. The obtained duality provides a way of explaining the complicated phenomenological forms of the effective fluid equation-of-state parameters that are being broadly used in the literature, since their microphysical origin may indeed lie in the non-extensive thermodynamics of spacetime. Finally, concerning the cosmological behavior, we show that at late times the effective fluid may drive the universe acceleration even in the absence of an explicit cosmological constant, and even if the initial fluid is the standard dust matter one. Similarly, at early times we obtain an effective cosmological constant which is enhanced through screening, and hence it can drive a successful inflation without spoiling the correct late-time acceleration. |
| publishDate |
2020 |
| dc.date.none.fl_str_mv |
2020 2021 2021 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/236777 |
| url |
http://hdl.handle.net/10261/236777 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
#PLACEHOLDER_PARENT_METADATA_VALUE# info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/FIS2016-76363-P https://doi.org/10.1016/j.nuclphysb.2019.114850 Sí |
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info:eu-repo/semantics/openAccess |
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openAccess |
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Elsevier |
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Elsevier |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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