Tsallis, Rényi and Sharma-Mittal holographic and new agegraphic dark energy models in D-dimensional fractal universe
. In this work, we explore the accelerated expansion of the Universe through a non-linear interaction of newly proposed dark energy models (namely Tsallis holographic dark energy (HDE), Rényi HDE, Sharma Mittal HDE, Tsallis new agegraphic dark energy (NADE), Rényi NADE and Sharma-Mittal NADE) with c...
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| Veröffentlicht in: | European physical journal plus 2019-10, Vol.134 (10), p.514, Article 514 |
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| creator | Maity, Sayani Debnath, Ujjal |
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In this work, we explore the accelerated expansion of the Universe through a non-linear interaction of newly proposed dark energy models (namely Tsallis holographic dark energy (HDE), Rényi HDE, Sharma Mittal HDE, Tsallis new agegraphic dark energy (NADE), Rényi NADE and Sharma-Mittal NADE) with cold dark matter in the background of flat
D
-dimensional fractal Universe. The effect of IR cutoffs including the Hubble radius and Granda-Oliveros (GO) on the properties of the considered dark energy models have been investigated in this context. The cosmological parameters such as equation of state (EoS) parameter, squared speed of sound and
ω
d
-
ω
d
cosmological plane during the cosmic evolution have been calculated. Analyzing the behavior of such cosmological parameters graphically, it is found that the considered HDE and NADE models can lead to the late time accelerated expansion in the presence of interaction between two dark sectors of the Universe in more general space-time. This result is similar to the standard interacting HDE model with Hubble cutoff in FRW Universe. |
| doi_str_mv | 10.1140/epjp/i2019-12884-6 |
| format | Article |
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In this work, we explore the accelerated expansion of the Universe through a non-linear interaction of newly proposed dark energy models (namely Tsallis holographic dark energy (HDE), Rényi HDE, Sharma Mittal HDE, Tsallis new agegraphic dark energy (NADE), Rényi NADE and Sharma-Mittal NADE) with cold dark matter in the background of flat
D
-dimensional fractal Universe. The effect of IR cutoffs including the Hubble radius and Granda-Oliveros (GO) on the properties of the considered dark energy models have been investigated in this context. The cosmological parameters such as equation of state (EoS) parameter, squared speed of sound and
ω
d
-
ω
d
cosmological plane during the cosmic evolution have been calculated. Analyzing the behavior of such cosmological parameters graphically, it is found that the considered HDE and NADE models can lead to the late time accelerated expansion in the presence of interaction between two dark sectors of the Universe in more general space-time. This result is similar to the standard interacting HDE model with Hubble cutoff in FRW Universe.</description><identifier>ISSN: 2190-5444</identifier><identifier>EISSN: 2190-5444</identifier><identifier>DOI: 10.1140/epjp/i2019-12884-6</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Applied and Technical Physics ; Astronomical models ; Atomic ; Cold dark matter ; Complex Systems ; Condensed Matter Physics ; Dark energy ; Equations of state ; Fractal models ; Fractals ; Holography ; Mathematical and Computational Physics ; Molecular ; Optical and Plasma Physics ; Parameters ; Physics ; Physics and Astronomy ; Regular Article ; Theoretical ; Universe</subject><ispartof>European physical journal plus, 2019-10, Vol.134 (10), p.514, Article 514</ispartof><rights>Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2019</rights><rights>Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2019.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c319t-53fd7e1b8180c2aa6a86e4af3fb8176b26bcb25de1f3beff57c27603ceec77cc3</citedby><cites>FETCH-LOGICAL-c319t-53fd7e1b8180c2aa6a86e4af3fb8176b26bcb25de1f3beff57c27603ceec77cc3</cites><orcidid>0000-0002-0718-6106</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1140/epjp/i2019-12884-6$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/2919611874?pq-origsite=primo$$EHTML$$P50$$Gproquest$$H</linktohtml><link.rule.ids>314,780,784,21388,27924,27925,33744,41488,42557,43805,51319,64385,64389,72469</link.rule.ids></links><search><creatorcontrib>Maity, Sayani</creatorcontrib><creatorcontrib>Debnath, Ujjal</creatorcontrib><title>Tsallis, Rényi and Sharma-Mittal holographic and new agegraphic dark energy models in D-dimensional fractal universe</title><title>European physical journal plus</title><addtitle>Eur. Phys. J. Plus</addtitle><description>.
In this work, we explore the accelerated expansion of the Universe through a non-linear interaction of newly proposed dark energy models (namely Tsallis holographic dark energy (HDE), Rényi HDE, Sharma Mittal HDE, Tsallis new agegraphic dark energy (NADE), Rényi NADE and Sharma-Mittal NADE) with cold dark matter in the background of flat
D
-dimensional fractal Universe. The effect of IR cutoffs including the Hubble radius and Granda-Oliveros (GO) on the properties of the considered dark energy models have been investigated in this context. The cosmological parameters such as equation of state (EoS) parameter, squared speed of sound and
ω
d
-
ω
d
cosmological plane during the cosmic evolution have been calculated. Analyzing the behavior of such cosmological parameters graphically, it is found that the considered HDE and NADE models can lead to the late time accelerated expansion in the presence of interaction between two dark sectors of the Universe in more general space-time. This result is similar to the standard interacting HDE model with Hubble cutoff in FRW Universe.</description><subject>Applied and Technical Physics</subject><subject>Astronomical models</subject><subject>Atomic</subject><subject>Cold dark matter</subject><subject>Complex Systems</subject><subject>Condensed Matter Physics</subject><subject>Dark energy</subject><subject>Equations of state</subject><subject>Fractal models</subject><subject>Fractals</subject><subject>Holography</subject><subject>Mathematical and Computational Physics</subject><subject>Molecular</subject><subject>Optical and Plasma Physics</subject><subject>Parameters</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Regular Article</subject><subject>Theoretical</subject><subject>Universe</subject><issn>2190-5444</issn><issn>2190-5444</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>AFKRA</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp9kE1OwzAQhSMEEhX0AqwsscXUdhwnWaLyKxUhQVlbjjNOXRIn2A2oR-IcXIy0BcGK2cxo5r2n0RdFJ5ScU8rJBLplN7GM0BxTlmUci71oxGhOcMI53_8zH0bjEJZkKJ5TnvNR1M-DqmsbztDj54dbW6RciZ4WyjcK39vVStVo0dZt5VW3sHp7dfCOVAU_q1L5FwQOfLVGTVtCHZB16BKXtgEXbOuGCOOV3kT1zr6BD3AcHRhVBxh_96Po-fpqPr3Fs4ebu-nFDOuY5iucxKZMgRYZzYhmSgmVCeDKxGZYpaJgotAFS0qgJi7AmCTVLBUk1gA6TbWOj6LTXW7n29cewkou294PHwXJcpoLSrOUDyq2U2nfhuDByM7bRvm1pERuCMsNYbklLLeEpRhM8c4UBrGrwP9G_-P6Apx3g44</recordid><startdate>20191001</startdate><enddate>20191001</enddate><creator>Maity, Sayani</creator><creator>Debnath, Ujjal</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><orcidid>https://orcid.org/0000-0002-0718-6106</orcidid></search><sort><creationdate>20191001</creationdate><title>Tsallis, Rényi and Sharma-Mittal holographic and new agegraphic dark energy models in D-dimensional fractal universe</title><author>Maity, Sayani ; Debnath, Ujjal</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c319t-53fd7e1b8180c2aa6a86e4af3fb8176b26bcb25de1f3beff57c27603ceec77cc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Applied and Technical Physics</topic><topic>Astronomical models</topic><topic>Atomic</topic><topic>Cold dark matter</topic><topic>Complex Systems</topic><topic>Condensed Matter Physics</topic><topic>Dark energy</topic><topic>Equations of state</topic><topic>Fractal models</topic><topic>Fractals</topic><topic>Holography</topic><topic>Mathematical and Computational Physics</topic><topic>Molecular</topic><topic>Optical and Plasma Physics</topic><topic>Parameters</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Regular Article</topic><topic>Theoretical</topic><topic>Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Maity, Sayani</creatorcontrib><creatorcontrib>Debnath, Ujjal</creatorcontrib><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><jtitle>European physical journal plus</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Maity, Sayani</au><au>Debnath, Ujjal</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Tsallis, Rényi and Sharma-Mittal holographic and new agegraphic dark energy models in D-dimensional fractal universe</atitle><jtitle>European physical journal plus</jtitle><stitle>Eur. Phys. J. Plus</stitle><date>2019-10-01</date><risdate>2019</risdate><volume>134</volume><issue>10</issue><spage>514</spage><pages>514-</pages><artnum>514</artnum><issn>2190-5444</issn><eissn>2190-5444</eissn><abstract>.
In this work, we explore the accelerated expansion of the Universe through a non-linear interaction of newly proposed dark energy models (namely Tsallis holographic dark energy (HDE), Rényi HDE, Sharma Mittal HDE, Tsallis new agegraphic dark energy (NADE), Rényi NADE and Sharma-Mittal NADE) with cold dark matter in the background of flat
D
-dimensional fractal Universe. The effect of IR cutoffs including the Hubble radius and Granda-Oliveros (GO) on the properties of the considered dark energy models have been investigated in this context. The cosmological parameters such as equation of state (EoS) parameter, squared speed of sound and
ω
d
-
ω
d
cosmological plane during the cosmic evolution have been calculated. Analyzing the behavior of such cosmological parameters graphically, it is found that the considered HDE and NADE models can lead to the late time accelerated expansion in the presence of interaction between two dark sectors of the Universe in more general space-time. This result is similar to the standard interacting HDE model with Hubble cutoff in FRW Universe.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1140/epjp/i2019-12884-6</doi><orcidid>https://orcid.org/0000-0002-0718-6106</orcidid></addata></record> |
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| subjects | Applied and Technical Physics Astronomical models Atomic Cold dark matter Complex Systems Condensed Matter Physics Dark energy Equations of state Fractal models Fractals Holography Mathematical and Computational Physics Molecular Optical and Plasma Physics Parameters Physics Physics and Astronomy Regular Article Theoretical Universe |
| title | Tsallis, Rényi and Sharma-Mittal holographic and new agegraphic dark energy models in D-dimensional fractal universe |
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