Anisotropic holographic dark energy model in Bianchi type-VI sub(0) universe in a scalar-tensor theory of gravitation
In this paper, we investigate Bianchi type VI sub(0) universe filled with two minimally interacting fields, matter and anisotropic holographic dark energy components in the scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113: 467, 1986). Solving the field equations...
Gespeichert in:
| Veröffentlicht in: | Astrophysics and space science 2016-10, Vol.361 (10), p.1-7 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 7 |
|---|---|
| container_issue | 10 |
| container_start_page | 1 |
| container_title | Astrophysics and space science |
| container_volume | 361 |
| creator | Reddy, DRK Anitha, S Umadevi, S |
| description | In this paper, we investigate Bianchi type VI sub(0) universe filled with two minimally interacting fields, matter and anisotropic holographic dark energy components in the scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113: 467, 1986). Solving the field equations of the theory using a relation between metric potentials and special law of variation for Hubble's parameter proposed by Bermann (Nuovo Cimento B 74:182, 1983) we have presented an anisotropic holographic dark energy model in this theory. The physical aspects of the model are also discussed. |
| doi_str_mv | 10.1007/s10509-016-2942-6 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_miscellaneous_1845818100</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1827928485</sourcerecordid><originalsourceid>FETCH-LOGICAL-p660-3ddc7c2e8bbf8ae92fb271517a4d2f0b8e1f0913340b1467605f23118b8785b3</originalsourceid><addsrcrecordid>eNqNkLtOwzAYhS0EEqXwAGwey2D47Ti-jKXiUqkSAwh1q-zEaQ2pHeykUt-eIHgApnOO9OkbDkLXFG4pgLzLFErQBKggTHNGxAma0FIyorlYn6IJAHAiOKzP0UXOH-PUQssJGubB59in2PkK72Ibt8l0u7HXJn1iF1zaHvE-1q7FPuB7b0K187g_do68L3Ee7Axu8BD8waXsfhCDc2Vak0jvQo4J9zsX0xHHBo_mg-9N72O4RGeNabO7-sspen18eFs8k9XL03IxX5FOCCBFXVeyYk5Z2yjjNGssk7Sk0vCaNWCVow1oWhQcLOVCCigbVlCqrJKqtMUUzX6tXYpfg8v9Zu9z5drWBBeHvKGKl4qq8b9_oExqprgqi28flG21</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1827928485</pqid></control><display><type>article</type><title>Anisotropic holographic dark energy model in Bianchi type-VI sub(0) universe in a scalar-tensor theory of gravitation</title><source>SpringerLink E-Journals</source><creator>Reddy, DRK ; Anitha, S ; Umadevi, S</creator><creatorcontrib>Reddy, DRK ; Anitha, S ; Umadevi, S</creatorcontrib><description>In this paper, we investigate Bianchi type VI sub(0) universe filled with two minimally interacting fields, matter and anisotropic holographic dark energy components in the scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113: 467, 1986). Solving the field equations of the theory using a relation between metric potentials and special law of variation for Hubble's parameter proposed by Bermann (Nuovo Cimento B 74:182, 1983) we have presented an anisotropic holographic dark energy model in this theory. The physical aspects of the model are also discussed.</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1007/s10509-016-2942-6</identifier><language>eng</language><subject>Anisotropy ; Astrophysics ; Dark energy ; Gravitation ; Mathematical analysis ; Mathematical models ; Parameters ; Universe</subject><ispartof>Astrophysics and space science, 2016-10, Vol.361 (10), p.1-7</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Reddy, DRK</creatorcontrib><creatorcontrib>Anitha, S</creatorcontrib><creatorcontrib>Umadevi, S</creatorcontrib><title>Anisotropic holographic dark energy model in Bianchi type-VI sub(0) universe in a scalar-tensor theory of gravitation</title><title>Astrophysics and space science</title><description>In this paper, we investigate Bianchi type VI sub(0) universe filled with two minimally interacting fields, matter and anisotropic holographic dark energy components in the scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113: 467, 1986). Solving the field equations of the theory using a relation between metric potentials and special law of variation for Hubble's parameter proposed by Bermann (Nuovo Cimento B 74:182, 1983) we have presented an anisotropic holographic dark energy model in this theory. The physical aspects of the model are also discussed.</description><subject>Anisotropy</subject><subject>Astrophysics</subject><subject>Dark energy</subject><subject>Gravitation</subject><subject>Mathematical analysis</subject><subject>Mathematical models</subject><subject>Parameters</subject><subject>Universe</subject><issn>0004-640X</issn><issn>1572-946X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNqNkLtOwzAYhS0EEqXwAGwey2D47Ti-jKXiUqkSAwh1q-zEaQ2pHeykUt-eIHgApnOO9OkbDkLXFG4pgLzLFErQBKggTHNGxAma0FIyorlYn6IJAHAiOKzP0UXOH-PUQssJGubB59in2PkK72Ibt8l0u7HXJn1iF1zaHvE-1q7FPuB7b0K187g_do68L3Ee7Axu8BD8waXsfhCDc2Vak0jvQo4J9zsX0xHHBo_mg-9N72O4RGeNabO7-sspen18eFs8k9XL03IxX5FOCCBFXVeyYk5Z2yjjNGssk7Sk0vCaNWCVow1oWhQcLOVCCigbVlCqrJKqtMUUzX6tXYpfg8v9Zu9z5drWBBeHvKGKl4qq8b9_oExqprgqi28flG21</recordid><startdate>20161001</startdate><enddate>20161001</enddate><creator>Reddy, DRK</creator><creator>Anitha, S</creator><creator>Umadevi, S</creator><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20161001</creationdate><title>Anisotropic holographic dark energy model in Bianchi type-VI sub(0) universe in a scalar-tensor theory of gravitation</title><author>Reddy, DRK ; Anitha, S ; Umadevi, S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p660-3ddc7c2e8bbf8ae92fb271517a4d2f0b8e1f0913340b1467605f23118b8785b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Anisotropy</topic><topic>Astrophysics</topic><topic>Dark energy</topic><topic>Gravitation</topic><topic>Mathematical analysis</topic><topic>Mathematical models</topic><topic>Parameters</topic><topic>Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Reddy, DRK</creatorcontrib><creatorcontrib>Anitha, S</creatorcontrib><creatorcontrib>Umadevi, S</creatorcontrib><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Reddy, DRK</au><au>Anitha, S</au><au>Umadevi, S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Anisotropic holographic dark energy model in Bianchi type-VI sub(0) universe in a scalar-tensor theory of gravitation</atitle><jtitle>Astrophysics and space science</jtitle><date>2016-10-01</date><risdate>2016</risdate><volume>361</volume><issue>10</issue><spage>1</spage><epage>7</epage><pages>1-7</pages><issn>0004-640X</issn><eissn>1572-946X</eissn><abstract>In this paper, we investigate Bianchi type VI sub(0) universe filled with two minimally interacting fields, matter and anisotropic holographic dark energy components in the scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113: 467, 1986). Solving the field equations of the theory using a relation between metric potentials and special law of variation for Hubble's parameter proposed by Bermann (Nuovo Cimento B 74:182, 1983) we have presented an anisotropic holographic dark energy model in this theory. The physical aspects of the model are also discussed.</abstract><doi>10.1007/s10509-016-2942-6</doi><tpages>7</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-640X |
| ispartof | Astrophysics and space science, 2016-10, Vol.361 (10), p.1-7 |
| issn | 0004-640X 1572-946X |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1845818100 |
| source | SpringerLink E-Journals |
| subjects | Anisotropy Astrophysics Dark energy Gravitation Mathematical analysis Mathematical models Parameters Universe |
| title | Anisotropic holographic dark energy model in Bianchi type-VI sub(0) universe in a scalar-tensor theory of gravitation |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-24T20%3A08%3A36IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Anisotropic%20holographic%20dark%20energy%20model%20in%20Bianchi%20type-VI%20sub(0)%20universe%20in%20a%20scalar-tensor%20theory%20of%20gravitation&rft.jtitle=Astrophysics%20and%20space%20science&rft.au=Reddy,%20DRK&rft.date=2016-10-01&rft.volume=361&rft.issue=10&rft.spage=1&rft.epage=7&rft.pages=1-7&rft.issn=0004-640X&rft.eissn=1572-946X&rft_id=info:doi/10.1007/s10509-016-2942-6&rft_dat=%3Cproquest%3E1827928485%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1827928485&rft_id=info:pmid/&rfr_iscdi=true |