GUP corrected Casimir wormholes in f(Q) gravity
We have systematically presented the effect of the generalized uncertainty principle (GUP) in Casimir wormhole space-time in the recently proposed modified gravity, the so-called symmetric teleparallel gravity, or f ( Q ) gravity. We consider two famous GUP models, such as the Kempf, Mangano, and Ma...
Gespeichert in:
Veröffentlicht in: | General relativity and gravitation 2023-08, Vol.55 (8), Article 90 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 8 |
container_start_page | |
container_title | General relativity and gravitation |
container_volume | 55 |
creator | Hassan, Zinnat Ghosh, Sayantan Sahoo, P. K. Rao, V. Sree Hari |
description | We have systematically presented the effect of the generalized uncertainty principle (GUP) in Casimir wormhole space-time in the recently proposed modified gravity, the so-called symmetric teleparallel gravity, or
f
(
Q
) gravity. We consider two famous GUP models, such as the Kempf, Mangano, and Mann (KMM) model and the Detournay, Gabriel, and Spindel (DGS) model, in this study. Also, to find the solutions, we assumed two different
f
(
Q
) forms and obtained analytic as well as numerical solutions under the effect of GUP. Besides this, we investigate the solutions with three different redshift functions under an anisotropic fluid located at the throat. Further, we analyzed the obtained wormhole solutions with energy conditions, especially null energy conditions at the wormhole’s throat, and encountered that some arbitrary quantity disrespects the classical energy conditions at the wormhole throat of radius
r
0
. Later, the ADM mass and the volume integral quantifier are also discussed to calculate the amount of exotic matter required near the wormhole throat. Additionally, we show the behavior of the equation of state parameters under the effect of GUP. |
doi_str_mv | 10.1007/s10714-023-03139-y |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2848983341</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2848983341</sourcerecordid><originalsourceid>FETCH-LOGICAL-c319t-8692010739e2142878af5a6447a1dd27321431668bb9e9ac36e32a7d195fc85d3</originalsourceid><addsrcrecordid>eNp9kEFLxDAQhYMoWFf_gKeCFz3EzWTSJjnK4q7CggruOWTbdO2ybdekq_TfG63gzdMww3tvHh8hl8BugTE5DcAkCMo4UoaAmg5HJIFMcqoz5MckYYwBlZLBKTkLYRtXLXOZkOli9ZwWnfeu6F2Zzmyom9qnn51v3rqdC2ndptX1y0268faj7odzclLZXXAXv3NCVvP719kDXT4tHmd3S1og6J6qXHMWO6F2HARXUtkqs7kQ0kJZconxipDnar3WTtsCc4fcyhJ0VhUqK3FCrsbcve_eDy70ZtsdfBtfGq6E0gpRQFTxUVX4LgTvKrP3dWP9YICZbzBmBGMiGPMDxgzRhKMpRHG7cf4v-h_XFwIDY2w</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2848983341</pqid></control><display><type>article</type><title>GUP corrected Casimir wormholes in f(Q) gravity</title><source>SpringerLink</source><creator>Hassan, Zinnat ; Ghosh, Sayantan ; Sahoo, P. K. ; Rao, V. Sree Hari</creator><creatorcontrib>Hassan, Zinnat ; Ghosh, Sayantan ; Sahoo, P. K. ; Rao, V. Sree Hari</creatorcontrib><description>We have systematically presented the effect of the generalized uncertainty principle (GUP) in Casimir wormhole space-time in the recently proposed modified gravity, the so-called symmetric teleparallel gravity, or
f
(
Q
) gravity. We consider two famous GUP models, such as the Kempf, Mangano, and Mann (KMM) model and the Detournay, Gabriel, and Spindel (DGS) model, in this study. Also, to find the solutions, we assumed two different
f
(
Q
) forms and obtained analytic as well as numerical solutions under the effect of GUP. Besides this, we investigate the solutions with three different redshift functions under an anisotropic fluid located at the throat. Further, we analyzed the obtained wormhole solutions with energy conditions, especially null energy conditions at the wormhole’s throat, and encountered that some arbitrary quantity disrespects the classical energy conditions at the wormhole throat of radius
r
0
. Later, the ADM mass and the volume integral quantifier are also discussed to calculate the amount of exotic matter required near the wormhole throat. Additionally, we show the behavior of the equation of state parameters under the effect of GUP.</description><identifier>ISSN: 0001-7701</identifier><identifier>EISSN: 1572-9532</identifier><identifier>DOI: 10.1007/s10714-023-03139-y</identifier><language>eng</language><publisher>New York: Springer US</publisher><subject>Anisotropic fluids ; Astronomy ; Astrophysics and Cosmology ; Classical and Quantum Gravitation ; Differential Geometry ; Equations of state ; Gravity ; Mathematical and Computational Physics ; Physics ; Physics and Astronomy ; Quantum Physics ; Red shift ; Relativity Theory ; Theoretical ; Throats ; Uncertainty principles ; Wormholes</subject><ispartof>General relativity and gravitation, 2023-08, Vol.55 (8), Article 90</ispartof><rights>The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c319t-8692010739e2142878af5a6447a1dd27321431668bb9e9ac36e32a7d195fc85d3</citedby><cites>FETCH-LOGICAL-c319t-8692010739e2142878af5a6447a1dd27321431668bb9e9ac36e32a7d195fc85d3</cites><orcidid>0000-0002-6608-2075 ; 0000-0003-2130-8832 ; 0000-0002-3875-0849</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10714-023-03139-y$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10714-023-03139-y$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Hassan, Zinnat</creatorcontrib><creatorcontrib>Ghosh, Sayantan</creatorcontrib><creatorcontrib>Sahoo, P. K.</creatorcontrib><creatorcontrib>Rao, V. Sree Hari</creatorcontrib><title>GUP corrected Casimir wormholes in f(Q) gravity</title><title>General relativity and gravitation</title><addtitle>Gen Relativ Gravit</addtitle><description>We have systematically presented the effect of the generalized uncertainty principle (GUP) in Casimir wormhole space-time in the recently proposed modified gravity, the so-called symmetric teleparallel gravity, or
f
(
Q
) gravity. We consider two famous GUP models, such as the Kempf, Mangano, and Mann (KMM) model and the Detournay, Gabriel, and Spindel (DGS) model, in this study. Also, to find the solutions, we assumed two different
f
(
Q
) forms and obtained analytic as well as numerical solutions under the effect of GUP. Besides this, we investigate the solutions with three different redshift functions under an anisotropic fluid located at the throat. Further, we analyzed the obtained wormhole solutions with energy conditions, especially null energy conditions at the wormhole’s throat, and encountered that some arbitrary quantity disrespects the classical energy conditions at the wormhole throat of radius
r
0
. Later, the ADM mass and the volume integral quantifier are also discussed to calculate the amount of exotic matter required near the wormhole throat. Additionally, we show the behavior of the equation of state parameters under the effect of GUP.</description><subject>Anisotropic fluids</subject><subject>Astronomy</subject><subject>Astrophysics and Cosmology</subject><subject>Classical and Quantum Gravitation</subject><subject>Differential Geometry</subject><subject>Equations of state</subject><subject>Gravity</subject><subject>Mathematical and Computational Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Physics</subject><subject>Red shift</subject><subject>Relativity Theory</subject><subject>Theoretical</subject><subject>Throats</subject><subject>Uncertainty principles</subject><subject>Wormholes</subject><issn>0001-7701</issn><issn>1572-9532</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp9kEFLxDAQhYMoWFf_gKeCFz3EzWTSJjnK4q7CggruOWTbdO2ybdekq_TfG63gzdMww3tvHh8hl8BugTE5DcAkCMo4UoaAmg5HJIFMcqoz5MckYYwBlZLBKTkLYRtXLXOZkOli9ZwWnfeu6F2Zzmyom9qnn51v3rqdC2ndptX1y0268faj7odzclLZXXAXv3NCVvP719kDXT4tHmd3S1og6J6qXHMWO6F2HARXUtkqs7kQ0kJZconxipDnar3WTtsCc4fcyhJ0VhUqK3FCrsbcve_eDy70ZtsdfBtfGq6E0gpRQFTxUVX4LgTvKrP3dWP9YICZbzBmBGMiGPMDxgzRhKMpRHG7cf4v-h_XFwIDY2w</recordid><startdate>20230801</startdate><enddate>20230801</enddate><creator>Hassan, Zinnat</creator><creator>Ghosh, Sayantan</creator><creator>Sahoo, P. K.</creator><creator>Rao, V. Sree Hari</creator><general>Springer US</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-6608-2075</orcidid><orcidid>https://orcid.org/0000-0003-2130-8832</orcidid><orcidid>https://orcid.org/0000-0002-3875-0849</orcidid></search><sort><creationdate>20230801</creationdate><title>GUP corrected Casimir wormholes in f(Q) gravity</title><author>Hassan, Zinnat ; Ghosh, Sayantan ; Sahoo, P. K. ; Rao, V. Sree Hari</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c319t-8692010739e2142878af5a6447a1dd27321431668bb9e9ac36e32a7d195fc85d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Anisotropic fluids</topic><topic>Astronomy</topic><topic>Astrophysics and Cosmology</topic><topic>Classical and Quantum Gravitation</topic><topic>Differential Geometry</topic><topic>Equations of state</topic><topic>Gravity</topic><topic>Mathematical and Computational Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Physics</topic><topic>Red shift</topic><topic>Relativity Theory</topic><topic>Theoretical</topic><topic>Throats</topic><topic>Uncertainty principles</topic><topic>Wormholes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hassan, Zinnat</creatorcontrib><creatorcontrib>Ghosh, Sayantan</creatorcontrib><creatorcontrib>Sahoo, P. K.</creatorcontrib><creatorcontrib>Rao, V. Sree Hari</creatorcontrib><collection>CrossRef</collection><jtitle>General relativity and gravitation</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hassan, Zinnat</au><au>Ghosh, Sayantan</au><au>Sahoo, P. K.</au><au>Rao, V. Sree Hari</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>GUP corrected Casimir wormholes in f(Q) gravity</atitle><jtitle>General relativity and gravitation</jtitle><stitle>Gen Relativ Gravit</stitle><date>2023-08-01</date><risdate>2023</risdate><volume>55</volume><issue>8</issue><artnum>90</artnum><issn>0001-7701</issn><eissn>1572-9532</eissn><abstract>We have systematically presented the effect of the generalized uncertainty principle (GUP) in Casimir wormhole space-time in the recently proposed modified gravity, the so-called symmetric teleparallel gravity, or
f
(
Q
) gravity. We consider two famous GUP models, such as the Kempf, Mangano, and Mann (KMM) model and the Detournay, Gabriel, and Spindel (DGS) model, in this study. Also, to find the solutions, we assumed two different
f
(
Q
) forms and obtained analytic as well as numerical solutions under the effect of GUP. Besides this, we investigate the solutions with three different redshift functions under an anisotropic fluid located at the throat. Further, we analyzed the obtained wormhole solutions with energy conditions, especially null energy conditions at the wormhole’s throat, and encountered that some arbitrary quantity disrespects the classical energy conditions at the wormhole throat of radius
r
0
. Later, the ADM mass and the volume integral quantifier are also discussed to calculate the amount of exotic matter required near the wormhole throat. Additionally, we show the behavior of the equation of state parameters under the effect of GUP.</abstract><cop>New York</cop><pub>Springer US</pub><doi>10.1007/s10714-023-03139-y</doi><orcidid>https://orcid.org/0000-0002-6608-2075</orcidid><orcidid>https://orcid.org/0000-0003-2130-8832</orcidid><orcidid>https://orcid.org/0000-0002-3875-0849</orcidid></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0001-7701 |
ispartof | General relativity and gravitation, 2023-08, Vol.55 (8), Article 90 |
issn | 0001-7701 1572-9532 |
language | eng |
recordid | cdi_proquest_journals_2848983341 |
source | SpringerLink |
subjects | Anisotropic fluids Astronomy Astrophysics and Cosmology Classical and Quantum Gravitation Differential Geometry Equations of state Gravity Mathematical and Computational Physics Physics Physics and Astronomy Quantum Physics Red shift Relativity Theory Theoretical Throats Uncertainty principles Wormholes |
title | GUP corrected Casimir wormholes in f(Q) gravity |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T19%3A00%3A41IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=GUP%20corrected%20Casimir%20wormholes%20in%20f(Q)%20gravity&rft.jtitle=General%20relativity%20and%20gravitation&rft.au=Hassan,%20Zinnat&rft.date=2023-08-01&rft.volume=55&rft.issue=8&rft.artnum=90&rft.issn=0001-7701&rft.eissn=1572-9532&rft_id=info:doi/10.1007/s10714-023-03139-y&rft_dat=%3Cproquest_cross%3E2848983341%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2848983341&rft_id=info:pmid/&rfr_iscdi=true |