Stability of charged thin-shell gravastars with quintessence

This paper develops a new solution of gravitational vacuum star in the background of charged Kiselev black holes as an exterior manifold. We explore physical features and stability of thin-shell gravastars with radial perturbation. The matter thin layer located at thin-shell greatly affects stable c...

Full description

Saved in:
Bibliographic Details
Published in:The European physical journal. C, Particles and fields Particles and fields, 2021, Vol.81 (1), p.1-11, Article 47
Main Authors: Sharif, M., Javed, Faisal
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics and Cosmology
Chaplygin gas
Configurations
Elementary Particles
Equations of state
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Perturbation
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article – Theoretical Physics
Shell stability
Shells
String Theory
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c522t-867772630a6afea57457d6fb80937f69540686a9dd3559cd02c06042126e24293
cites cdi_FETCH-LOGICAL-c522t-867772630a6afea57457d6fb80937f69540686a9dd3559cd02c06042126e24293
container_end_page 11
container_issue 1
container_start_page 1
container_title The European physical journal. C, Particles and fields
container_volume 81
creator Sharif, M.
Javed, Faisal
description This paper develops a new solution of gravitational vacuum star in the background of charged Kiselev black holes as an exterior manifold. We explore physical features and stability of thin-shell gravastars with radial perturbation. The matter thin layer located at thin-shell greatly affects stable configuration of the developed structure. We assume three different choices of matter distribution such as barotropic, generalized Chaplygin gas and generalized phantomlike equation of state. The last two models depend on the shell radius, also known as variable equation of state. For barotropic model, the structure of thin-shell gravastar is mostly unstable while it shows stable configuration for such type of matter distribution with extraordinary quintessence parameter. The resulting gravastar structure indicates stable behavior for generalized Chaplygin gas but unstable for generalized phantomlike model. It is also found that proper length, entropy and energy within the shell show linear relation with thickness of the shell.
doi_str_mv 10.1140/epjc/s10052-020-08802-1
format article
fullrecord <record><control><sourceid>gale_doaj_</sourceid><recordid>TN_cdi_doaj_primary_oai_doaj_org_article_7dfed2c953d14263846842aad76b01b6</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><galeid>A650882257</galeid><doaj_id>oai_doaj_org_article_7dfed2c953d14263846842aad76b01b6</doaj_id><sourcerecordid>A650882257</sourcerecordid><originalsourceid>FETCH-LOGICAL-c522t-867772630a6afea57457d6fb80937f69540686a9dd3559cd02c06042126e24293</originalsourceid><addsrcrecordid>eNqFkVtrFTEUhQdRsFZ_gwM--TDtzp7cBnwpxcuBgmD1OeyTy5wcpjOnSY7af2_akUqfJA8Ji2-t7GQ1zVsGZ4xxOPeHvT3PDEBgBwgdaA3YsWfNCeM972TVnz-eOX_ZvMp5DwDIQZ80H64LbeMUy127hNbuKI3etWUX5y7v_DS1Y6KflAul3P6KZdfeHuNcfM5-tv518yLQlP2bv_tp8-PTx--XX7qrr583lxdXnRWIpdNSKYWyB5IUPAnFhXIybDUMvQpyEBykljQ41wsxWAdooY6KDKVHjkN_2mzWXLfQ3hxSvKF0ZxaK5kFY0mgolWgnb5QL3qEdRO8Yr3dqLjVHIqfkFthW1qx3a9YhLbdHn4vZL8c01_ENcqV1xTVW6mylRqqhcQ5LSWTrcv4m2mX2IVb9Qor624hCVcP7J4bKFP-7jHTM2Wyuvz1l1cratOScfHh8EgNz36m579SsnZraqXno1LDq1KszV8c8-vRv-P9Z_wAOBaRa</addsrcrecordid><sourcetype>Open Website</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2478868482</pqid></control><display><type>article</type><title>Stability of charged thin-shell gravastars with quintessence</title><source>Springer Nature - SpringerLink Journals - Fully Open Access </source><source>ProQuest - Publicly Available Content Database</source><creator>Sharif, M. ; Javed, Faisal</creator><creatorcontrib>Sharif, M. ; Javed, Faisal</creatorcontrib><description>This paper develops a new solution of gravitational vacuum star in the background of charged Kiselev black holes as an exterior manifold. We explore physical features and stability of thin-shell gravastars with radial perturbation. The matter thin layer located at thin-shell greatly affects stable configuration of the developed structure. We assume three different choices of matter distribution such as barotropic, generalized Chaplygin gas and generalized phantomlike equation of state. The last two models depend on the shell radius, also known as variable equation of state. For barotropic model, the structure of thin-shell gravastar is mostly unstable while it shows stable configuration for such type of matter distribution with extraordinary quintessence parameter. The resulting gravastar structure indicates stable behavior for generalized Chaplygin gas but unstable for generalized phantomlike model. It is also found that proper length, entropy and energy within the shell show linear relation with thickness of the shell.</description><identifier>ISSN: 1434-6044</identifier><identifier>EISSN: 1434-6052</identifier><identifier>DOI: 10.1140/epjc/s10052-020-08802-1</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Astronomy ; Astrophysics and Cosmology ; Chaplygin gas ; Configurations ; Elementary Particles ; Equations of state ; Hadrons ; Heavy Ions ; Measurement Science and Instrumentation ; Nuclear Energy ; Nuclear Physics ; Perturbation ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Regular Article – Theoretical Physics ; Shell stability ; Shells ; String Theory</subject><ispartof>The European physical journal. C, Particles and fields, 2021, Vol.81 (1), p.1-11, Article 47</ispartof><rights>The Author(s) 2021</rights><rights>COPYRIGHT 2021 Springer</rights><rights>The Author(s) 2021. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c522t-867772630a6afea57457d6fb80937f69540686a9dd3559cd02c06042126e24293</citedby><cites>FETCH-LOGICAL-c522t-867772630a6afea57457d6fb80937f69540686a9dd3559cd02c06042126e24293</cites><orcidid>0000-0001-6845-3506</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/2478868482/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/2478868482?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25753,27924,27925,37012,44590,75126</link.rule.ids></links><search><creatorcontrib>Sharif, M.</creatorcontrib><creatorcontrib>Javed, Faisal</creatorcontrib><title>Stability of charged thin-shell gravastars with quintessence</title><title>The European physical journal. C, Particles and fields</title><addtitle>Eur. Phys. J. C</addtitle><description>This paper develops a new solution of gravitational vacuum star in the background of charged Kiselev black holes as an exterior manifold. We explore physical features and stability of thin-shell gravastars with radial perturbation. The matter thin layer located at thin-shell greatly affects stable configuration of the developed structure. We assume three different choices of matter distribution such as barotropic, generalized Chaplygin gas and generalized phantomlike equation of state. The last two models depend on the shell radius, also known as variable equation of state. For barotropic model, the structure of thin-shell gravastar is mostly unstable while it shows stable configuration for such type of matter distribution with extraordinary quintessence parameter. The resulting gravastar structure indicates stable behavior for generalized Chaplygin gas but unstable for generalized phantomlike model. It is also found that proper length, entropy and energy within the shell show linear relation with thickness of the shell.</description><subject>Astronomy</subject><subject>Astrophysics and Cosmology</subject><subject>Chaplygin gas</subject><subject>Configurations</subject><subject>Elementary Particles</subject><subject>Equations of state</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Measurement Science and Instrumentation</subject><subject>Nuclear Energy</subject><subject>Nuclear Physics</subject><subject>Perturbation</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Regular Article – Theoretical Physics</subject><subject>Shell stability</subject><subject>Shells</subject><subject>String Theory</subject><issn>1434-6044</issn><issn>1434-6052</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNqFkVtrFTEUhQdRsFZ_gwM--TDtzp7cBnwpxcuBgmD1OeyTy5wcpjOnSY7af2_akUqfJA8Ji2-t7GQ1zVsGZ4xxOPeHvT3PDEBgBwgdaA3YsWfNCeM972TVnz-eOX_ZvMp5DwDIQZ80H64LbeMUy127hNbuKI3etWUX5y7v_DS1Y6KflAul3P6KZdfeHuNcfM5-tv518yLQlP2bv_tp8-PTx--XX7qrr583lxdXnRWIpdNSKYWyB5IUPAnFhXIybDUMvQpyEBykljQ41wsxWAdooY6KDKVHjkN_2mzWXLfQ3hxSvKF0ZxaK5kFY0mgolWgnb5QL3qEdRO8Yr3dqLjVHIqfkFthW1qx3a9YhLbdHn4vZL8c01_ENcqV1xTVW6mylRqqhcQ5LSWTrcv4m2mX2IVb9Qor624hCVcP7J4bKFP-7jHTM2Wyuvz1l1cratOScfHh8EgNz36m579SsnZraqXno1LDq1KszV8c8-vRv-P9Z_wAOBaRa</recordid><startdate>2021</startdate><enddate>2021</enddate><creator>Sharif, M.</creator><creator>Javed, Faisal</creator><general>Springer Berlin Heidelberg</general><general>Springer</general><general>Springer Nature B.V</general><general>SpringerOpen</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>ISR</scope><scope>7U5</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0001-6845-3506</orcidid></search><sort><creationdate>2021</creationdate><title>Stability of charged thin-shell gravastars with quintessence</title><author>Sharif, M. ; Javed, Faisal</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c522t-867772630a6afea57457d6fb80937f69540686a9dd3559cd02c06042126e24293</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Astronomy</topic><topic>Astrophysics and Cosmology</topic><topic>Chaplygin gas</topic><topic>Configurations</topic><topic>Elementary Particles</topic><topic>Equations of state</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Measurement Science and Instrumentation</topic><topic>Nuclear Energy</topic><topic>Nuclear Physics</topic><topic>Perturbation</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Regular Article – Theoretical Physics</topic><topic>Shell stability</topic><topic>Shells</topic><topic>String Theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sharif, M.</creatorcontrib><creatorcontrib>Javed, Faisal</creatorcontrib><collection>Springer_OA刊</collection><collection>CrossRef</collection><collection>Gale In Context: Science</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest advanced technologies &amp; aerospace journals</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest - Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Directory of Open Access Journals (DOAJ)</collection><jtitle>The European physical journal. C, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sharif, M.</au><au>Javed, Faisal</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Stability of charged thin-shell gravastars with quintessence</atitle><jtitle>The European physical journal. C, Particles and fields</jtitle><stitle>Eur. Phys. J. C</stitle><date>2021</date><risdate>2021</risdate><volume>81</volume><issue>1</issue><spage>1</spage><epage>11</epage><pages>1-11</pages><artnum>47</artnum><issn>1434-6044</issn><eissn>1434-6052</eissn><abstract>This paper develops a new solution of gravitational vacuum star in the background of charged Kiselev black holes as an exterior manifold. We explore physical features and stability of thin-shell gravastars with radial perturbation. The matter thin layer located at thin-shell greatly affects stable configuration of the developed structure. We assume three different choices of matter distribution such as barotropic, generalized Chaplygin gas and generalized phantomlike equation of state. The last two models depend on the shell radius, also known as variable equation of state. For barotropic model, the structure of thin-shell gravastar is mostly unstable while it shows stable configuration for such type of matter distribution with extraordinary quintessence parameter. The resulting gravastar structure indicates stable behavior for generalized Chaplygin gas but unstable for generalized phantomlike model. It is also found that proper length, entropy and energy within the shell show linear relation with thickness of the shell.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1140/epjc/s10052-020-08802-1</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0001-6845-3506</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1434-6044
ispartof The European physical journal. C, Particles and fields, 2021, Vol.81 (1), p.1-11, Article 47
issn 1434-6044
1434-6052
language eng
recordid cdi_doaj_primary_oai_doaj_org_article_7dfed2c953d14263846842aad76b01b6
source Springer Nature - SpringerLink Journals - Fully Open Access ; ProQuest - Publicly Available Content Database
subjects Astronomy
Astrophysics and Cosmology
Chaplygin gas
Configurations
Elementary Particles
Equations of state
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Perturbation
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article – Theoretical Physics
Shell stability
Shells
String Theory
title Stability of charged thin-shell gravastars with quintessence
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-27T07%3A18%3A33IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-gale_doaj_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Stability%20of%20charged%20thin-shell%20gravastars%20with%20quintessence&rft.jtitle=The%20European%20physical%20journal.%20C,%20Particles%20and%20fields&rft.au=Sharif,%20M.&rft.date=2021&rft.volume=81&rft.issue=1&rft.spage=1&rft.epage=11&rft.pages=1-11&rft.artnum=47&rft.issn=1434-6044&rft.eissn=1434-6052&rft_id=info:doi/10.1140/epjc/s10052-020-08802-1&rft_dat=%3Cgale_doaj_%3EA650882257%3C/gale_doaj_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c522t-867772630a6afea57457d6fb80937f69540686a9dd3559cd02c06042126e24293%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2478868482&rft_id=info:pmid/&rft_galeid=A650882257&rfr_iscdi=true