Jeans analysis with κ-deformed Kaniadakis distribution in f (R) gravity

The influence of the κ -deformed Kaniadakis distribution on Jeans instability in the background of f R gravity is investigated, the dispersion relation considering the κ -deformed Kaniadakis distribution is derived by exploiting the kinetic theory. The cases of high and low frequency perturbations a...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physica scripta 2022-02, Vol.97 (2), p.25601
1. Verfasser: He, Ke-Rong
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 2
container_start_page 25601
container_title Physica scripta
container_volume 97
creator He, Ke-Rong
description The influence of the κ -deformed Kaniadakis distribution on Jeans instability in the background of f R gravity is investigated, the dispersion relation considering the κ -deformed Kaniadakis distribution is derived by exploiting the kinetic theory. The cases of high and low frequency perturbations are analyzed, respectively, it is found that the range of the unstable modes and the growth rates decrease with the increased distribution index κ in both of high and low frequency regime. Finally, based on the derivation of effective temperature, the relation between Jeans mass and temperature is studied, it is found that lower Jeans mass means that the system is more likely to collapse due to gravitational instability, the system is unstable for lower distribution index κ .
doi_str_mv 10.1088/1402-4896/ac485e
format Article
fullrecord <record><control><sourceid>iop_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1088_1402_4896_ac485e</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>psac485e</sourcerecordid><originalsourceid>FETCH-LOGICAL-c311t-8ed1350021fa7244b0b70765a3df20aa4ad8c592feb1e51a9689fb517383a453</originalsourceid><addsrcrecordid>eNp1kM1KAzEUhYMoWKt7l1mJgmPzO5MspahVC4J0H-5MEk1tZ4ZkqvTVfAifyRkqrnR14d5zzuU7CJ1SckWJUhMqCMuE0vkEKqGk20Oj39U-GhHCaaa00IfoKKUlISxnuR6h2YODOmGoYbVNIeGP0L3ir8_MOt_EtbP4EeoAFt76mw2pi6HcdKGpcaixx-fPF_glwnvotsfowMMquZOfOUaL25vFdJbNn-7up9fzrOKUdplylnLZv6ceCiZEScqCFLkEbj0jAAKsqqRm3pXUSQo6V9qXkhZccRCSjxHZxVaxSSk6b9oY1hC3hhIzFGEGajNQm10RveVsZwlNa5bNJvasybTJ6MIwQ5jMCTWt9b3w8g_hv7nf1dBsFQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Jeans analysis with κ-deformed Kaniadakis distribution in f (R) gravity</title><source>IOP Publishing Journals</source><source>Institute of Physics (IOP) Journals - HEAL-Link</source><creator>He, Ke-Rong</creator><creatorcontrib>He, Ke-Rong</creatorcontrib><description>The influence of the κ -deformed Kaniadakis distribution on Jeans instability in the background of f R gravity is investigated, the dispersion relation considering the κ -deformed Kaniadakis distribution is derived by exploiting the kinetic theory. The cases of high and low frequency perturbations are analyzed, respectively, it is found that the range of the unstable modes and the growth rates decrease with the increased distribution index κ in both of high and low frequency regime. Finally, based on the derivation of effective temperature, the relation between Jeans mass and temperature is studied, it is found that lower Jeans mass means that the system is more likely to collapse due to gravitational instability, the system is unstable for lower distribution index κ .</description><identifier>ISSN: 0031-8949</identifier><identifier>EISSN: 1402-4896</identifier><identifier>DOI: 10.1088/1402-4896/ac485e</identifier><identifier>CODEN: PHSTBO</identifier><language>eng</language><publisher>IOP Publishing</publisher><subject>deformed Kaniadakis distribution ; gravity ; Jeans instability</subject><ispartof>Physica scripta, 2022-02, Vol.97 (2), p.25601</ispartof><rights>2022 IOP Publishing Ltd</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c311t-8ed1350021fa7244b0b70765a3df20aa4ad8c592feb1e51a9689fb517383a453</citedby><cites>FETCH-LOGICAL-c311t-8ed1350021fa7244b0b70765a3df20aa4ad8c592feb1e51a9689fb517383a453</cites><orcidid>0000-0002-9842-2345</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1402-4896/ac485e/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,778,782,27907,27908,53829,53876</link.rule.ids></links><search><creatorcontrib>He, Ke-Rong</creatorcontrib><title>Jeans analysis with κ-deformed Kaniadakis distribution in f (R) gravity</title><title>Physica scripta</title><addtitle>PS</addtitle><addtitle>Phys. Scr</addtitle><description>The influence of the κ -deformed Kaniadakis distribution on Jeans instability in the background of f R gravity is investigated, the dispersion relation considering the κ -deformed Kaniadakis distribution is derived by exploiting the kinetic theory. The cases of high and low frequency perturbations are analyzed, respectively, it is found that the range of the unstable modes and the growth rates decrease with the increased distribution index κ in both of high and low frequency regime. Finally, based on the derivation of effective temperature, the relation between Jeans mass and temperature is studied, it is found that lower Jeans mass means that the system is more likely to collapse due to gravitational instability, the system is unstable for lower distribution index κ .</description><subject>deformed Kaniadakis distribution</subject><subject>gravity</subject><subject>Jeans instability</subject><issn>0031-8949</issn><issn>1402-4896</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp1kM1KAzEUhYMoWKt7l1mJgmPzO5MspahVC4J0H-5MEk1tZ4ZkqvTVfAifyRkqrnR14d5zzuU7CJ1SckWJUhMqCMuE0vkEKqGk20Oj39U-GhHCaaa00IfoKKUlISxnuR6h2YODOmGoYbVNIeGP0L3ir8_MOt_EtbP4EeoAFt76mw2pi6HcdKGpcaixx-fPF_glwnvotsfowMMquZOfOUaL25vFdJbNn-7up9fzrOKUdplylnLZv6ceCiZEScqCFLkEbj0jAAKsqqRm3pXUSQo6V9qXkhZccRCSjxHZxVaxSSk6b9oY1hC3hhIzFGEGajNQm10RveVsZwlNa5bNJvasybTJ6MIwQ5jMCTWt9b3w8g_hv7nf1dBsFQ</recordid><startdate>20220201</startdate><enddate>20220201</enddate><creator>He, Ke-Rong</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-9842-2345</orcidid></search><sort><creationdate>20220201</creationdate><title>Jeans analysis with κ-deformed Kaniadakis distribution in f (R) gravity</title><author>He, Ke-Rong</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c311t-8ed1350021fa7244b0b70765a3df20aa4ad8c592feb1e51a9689fb517383a453</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>deformed Kaniadakis distribution</topic><topic>gravity</topic><topic>Jeans instability</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>He, Ke-Rong</creatorcontrib><collection>CrossRef</collection><jtitle>Physica scripta</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>He, Ke-Rong</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Jeans analysis with κ-deformed Kaniadakis distribution in f (R) gravity</atitle><jtitle>Physica scripta</jtitle><stitle>PS</stitle><addtitle>Phys. Scr</addtitle><date>2022-02-01</date><risdate>2022</risdate><volume>97</volume><issue>2</issue><spage>25601</spage><pages>25601-</pages><issn>0031-8949</issn><eissn>1402-4896</eissn><coden>PHSTBO</coden><abstract>The influence of the κ -deformed Kaniadakis distribution on Jeans instability in the background of f R gravity is investigated, the dispersion relation considering the κ -deformed Kaniadakis distribution is derived by exploiting the kinetic theory. The cases of high and low frequency perturbations are analyzed, respectively, it is found that the range of the unstable modes and the growth rates decrease with the increased distribution index κ in both of high and low frequency regime. Finally, based on the derivation of effective temperature, the relation between Jeans mass and temperature is studied, it is found that lower Jeans mass means that the system is more likely to collapse due to gravitational instability, the system is unstable for lower distribution index κ .</abstract><pub>IOP Publishing</pub><doi>10.1088/1402-4896/ac485e</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0002-9842-2345</orcidid></addata></record>
fulltext fulltext
identifier ISSN: 0031-8949
ispartof Physica scripta, 2022-02, Vol.97 (2), p.25601
issn 0031-8949
1402-4896
language eng
recordid cdi_crossref_primary_10_1088_1402_4896_ac485e
source IOP Publishing Journals; Institute of Physics (IOP) Journals - HEAL-Link
subjects deformed Kaniadakis distribution
gravity
Jeans instability
title Jeans analysis with κ-deformed Kaniadakis distribution in f (R) gravity
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-16T13%3A42%3A34IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-iop_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Jeans%20analysis%20with%20%CE%BA-deformed%20Kaniadakis%20distribution%20in%20f%20(R)%20gravity&rft.jtitle=Physica%20scripta&rft.au=He,%20Ke-Rong&rft.date=2022-02-01&rft.volume=97&rft.issue=2&rft.spage=25601&rft.pages=25601-&rft.issn=0031-8949&rft.eissn=1402-4896&rft.coden=PHSTBO&rft_id=info:doi/10.1088/1402-4896/ac485e&rft_dat=%3Ciop_cross%3Epsac485e%3C/iop_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true