Flat-space holography and stress tensor of Kerr black hole

We propose a stress tensor for the Kerr black hole written in the Boyer–Lindquist coordinate. To achieve this, we use the dictionary of the Flat/CCFT correspondence and take the flat-space limit from the quasi-local stress tensor of the four-dimensional Kerr–AdS black hole. The proposed stress tenso...

Full description

Saved in:
Bibliographic Details
Published in:Physics letters. B 2016-09, Vol.760 (C), p.713-719
Main Authors: Baghchesaraei, Omid, Fareghbal, Reza, Izadi, Yousef
Format: Article
Language:English
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-c426t-83ef35b8982f6d5c2663b729605df2d72829534608e6cca2d69b13ce920070f03
cites cdi_FETCH-LOGICAL-c426t-83ef35b8982f6d5c2663b729605df2d72829534608e6cca2d69b13ce920070f03
container_end_page 719
container_issue C
container_start_page 713
container_title Physics letters. B
container_volume 760
creator Baghchesaraei, Omid
Fareghbal, Reza
Izadi, Yousef
description We propose a stress tensor for the Kerr black hole written in the Boyer–Lindquist coordinate. To achieve this, we use the dictionary of the Flat/CCFT correspondence and take the flat-space limit from the quasi-local stress tensor of the four-dimensional Kerr–AdS black hole. The proposed stress tensor yields the correct values for the mass and angular momentum of the Kerr black hole at spatial infinity. We also calculate some components of the energy momentum tensor of the three dimensional CCFT and show that they are consistent with the holographic calculation of the Kerr black hole. The calculation we present in this paper is another confirmation for the Flat/CCFT proposal.
doi_str_mv 10.1016/j.physletb.2016.07.062
format article
fullrecord <record><control><sourceid>elsevier_doaj_</sourceid><recordid>TN_cdi_doaj_primary_oai_doaj_org_article_735d2b0c78e6402e9d75b614194fc410</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0370269316304038</els_id><doaj_id>oai_doaj_org_article_735d2b0c78e6402e9d75b614194fc410</doaj_id><sourcerecordid>S0370269316304038</sourcerecordid><originalsourceid>FETCH-LOGICAL-c426t-83ef35b8982f6d5c2663b729605df2d72829534608e6cca2d69b13ce920070f03</originalsourceid><addsrcrecordid>eNqFkMFOwzAMQCMEEmPwC6g_0OIkbdJwAk0MJiZxgXOUJs7WUZYpqZD292Rs4srJsmU_24-QWwoVBSruNtVuvU8Djl3Fcl6BrECwMzKhreQlq-vmnEyASyiZUPySXKW0AQDagJiQ-_lgxjLtjMViHYawiibTCrN1RRojplSMuE0hFsEXrxhj0Q3Gfh5a8ZpceDMkvDnFKfmYP73PXsrl2_Ni9rgsbc3EWLYcPW-6VrXMC9dYJgTvJFMCGueZk6xlquG1gBaFtYY5oTrKLSoGIMEDn5LFkeuC2ehd7L9M3Otgev1bCHGlTRx7O6CWvHGsAyszqwaGysmmE7Smqva2pgeWOLJsDClF9H88CvpgU-cNJ5v6YFOD1NlmHnw4DmL-9LvHqJPtcWvR9RHtmE_p_0P8ANuff38</addsrcrecordid><sourcetype>Open Website</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Flat-space holography and stress tensor of Kerr black hole</title><source>ScienceDirect</source><source>Elsevier:Jisc Collections:Elsevier Read and Publish Agreement 2022-2024:Freedom Collection (Reading list)</source><creator>Baghchesaraei, Omid ; Fareghbal, Reza ; Izadi, Yousef</creator><creatorcontrib>Baghchesaraei, Omid ; Fareghbal, Reza ; Izadi, Yousef</creatorcontrib><description>We propose a stress tensor for the Kerr black hole written in the Boyer–Lindquist coordinate. To achieve this, we use the dictionary of the Flat/CCFT correspondence and take the flat-space limit from the quasi-local stress tensor of the four-dimensional Kerr–AdS black hole. The proposed stress tensor yields the correct values for the mass and angular momentum of the Kerr black hole at spatial infinity. We also calculate some components of the energy momentum tensor of the three dimensional CCFT and show that they are consistent with the holographic calculation of the Kerr black hole. The calculation we present in this paper is another confirmation for the Flat/CCFT proposal.</description><identifier>ISSN: 0370-2693</identifier><identifier>EISSN: 1873-2445</identifier><identifier>DOI: 10.1016/j.physletb.2016.07.062</identifier><language>eng</language><publisher>Elsevier B.V</publisher><ispartof>Physics letters. B, 2016-09, Vol.760 (C), p.713-719</ispartof><rights>2016 The Author(s)</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c426t-83ef35b8982f6d5c2663b729605df2d72829534608e6cca2d69b13ce920070f03</citedby><cites>FETCH-LOGICAL-c426t-83ef35b8982f6d5c2663b729605df2d72829534608e6cca2d69b13ce920070f03</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0370269316304038$$EHTML$$P50$$Gelsevier$$Hfree_for_read</linktohtml><link.rule.ids>314,776,780,3536,27901,27902,45756</link.rule.ids></links><search><creatorcontrib>Baghchesaraei, Omid</creatorcontrib><creatorcontrib>Fareghbal, Reza</creatorcontrib><creatorcontrib>Izadi, Yousef</creatorcontrib><title>Flat-space holography and stress tensor of Kerr black hole</title><title>Physics letters. B</title><description>We propose a stress tensor for the Kerr black hole written in the Boyer–Lindquist coordinate. To achieve this, we use the dictionary of the Flat/CCFT correspondence and take the flat-space limit from the quasi-local stress tensor of the four-dimensional Kerr–AdS black hole. The proposed stress tensor yields the correct values for the mass and angular momentum of the Kerr black hole at spatial infinity. We also calculate some components of the energy momentum tensor of the three dimensional CCFT and show that they are consistent with the holographic calculation of the Kerr black hole. The calculation we present in this paper is another confirmation for the Flat/CCFT proposal.</description><issn>0370-2693</issn><issn>1873-2445</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>DOA</sourceid><recordid>eNqFkMFOwzAMQCMEEmPwC6g_0OIkbdJwAk0MJiZxgXOUJs7WUZYpqZD292Rs4srJsmU_24-QWwoVBSruNtVuvU8Djl3Fcl6BrECwMzKhreQlq-vmnEyASyiZUPySXKW0AQDagJiQ-_lgxjLtjMViHYawiibTCrN1RRojplSMuE0hFsEXrxhj0Q3Gfh5a8ZpceDMkvDnFKfmYP73PXsrl2_Ni9rgsbc3EWLYcPW-6VrXMC9dYJgTvJFMCGueZk6xlquG1gBaFtYY5oTrKLSoGIMEDn5LFkeuC2ehd7L9M3Otgev1bCHGlTRx7O6CWvHGsAyszqwaGysmmE7Smqva2pgeWOLJsDClF9H88CvpgU-cNJ5v6YFOD1NlmHnw4DmL-9LvHqJPtcWvR9RHtmE_p_0P8ANuff38</recordid><startdate>20160910</startdate><enddate>20160910</enddate><creator>Baghchesaraei, Omid</creator><creator>Fareghbal, Reza</creator><creator>Izadi, Yousef</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>6I.</scope><scope>AAFTH</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>DOA</scope></search><sort><creationdate>20160910</creationdate><title>Flat-space holography and stress tensor of Kerr black hole</title><author>Baghchesaraei, Omid ; Fareghbal, Reza ; Izadi, Yousef</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c426t-83ef35b8982f6d5c2663b729605df2d72829534608e6cca2d69b13ce920070f03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Baghchesaraei, Omid</creatorcontrib><creatorcontrib>Fareghbal, Reza</creatorcontrib><creatorcontrib>Izadi, Yousef</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>CrossRef</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>Physics letters. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Baghchesaraei, Omid</au><au>Fareghbal, Reza</au><au>Izadi, Yousef</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Flat-space holography and stress tensor of Kerr black hole</atitle><jtitle>Physics letters. B</jtitle><date>2016-09-10</date><risdate>2016</risdate><volume>760</volume><issue>C</issue><spage>713</spage><epage>719</epage><pages>713-719</pages><issn>0370-2693</issn><eissn>1873-2445</eissn><abstract>We propose a stress tensor for the Kerr black hole written in the Boyer–Lindquist coordinate. To achieve this, we use the dictionary of the Flat/CCFT correspondence and take the flat-space limit from the quasi-local stress tensor of the four-dimensional Kerr–AdS black hole. The proposed stress tensor yields the correct values for the mass and angular momentum of the Kerr black hole at spatial infinity. We also calculate some components of the energy momentum tensor of the three dimensional CCFT and show that they are consistent with the holographic calculation of the Kerr black hole. The calculation we present in this paper is another confirmation for the Flat/CCFT proposal.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.physletb.2016.07.062</doi><tpages>7</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0370-2693
ispartof Physics letters. B, 2016-09, Vol.760 (C), p.713-719
issn 0370-2693
1873-2445
language eng
recordid cdi_doaj_primary_oai_doaj_org_article_735d2b0c78e6402e9d75b614194fc410
source ScienceDirect; Elsevier:Jisc Collections:Elsevier Read and Publish Agreement 2022-2024:Freedom Collection (Reading list)
title Flat-space holography and stress tensor of Kerr black hole
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-04T09%3A38%3A52IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-elsevier_doaj_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Flat-space%20holography%20and%20stress%20tensor%20of%20Kerr%20black%20hole&rft.jtitle=Physics%20letters.%20B&rft.au=Baghchesaraei,%20Omid&rft.date=2016-09-10&rft.volume=760&rft.issue=C&rft.spage=713&rft.epage=719&rft.pages=713-719&rft.issn=0370-2693&rft.eissn=1873-2445&rft_id=info:doi/10.1016/j.physletb.2016.07.062&rft_dat=%3Celsevier_doaj_%3ES0370269316304038%3C/elsevier_doaj_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c426t-83ef35b8982f6d5c2663b729605df2d72829534608e6cca2d69b13ce920070f03%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true