No Cover Image

Journal article 611 views 97 downloads

Holographic entanglement entropy of the Coulomb branch

Adam Chalabi, Prem Kumar Orcid Logo, Andy O’Bannon, Anton Pribytok, Ronnie Rodgers, Jacopo Sisti

Journal of High Energy Physics, Volume: 2021, Issue: 4

Swansea University Author: Prem Kumar Orcid Logo

  • Chalabi2021_Article_HolographicEntanglementEntropy.pdf

    PDF | Version of Record

    ©The Authors. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0)

    Download (1.48MB)

Abstract

We compute entanglement entropy (EE) of a spherical region in (3 + 1)- dimensional N = 4 supersymmetric SU(N) Yang-Mills theory in states described holographically by probe D3-branes in AdS5 × S5. We do so by generalising methods for computing EE from a probe brane action without having to determine...

Full description

Published in: Journal of High Energy Physics
ISSN: 1029-8479
Published: Springer Science and Business Media LLC 2021
Online Access: Check full text

URI: https://cronfa.swan.ac.uk/Record/cronfa56387
Tags: Add Tag
No Tags, Be the first to tag this record!
first_indexed 2021-03-22T13:10:07Z
last_indexed 2023-01-11T14:35:34Z
id cronfa56387
recordtype SURis
fullrecord <?xml version="1.0"?><rfc1807><datestamp>2022-10-25T13:56:57.3667705</datestamp><bib-version>v2</bib-version><id>56387</id><entry>2021-03-09</entry><title>Holographic entanglement entropy of the Coulomb branch</title><swanseaauthors><author><sid>087fd097167d724ce1b13cb285741ef5</sid><ORCID>0000-0003-0867-4213</ORCID><firstname>Prem</firstname><surname>Kumar</surname><name>Prem Kumar</name><active>true</active><ethesisStudent>false</ethesisStudent></author></swanseaauthors><date>2021-03-09</date><deptcode>SPH</deptcode><abstract>We compute entanglement entropy (EE) of a spherical region in (3 + 1)- dimensional N = 4 supersymmetric SU(N) Yang-Mills theory in states described holographically by probe D3-branes in AdS5 &#xD7; S5. We do so by generalising methods for computing EE from a probe brane action without having to determine the probe&#x2019;s back- reaction. On the Coulomb branch with SU(N) broken to SU(N &#x2212; 1) &#xD7; U(1), we find the EE monotonically decreases as the sphere&#x2019;s radius increases, consistent with the a-theorem. The EE of a symmetric-representation Wilson line screened in SU(N &#x2212; 1) also monotonically decreases, although no known physical principle requires this. A spherical soliton separating SU(N) inside from SU(N &#x2212; 1) &#xD7; U(1) outside had been proposed to model an extremal black hole. However, we find the EE of a sphere at the soliton&#x2019;s radius does not scale with the surface area. For both the screened Wilson line and soliton, the EE at large radius is described by a position-dependent W-boson mass as a short-distance cutoff. Our holographic results for EE and one-point functions of the Lagrangian and stress-energy tensor show that at large distance the soliton looks like a Wilson line in a direct product of fundamental representations.</abstract><type>Journal Article</type><journal>Journal of High Energy Physics</journal><volume>2021</volume><journalNumber>4</journalNumber><paginationStart/><paginationEnd/><publisher>Springer Science and Business Media LLC</publisher><placeOfPublication/><isbnPrint/><isbnElectronic/><issnPrint/><issnElectronic>1029-8479</issnElectronic><keywords>AdS-CFT Correspondence; Conformal Field Theory; Gauge-gravity correspondence; Supersymmetric Gauge Theory</keywords><publishedDay>15</publishedDay><publishedMonth>4</publishedMonth><publishedYear>2021</publishedYear><publishedDate>2021-04-15</publishedDate><doi>10.1007/jhep04(2021)153</doi><url/><notes/><college>COLLEGE NANME</college><department>Physics</department><CollegeCode>COLLEGE CODE</CollegeCode><DepartmentCode>SPH</DepartmentCode><institution>Swansea University</institution><apcterm>Another institution paid the OA fee</apcterm><funders>STFC</funders><projectreference/><lastEdited>2022-10-25T13:56:57.3667705</lastEdited><Created>2021-03-09T23:00:34.2244158</Created><path><level id="1">Faculty of Science and Engineering</level><level id="2">School of Biosciences, Geography and Physics - Physics</level></path><authors><author><firstname>Adam</firstname><surname>Chalabi</surname><order>1</order></author><author><firstname>Prem</firstname><surname>Kumar</surname><orcid>0000-0003-0867-4213</orcid><order>2</order></author><author><firstname>Andy</firstname><surname>O&#x2019;Bannon</surname><order>3</order></author><author><firstname>Anton</firstname><surname>Pribytok</surname><order>4</order></author><author><firstname>Ronnie</firstname><surname>Rodgers</surname><order>5</order></author><author><firstname>Jacopo</firstname><surname>Sisti</surname><order>6</order></author></authors><documents><document><filename>56387__19727__f8113321518e4dca93d6205bd02d8f65.pdf</filename><originalFilename>Chalabi2021_Article_HolographicEntanglementEntropy.pdf</originalFilename><uploaded>2021-04-22T09:56:29.4478105</uploaded><type>Output</type><contentLength>1549115</contentLength><contentType>application/pdf</contentType><version>Version of Record</version><cronfaStatus>true</cronfaStatus><documentNotes>&#xA9;The Authors. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0)</documentNotes><copyrightCorrect>true</copyrightCorrect><language>eng</language><licence>https://creativecommons.org/licenses/by/4.0/</licence></document></documents><OutputDurs/></rfc1807>
spelling 2022-10-25T13:56:57.3667705 v2 56387 2021-03-09 Holographic entanglement entropy of the Coulomb branch 087fd097167d724ce1b13cb285741ef5 0000-0003-0867-4213 Prem Kumar Prem Kumar true false 2021-03-09 SPH We compute entanglement entropy (EE) of a spherical region in (3 + 1)- dimensional N = 4 supersymmetric SU(N) Yang-Mills theory in states described holographically by probe D3-branes in AdS5 × S5. We do so by generalising methods for computing EE from a probe brane action without having to determine the probe’s back- reaction. On the Coulomb branch with SU(N) broken to SU(N − 1) × U(1), we find the EE monotonically decreases as the sphere’s radius increases, consistent with the a-theorem. The EE of a symmetric-representation Wilson line screened in SU(N − 1) also monotonically decreases, although no known physical principle requires this. A spherical soliton separating SU(N) inside from SU(N − 1) × U(1) outside had been proposed to model an extremal black hole. However, we find the EE of a sphere at the soliton’s radius does not scale with the surface area. For both the screened Wilson line and soliton, the EE at large radius is described by a position-dependent W-boson mass as a short-distance cutoff. Our holographic results for EE and one-point functions of the Lagrangian and stress-energy tensor show that at large distance the soliton looks like a Wilson line in a direct product of fundamental representations. Journal Article Journal of High Energy Physics 2021 4 Springer Science and Business Media LLC 1029-8479 AdS-CFT Correspondence; Conformal Field Theory; Gauge-gravity correspondence; Supersymmetric Gauge Theory 15 4 2021 2021-04-15 10.1007/jhep04(2021)153 COLLEGE NANME Physics COLLEGE CODE SPH Swansea University Another institution paid the OA fee STFC 2022-10-25T13:56:57.3667705 2021-03-09T23:00:34.2244158 Faculty of Science and Engineering School of Biosciences, Geography and Physics - Physics Adam Chalabi 1 Prem Kumar 0000-0003-0867-4213 2 Andy O’Bannon 3 Anton Pribytok 4 Ronnie Rodgers 5 Jacopo Sisti 6 56387__19727__f8113321518e4dca93d6205bd02d8f65.pdf Chalabi2021_Article_HolographicEntanglementEntropy.pdf 2021-04-22T09:56:29.4478105 Output 1549115 application/pdf Version of Record true ©The Authors. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0) true eng https://creativecommons.org/licenses/by/4.0/
title Holographic entanglement entropy of the Coulomb branch
spellingShingle Holographic entanglement entropy of the Coulomb branch
Prem Kumar
title_short Holographic entanglement entropy of the Coulomb branch
title_full Holographic entanglement entropy of the Coulomb branch
title_fullStr Holographic entanglement entropy of the Coulomb branch
title_full_unstemmed Holographic entanglement entropy of the Coulomb branch
title_sort Holographic entanglement entropy of the Coulomb branch
author_id_str_mv 087fd097167d724ce1b13cb285741ef5
author_id_fullname_str_mv 087fd097167d724ce1b13cb285741ef5_***_Prem Kumar
author Prem Kumar
author2 Adam Chalabi
Prem Kumar
Andy O’Bannon
Anton Pribytok
Ronnie Rodgers
Jacopo Sisti
format Journal article
container_title Journal of High Energy Physics
container_volume 2021
container_issue 4
publishDate 2021
institution Swansea University
issn 1029-8479
doi_str_mv 10.1007/jhep04(2021)153
publisher Springer Science and Business Media LLC
college_str Faculty of Science and Engineering
hierarchytype
hierarchy_top_id facultyofscienceandengineering
hierarchy_top_title Faculty of Science and Engineering
hierarchy_parent_id facultyofscienceandengineering
hierarchy_parent_title Faculty of Science and Engineering
department_str School of Biosciences, Geography and Physics - Physics{{{_:::_}}}Faculty of Science and Engineering{{{_:::_}}}School of Biosciences, Geography and Physics - Physics
document_store_str 1
active_str 0
description We compute entanglement entropy (EE) of a spherical region in (3 + 1)- dimensional N = 4 supersymmetric SU(N) Yang-Mills theory in states described holographically by probe D3-branes in AdS5 × S5. We do so by generalising methods for computing EE from a probe brane action without having to determine the probe’s back- reaction. On the Coulomb branch with SU(N) broken to SU(N − 1) × U(1), we find the EE monotonically decreases as the sphere’s radius increases, consistent with the a-theorem. The EE of a symmetric-representation Wilson line screened in SU(N − 1) also monotonically decreases, although no known physical principle requires this. A spherical soliton separating SU(N) inside from SU(N − 1) × U(1) outside had been proposed to model an extremal black hole. However, we find the EE of a sphere at the soliton’s radius does not scale with the surface area. For both the screened Wilson line and soliton, the EE at large radius is described by a position-dependent W-boson mass as a short-distance cutoff. Our holographic results for EE and one-point functions of the Lagrangian and stress-energy tensor show that at large distance the soliton looks like a Wilson line in a direct product of fundamental representations.
published_date 2021-04-15T04:11:18Z
_version_ 1763753778059673600
score 11.016235