<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article SYSTEM "http://jats.nlm.nih.gov/archiving/1.2/JATS-archivearticle1.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="1.2" article-type="research-article" xml:lang="en"><?properties open_access?><front><journal-meta><journal-id journal-id-type="publisher-id">13130</journal-id><journal-id journal-id-type="doi">10.1007/13130.1029-8479</journal-id><journal-title-group><journal-title>Journal of High Energy Physics</journal-title><abbrev-journal-title abbrev-type="publisher">J. High Energ. Phys.</abbrev-journal-title></journal-title-group><issn pub-type="epub">1029-8479</issn><publisher><publisher-name>Springer Berlin Heidelberg</publisher-name><publisher-loc>Berlin/Heidelberg</publisher-loc></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">JHEP09(2019)033</article-id><article-id pub-id-type="manuscript">11216</article-id><article-id pub-id-type="arxiv">1805.06463</article-id><article-id pub-id-type="doi">10.1007/JHEP09(2019)033</article-id><article-categories><subj-group subj-group-type="heading"><subject>Regular Article - Theoretical Physics</subject></subj-group></article-categories><title-group><article-title xml:lang="en">Holographic dual of hot Polchinski-Strassler quark-gluon plasma</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>Bena</surname><given-names>Iosif</given-names></name><xref ref-type="aff" rid="Aff1">1</xref></contrib><contrib contrib-type="author"><name><surname>Dias</surname><given-names>Óscar J.C.</given-names></name><xref ref-type="aff" rid="Aff2">2</xref></contrib><contrib contrib-type="author"><name><surname>Hartnett</surname><given-names>Gavin S.</given-names></name><xref ref-type="aff" rid="Aff2">2</xref></contrib><contrib contrib-type="author" corresp="yes"><name><surname>Niehoff</surname><given-names>Benjamin E.</given-names></name><xref ref-type="aff" rid="Aff3">3</xref><xref ref-type="corresp" rid="IDJHEP092019033_cor4">d</xref></contrib><contrib contrib-type="author"><name><surname>Santos</surname><given-names>Jorge E.</given-names></name><xref ref-type="aff" rid="Aff4">4</xref></contrib><aff id="Aff1"><label>1</label><institution-wrap><institution-id institution-id-type="GRID">grid.460789.4</institution-id><institution-id institution-id-type="ISNI">0000 0004 4910 6535</institution-id><institution content-type="org-division">Institut de Physique Théorique</institution><institution content-type="org-name">Université Paris Saclay</institution></institution-wrap><addr-line content-type="street">CEA, CNRS</addr-line><addr-line content-type="postcode">91191</addr-line><addr-line content-type="city">Gif-sur-Yvette Cedex</addr-line><country country="FR">France</country></aff><aff id="Aff2"><label>2</label><institution-wrap><institution-id institution-id-type="GRID">grid.5491.9</institution-id><institution-id institution-id-type="ISNI">0000 0004 1936 9297</institution-id><institution content-type="org-division">STAG research centre and School of Mathematical Sciences</institution><institution content-type="org-name">University of Southampton</institution></institution-wrap><addr-line content-type="street">Highfield Campus</addr-line><addr-line content-type="postcode">SO17 1BJ</addr-line><addr-line content-type="city">Southampton</addr-line><country country="GB">U.K.</country></aff><aff id="Aff3"><label>3</label><institution-wrap><institution-id institution-id-type="GRID">grid.5596.f</institution-id><institution-id institution-id-type="ISNI">0000 0001 0668 7884</institution-id><institution content-type="org-division">Institute for Theoretical Physics</institution><institution content-type="org-name">KU Leuven</institution></institution-wrap><addr-line content-type="street">Celestijnenlaan 200D</addr-line><addr-line content-type="postcode">B-3001</addr-line><addr-line content-type="city">Leuven</addr-line><country country="BE">Belgium</country></aff><aff id="Aff4"><label>4</label><institution-wrap><institution-id institution-id-type="GRID">grid.5335.0</institution-id><institution-id institution-id-type="ISNI">0000000121885934</institution-id><institution content-type="org-division">Department of Applied Mathematics and Theoretical Physics</institution><institution content-type="org-name">University of Cambridge</institution></institution-wrap><addr-line content-type="street">Wilberforce Road</addr-line><addr-line content-type="postcode">CB3 0WA</addr-line><addr-line content-type="city">Cambridge</addr-line><country country="GB">U.K.</country></aff></contrib-group><author-notes><corresp id="IDJHEP092019033_cor4"><label>d</label><email>ben.niehoff@kuleuven.be</email></corresp></author-notes><pub-date date-type="epub"><day>5</day><month>9</month><year>2019</year></pub-date><pub-date date-type="collection"><month>9</month><year>2019</year></pub-date><volume>2019</volume><issue seq="33">9</issue><elocation-id>33</elocation-id><history><date date-type="registration"><day>5</day><month>9</month><year>2019</year></date><date date-type="received"><day>9</day><month>7</month><year>2018</year></date><date date-type="rev-recd"><day>27</day><month>10</month><year>2018</year></date><date date-type="accepted"><day>24</day><month>8</month><year>2019</year></date><date date-type="online"><day>5</day><month>9</month><year>2019</year></date></history><permissions><copyright-statement>© The Author(s) 2019</copyright-statement><copyright-year>2019</copyright-year></permissions><abstract id="Abs1" xml:lang="en"><title>A<sc>bstract</sc></title><p id="Par1">We construct the supergravity dual of the hot quark-gluon plasma in the mass-deformed <inline-formula id="IEq1"><alternatives><mml:math display="inline"><mml:mi mathvariant="script">N</mml:mi></mml:math><tex-math id="IEq1_TeX">\documentclass[12pt]{minimal}
				\usepackage{amsmath}
				\usepackage{wasysym}
				\usepackage{amsfonts}
				\usepackage{amssymb}
				\usepackage{amsbsy}
				\usepackage{mathrsfs}
				\usepackage{upgreek}
				\setlength{\oddsidemargin}{-69pt}
				\begin{document}$$ \mathcal{N} $$\end{document}</tex-math><inline-graphic xlink:href="13130_2019_11216_Article_IEq1.gif"/></alternatives></inline-formula> = 4 Super-Yang-Mills theory (also known as <inline-formula id="IEq2"><alternatives><mml:math display="inline"><mml:mi mathvariant="script">N</mml:mi></mml:math><tex-math id="IEq2_TeX">\documentclass[12pt]{minimal}
				\usepackage{amsmath}
				\usepackage{wasysym}
				\usepackage{amsfonts}
				\usepackage{amssymb}
				\usepackage{amsbsy}
				\usepackage{mathrsfs}
				\usepackage{upgreek}
				\setlength{\oddsidemargin}{-69pt}
				\begin{document}$$ \mathcal{N} $$\end{document}</tex-math><inline-graphic xlink:href="13130_2019_11216_Article_IEq2.gif"/></alternatives></inline-formula> = 1<sup>∗</sup>). The full ten-dimensional type IIB holographic dual is described by 20 functions of two variables, which we determine numerically, and it contains a black hole with <italic>S</italic><sup>5</sup> horizon topology. As we lower the temperature to around half of the mass of the chiral multiplets, we find evidence for (most likely a first-order) phase transition, which could lead either to one of the Polchinski-Strassler confining, screening, or oblique vacua with polarized branes, or to an intermediate phase corresponding to blackened polarized branes with an <italic>S</italic><sup>2</sup> ×<italic>S</italic><sup>3</sup> horizon topology. This phase transition is a feature that could in principle be seen by putting the theory on the lattice, and thus our result for the ratio of the chiral multiplet mass to the phase transition temperature, <italic>m</italic><sub>c</sub><italic>/T</italic> = 2<italic>.</italic>15467491205(6), constitutes the first prediction of string theory and AdS/CFT that could be independently checked via four-dimensional super-QCD lattice computation. We also construct the black-hole solution in certain five-dimensional gauged supergravity truncations and, without directly using uplift/reduction formulae, we find strong evidence that the five- and ten-dimensional solutions are the same. This indicates that five-dimensional gauged supergravity is powerful enough to capture the physics of the high-temperature deconfined phase of the Polchinski-Strassler quark-gluon plasma.</p></abstract><kwd-group xml:lang="en"><title>K<sc>eywords</sc></title><kwd>Gauge-gravity correspondence</kwd><kwd>Holography and quark-gluon plasmas</kwd><kwd>Confinement</kwd><kwd>Black Holes in String Theory</kwd></kwd-group><custom-meta-group><custom-meta><meta-name>publisher-imprint-name</meta-name><meta-value>Springer</meta-value></custom-meta><custom-meta><meta-name>volume-issue-count</meta-name><meta-value>12</meta-value></custom-meta><custom-meta><meta-name>issue-article-count</meta-name><meta-value>124</meta-value></custom-meta><custom-meta><meta-name>issue-toc-levels</meta-name><meta-value>0</meta-value></custom-meta><custom-meta><meta-name>issue-pricelist-year</meta-name><meta-value>2019</meta-value></custom-meta><custom-meta><meta-name>issue-copyright-holder</meta-name><meta-value>The Author(s)</meta-value></custom-meta><custom-meta><meta-name>issue-copyright-year</meta-name><meta-value>2019</meta-value></custom-meta><custom-meta><meta-name>article-contains-esm</meta-name><meta-value>No</meta-value></custom-meta><custom-meta><meta-name>article-numbering-style</meta-name><meta-value>ContentOnly</meta-value></custom-meta><custom-meta><meta-name>article-registration-date-year</meta-name><meta-value>2019</meta-value></custom-meta><custom-meta><meta-name>article-registration-date-month</meta-name><meta-value>9</meta-value></custom-meta><custom-meta><meta-name>article-registration-date-day</meta-name><meta-value>5</meta-value></custom-meta><custom-meta><meta-name>article-toc-levels</meta-name><meta-value>0</meta-value></custom-meta><custom-meta><meta-name>toc-levels</meta-name><meta-value>0</meta-value></custom-meta><custom-meta><meta-name>volume-type</meta-name><meta-value>Regular</meta-value></custom-meta><custom-meta><meta-name>journal-product</meta-name><meta-value>ArchiveJournal</meta-value></custom-meta><custom-meta><meta-name>numbering-style</meta-name><meta-value>Unnumbered</meta-value></custom-meta><custom-meta><meta-name>article-grants-type</meta-name><meta-value>OpenChoice</meta-value></custom-meta><custom-meta><meta-name>metadata-grant</meta-name><meta-value>OpenAccess</meta-value></custom-meta><custom-meta><meta-name>abstract-grant</meta-name><meta-value>OpenAccess</meta-value></custom-meta><custom-meta><meta-name>bodypdf-grant</meta-name><meta-value>OpenAccess</meta-value></custom-meta><custom-meta><meta-name>bodyhtml-grant</meta-name><meta-value>OpenAccess</meta-value></custom-meta><custom-meta><meta-name>bibliography-grant</meta-name><meta-value>OpenAccess</meta-value></custom-meta><custom-meta><meta-name>esm-grant</meta-name><meta-value>OpenAccess</meta-value></custom-meta><custom-meta><meta-name>online-first</meta-name><meta-value>false</meta-value></custom-meta><custom-meta><meta-name>pdf-file-reference</meta-name><meta-value>BodyRef/PDF/13130_2019_Article_11216.pdf</meta-value></custom-meta><custom-meta><meta-name>target-type</meta-name><meta-value>OnlinePDF</meta-value></custom-meta><custom-meta><meta-name>issue-online-date-year</meta-name><meta-value>2019</meta-value></custom-meta><custom-meta><meta-name>issue-online-date-month</meta-name><meta-value>12</meta-value></custom-meta><custom-meta><meta-name>issue-online-date-day</meta-name><meta-value>25</meta-value></custom-meta><custom-meta><meta-name>issue-type</meta-name><meta-value>Regular</meta-value></custom-meta><custom-meta><meta-name>article-type</meta-name><meta-value>OriginalPaper</meta-value></custom-meta><custom-meta><meta-name>journal-subject-primary</meta-name><meta-value>Physics</meta-value></custom-meta><custom-meta><meta-name>journal-subject-secondary</meta-name><meta-value>Elementary Particles, Quantum Field Theory</meta-value></custom-meta><custom-meta><meta-name>journal-subject-secondary</meta-name><meta-value>Quantum Field Theories, String Theory</meta-value></custom-meta><custom-meta><meta-name>journal-subject-secondary</meta-name><meta-value>Classical and Quantum Gravitation, Relativity Theory</meta-value></custom-meta><custom-meta><meta-name>journal-subject-secondary</meta-name><meta-value>Quantum Physics</meta-value></custom-meta><custom-meta><meta-name>journal-subject-collection</meta-name><meta-value>Physics and Astronomy</meta-value></custom-meta><custom-meta><meta-name>open-access</meta-name><meta-value>true</meta-value></custom-meta></custom-meta-group></article-meta><notes notes-type="Misc"><p>A<sc>r</sc>X<sc>iv e</sc>P<sc>rint</sc>: <ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/1805.06463">1805.06463</ext-link></p></notes></front><back><ack><title><bold>Open Access</bold></title><p>This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited</p></ack><ref-list id="Bib1"><title>References</title><ref-list><ref id="CR1"><label>[1]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Policastro</surname><given-names>G</given-names></name><name><surname>Son</surname><given-names>DT</given-names></name><name><surname>Starinets</surname><given-names>AO</given-names></name></person-group><article-title xml:lang="en"><italic>The Shear viscosity of strongly coupled N</italic> = 4 <italic>supersymmetric Yang-Mills plasma</italic></article-title><source>Phys. Rev. Lett.</source><year>2001</year><volume>87</volume><fpage>081601</fpage>2001PhRvL..87h1601P</mixed-citation></ref><ref id="CR2"><label>[2]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Kovtun</surname><given-names>P</given-names></name><name><surname>Son</surname><given-names>DT</given-names></name><name><surname>Starinets</surname><given-names>AO</given-names></name></person-group><article-title xml:lang="en"><italic>Viscosity in strongly interacting quantum field theories from black hole physics</italic></article-title><source>Phys. Rev. Lett.</source><year>2005</year><volume>94</volume><fpage>111601</fpage>2005PhRvL..94k1601K</mixed-citation></ref><ref id="CR3"><label>[3]</label><mixed-citation publication-type="other">T. Banks, M.R. Douglas, G.T. Horowitz and E.J. Martinec, <italic>AdS dynamics from conformal field theory</italic>, <ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/hep-th/9808016">hep-th/9808016</ext-link> [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+hep-th/9808016">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR4"><label>[4]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Balasubramanian</surname><given-names>V</given-names></name><name><surname>Kraus</surname><given-names>P</given-names></name><name><surname>Lawrence</surname><given-names>AE</given-names></name><name><surname>Trivedi</surname><given-names>SP</given-names></name></person-group><article-title xml:lang="en"><italic>Holographic probes of anti-de Sitter space-times</italic></article-title><source>Phys. Rev.</source><year>1999</year><volume>D 59</volume><fpage>104021</fpage>1999PhRvD..59j4021B</mixed-citation></ref><ref id="CR5"><label>[5]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Donagi</surname><given-names>R</given-names></name><name><surname>Witten</surname><given-names>E</given-names></name></person-group><article-title xml:lang="en"><italic>Supersymmetric Yang-Mills theory and integrable systems</italic></article-title><source>Nucl. Phys.</source><year>1996</year><volume>B 460</volume><fpage>299</fpage>1996NuPhB.460..299D13771670996.37507</mixed-citation></ref><ref id="CR6"><label>[6]</label><mixed-citation publication-type="other">J. Polchinski and M.J. Strassler, <italic>The String dual of a confining four-dimensional gauge theory</italic>, <ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/hep-th/0003136">hep-th/0003136</ext-link> [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+hep-th/0003136">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR7"><label>[7]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Myers</surname><given-names>RC</given-names></name></person-group><article-title xml:lang="en"><italic>Dielectric branes</italic></article-title><source>JHEP</source><year>1999</year><volume>12</volume><fpage>022</fpage>1999JHEP...12..022M17430600958.81091</mixed-citation></ref><ref id="CR8"><label>[8]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Freedman</surname><given-names>DZ</given-names></name><name><surname>Minahan</surname><given-names>JA</given-names></name></person-group><article-title xml:lang="en"><italic>Finite temperature effects in the supergravity dual of the N</italic> = 1<sup>∗</sup><italic>gauge theory</italic></article-title><source>JHEP</source><year>2001</year><volume>01</volume><fpage>036</fpage>2001JHEP...01..036F1818346</mixed-citation></ref><ref id="CR9"><label>[9]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Sakai</surname><given-names>T</given-names></name><name><surname>Sugimoto</surname><given-names>S</given-names></name></person-group><article-title xml:lang="en"><italic>Low energy hadron physics in holographic QCD</italic></article-title><source>Prog. Theor. Phys.</source><year>2005</year><volume>113</volume><fpage>843</fpage>2005PThPh.113..843S1076.81623</mixed-citation></ref><ref id="CR10"><label>[10]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Witten</surname><given-names>E</given-names></name></person-group><article-title xml:lang="en"><italic>Branes and the dynamics of QCD</italic></article-title><source>Nucl. Phys.</source><year>1997</year><volume>B 507</volume><fpage>658</fpage>1997NuPhB.507..658W14910320925.81388</mixed-citation></ref><ref id="CR11"><label>[11]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Giveon</surname><given-names>A</given-names></name><name><surname>Kutasov</surname><given-names>D</given-names></name></person-group><article-title xml:lang="en"><italic>Brane dynamics and gauge theory</italic></article-title><source>Rev. Mod. Phys.</source><year>1999</year><volume>71</volume><fpage>983</fpage>1999RvMP...71..983G17123161205.81115</mixed-citation></ref><ref id="CR12"><label>[12]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Witten</surname><given-names>E</given-names></name></person-group><article-title xml:lang="en"><italic>Anti-de Sitter space, thermal phase transition and confinement in gauge theories</italic></article-title><source>Adv. Theor. Math. Phys.</source><year>1998</year><volume>2</volume><fpage>505</fpage>16468951057.81550</mixed-citation></ref><ref id="CR13"><label>[13]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Klebanov</surname><given-names>IR</given-names></name><name><surname>Strassler</surname><given-names>MJ</given-names></name></person-group><article-title xml:lang="en"><italic>Supergravity and a confining gauge theory: Duality cascades and chi SB resolution of naked singularities</italic></article-title><source>JHEP</source><year>2000</year><volume>08</volume><fpage>052</fpage>2000JHEP...08..052K0986.83041</mixed-citation></ref><ref id="CR14"><label>[14]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Gauntlett</surname><given-names>JP</given-names></name><name><surname>Martelli</surname><given-names>D</given-names></name><name><surname>Pakis</surname><given-names>S</given-names></name><name><surname>Waldram</surname><given-names>D</given-names></name></person-group><article-title xml:lang="en"><italic>G structures and wrapped NS5-branes</italic></article-title><source>Commun. Math. Phys.</source><year>2004</year><volume>247</volume><fpage>421</fpage>2004CMaPh.247..421G20632671061.81058</mixed-citation></ref><ref id="CR15"><label>[15]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Gowdigere</surname><given-names>CN</given-names></name><name><surname>Nemeschansky</surname><given-names>D</given-names></name><name><surname>Warner</surname><given-names>NP</given-names></name></person-group><article-title xml:lang="en"><italic>Supersymmetric solutions with fluxes from algebraic Killing spinors</italic></article-title><source>Adv. Theor. Math. Phys.</source><year>2003</year><volume>7</volume><fpage>787</fpage>20453011056.81057</mixed-citation></ref><ref id="CR16"><label>[16]</label><mixed-citation publication-type="other">D. Nemeschansky and N.P. Warner, <italic>A Family of M-theory flows with four supersymmetries</italic>, <ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/hep-th/0403006">hep-th/0403006</ext-link> [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+hep-th/0403006">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR17"><label>[17]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Lin</surname><given-names>H</given-names></name><name><surname>Lunin</surname><given-names>O</given-names></name><name><surname>Maldacena</surname><given-names>JM</given-names></name></person-group><article-title xml:lang="en"><italic>Bubbling AdS space and</italic> 1<italic>/</italic>2 <italic>BPS geometries</italic></article-title><source>JHEP</source><year>2004</year><volume>10</volume><fpage>025</fpage>2004JHEP...10..025L2116025</mixed-citation></ref><ref id="CR18"><label>[18]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Headrick</surname><given-names>M</given-names></name><name><surname>Kitchen</surname><given-names>S</given-names></name><name><surname>Wiseman</surname><given-names>T</given-names></name></person-group><article-title xml:lang="en"><italic>A New approach to static numerical relativity and its application to Kaluza-Klein black holes</italic></article-title><source>Class. Quant. Grav.</source><year>2010</year><volume>27</volume><fpage>035002</fpage>2010CQGra..27c5002H25855271186.83083</mixed-citation></ref><ref id="CR19"><label>[19]</label><mixed-citation publication-type="other">T. Wiseman, <italic>Numerical construction of static and stationary black holes</italic>, in <italic>Black holes in higher dimensions</italic>, G.T. Horowitz ed., pp. 233-270 (2012) [<ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/1107.5513">arXiv:1107.5513</ext-link>] [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+arXiv:1107.5513">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR20"><label>[20]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Dias</surname><given-names>ÓJC</given-names></name><name><surname>Santos</surname><given-names>JE</given-names></name><name><surname>Way</surname><given-names>B</given-names></name></person-group><article-title xml:lang="en"><italic>Numerical Methods for Finding Stationary Gravitational Solutions</italic></article-title><source>Class. Quant. Grav.</source><year>2016</year><volume>33</volume><fpage>133001</fpage>2016CQGra..33m3001D35134561346.83002</mixed-citation></ref><ref id="CR21"><label>[21]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Girardello</surname><given-names>L</given-names></name><name><surname>Petrini</surname><given-names>M</given-names></name><name><surname>Porrati</surname><given-names>M</given-names></name><name><surname>Zaffaroni</surname><given-names>A</given-names></name></person-group><article-title xml:lang="en"><italic>The Supergravity dual of N</italic> = 1 <italic>superYang-Mills theory</italic></article-title><source>Nucl. Phys.</source><year>2000</year><volume>B 569</volume><fpage>451</fpage>2000NuPhB.569..451G0951.81056</mixed-citation></ref><ref id="CR22"><label>[22]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Petrini</surname><given-names>M</given-names></name><name><surname>Samtleben</surname><given-names>H</given-names></name><name><surname>Schmidt</surname><given-names>S</given-names></name><name><surname>Skenderis</surname><given-names>K</given-names></name></person-group><article-title xml:lang="en"><italic>The</italic> 10<italic>d Uplift of the GPPZ Solution</italic></article-title><source>JHEP</source><year>2018</year><volume>07</volume><fpage>026</fpage>2018JHEP...07..026P38620271395.83130</mixed-citation></ref><ref id="CR23"><label>[23]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Bobev</surname><given-names>N</given-names></name><name><surname>Gautason</surname><given-names>FF</given-names></name><name><surname>Niehoff</surname><given-names>BE</given-names></name><name><surname>van Muiden</surname><given-names>J</given-names></name><name><surname>Uplifting</surname><given-names>GPPZ</given-names></name></person-group><article-title xml:lang="en"><italic>a ten-dimensional dual of</italic><inline-formula id="IEq3"><alternatives><mml:math display="inline"><mml:mi mathvariant="script">N</mml:mi></mml:math><tex-math id="IEq3_TeX">\documentclass[12pt]{minimal}
				\usepackage{amsmath}
				\usepackage{wasysym}
				\usepackage{amsfonts}
				\usepackage{amssymb}
				\usepackage{amsbsy}
				\usepackage{mathrsfs}
				\usepackage{upgreek}
				\setlength{\oddsidemargin}{-69pt}
				\begin{document}$$ \mathcal{N} $$\end{document}</tex-math><inline-graphic xlink:href="13130_2019_11216_Article_IEq3.gif"/></alternatives></inline-formula> = 1<sup>∗</sup></article-title><source>JHEP</source><year>2018</year><volume>10</volume><fpage>058</fpage>2018JHEP...10..058B</mixed-citation></ref><ref id="CR24"><label>[24]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Pilch</surname><given-names>K</given-names></name><name><surname>Warner</surname><given-names>NP</given-names></name></person-group><article-title xml:lang="en"><italic>N</italic> = 1 <italic>supersymmetric renormalization group flows from IIB supergravity</italic></article-title><source>Adv. Theor. Math. Phys.</source><year>2002</year><volume>4</volume><fpage>627</fpage>18387221063.81626</mixed-citation></ref><ref id="CR25"><label>[25]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Baguet</surname><given-names>A</given-names></name><name><surname>Hohm</surname><given-names>O</given-names></name><name><surname>Samtleben</surname><given-names>H</given-names></name></person-group><article-title xml:lang="en"><italic>Consistent Type IIB Reductions to Maximal</italic> 5<italic>D Supergravity</italic></article-title><source>Phys. Rev.</source><year>2015</year><volume>D 92</volume><fpage>065004</fpage>2015PhRvD..92f5004B3440975</mixed-citation></ref><ref id="CR26"><label>[26]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Pilch</surname><given-names>K</given-names></name><name><surname>Warner</surname><given-names>NP</given-names></name></person-group><article-title xml:lang="en"><italic>N</italic> = 2 <italic>supersymmetric RG flows and the IIB dilaton</italic></article-title><source>Nucl. Phys.</source><year>2001</year><volume>B 594</volume><fpage>209</fpage>2001NuPhB.594..209P18089340971.83513</mixed-citation></ref><ref id="CR27"><label>[27]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Leigh</surname><given-names>RG</given-names></name><name><surname>Strassler</surname><given-names>MJ</given-names></name></person-group><article-title xml:lang="en"><italic>Exactly marginal operators and duality in four-dimensional N</italic> = 1 <italic>supersymmetric gauge theory</italic></article-title><source>Nucl. Phys.</source><year>1995</year><volume>B 447</volume><fpage>95</fpage>1995NuPhB.447...95L13436721009.81570</mixed-citation></ref><ref id="CR28"><label>[28]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Vafa</surname><given-names>C</given-names></name><name><surname>Witten</surname><given-names>E</given-names></name></person-group><article-title xml:lang="en"><italic>A Strong coupling test of S duality</italic></article-title><source>Nucl. Phys.</source><year>1994</year><volume>B 431</volume><fpage>3</fpage>1994NuPhB.431....3V13050960964.81522</mixed-citation></ref><ref id="CR29"><label>[29]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Günaydin</surname><given-names>M</given-names></name><name><surname>Romans</surname><given-names>LJ</given-names></name><name><surname>Warner</surname><given-names>NP</given-names></name></person-group><article-title xml:lang="en"><italic>Gauged N</italic> = 8 <italic>Supergravity in Five-Dimensions</italic></article-title><source>Phys. Lett.</source><year>1985</year><volume>154B</volume><fpage>268</fpage>1985PhLB..154..268G789042</mixed-citation></ref><ref id="CR30"><label>[30]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Pernici</surname><given-names>M</given-names></name><name><surname>Pilch</surname><given-names>K</given-names></name><name><surname>van Nieuwenhuizen</surname><given-names>P</given-names></name></person-group><article-title xml:lang="en"><italic>Gauged N</italic> = 8 <italic>D</italic> = 5 <italic>Supergravity</italic></article-title><source>Nucl. Phys.</source><year>1985</year><volume>B 259</volume><fpage>460</fpage>1985NuPhB.259..460P</mixed-citation></ref><ref id="CR31"><label>[31]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Günaydin</surname><given-names>M</given-names></name><name><surname>Romans</surname><given-names>LJ</given-names></name><name><surname>Warner</surname><given-names>NP</given-names></name></person-group><article-title xml:lang="en"><italic>Compact and Noncompact Gauged Supergravity Theories in Five-Dimensions</italic></article-title><source>Nucl. Phys.</source><year>1986</year><volume>B 272</volume><fpage>598</fpage>1986NuPhB.272..598G</mixed-citation></ref><ref id="CR32"><label>[32]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Cvetič</surname><given-names>M</given-names></name><name><surname>Lü</surname><given-names>H</given-names></name><name><surname>Pope</surname><given-names>CN</given-names></name></person-group><article-title xml:lang="en"><italic>Consistent Kaluza-Klein sphere reductions</italic></article-title><source>Phys. Rev.</source><year>2000</year><volume>D 62</volume><fpage>064028</fpage>2000PhRvD..62f4028C1791031</mixed-citation></ref><ref id="CR33"><label>[33]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Gibbons</surname><given-names>GW</given-names></name><name><surname>Pope</surname><given-names>CN</given-names></name></person-group><article-title xml:lang="en"><italic>Consistent S</italic><sup>2</sup><italic>Pauli reduction of six-dimensional chiral gauged Einstein-Maxwell supergravity</italic></article-title><source>Nucl. Phys.</source><year>2004</year><volume>B 697</volume><fpage>225</fpage>2004NuPhB.697..225G1236.83025</mixed-citation></ref><ref id="CR34"><label>[34]</label><mixed-citation publication-type="other">B. de Wit and H. Nicolai, <italic>Deformations of gauged</italic> SO(8) <italic>supergravity and supergravity in eleven dimensions</italic>, <italic>JHEP</italic><bold>05</bold> (2013) 077 [<ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/1302.6219">arXiv:1302.6219</ext-link>] [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+arXiv:1302.6219">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR35"><label>[35]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Godazgar</surname><given-names>H</given-names></name><name><surname>Godazgar</surname><given-names>M</given-names></name><name><surname>Nicolai</surname><given-names>H</given-names></name></person-group><article-title xml:lang="en"><italic>Nonlinear Kaluza-Klein theory for dual fields</italic></article-title><source>Phys. Rev.</source><year>2013</year><volume>D 88</volume><fpage>125002</fpage>2013PhRvD..88l5002G</mixed-citation></ref><ref id="CR36"><label>[36]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Godazgar</surname><given-names>H</given-names></name><name><surname>Godazgar</surname><given-names>M</given-names></name><name><surname>Nicolai</surname><given-names>H</given-names></name></person-group><article-title xml:lang="en"><italic>Testing the non-linear flux ansatz for maximal supergravity</italic></article-title><source>Phys. Rev.</source><year>2013</year><volume>D 87</volume><fpage>085038</fpage>2013PhRvD..87h5038G</mixed-citation></ref><ref id="CR37"><label>[37]</label><mixed-citation publication-type="other">H. Godazgar, M. Godazgar and H. Nicolai, <italic>Generalised geometry from the ground up</italic>, <italic>JHEP</italic><bold>02</bold> (2014) 075 [<ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/1307.8295">arXiv:1307.8295</ext-link>] [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+arXiv:1307.8295">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR38"><label>[38]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Godazgar</surname><given-names>H</given-names></name><name><surname>Godazgar</surname><given-names>M</given-names></name><name><surname>Nicolai</surname><given-names>H</given-names></name></person-group><article-title xml:lang="en"><italic>Embedding tensor of Scherk-Schwarz flux compactifications from eleven dimensions</italic></article-title><source>Phys. Rev.</source><year>2014</year><volume>D 89</volume><fpage>045009</fpage>2014PhRvD..89d5009G1333.83237</mixed-citation></ref><ref id="CR39"><label>[39]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Lee</surname><given-names>K</given-names></name><name><surname>Strickland-Constable</surname><given-names>C</given-names></name><name><surname>Waldram</surname><given-names>D</given-names></name></person-group><article-title xml:lang="en"><italic>Spheres, generalised parallelisability and consistent truncations</italic></article-title><source>Fortsch. Phys.</source><year>2017</year><volume>65</volume><fpage>1700048</fpage>3715652</mixed-citation></ref><ref id="CR40"><label>[40]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Intriligator</surname><given-names>KA</given-names></name></person-group><article-title xml:lang="en"><italic>Bonus symmetries of N</italic> = 4 <italic>superYang-Mills correlation functions via AdS duality</italic></article-title><source>Nucl. Phys.</source><year>1999</year><volume>B 551</volume><fpage>575</fpage>1999NuPhB.551..575I0947.81121</mixed-citation></ref><ref id="CR41"><label>[41]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Bianchi</surname><given-names>M</given-names></name><name><surname>Freedman</surname><given-names>DZ</given-names></name><name><surname>Skenderis</surname><given-names>K</given-names></name></person-group><article-title xml:lang="en"><italic>Holographic renormalization</italic></article-title><source>Nucl. Phys.</source><year>2002</year><volume>B 631</volume><fpage>159</fpage>2002NuPhB.631..159B19080680995.81075</mixed-citation></ref><ref id="CR42"><label>[42]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Bianchi</surname><given-names>M</given-names></name><name><surname>Freedman</surname><given-names>DZ</given-names></name><name><surname>Skenderis</surname><given-names>K</given-names></name></person-group><article-title xml:lang="en"><italic>How to go with an RG flow</italic></article-title><source>JHEP</source><year>2001</year><volume>08</volume><fpage>041</fpage>2001JHEP...08..041B1866236</mixed-citation></ref><ref id="CR43"><label>[43]</label><mixed-citation publication-type="other">R.M. Wald, <italic>Dynamic and Thermodynamic Stability of Black Holes and Black Branes</italic>, <italic>Fundam. Theor. Phys.</italic><bold>177</bold> (2014) 229 [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+J+%22Fundam.Theor.Phys.,177,229%22">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR44"><label>[44]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Schiffrin</surname><given-names>JS</given-names></name><name><surname>Wald</surname><given-names>RM</given-names></name></person-group><article-title xml:lang="en"><italic>Turning Point Instabilities for Relativistic Stars and Black Holes</italic></article-title><source>Class. Quant. Grav.</source><year>2014</year><volume>31</volume><fpage>035024</fpage>2014CQGra..31c5024S1285.83013</mixed-citation></ref><ref id="CR45"><label>[45]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Schwarz</surname><given-names>JH</given-names></name></person-group><article-title xml:lang="en"><italic>Covariant Field Equations of Chiral N</italic> = 2 <italic>D</italic> = 10 <italic>Supergravity</italic></article-title><source>Nucl. Phys.</source><year>1983</year><volume>B 226</volume><fpage>269</fpage>1983NuPhB.226..269S</mixed-citation></ref><ref id="CR46"><label>[46]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Graña</surname><given-names>M</given-names></name><name><surname>Polchinski</surname><given-names>J</given-names></name></person-group><article-title xml:lang="en"><italic>Gauge/gravity duals with holomorphic dilaton</italic></article-title><source>Phys. Rev.</source><year>2002</year><volume>D 65</volume><fpage>126005</fpage>2002PhRvD..65l6005G1926698</mixed-citation></ref><ref id="CR47"><label>[47]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Bena</surname><given-names>I</given-names></name><name><surname>Graña</surname><given-names>M</given-names></name><name><surname>Kuperstein</surname><given-names>S</given-names></name><name><surname>Ntokos</surname><given-names>P</given-names></name><name><surname>Petrini</surname><given-names>M</given-names></name></person-group><article-title xml:lang="en"><italic>Fermionic and bosonic mass deformations of</italic><inline-formula id="IEq5"><alternatives><mml:math display="inline"><mml:mi mathvariant="script">N</mml:mi></mml:math><tex-math id="IEq5_TeX">\documentclass[12pt]{minimal}
				\usepackage{amsmath}
				\usepackage{wasysym}
				\usepackage{amsfonts}
				\usepackage{amssymb}
				\usepackage{amsbsy}
				\usepackage{mathrsfs}
				\usepackage{upgreek}
				\setlength{\oddsidemargin}{-69pt}
				\begin{document}$$ \mathcal{N} $$\end{document}</tex-math><inline-graphic xlink:href="13130_2019_11216_Article_IEq5.gif"/></alternatives></inline-formula> = 4 <italic>SYM and their bulk supergravity dual</italic></article-title><source>JHEP</source><year>2016</year><volume>05</volume><fpage>149</fpage>2016JHEP...05..149B1388.83740</mixed-citation></ref><ref id="CR48"><label>[48]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Figueras</surname><given-names>P</given-names></name><name><surname>Lucietti</surname><given-names>J</given-names></name><name><surname>Wiseman</surname><given-names>T</given-names></name></person-group><article-title xml:lang="en"><italic>Ricci solitons, Ricci flow and strongly coupled CFT in the Schwarzschild Unruh or Boulware vacua</italic></article-title><source>Class. Quant. Grav.</source><year>2011</year><volume>28</volume><fpage>215018</fpage>2011CQGra..28u5018F28515671230.83015</mixed-citation></ref><ref id="CR49"><label>[49]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Figueras</surname><given-names>P</given-names></name><name><surname>Wiseman</surname><given-names>T</given-names></name></person-group><article-title xml:lang="en"><italic>On the existence of stationary Ricci solitons</italic></article-title><source>Class. Quant. Grav.</source><year>2017</year><volume>34</volume><fpage>145007</fpage>2017CQGra..34n5007F36824871373.83054</mixed-citation></ref><ref id="CR50"><label>[50]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Dias</surname><given-names>ÓJC</given-names></name><name><surname>Horowitz</surname><given-names>GT</given-names></name><name><surname>Santos</surname><given-names>JE</given-names></name></person-group><article-title xml:lang="en"><italic>Black holes with only one Killing field</italic></article-title><source>JHEP</source><year>2011</year><volume>07</volume><fpage>115</fpage>2011JHEP...07..115D28759371298.83075</mixed-citation></ref><ref id="CR51"><label>[51]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Dias</surname><given-names>ÓJC</given-names></name><name><surname>Santos</surname><given-names>JE</given-names></name><name><surname>Way</surname><given-names>B</given-names></name></person-group><article-title xml:lang="en"><italic>Black holes with a single Killing vector field: black resonators</italic></article-title><source>JHEP</source><year>2015</year><volume>12</volume><fpage>171</fpage>2015JHEP...12..171D34646311388.83425</mixed-citation></ref><ref id="CR52"><label>[52]</label><mixed-citation publication-type="other">O.J.C. Dias, G.S. Hartnett, B.E. Niehoff and J.E. Santos, <italic>Energy in M-Theory and IIB</italic>, to be submitted (2018).</mixed-citation></ref><ref id="CR53"><label>[53]</label><mixed-citation publication-type="other">M. Taylor, <italic>Anomalies, counterterms and the N</italic> = 0 <italic>Polchinski-Strassler solutions</italic>, <ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/hep-th/0103162">hep-th/0103162</ext-link> [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+hep-th/0103162">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR54"><label>[54]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Dias</surname><given-names>ÓJC</given-names></name><name><surname>Hartnett</surname><given-names>GS</given-names></name><name><surname>Niehoff</surname><given-names>BE</given-names></name><name><surname>Santos</surname><given-names>JE</given-names></name></person-group><article-title xml:lang="en"><italic>Mass-deformed M2 branes in Stenzel space</italic></article-title><source>JHEP</source><year>2017</year><volume>11</volume><fpage>105</fpage>2017JHEP...11..105D37472031383.83204</mixed-citation></ref><ref id="CR55"><label>[55]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Gregory</surname><given-names>R</given-names></name><name><surname>Laflamme</surname><given-names>R</given-names></name></person-group><article-title xml:lang="en"><italic>Black strings and p-branes are unstable</italic></article-title><source>Phys. Rev. Lett.</source><year>1993</year><volume>70</volume><fpage>2837</fpage>1993PhRvL..70.2837G12154081051.83544</mixed-citation></ref><ref id="CR56"><label>[56]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Wiseman</surname><given-names>T</given-names></name></person-group><article-title xml:lang="en"><italic>Static axisymmetric vacuum solutions and nonuniform black strings</italic></article-title><source>Class. Quant. Grav.</source><year>2003</year><volume>20</volume><fpage>1137</fpage>2003CQGra..20.1137W1051.83018</mixed-citation></ref><ref id="CR57"><label>[57]</label><mixed-citation publication-type="other">M. Kalisch and M. Ansorg, <italic>Highly Deformed Non-uniform Black Strings in Six Dimensions</italic>, in <italic>Proceedings, 14th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories (MG14)</italic>, (in 4 volumes), Rome, Italy, 12-18 July 2015, vol. 2, pp. 1799-1804 (2017) [DOI:10.1142/9789813226609 0185] [<ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/1509.03083">arXiv:1509.03083</ext-link>] [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+arXiv:1509.03083">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR58"><label>[58]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Kalisch</surname><given-names>M</given-names></name><name><surname>Ansorg</surname><given-names>M</given-names></name></person-group><article-title xml:lang="en"><italic>Pseudo-spectral construction of non-uniform black string solutions in five and six spacetime dimensions</italic></article-title><source>Class. Quant. Grav.</source><year>2016</year><volume>33</volume><fpage>215005</fpage>2016CQGra..33u5005K35626681351.83028</mixed-citation></ref><ref id="CR59"><label>[59]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Dias</surname><given-names>ÓJC</given-names></name><name><surname>Santos</surname><given-names>JE</given-names></name><name><surname>Way</surname><given-names>B</given-names></name></person-group><article-title xml:lang="en"><italic>Rings, Ripples and Rotation: Connecting Black Holes to Black Rings</italic></article-title><source>JHEP</source><year>2014</year><volume>07</volume><fpage>045</fpage>2014JHEP...07..045D</mixed-citation></ref><ref id="CR60"><label>[60]</label><mixed-citation publication-type="other">R. Emparan, P. Figueras and M. Martinez, <italic>Bumpy black holes</italic>, <italic>JHEP</italic><bold>12</bold> (2014) 072 [<ext-link ext-link-type="uri" xlink:href="https://arxiv.org/abs/1410.4764">arXiv:1410.4764</ext-link>] [<ext-link ext-link-type="uri" xlink:href="https://inspirehep.net/search?p=find+EPRINT+arXiv:1410.4764">INSPIRE</ext-link>].</mixed-citation></ref><ref id="CR61"><label>[61]</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><name><surname>Dias</surname><given-names>ÓJC</given-names></name><name><surname>Santos</surname><given-names>JE</given-names></name><name><surname>Way</surname><given-names>B</given-names></name></person-group><article-title xml:lang="en"><italic>Lumpy AdS</italic><sub>5</sub><italic>× S</italic><sup>5</sup><italic>black holes and black belts</italic></article-title><source>JHEP</source><year>2015</year><volume>04</volume><fpage>060</fpage>2015JHEP...04..060D</mixed-citation></ref></ref-list></ref-list></back></article>