<?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">JHEP06(2020)104</article-id><article-id pub-id-type="manuscript">13203</article-id><article-id pub-id-type="arxiv">2003.05454</article-id><article-id pub-id-type="doi">10.1007/JHEP06(2020)104</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">To go or not to go with the flow: Hawking radiation at strong coupling</article-title></title-group><contrib-group><contrib contrib-type="author" corresp="yes" id="Au1"><name><surname>Santos</surname><given-names>Jorge E.</given-names></name><xref ref-type="aff" rid="Aff1">1</xref><xref ref-type="aff" rid="Aff2">2</xref><xref ref-type="corresp" rid="IDJHEP062020104_cor1">a</xref></contrib><aff id="Aff1"><label>1</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><aff id="Aff2"><label>2</label><institution-wrap><institution-id institution-id-type="GRID">grid.78989.37</institution-id><institution-id institution-id-type="ISNI">0000 0001 2160 7918</institution-id><institution content-type="org-name">Institute for Advanced Study</institution></institution-wrap><addr-line content-type="postcode">08540</addr-line><addr-line content-type="city">Princeton</addr-line><addr-line content-type="state">NJ</addr-line><country country="US">U.S.A.</country></aff></contrib-group><author-notes><corresp id="IDJHEP062020104_cor1"><label>a</label><email>jss55@cam.ac.uk</email></corresp></author-notes><pub-date date-type="epub"><day>16</day><month>6</month><year>2020</year></pub-date><pub-date date-type="collection"><month>6</month><year>2020</year></pub-date><volume>2020</volume><issue seq="104">6</issue><elocation-id>104</elocation-id><history><date date-type="registration"><day>16</day><month>6</month><year>2020</year></date><date date-type="received"><day>17</day><month>4</month><year>2020</year></date><date date-type="accepted"><day>24</day><month>5</month><year>2020</year></date><date date-type="online"><day>16</day><month>6</month><year>2020</year></date></history><permissions><copyright-statement>© The Author(s) 2020</copyright-statement><copyright-year>2020</copyright-year></permissions><abstract id="Abs1" xml:lang="en"><title>A<sc>bstract</sc></title><p id="Par1">We construct the gravitational dual of a one-parameter class of states of strongly coupled SU(<italic>N</italic>) <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}
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				\begin{document}$$ \mathcal{N} $$\end{document}</tex-math><inline-graphic xlink:href="13130_2020_13203_Article_IEq1.gif"/></alternatives></inline-formula> = 4 SYM at infinite <italic>N</italic> and asymptotic temperature <italic>T</italic><sub>∞</sub>, on a fixed Schwarzschild black hole background with temperature <italic>T</italic><sub>BH</sub>. The resulting bulk geometry is of the flowing type and allow us to measure Hawking radiation at strong coupling. The outgoing Hawking flux is a function of the dimensionless ratio <italic>τ ≡ T</italic><sub><italic>∞</italic></sub><italic>/T</italic><sub>BH</sub> and appears to be non-monotonic in <italic>τ</italic>. At present, we have no field theory understanding for this behaviour.</p></abstract><kwd-group xml:lang="en"><title>K<sc>eywords</sc></title><kwd>AdS-CFT Correspondence</kwd><kwd>Black Holes</kwd><kwd>Nonperturbative Effects</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>187</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>2020</meta-value></custom-meta><custom-meta><meta-name>issue-copyright-holder</meta-name><meta-value>The 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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/2003.05454">2003.05454</ext-link></p></notes></front><back><ack><title><bold>Open Access</bold></title><p>This article is distributed under the terms of the 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