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We perform a global analysis of effective field theory (EFT) operators describing the interactions between a gauge-singlet Dirac fermion and the Standard Model quarks, the gluons and the photon. In this bottom-up approach, we simultaneously vary the coefficients of 14 such operators up to dimension 7, along with the DM mass, the scale of new physics and several nuisance parameters. Our likelihood functions include the latest data from Planck, direct and indirect detection experiments, and the LHC. For DM masses below 100 GeV, we find that it is impossible to satisfy all constraints simultaneously while maintaining EFT validity at LHC energies. For new physics scales around 1 TeV, our results are influenced by several small excesses in the LHC data and depend on the prescription that we adopt to ensure EFT validity. Furthermore, we find large regions of viable parameter space where the EFT is valid and the relic density can be reproduced, implying that WIMPs can still account for the DM of the universe while being consistent with the latest data. We assess the status of a wide class of WIMP dark matter (DM) models in light of the latest experimental results using the global fitting framework $\textsf{GAMBIT}$. We perform a global analysis of effective field theory (EFT) operators describing the interactions between a gauge-singlet Dirac fermion and the Standard Model quarks, the gluons and the photon. In this bottom-up approach, we simultaneously vary the coefficients of 14 such operators up to dimension 7, along with the DM mass, the scale of new physics and several nuisance parameters. Our likelihood functions include the latest data from $\mathit{Planck}$, direct and indirect detection experiments, and the LHC. For DM masses below 100 GeV, we find that it is impossible to satisfy all constraints simultaneously while maintaining EFT validity at LHC energies. For new physics scales around 1 TeV, our results are influenced by several small excesses in the LHC data and depend on the prescription that we adopt to ensure EFT validity. Furthermore, we find large regions of viable parameter space where the EFT is valid and the relic density can be reproduced, implying that WIMPs can still account for the DM of the universe while being consistent with the latest data. Athron, Peter; Kozar, Neal Avis; Balázs, Csaba; Beniwal, Ankit; Bloor, Sanjay; Bringmann, Torsten; Brod, Joachim; Chang, Christopher; Cornell, Jonathan M.; Farmer, Ben; Fowlie, Andrew; Gonzalo, Tomás E.; Handley, Will; Kahlhoefer, Felix; Kvellestad, Anders; Mahmoudi, Farvah; Prim, Markus T.; Raklev, Are; Renk, Janina J.; Scaffidi, Andre; Scott, Pat; Stöcker, Patrick; Vincent, Aaron C.; White, Martin; Wild, Sebastian; Zupan, Jure" /> <meta name="keywords" content="CERN Document Server, WebSearch, CERN Document Server" /> <script type="text/javascript" src="https://cds.cern.ch/js/jquery.min.js"></script>  <link rel="stylesheet" href="https://cds.cern.ch/img/webnews.css" type="text/css" />  <script type="text/javascript" src="https://cds.cern.ch/js/webnews.js?v=20131009"></script> <meta property="fb:app_id" content="137353533001720"/> <script type="text/x-mathjax-config"> MathJax.Hub.Config({ tex2jax: {inlineMath: [['$','$']], processEscapes: true}, showProcessingMessages: false, messageStyle: "none" }); </script> <script src="/MathJax/MathJax.js?config=TeX-AMS_CHTML" type="text/javascript"> </script>  <meta content="Springer : Thermal WIMPs and the Scale of New Physics: Global Fits of Dirac Dark Matter Effective Field Theories" name="citation_title" /> <meta content="Athron, Peter" name="citation_author" /> <meta content="Renk, Janina J." name="citation_author" /> <meta content="Kahlhoefer, Felix" name="citation_author" /> <meta content="Farmer, Ben" name="citation_author" /> <meta content="Kvellestad, Anders" name="citation_author" /> <meta content="Vincent, Aaron C." name="citation_author" /> <meta content="Brod, Joachim" name="citation_author" /> <meta content="Zupan, Jure" name="citation_author" /> <meta content="Balázs, Csaba" name="citation_author" /> <meta content="Cornell, Jonathan M." name="citation_author" /> <meta content="White, Martin" name="citation_author" /> <meta content="Wild, Sebastian" name="citation_author" /> <meta content="Stöcker, Patrick" name="citation_author" /> <meta content="Prim, Markus T." name="citation_author" /> <meta content="Beniwal, Ankit" name="citation_author" /> <meta content="Handley, Will" name="citation_author" /> <meta content="Bringmann, Torsten" name="citation_author" /> <meta content="Chang, Christopher" name="citation_author" /> <meta content="Scott, Pat" name="citation_author" /> <meta content="Scaffidi, Andre" name="citation_author" /> <meta content="Mahmoudi, Farvah" name="citation_author" /> <meta content="Gonzalo, Tomás E." name="citation_author" /> <meta content="Fowlie, Andrew" name="citation_author" /> <meta content="Bloor, Sanjay" name="citation_author" /> <meta content="Kozar, Neal Avis" name="citation_author" /> <meta content="Raklev, Are" name="citation_author" /> <meta content="10.1140/epjc/s10052-021-09712-6" name="citation_doi" /> <meta content="Eur. 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Furthermore, we find large regions of viable parameter space where the EFT is valid and the relic density can be reproduced, implying that WIMPs can still account for the DM of the universe while being consistent with the latest data." property="og:description" />  <meta content="summary" name="twitter:card" /> <style></style> </head> <body class="CERN32Document32Server search" lang="ka">  <div id="cern-toolbar"> <h1><a href="http://cern.ch" title="CERN">CERN <span>Accelerating science</span></a></h1> <ul> <li class="cern-accountlinks"><a class="cern-account" href="https://cds.cern.ch/youraccount/login?ln=ka&referer=https%3A//cds.cern.ch/record/2771846%3Fln%3Dka" title="Sign in to your CERN account">Sign in</a></li> <li><a class="cern-directory" href="http://cern.ch/directory" title="Search CERN resources and browse the directory">Directory</a></li> </ul> </div>   <div role="banner" class="clearfix" id="header"> <div class="header-inner inner"> <hgroup class="clearfix"> <h2 id="site-name"> <a rel="home" title="Home" href="/"><span>CERN Document Server</span></a> </h2> <h3 id="site-slogan">Access articles, reports and multimedia content in HEP</h3> </hgroup> <div role="navigation" id="main-navigation" class="cdsmenu"> <h2 class="element-invisible">Main menu</h2><ul class="links inline clearfix"> <li class="menu-386 first active-trail"><a class="active-trail" href="https://cds.cern.ch/?ln=ka">ძებნა</a></li> <li class="menu-444 "><a class="" title="" href="https://cds.cern.ch/submit?ln=ka">დაყენება</a></li> <li class="menu-426 "><a class="" href="https://cds.cern.ch/help/?ln=ka">დახმარება</a></li> <li class="leaf hassubcdsmenu"> <a hreflang="en" class="header" href="https://cds.cern.ch/youraccount/display?ln=ka">პერს</a> <ul class="subsubcdsmenu"><li><a href="https://cds.cern.ch/youralerts/list?ln=ka">თქვენი ცვლილებები</a></li><li><a href="https://cds.cern.ch/yourbaskets/display?ln=ka">თქვენი კალათები</a></li><li><a href="https://cds.cern.ch/yourcomments?ln=ka">Your comments</a></li><li><a href="https://cds.cern.ch/youralerts/display?ln=ka">თქვენი ძებნა</a></li></ul></li> </ul> </div> </div> </div>  <table class="navtrailbox"> <tr> <td class="navtrailboxbody"> <a href="/?ln=ka" class="navtrail">მთავარი</a> > Thermal WIMPs and the Scale of New Physics: Global Fits of Dirac Dark Matter Effective Field Theories </td> </tr> </table> </div> <div class="pagebody"><div class="pagebodystripemiddle"> <div class="detailedrecordbox"> <div class="detailedrecordtabs"> <div> <ul class="detailedrecordtabs"><li class="on first"><a href="/record/2771846/?ln=ka">ინფორმაცია </a></li><li class=""><a href="/record/2771846/files?ln=ka">Files </a></li></ul> <div id="tabsSpacer" style="clear:both;height:0px"> </div></div> </div> <div class="detailedrecordboxcontent"> <div class="top-left-folded"></div> <div class="top-right-folded"></div> <div class="inside">  <abbr class="unapi-id" title="2771846"></abbr> <style type="text/css">  </style> <table class="formatRecordTableFullWidth" > <tr> <td class="formatRecordHeader" style="background-image: url('https://cds.cern.ch/img/journals.jpg');" colspan="2">  Article </td> </tr> <script type="text/javascript"> $( document ).ready(function() { $('.showAuthor').on('click', function() { var author = '<p>' + $(this).data('name') + '</p>'; var affiliation = $(this).data('affiliation') + '</br>'; var contribution = $(this).data('contribution') + '</br>'; $.magnificPopup.open({ items: { src: '<div id="ovelary-mathjax" class="overlay-white oc-content overlay-white-500">' + author + affiliation + contribution + '</div>', type: 'inline' }, callbacks: { open: function() { var div = document.getElementById("overlay-mathjax") MathJax.Hub.Queue(["Typeset", MathJax.Hub, div]); }, } }) }) }); </script> <tr><td class="formatRecordLabel"> Report number </td><td style="padding-left:5px;"><a href="http://arxiv.org/abs/arXiv:2106.02056">arXiv:2106.02056</a> ; ADP-21-9/T1156 ; CERN-TH-2021-084 ; CP3-21-15 ; P3H-21-038 ; TTK-21-19, gambit-physics-21 ; TTK-21-19, gambit-physics-2021</td></tr> <tr><td class="formatRecordLabel"> Title </td><td style="padding-left:5px;"><b>Thermal WIMPs and the Scale of New Physics: Global Fits of Dirac Dark Matter Effective Field Theories</b></td></tr> <tr><td class="formatRecordLabel"><span style="white-space:nowrap;"> Author(s) </span> </td><td style="padding-left:5px;"> <script type="text/javascript"> function toggle_authors_visibility(){ var more = document.getElementById('more'); var link = document.getElementById('link'); var extension = document.getElementById('extension'); if (more.style.display=='none'){ more.style.display = ''; extension.style.display = 'none'; link.innerHTML = "დამალვა" } else { more.style.display = 'none'; extension.style.display = ''; link.innerHTML = "ყველა 26 ავტორის ჩვენება " } link.style.color = "rgb(204,0,0);" } function set_up(){ var extension = document.getElementById('extension'); extension.innerHTML = "GAMBIT Collaboration "; toggle_authors_visibility(); } </script> <a name="show_hide" /><p id="more" style=""><a href="https://cds.cern.ch/search?f=author&p=Athron%2C%20Peter&ln=ka">Athron, Peter</a> (Monash U. ; Nanjing Normal U.) ; <a href="https://cds.cern.ch/search?f=author&p=Kozar%2C%20Neal%20Avis&ln=ka">Kozar, Neal Avis</a> (CPARC ; Queen's U., Kingston) ; <a href="https://cds.cern.ch/search?f=author&p=Bal%C3%A1zs%2C%20Csaba&ln=ka">Balázs, Csaba</a> (Monash U.) ; <a href="https://cds.cern.ch/search?f=author&p=Beniwal%2C%20Ankit&ln=ka">Beniwal, Ankit</a> (Louvain U., CP3) ; <a href="https://cds.cern.ch/search?f=author&p=Bloor%2C%20Sanjay&ln=ka">Bloor, Sanjay</a> (Imperial Coll., London ; Queensland U.) ; <a href="https://cds.cern.ch/search?f=author&p=Bringmann%2C%20Torsten&ln=ka">Bringmann, Torsten</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Brod%2C%20Joachim&ln=ka">Brod, Joachim</a> (Cincinnati U.) ; <a href="https://cds.cern.ch/search?f=author&p=Chang%2C%20Christopher&ln=ka">Chang, Christopher</a> (Queensland U.) ; <a href="https://cds.cern.ch/search?f=author&p=Cornell%2C%20Jonathan%20M.&ln=ka">Cornell, Jonathan M.</a> (Weber State U.) ; <a href="https://cds.cern.ch/search?f=author&p=Farmer%2C%20Ben&ln=ka">Farmer, Ben</a> (ASP, Melbourne) ; <a href="https://cds.cern.ch/search?f=author&p=Fowlie%2C%20Andrew&ln=ka">Fowlie, Andrew</a> (Nanjing Normal U.) ; <a href="https://cds.cern.ch/search?f=author&p=Gonzalo%2C%20Tom%C3%A1s%20E.&ln=ka">Gonzalo, Tomás E.</a> (Monash U. ; Aachen, Tech. Hochsch.) ; <a href="https://cds.cern.ch/search?f=author&p=Handley%2C%20Will&ln=ka">Handley, Will</a> (Cambridge U., KICC ; Cambridge U.) ; <a href="https://cds.cern.ch/search?f=author&p=Kahlhoefer%2C%20Felix&ln=ka">Kahlhoefer, Felix</a> (Aachen, Tech. Hochsch.) ; <a href="https://cds.cern.ch/search?f=author&p=Kvellestad%2C%20Anders&ln=ka">Kvellestad, Anders</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Mahmoudi%2C%20Farvah&ln=ka">Mahmoudi, Farvah</a> (IP2I, Lyon ; CERN) ; <a href="https://cds.cern.ch/search?f=author&p=Prim%2C%20Markus%20T.&ln=ka">Prim, Markus T.</a> (Bonn U.) ; <a href="https://cds.cern.ch/search?f=author&p=Raklev%2C%20Are&ln=ka">Raklev, Are</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Renk%2C%20Janina%20J.&ln=ka">Renk, Janina J.</a> (Imperial Coll., London ; Stockholm U. (main)) ; <a href="https://cds.cern.ch/search?f=author&p=Scaffidi%2C%20Andre&ln=ka">Scaffidi, Andre</a> (ARC, CoEPP, Australia ; Adelaide U. ; INFN, Turin) ; <a href="https://cds.cern.ch/search?f=author&p=Scott%2C%20Pat&ln=ka">Scott, Pat</a> (Imperial Coll., London ; Queensland U.) ; <a href="https://cds.cern.ch/search?f=author&p=St%C3%B6cker%2C%20Patrick&ln=ka">Stöcker, Patrick</a> (Aachen, Tech. Hochsch.) ; <a href="https://cds.cern.ch/search?f=author&p=Vincent%2C%20Aaron%20C.&ln=ka">Vincent, Aaron C.</a> (CPARC ; Queen's U., Kingston ; Perimeter Inst. Theor. Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=White%2C%20Martin&ln=ka">White, Martin</a> (ARC, CoEPP, Australia ; Adelaide U.) ; <a href="https://cds.cern.ch/search?f=author&p=Wild%2C%20Sebastian&ln=ka">Wild, Sebastian</a> (DESY) ; <a href="https://cds.cern.ch/search?f=author&p=Zupan%2C%20Jure&ln=ka">Zupan, Jure</a> (Cincinnati U.)</p> <span id="extension"></span> <small><i><a id="link" href="#" onclick="toggle_authors_visibility()" style="color:rgb(204,0,0);"></a></i></small><script type="text/javascript">set_up()</script></td></tr> <tr><td class="formatRecordLabel"> Publication </td><td style="padding-left:5px;">2021-11-11</td></tr> <tr><td class="formatRecordLabel"> Imprint </td><td style="padding-left:5px;">2021-06-03</td></tr> <tr><td class="formatRecordLabel"> Number of pages </td><td style="padding-left:5px;">37</td></tr> <tr><td class="formatRecordLabel"> Note </td><td style="padding-left:5px;">37 pages, 11 figures, 5 tables; v2: matches EPJC version</td></tr> <tr><td class="formatRecordLabel"> In: </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1140/epjc/s10052-021-09712-6"><i>Eur. Phys. J. C</i> 81 (2021) 992</a> </a></td></tr> <tr><td class="formatRecordLabel"> DOI </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1140/epjc/s10052-021-09712-6" title="DOI" target="_blank">10.1140/epjc/s10052-021-09712-6</a> (publication) <tr><td class="formatRecordLabel"> Subject category </td><td style="padding-left:5px;">astro-ph.CO ; Astrophysics and Astronomy ; hep-ph ; Particle Physics - Phenomenology</td></tr> <tr><td class="formatRecordLabel"> Accelerator/Facility, Experiment </td><td style="padding-left:5px;"><a href="https://cds.cern.ch/search?p=GAMBIT&f=693__a">GAMBIT</a></td></tr> <tr><td class="formatRecordLabel"> Abstract </td><td style="padding-left:5px;">We assess the status of a wide class of WIMP dark matter (DM) models in light of the latest experimental results using the global fitting framework $\textsf{GAMBIT}$. We perform a global analysis of effective field theory (EFT) operators describing the interactions between a gauge-singlet Dirac fermion and the Standard Model quarks, the gluons and the photon. In this bottom-up approach, we simultaneously vary the coefficients of 14 such operators up to dimension 7, along with the DM mass, the scale of new physics and several nuisance parameters. Our likelihood functions include the latest data from $\mathit{Planck}$, direct and indirect detection experiments, and the LHC. For DM masses below 100 GeV, we find that it is impossible to satisfy all constraints simultaneously while maintaining EFT validity at LHC energies. For new physics scales around 1 TeV, our results are influenced by several small excesses in the LHC data and depend on the prescription that we adopt to ensure EFT validity. Furthermore, we find large regions of viable parameter space where the EFT is valid and the relic density can be reproduced, implying that WIMPs can still account for the DM of the universe while being consistent with the latest data.</td></tr> <tr><td class="formatRecordLabel"> Copyright/License </td><td style="padding-left:5px;">publication: © 2021-2024 The Author(s)<br/>preprint: (License: <a href="http://creativecommons.org/licenses/by/4.0/">CC BY 4.0</a>)</td></tr> </table> <br /><div style="max-width:1024px;margin:auto"><div style="overflow-x:auto;display:inline;width:100%;"><a href="/record/2771846/plots#0"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2771846/files/EFT_illustration.png" title=" Illustration of our approach for studying DM EFTs compared to a more naive approach, in which one only uses the experiment that yields the strongest bound on $C / \La^2$. The resulting exclusion is indicated by the red shaded region. By independently varying $\La$, we can include additional information from experiments that give weaker bounds on $C / \La^2$ but for which the EFT has a larger range of validity. The additional exclusion obtained in this way is indicated by the blue shaded region. The region of parameter space that corresponds to the non-perturbative values of Wilson coefficient $C$ is excluded in either approach (shaded brown)." width="200px"/></a> <a href="/record/2771846/plots#1"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2771846/files/Dim_6_DMEFT_22_21_like2D_capped_hard_ext.png" title=" Profile likelihood in the $m_\chi$--$\La$ plane when considering only dimension-6 operators and capping the LHC likelihood at the value of the background-only hypothesis. The white contours indicate the $1\sigma$ and $2\sigma$ confidence regions and the best-fit point is indicated by the white star. The shaded region (corresponding to $\La \leq 2 m_\chi$) is excluded by the EFT validity requirement. In the right panel, the parameter ranges have been restricted to the most interesting region. Note that the position of the best-fit points in the two panels is somewhat arbitrary, as there is a degeneracy between $\La$ and $\mathcal{C}_{3,4}^{(6)}$ and hence the likelihood is essentially constant across the entire yellow region (see also Fig.~\ref{fig:dim_6_capped_coefficients})." width="200px"/></a> <a href="/record/2771846/plots#2"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2771846/files/Dim_6_DMEFT_22_21_like2D_capped_hard.png" title=" Profile likelihood in the $m_\chi$--$\La$ plane when considering only dimension-6 operators and capping the LHC likelihood at the value of the background-only hypothesis. The white contours indicate the $1\sigma$ and $2\sigma$ confidence regions and the best-fit point is indicated by the white star. The shaded region (corresponding to $\La \leq 2 m_\chi$) is excluded by the EFT validity requirement. In the right panel, the parameter ranges have been restricted to the most interesting region. Note that the position of the best-fit points in the two panels is somewhat arbitrary, as there is a degeneracy between $\La$ and $\mathcal{C}_{3,4}^{(6)}$ and hence the likelihood is essentially constant across the entire yellow region (see also Fig.~\ref{fig:dim_6_capped_coefficients})." width="200px"/></a> <a href='/record/2771846/plots'>Show more plots</a></div></div><br /> <br/>Corresponding record in: <a href="http://inspirehep.net/record/1867194">Inspire</a> <small> </small> <br/> <br/><br/><div align="right"><div style="padding-bottom:2px;padding-top:30px;"><span class="moreinfo" style="margin-right:10px;"> <a href="" class="moreinfo">Back to search</a> </span></div></div> <div class="bottom-left-folded"><div class="recordlastmodifiedbox" style="position:relative;margin-left:1px"> ჩანაწერი შექმნილია 2021-06-08, ბოლოს შესწორებულია 2024-01-19</div></div> <div class="bottom-right-folded" style="text-align:right;padding-bottom:2px;"> <span class="moreinfo" style="margin-right:10px;"><a href="/search?ln=ka&p=recid%3A2771846&rm=wrd" class="moreinfo">მსგავსი ჩანაწერები</a></span></div> </div> </div> </div> <br/> <br /> <div class="detailedrecordminipanel"> <div class="top-left"></div><div class="top-right"></div> <div class="inside"> <div id="detailedrecordminipanelfile" style="width:33%;float:left;text-align:center;margin-top:0"> <div><small class="detailedRecordActions">სრული ტექსტი:</small> <br /><em>2106.02056</em> - <a href="/record/2771846/files/2106.02056.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="სრული ტექსტის ჩამოტვირთვა"/>PDF</a><br /><em>document</em> - <a href="/record/2771846/files/document.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="სრული ტექსტის ჩამოტვირთვა"/>PDF</a><br /></div> </div> <div id="detailedrecordminipanelreview" style="width:30%;float:left;text-align:center"> </div> <div id="detailedrecordminipanelactions" style="width:36%;float:right;text-align:right;"> <ul class="detailedrecordactions"> <li><a href="/yourbaskets/add?ln=ka&recid=2771846">პირად კალათაში დამატება</a></li> <li>ექსპორტირება <a style="text-decoration:underline;font-weight:normal" href="/record/2771846/export/hx?ln=ka">BibTeX</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2771846/export/hm?ln=ka">MARC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2771846/export/xm?ln=ka">MARCXML</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2771846/export/xd?ln=ka">DC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2771846/export/xe?ln=ka">EndNote</a>,  <a style="text-decoration:underline;font-weight:normal" href="/record/2771846/export/xn?ln=ka">NLM</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2771846/export/xw?ln=ka">RefWorks</a> </li> </ul> <div style='padding-left: 13px;'>  <div id="bookmark"></div> <div id="bookmark_sciencewise"></div> <style type="text/css"> #bookmark_sciencewise, #bookmark {float: left;} #bookmark_sciencewise li {padding: 2px; width: 25px;} #bookmark_sciencewise ul, #bookmark ul {list-style-image: none;} </style> <script type="text/javascript" src="/js/jquery.bookmark.min.js"></script> <style type="text/css">@import "/css/jquery.bookmark.css";</style> <script type="text/javascript">// <![CDATA[ $.bookmark.addSite('sciencewise', 'ScienceWise.info', 'https://cds.cern.ch/img/sciencewise.png', 'en', 'bookmark', 'http://sciencewise.info/bookmarks/2106.0205/add'); $('#bookmark_sciencewise').bookmark({sites: ['sciencewise']}); $('#bookmark').bookmark({ sites: ['facebook', 'twitter', 'linkedin', 'google_plusone'], icons: '/img/bookmarks.png', url: 'https://cds.cern.ch/record/2771846', addEmail: true, title: "Thermal WIMPs and the Scale of New Physics: Global Fits of Dirac Dark Matter Effective Field Theories", description: "We assess the status of a wide class of WIMP dark matter (DM) models in light of the latest experimental results using the global fitting framework GAMBIT. We perform a global analysis of effective field theory (EFT) operators describing the interactions between a gauge-singlet Dirac fermion and the Standard Model quarks, the gluons and the photon. In this bottom-up approach, we simultaneously vary the coefficients of 14 such operators up to dimension 7, along with the DM mass, the scale of new physics and several nuisance parameters. Our likelihood functions include the latest data from Planck, direct and indirect detection experiments, and the LHC. For DM masses below 100\u00a0GeV, we find that it is impossible to satisfy all constraints simultaneously while maintaining EFT validity at LHC energies. For new physics scales around 1\u00a0TeV, our results are influenced by several small excesses in the LHC data and depend on the prescription that we adopt to ensure EFT validity. 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