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Collider constraints on electroweakinos in the presence of a light gravitino - CERN Document Server

<!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.0 Transitional//EN" "http://www.w3.org/TR/xhtml1/DTD/xhtml1-transitional.dtd"> <!--[if IEMobile 7]><html class="iem7" xmlns="http://www.w3.org/1999/xhtml" lang="en" xml:lang="en" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if lte IE 6]><html class="ie6 ie6-7 ie6-8" xmlns="http://www.w3.org/1999/xhtml" lang="en" xml:lang="en" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if (IE 7)&(!IEMobile)]><html class="ie7 ie6-7 ie6-8" xmlns="http://www.w3.org/1999/xhtml" lang="en" xml:lang="en" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if IE 8]><html class="ie8 ie6-8" xmlns="http://www.w3.org/1999/xhtml" lang="en" xml:lang="en" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if (gte IE 9)|(gt IEMobile 7)]><!--><html xmlns="http://www.w3.org/1999/xhtml" lang="en" xml:lang="en" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><!--<![endif]--> <head> <title>Collider constraints on electroweakinos in the presence of a light gravitino - CERN Document Server</title> <link href='https://framework.web.cern.ch/framework/2.0/fonts/PTSansWeb/PTSansWeb.css' rel='stylesheet' type='text/css' /> <link rel="stylesheet" href="https://cds.cern.ch/img/invenio.css?v=20141127" type="text/css" /> <link rel="stylesheet" href="https://cds.cern.ch/img/cern_theme/css/cern_theme.css?v=20141127" type="text/css" /> <link rel="stylesheet"href="/css/font-awesome.min.css"> <meta http-equiv="X-UA-Compatible" content="IE=Edge"/> <link rel="stylesheet" href="https://cds.cern.ch/img/cern_toolbar/css/toolbar.css" type="text/css" /> <!--[if lt IE 8]> <link href="https://cds.cern.ch/img/cern_toolbar/css/toolbar-ie.css" rel="stylesheet" type="text/css"> <![endif]--> <!--[if lt IE 8]> <link rel="stylesheet" type="text/css" href="https://cds.cern.ch/img/invenio-ie7.css" /> <![endif]--> <!--[if gt IE 8]> <style type="text/css">div.restrictedflag {filter:none;}</style> <![endif]--> <link rel="canonical" href="https://cds.cern.ch/record/2852808" /> <link rel="alternate" hreflang="el" href="https://cds.cern.ch/record/2852808?ln=el" /> <link rel="alternate" hreflang="fr" href="https://cds.cern.ch/record/2852808?ln=fr" /> <link rel="alternate" hreflang="bg" href="https://cds.cern.ch/record/2852808?ln=bg" /> <link rel="alternate" hreflang="zh-TW" href="https://cds.cern.ch/record/2852808?ln=zh_TW" /> <link rel="alternate" hreflang="pt" href="https://cds.cern.ch/record/2852808?ln=pt" /> <link rel="alternate" hreflang="no" href="https://cds.cern.ch/record/2852808?ln=no" /> <link rel="alternate" hreflang="hr" href="https://cds.cern.ch/record/2852808?ln=hr" /> <link rel="alternate" hreflang="ca" href="https://cds.cern.ch/record/2852808?ln=ca" /> <link rel="alternate" hreflang="de" href="https://cds.cern.ch/record/2852808?ln=de" /> <link rel="alternate" hreflang="it" href="https://cds.cern.ch/record/2852808?ln=it" /> <link rel="alternate" hreflang="zh-CN" href="https://cds.cern.ch/record/2852808?ln=zh_CN" /> <link rel="alternate" hreflang="sv" href="https://cds.cern.ch/record/2852808?ln=sv" /> <link rel="alternate" hreflang="sk" href="https://cds.cern.ch/record/2852808?ln=sk" /> <link rel="alternate" hreflang="en" href="https://cds.cern.ch/record/2852808?ln=en" /> <link rel="alternate" hreflang="pl" href="https://cds.cern.ch/record/2852808?ln=pl" /> <link rel="alternate" hreflang="ru" href="https://cds.cern.ch/record/2852808?ln=ru" /> <link rel="alternate" hreflang="ka" href="https://cds.cern.ch/record/2852808?ln=ka" /> <link rel="alternate" hreflang="ja" href="https://cds.cern.ch/record/2852808?ln=ja" /> <link rel="alternate" hreflang="es" href="https://cds.cern.ch/record/2852808?ln=es" /> <link rel="alternate" type="application/rss+xml" title="CERN Document Server RSS" href="/rss?ln=en" /> <link rel="search" type="application/opensearchdescription+xml" href="https://cds.cern.ch/opensearchdescription" title="CERN Document Server" /> <link rel="unapi-server" type="application/xml" title="unAPI" href="https://cds.cern.ch/unapi" /> <link rel="apple-touch-icon" href="/apple-touch-icon.png"/> <link rel="apple-touch-icon-precomposed" href="/apple-touch-icon-precomposed.png"/> <meta http-equiv="Content-Type" content="text/html; charset=utf-8" /> <meta http-equiv="Content-Language" content="en" /> <meta name="description" content="Using the GAMBIT global fitting framework, we constrain the MSSM with an eV-scale gravitino as the lightest supersymmetric particle, and the six electroweakinos (neutralinos and charginos) as the only other light new states. We combine 15 ATLAS and 12 CMS searches at 13 TeV, along with a large collection of ATLAS and CMS measurements of Standard Model signatures. This model, which we refer to as the ${{\tilde{G}}}$-EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic ${{\tilde{G}}}$-EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the ${{\tilde{G}}}$-EWMSSM parameter space is excluded, we find several viable parameter regions that predict phenomenologically rich scenarios with multiple neutralinos and charginos within the kinematic reach of the LHC during Run 3, or the High Luminosity LHC. In particular, we identify scenarios with Higgsino-dominated electroweakinos as light as 140 GeV that are consistent with our combined set of collider searches and measurements. The full set of ${{\tilde{G}}}$-EWMSSM parameter samples and GAMBIT input files generated for this work is available via Zenodo. Using the GAMBIT global fitting framework, we constrain the MSSM with an eV-scale gravitino as the lightest supersymmetric particle, and the six electroweakinos (neutralinos and charginos) as the only other light new states. We combine 15 ATLAS and 12 CMS searches at 13 TeV, along with a large collection of ATLAS and CMS measurements of Standard Model signatures. This model, which we refer to as the $\tilde G$-EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic $\tilde G$-EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the $\tilde G$-EWMSSM parameter space is excluded, we find several viable parameter regions that predict phenomenologically rich scenarios with multiple neutralinos and charginos within the kinematic reach of the LHC during Run 3, or the High Luminosity LHC. In particular, we identify scenarios with Higgsino-dominated electroweakinos as light as 140 GeV that are consistent with our combined set of collider searches and measurements. The full set of $\tilde G$-EWMSSM parameter samples and GAMBIT input files generated for this work is available via Zenodo. Ananyev, Viktor; Balázs, Csaba; Beniwal, Ankit; Braseth, Lasse Lorentz; Buckley, Andy; Butterworth, Jonathan; Chang, Christopher; Danninger, Matthias; Fowlie, Andrew; Gonzalo, Tomás E.; Kvellestad, Anders; Mahmoudi, Farvah; Martinez, Gregory D.; Prim, Markus T.; Procter, Tomasz; Raklev, Are; Scott, Pat; Stöcker, Patrick; Abeele, Jeriek Van den; White, Martin; Zhang, Yang" /> <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> <!-- WebNews CSS library --> <link rel="stylesheet" href="https://cds.cern.ch/img/webnews.css" type="text/css" /> <!-- WebNews JS library --> <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> <!-- GoogleScholar --> <meta content="Springer : Collider constraints on electroweakinos in the presence of a light gravitino" name="citation_title" /> <meta content="Ananyev, Viktor" name="citation_author" /> <meta content="Braseth, Lasse Lorentz" name="citation_author" /> <meta content="Scott, Pat" name="citation_author" /> <meta content="Danninger, Matthias" name="citation_author" /> <meta content="Mahmoudi, Farvah" name="citation_author" /> <meta content="Stöcker, Patrick" name="citation_author" /> <meta content="Raklev, Are" name="citation_author" /> <meta content="Gonzalo, Tomás E." name="citation_author" /> <meta content="White, Martin" name="citation_author" /> <meta content="Prim, Markus T." name="citation_author" /> <meta content="Beniwal, Ankit" name="citation_author" /> <meta content="Procter, Tomasz" name="citation_author" /> <meta content="Butterworth, Jonathan" name="citation_author" /> <meta content="Buckley, Andy" name="citation_author" /> <meta content="Fowlie, Andrew" name="citation_author" /> <meta content="Kvellestad, Anders" name="citation_author" /> <meta content="Zhang, Yang" name="citation_author" /> <meta content="Balázs, Csaba" name="citation_author" /> <meta content="Chang, Christopher" name="citation_author" /> <meta content="Martinez, Gregory D." name="citation_author" /> <meta content="Abeele, Jeriek Van den" name="citation_author" /> <meta content="10.1140/epjc/s10052-023-11574-z" name="citation_doi" /> <meta content="Eur. 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framework, we constrain the MSSM with an eV-scale gravitino as the lightest supersymmetric particle, and the six electroweakinos (neutralinos and charginos) as the only other light new states. We combine 15 ATLAS and 12 CMS searches at 13 TeV, along with a large collection of ATLAS and CMS measurements of Standard Model signatures. This model, which we refer to as the ${{\tilde{G}}}$-EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic ${{\tilde{G}}}$-EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the ${{\tilde{G}}}$-EWMSSM parameter space is excluded, we find several viable parameter regions that predict phenomenologically rich scenarios with multiple neutralinos and charginos within the kinematic reach of the LHC during Run 3, or the High Luminosity LHC. In particular, we identify scenarios with Higgsino-dominated electroweakinos as light as 140 GeV that are consistent with our combined set of collider searches and measurements. The full set of ${{\tilde{G}}}$-EWMSSM parameter samples and GAMBIT input files generated for this work is available via Zenodo." property="og:description" /> <meta content="arXiv" property="og:description" /> <meta content="Using the GAMBIT global fitting framework, we constrain the MSSM with an eV-scale gravitino as the lightest supersymmetric particle, and the six electroweakinos (neutralinos and charginos) as the only other light new states. We combine 15 ATLAS and 12 CMS searches at 13 TeV, along with a large collection of ATLAS and CMS measurements of Standard Model signatures. This model, which we refer to as the $\tilde G$-EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic $\tilde G$-EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the $\tilde G$-EWMSSM parameter space is excluded, we find several viable parameter regions that predict phenomenologically rich scenarios with multiple neutralinos and charginos within the kinematic reach of the LHC during Run 3, or the High Luminosity LHC. In particular, we identify scenarios with Higgsino-dominated electroweakinos as light as 140 GeV that are consistent with our combined set of collider searches and measurements. 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Collider constraints on electroweakinos in the presence of a light gravitino </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/2852808/?ln=en">Information </a></li><li class=""><a href="/record/2852808/files?ln=en">Files </a></li></ul> <div id="tabsSpacer" style="clear:both;height:0px">&nbsp;</div></div> </div> <div class="detailedrecordboxcontent"> <div class="top-left-folded"></div> <div class="top-right-folded"></div> <div class="inside"> <!--<div style="height:0.1em;">&nbsp;</div> <p class="notopgap">&nbsp;</p>--> <abbr class="unapi-id" title="2852808"></abbr> <style type="text/css"> <!-- ul.detailedrecordtabs li.on a{background-color:#4D94CC;color:#fff !important;border-bottom:1px solid #4D94CC!important;} div.detailedrecordboxcontent {padding-top:0px !important;} --> </style> <table class="formatRecordTableFullWidth" > <tr> <td class="formatRecordHeader" style="background-image: url('https://cds.cern.ch/img/journals.jpg');" colspan="2"> <!--YTD: record may have more than one 690C.a tag--> 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:2303.09082">arXiv:2303.09082</a> ; TTP23-009 ; KCL-PH-TH/2023-21 ; gambit-physics-23 ; MCnet-23-05, ADP-23-08/T1217 ; CERN-TH-2023-043</td></tr> <tr><td class="formatRecordLabel"> Title </td><td style="padding-left:5px;"><b>Collider constraints on electroweakinos in the presence of a light gravitino</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 = "Hide" } else { more.style.display = 'none'; extension.style.display = ''; link.innerHTML = "Show all 21 authors" } link.style.color = "rgb(204,0,0);" } function set_up(){ var extension = document.getElementById('extension'); extension.innerHTML = "GAMBIT Collaboration&nbsp;"; toggle_authors_visibility(); } </script> <a name="show_hide" /><p id="more" style=""><a href="https://cds.cern.ch/search?f=author&amp;p=Ananyev%2C%20Viktor&amp;ln=en">Ananyev, Viktor</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Bal%C3%A1zs%2C%20Csaba&amp;ln=en">Balázs, Csaba</a> (Monash U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Beniwal%2C%20Ankit&amp;ln=en">Beniwal, Ankit</a> (King's Coll. London (main)) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Braseth%2C%20Lasse%20Lorentz&amp;ln=en">Braseth, Lasse Lorentz</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Buckley%2C%20Andy&amp;ln=en">Buckley, Andy</a> (Glasgow U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Butterworth%2C%20Jonathan&amp;ln=en">Butterworth, Jonathan</a> (University Coll. London) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Chang%2C%20Christopher&amp;ln=en">Chang, Christopher</a> (Queensland U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Danninger%2C%20Matthias&amp;ln=en">Danninger, Matthias</a> (Simon Fraser U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Fowlie%2C%20Andrew&amp;ln=en">Fowlie, Andrew</a> (XJTLU, Suzhou) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Gonzalo%2C%20Tom%C3%A1s%20E.&amp;ln=en">Gonzalo, Tomás E.</a> (KIT, Karlsruhe, TTP) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Kvellestad%2C%20Anders&amp;ln=en">Kvellestad, Anders</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Mahmoudi%2C%20Farvah&amp;ln=en">Mahmoudi, Farvah</a> (IP2I, Lyon) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Martinez%2C%20Gregory%20D.&amp;ln=en">Martinez, Gregory D.</a> (Southern California U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Prim%2C%20Markus%20T.&amp;ln=en">Prim, Markus T.</a> (Bonn U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Procter%2C%20Tomasz&amp;ln=en">Procter, Tomasz</a> (Glasgow U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Raklev%2C%20Are&amp;ln=en">Raklev, Are</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Scott%2C%20Pat&amp;ln=en">Scott, Pat</a> (Australian Natl. U., Canberra (main)) ; <a href="https://cds.cern.ch/search?f=author&amp;p=St%C3%B6cker%2C%20Patrick&amp;ln=en">Stöcker, Patrick</a> (RWTH Aachen U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Abeele%2C%20Jeriek%20Van%20den&amp;ln=en">Abeele, Jeriek Van den</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=White%2C%20Martin&amp;ln=en">White, Martin</a> (Adelaide U.) ; <a href="https://cds.cern.ch/search?f=author&amp;p=Zhang%2C%20Yang&amp;ln=en">Zhang, Yang</a> (Zhengzhou U. ; Beijing, Inst. Theor. Phys.)</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;">2023-06-10</td></tr> <tr><td class="formatRecordLabel"> Imprint </td><td style="padding-left:5px;">2023-03-16</td></tr> <tr><td class="formatRecordLabel"> Number of pages </td><td style="padding-left:5px;">38</td></tr> <tr><td class="formatRecordLabel"> Note </td><td style="padding-left:5px;">38 pages, 12 figures, 5 tables</td></tr> <tr><td class="formatRecordLabel"> In: </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1140/epjc/s10052-023-11574-z"><i>Eur. Phys. J. C</i> 83 (2023) 493</a> </a></td></tr> <tr><td class="formatRecordLabel"> DOI </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1140/epjc/s10052-023-11574-z" title="DOI" target="_blank">10.1140/epjc/s10052-023-11574-z</a> <tr><td class="formatRecordLabel"> Subject category </td><td style="padding-left:5px;">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&amp;f=693__a">GAMBIT</a></td></tr> <tr><td class="formatRecordLabel"> Abstract </td><td style="padding-left:5px;">Using the GAMBIT global fitting framework, we constrain the MSSM with an eV-scale gravitino as the lightest supersymmetric particle, and the six electroweakinos (neutralinos and charginos) as the only other light new states. We combine 15 ATLAS and 12 CMS searches at 13 TeV, along with a large collection of ATLAS and CMS measurements of Standard Model signatures. This model, which we refer to as the $\tilde G$-EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic $\tilde G$-EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the $\tilde G$-EWMSSM parameter space is excluded, we find several viable parameter regions that predict phenomenologically rich scenarios with multiple neutralinos and charginos within the kinematic reach of the LHC during Run 3, or the High Luminosity LHC. In particular, we identify scenarios with Higgsino-dominated electroweakinos as light as 140 GeV that are consistent with our combined set of collider searches and measurements. The full set of $\tilde G$-EWMSSM parameter samples and GAMBIT input files generated for this work is available via Zenodo.</td></tr> <tr><td class="formatRecordLabel"> Copyright/License </td><td style="padding-left:5px;">publication: &copy; 2023-2024 The Author(s) (License: <a href="http://creativecommons.org/licenses/by/4.0/">CC-BY-4.0</a>), sponsored by <a href="http://scoap3.org">SCOAP&#179;</a><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/2852808/plots#0"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2852808/files/chi01_BRs__mu__M1_900__M2_400__tanb_1.png" title=" Branching ratios for the lightest neutralino as a function of $\mu$, with $M_1=900$\,GeV, $M_2=400$\,GeV, and $\tan\beta=1$ (top) or $\tan\beta=10$ (bottom). The wino and Higgsino NLSP regions are shown in red and green, respectively. The pink line (dash dot) shows the combined branching ratio for decays to all states other than on-shell $(Z,h,\gamma) + \tilde{G}$. The thin, grey bar marks a parameter region where $m_{\tilde\chi_1^\pm} < m_{\tilde\chi_1^0}$." width="200px"/></a> <a href="/record/2852808/plots#1"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2852808/files/chi01_BRs__mu__M1_900__M2_400__tanb_10.png" title=" Branching ratios for the lightest neutralino as a function of $\mu$, with $M_1=900$\,GeV, $M_2=400$\,GeV, and $\tan\beta=1$ (top) or $\tan\beta=10$ (bottom). The wino and Higgsino NLSP regions are shown in red and green, respectively. The pink line (dash dot) shows the combined branching ratio for decays to all states other than on-shell $(Z,h,\gamma) + \tilde{G}$. The thin, grey bar marks a parameter region where $m_{\tilde\chi_1^\pm} < m_{\tilde\chi_1^0}$." width="200px"/></a> <a href="/record/2852808/plots#2"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2852808/files/MSSMEW_gravitino_152_151_like2D.png" title=" Profile likelihood in the $(m_{\tilde{\chi}_2^0},m_{\tilde{\chi}_1^0})$ plane (left) and in the $(m_{\tilde{\chi}_1^{\pm}},m_{\tilde{\chi}_1^{0}})$ plane (right). The contour lines show the $1\sigma$ and $2\sigma$ confidence regions. The best-fit point is marked by the white star." width="200px"/></a> <a href='/record/2852808/plots'>Show more plots</a></div></div><br /> <br/>Corresponding record in: <a href="http://inspirehep.net/record/2643056">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">&nbsp;Record created 2023-03-18, last modified 2024-01-10</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=en&amp;p=recid%3A2852808&amp;rm=wrd" class="moreinfo">Similar records</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">Fulltext:</small> <br /><em>document</em> - <a href="/record/2852808/files/document.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="Download fulltext"/>PDF</a><br /><em>2303.09082</em> - <a href="/record/2852808/files/2303.09082.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="Download fulltext"/>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=en&amp;recid=2852808">Add to personal basket</a></li> <li>Export as <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/hx?ln=en">BibTeX</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/hm?ln=en">MARC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/xm?ln=en">MARCXML</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/xd?ln=en">DC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/xe?ln=en">EndNote</a>, <!-- <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/xe8x?ln=en">EndNote (8-X)</a>,--> <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/xn?ln=en">NLM</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2852808/export/xw?ln=en">RefWorks</a> </li> </ul> <div style='padding-left: 13px;'> <!-- JQuery Bookmark Button BEGIN --> <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/2303.0908/add'); $('#bookmark_sciencewise').bookmark({sites: ['sciencewise']}); $('#bookmark').bookmark({ sites: ['facebook', 'twitter', 'linkedin', 'google_plusone'], icons: '/img/bookmarks.png', url: 'https://cds.cern.ch/record/2852808', addEmail: true, title: "Collider constraints on electroweakinos in the presence of a light gravitino", description: "Using the GAMBIT global fitting framework, we constrain the MSSM with an eV-scale gravitino as the lightest supersymmetric particle, and the six electroweakinos (neutralinos and charginos) as the only other light new states. We combine 15 ATLAS and 12 CMS searches at 13\u00a0TeV, along with a large collection of ATLAS and CMS measurements of Standard Model signatures. This model, which we refer to as the ${{\\tilde{G}}}$-EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic ${{\\tilde{G}}}$-EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the ${{\\tilde{G}}}$-EWMSSM parameter space is excluded, we find several viable parameter regions that predict phenomenologically rich scenarios with multiple neutralinos and charginos within the kinematic reach of the LHC during Run 3, or the High Luminosity LHC. In particular, we identify scenarios with Higgsino-dominated electroweakinos as light as 140\u00a0GeV that are consistent with our combined set of collider searches and measurements. 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