TY - JOUR
T1 - Collider constraints on electroweakinos in the presence of a light gravitino
AU - GAMBIT Collaboration
AU - Ananyev, Viktor
AU - Balázs, Csaba
AU - Beniwal, Ankit
AU - Braseth, Lasse Lorentz
AU - Buckley, Andy
AU - Butterworth, Jonathan
AU - Chang, Christopher
AU - Danninger, Matthias
AU - Fowlie, Andrew
AU - Gonzalo, Tomás E.
AU - Kvellestad, Anders
AU - Mahmoudi, Farvah
AU - Martinez, Gregory D.
AU - Prim, Markus T.
AU - Procter, Tomasz
AU - Raklev, Are
AU - Scott, Pat
AU - Stöcker, Patrick
AU - Van den Abeele, Jeriek
AU - White, Martin
AU - Zhang, Yang
N1 - Funding Information:
We thank our colleagues in the GAMBIT Community for helpful discussions and comments. We also thank the ATLAS and CMS experiments for the resources they have made public to enable reinterpretations of their searches and measurements. For computing resources, we thank PRACE for awarding us access to Marconi at CINECA and Joliot-Curie at CEA. Computing resources were also provided by Sigma2, the National Infrastructure for HPC in Norway, under project NN9284K. AF was supported by the National Natural Science Foundation of China (NNSFC) Research Fund for International Excellent Young Scientists grant 1950410509. ABu and JB were supported by the UK Science and Technology Facilities Council (STFC) Consolidated Grant programme awards ST/S000887/1 and ST/S000666/1 respectively, ABe by STFC grant ST/T00679X/1, and TP by the STFC Doctoral Training Programme. The work of CB was supported by the Australian Research Council Discovery Project grant DP210101636. AK and AR were supported by the Research Council of Norway FRIPRO grant 323985. TEG was funded by the Deutsche Forschungsgemeinschaft (DFG) through the Emmy Noether Grant No. KA 4662/1-1. The work of VA was supported by the European Union Framework Programme for Research and Innovation Horizon 2020 (2014–2021) under the Marie Sklodowska-Curie Grant Agreement No. 765710. YZ was supported by the NNSFC under grant No. 12105248 and 12047503 (Peng-Huan-Wu Theoretical Physics Innovation Center). MJW is supported by the ARC Centre of Excellence for Dark Matter Particle Physics (CE200100008). We made use of pippi v2.2 [203] for this work.
Funding Information:
We thank our colleagues in the GAMBIT Community for helpful discussions and comments. We also thank the ATLAS and CMS experiments for the resources they have made public to enable reinterpretations of their searches and measurements. For computing resources, we thank PRACE for awarding us access to Marconi at CINECA and Joliot-Curie at CEA. Computing resources were also provided by Sigma2, the National Infrastructure for HPC in Norway, under project NN9284K. AF was supported by the National Natural Science Foundation of China (NNSFC) Research Fund for International Excellent Young Scientists grant 1950410509. ABu and JB were supported by the UK Science and Technology Facilities Council (STFC) Consolidated Grant programme awards ST/S000887/1 and ST/S000666/1 respectively, ABe by STFC grant ST/T00679X/1, and TP by the STFC Doctoral Training Programme. The work of CB was supported by the Australian Research Council Discovery Project grant DP210101636. AK and AR were supported by the Research Council of Norway FRIPRO grant 323985. TEG was funded by the Deutsche Forschungsgemeinschaft (DFG) through the Emmy Noether Grant No. KA 4662/1-1. The work of VA was supported by the European Union Framework Programme for Research and Innovation Horizon 2020 (2014–2021) under the Marie Sklodowska-Curie Grant Agreement No. 765710. YZ was supported by the NNSFC under grant No. 12105248 and 12047503 (Peng-Huan-Wu Theoretical Physics Innovation Center). MJW is supported by the ARC Centre of Excellence for Dark Matter Particle Physics (CE200100008). We made use of pippi v2.2 [] for this work.
Publisher Copyright:
© 2023, The Author(s).
PY - 2023/6
Y1 - 2023/6
N2 - 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 G~ -EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic G~ -EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the 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 G~ -EWMSSM parameter samples and GAMBIT input files generated for this work is available via Zenodo.
AB - 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 G~ -EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic G~ -EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the 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 G~ -EWMSSM parameter samples and GAMBIT input files generated for this work is available via Zenodo.
UR - http://www.scopus.com/inward/record.url?scp=85161903663&partnerID=8YFLogxK
U2 - 10.1140/epjc/s10052-023-11574-z
DO - 10.1140/epjc/s10052-023-11574-z
M3 - Article
AN - SCOPUS:85161903663
SN - 1434-6044
VL - 83
JO - European Physical Journal C
JF - European Physical Journal C
IS - 6
M1 - 493
ER -