Search for pair-produced third-generation squarks decaying via charm quarks or in compressed supersymmetric scenarios in pp collisions at √s=8 TeV with the ATLAS detector
Metadatos
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American Physical Society
Fecha
2014-09-24Referencia bibliográfica
Aad, G., Abbott, B., Abdallah, J., Khalek, S. A., Aben, R., Abi, B., ... & Abreu, R. (2014). Search for pair-produced third-generation squarks decaying via charm quarks or in compressed supersymmetric scenarios in p p collisions at s= 8 TeV with the ATLAS detector. Physical Review D, 90(5), 052008. [https://doi.org/10.1103/PhysRevD.90.052008]
Patrocinador
ANPCyT; YerPhI, Armenia; Australian Research Council; BMWF, Austria; Austrian Science Fund (FWF); Azerbaijan National Academy of Sciences (ANAS); SSTC, Belarus; National Council for Scientific and Technological Development (CNPq); Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); Natural Sciences and Engineering Research Council of Canada; NRC, Canada; Canada Foundation for Innovation; CERN, Chile; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT); Chinese Academy of Sciences; Ministry of Science and Technology, China; National Natural Science Foundation of China; Departamento Administrativo de Ciencia, Tecnologia e Innovacion Colciencias; Ministry of Education, Youth & Sports - Czech Republic Czech Republic Government; DNRF, Denmark; Danish Natural Science Research Council; Lundbeckfonden; European Union (EU) European Union (EU) European Research Council (ERC); Centre National de la Recherche Scientifique (CNRS); CEA-DSM/IRFU, France; GNSF, Georgia; Federal Ministry of Education & Research (BMBF); German Research Foundation (DFG); HGF, Germany; Max Planck Society; Alexander von Humboldt Foundation; Greek Ministry of Development-GSRT; NSRF, Greece; Israel Science Foundation; MINERVA, Israel; German-Israeli Foundation for Scientific Research and Development; I-CORE, Israel; Benoziyo Center, Israel; Istituto Nazionale di Fisica Nucleare (INFN); Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science; CNRST, Morocco; FOM (The Netherlands) Netherlands Government; Netherlands Organization for Scientific Research (NWO) Netherlands Government; BRF, Norway; RCN, Norway; Ministry of Science and Higher Education, Poland; NCN, Poland; GRICES, Portugal; Portuguese Foundation for Science and Technology; MNE/IFA, Romania; Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; Slovenian Research Agency - Slovenia; MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC, Sweden; Wallenberg Foundation, Sweden; SER, Switzerland; Swiss National Science Foundation (SNSF); Cantons of Bern, Switzerland; Geneva, Switzerland; National Science Council of Taiwan; Ministry of Energy & Natural Resources - Turkey; Leverhulme Trust; United States Department of Energy (DOE); National Science Foundation (NSF); ICREA; Science & Technology Facilities Council (STFC) ST/J005533/1 ST/M001431/1 ST/L001144/1 ST/K50208X/1 ST/I000186/1 ST/H00095X/1 ST/L001179/1 ATLAS Upgrades ST/J004928/1 ATLAS Upgrade ST/M003213/1 ST/M002306/1 ST/K001361/1 MINOS/MINOS+ ST/H00100X/1 ST/J005525/1 ST/J005576/1 ST/K003658/1 GRIDPP PP/E000487/1 ST/M001474/1 ST/K003437/1 GRIDPP ST/K501840/1 GRIDPP ST/M001733/1 ST/H001026/1 ST/K001361/1 LHCb Upgrades ST/K001361/1 ATLAS Upgrades ST/K001310/1 LHCb Upgrades ST/K001310/1 ATLAS Upgrades ST/J500641/1 ST/I006056/1 ST/G006717/1 ST/F00754X/1 ST/K00140X/1 ATLAS ST/H001093/1 ST/K003658/1 ST/I505756/1 ST/I006080/1 PP/E000444/1 ST/L006480/1 ST/L00352X/1 ST/L003112/1 ST/K001329/1 ATLAS ST/K001361/1 ST/K001310/1 ST/I006056/1 ATLAS Upgrades PP/D002915/1 ST/K001302/1 ST/J004928/1 ST/I00372X/1 GRIDPP ST/K00073X/1 ST/I000178/1 GRIDPP PP/E000347/1 ST/H00100X/2 ST/I005811/1 ST/K000713/1 ST/H00095X/2 ST/H001042/1 ST/I00372X/1 ST/J00474X/1 ATLAS Upgrades PP/E003087/1 ST/K001248/1 ST/K00137X/1 ST/L001209/1 ATLAS Upgrades ST/K001264/1 ATLAS ST/K000705/1 ST/I005803/1 ST/K001310/1 ATLAS ST/M000761/1 ST/L001195/1 ST/M007103/1 ATLAS Upgrades ST/G50228X/1 ST/K003437/1 ST/J00474X/1 ST/K001361/1 ATLAS ST/L003325/1 ST/M000664/1 ST/L001179/1 ST/J005487/1 ST/H001042/2 ST/M002306/1 ATLAS Upgrades ST/L006464/1 ST/K00140X/1 ST/K001337/1 ATLAS ST/H001093/2 ST/H001026/2 ST/K502236/1 ST/M002071/1 ATLAS Upgrades ST/K501840/1 ST/K001388/1 PP/E002846/1 ST/J002798/1 ST/L000970/1 ST/F007418/1 ST/I006056/1 ATLAS Upgrade ST/L000970/1 ATLAS Upgrade ST/K001426/1 ATLAS ST/K001361/1 LHCb ST/K001337/1 ST/K001310/1 LHCb ST/I005803/1 GRIDPP PP/E002757/1 PP/E000355/1 ST/K000659/1 ST/K001418/1 ST/L001179/1 ATLAS Upgrade ATLAS ST/G502320/1 ST/H001069/2 ST/J004944/1 ST/J005460/1 ST/J501074/1; Royal Society of LondonResumen
Results of a search for supersymmetry via direct production of third-generation squarks are reported, using 20.3 fb−1 of proton-proton collision data at √s=8 TeV recorded by the ATLAS experiment at the LHC in 2012. Two different analysis strategies based on monojetlike and c-tagged event selections are carried out to optimize the sensitivity for direct top squark-pair production in the decay channel to a charm quark and the lightest neutralino (˜t1→c+˜χ01) across the top squark–neutralino mass parameter space. No excess above the Standard Model background expectation is observed. The results are interpreted in the context of direct pair production of top squarks and presented in terms of exclusion limits in the (m˜t1, m˜χ01) parameter space. A top squark of mass up to about 240 GeV is excluded at 95% confidence level for arbitrary neutralino masses, within the kinematic boundaries. Top squark masses up to 270 GeV are excluded for a neutralino mass of 200 GeV. In a scenario where the top squark and the lightest neutralino are nearly degenerate in mass, top squark masses up to 260 GeV are excluded. The results from the monojetlike analysis are also interpreted in terms of compressed scenarios for top squark-pair production in the decay channel ˜t1→b+ff′+˜χ01 and sbottom pair production with ˜b1→b+˜χ01, leading to a similar exclusion for nearly mass-degenerate third-generation squarks and the lightest neutralino. The results in this paper significantly extend previous results at colliders.