4.7 Article

Search for supersymmetry at √s=13 TeV in final states with jets and two same-sign leptons or three leptons with the ATLAS detector

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EUROPEAN PHYSICAL JOURNAL C
卷 76, 期 5, 页码 -

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SPRINGER
DOI: 10.1140/epjc/s10052-016-4095-8

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资金

  1. ANPCyT, Argentina
  2. YerPhI, Armenia
  3. ARC, Australia
  4. BMWFW, Austria
  5. FWF, Austria
  6. ANAS, Azerbaijan
  7. SSTC, Belarus
  8. CNPq, Brazil
  9. FAPESP, Brazil
  10. NSERC, Canada
  11. NRC, Canada
  12. CFI, Canada
  13. CERN
  14. CONICYT, Chile
  15. CAS, China
  16. MOST, China
  17. NSFC, China
  18. COLCIENCIAS, Colombia
  19. MSMT CR, Czech Republic
  20. MPO CR, Czech Republic
  21. VSC CR, Czech Republic
  22. DNRF, Denmark
  23. DNSRC, Denmark
  24. IN2P3-CNRS, France
  25. CEA-DSM/IRFU, France
  26. GNSF, Georgia
  27. BMBF, Germany
  28. HGF, Germany
  29. MPG, Germany
  30. GSRT, Greece
  31. RGC, Hong Kong SAR, China
  32. ISF, Israel
  33. I-CORE, Israel
  34. Benoziyo Center, Israel
  35. INFN, Italy
  36. MEXT, Japan
  37. JSPS, Japan
  38. CNRST, Morocco
  39. FOM, Netherlands
  40. NWO, Netherlands
  41. RCN, Norway
  42. MNiSW, Poland
  43. NCN, Poland
  44. FCT, Portugal
  45. MNE/IFA, Romania
  46. MES of Russia, Russian Federation
  47. NRC KI, Russian Federation
  48. JINR
  49. MESTD, Serbia
  50. MSSR, Slovakia
  51. ARRS, Slovenia
  52. MIZS, Slovenia
  53. DST/NRF, South Africa
  54. MINECO, Spain
  55. SRC, Sweden
  56. Wallenberg Foundation, Sweden
  57. SERI, Switzerland
  58. SNSF, Switzerland
  59. Cantons of Bern, Switzerland
  60. Geneva, Switzerland
  61. MOST, Taiwan
  62. TAEK, Turkey
  63. STFC, United Kingdom
  64. DOE, United States of America
  65. NSF, United States of America
  66. BCKDF
  67. Canada Council, Canada
  68. CANARIE, Canada
  69. CRC, Canada
  70. Compute Canada, Canada
  71. FQRNT, Canada
  72. Ontario InnovationTrust, Canada
  73. EPLANET, European Union
  74. ERC, European Union
  75. FP7, European Union
  76. Horizon 2020, European Union
  77. Marie Sklodowska-Curie Actions, European Union
  78. Investissements d'Avenir Labex and Idex, France
  79. ANR, France
  80. Region Auvergne, France
  81. Fondation Partager le Savoir, France
  82. DFG, Germany
  83. AvH Foundation, Germany
  84. Herakleitos, Thales
  85. Aristeia programmes - EU-ESF
  86. Greek NSRF
  87. BSF, Israel
  88. GIF, Israel
  89. Minerva, Israel
  90. BRF, Norway
  91. Royal Society, United Kingdom
  92. Leverhulme Trust, United Kingdom
  93. Direct For Mathematical & Physical Scien
  94. Division Of Physics [1119200, 1410972] Funding Source: National Science Foundation
  95. Direct For Mathematical & Physical Scien
  96. Division Of Physics [1506173] Funding Source: National Science Foundation
  97. ICREA Funding Source: Custom
  98. STFC [ST/M000753/1, ST/N000307/1, ST/J005533/1, ST/J004804/1, ST/I005846/1, ST/L006162/1, ST/M006417/1, ST/K003666/1, ST/N000331/1, ST/K001361/1, ST/N000277/1, ST/J00488X/1, ST/L003449/1, ST/K001329/1, ST/L000997/1, ST/L001144/1, ST/L005662/1, ST/N000463/1, ST/M001431/1, ST/H001093/2] Funding Source: UKRI

向作者/读者索取更多资源

A search for strongly produced supersymmetric particles is conducted using signatures involving multiple energetic jets and either two isolated leptons (e or mu) with the same electric charge or at least three isolated leptons. The search also utilises b-tagged jets, missing transverse momentum and other observables to extend its sensitivity. The analysis uses a data sample of proton-proton collisions at root s = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 corresponding to a total integrated luminosity of 3.2 fb(-1). No significant excess over the Standard Model expectation is observed. The results are interpreted in several simplified supersymmetric models and extend the exclusion limits from previous searches. In the context of exclusive production and simplified decay modes, gluino masses are excluded at 95% confidence level up to 1.1-1.3 TeV for light neutralinos (depending on the decay channel), and bottom squark masses are also excluded up to 540 GeV. In the former scenarios, neutralino masses are also excluded up to 550-850 GeV for gluino masses around 1 TeV.

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