4.7 Article

Search for dark matter in events with heavy quarks and missing transverse momentum in pp collisions with the ATLAS detector

Journal

EUROPEAN PHYSICAL JOURNAL C
Volume 75, Issue 2, Pages -

Publisher

SPRINGER
DOI: 10.1140/epjc/s10052-015-3306-z

Keywords

-

Funding

  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. COLCIEN-CIAS, Colombia
  19. MSMT CR, Czech Republic
  20. MPO CR, Czech Republic
  21. VSC CR, Czech Republic
  22. DNRF, Denmark
  23. DNSRC, Denmark
  24. Lundbeck Foundation, Denmark
  25. EPLANET, European Union
  26. ERC, European Union
  27. NSRF, European Union
  28. IN2P3-CNRS, France
  29. CEA-DSM/IRFU, France
  30. GNSF, Georgia
  31. BMBF, Germany
  32. DFG, Germany
  33. HGF, Germany
  34. MPG, Germany
  35. AvH Foundation, Germany
  36. GSRT, Greece
  37. NSRF, Greece
  38. ISF, Israel
  39. MINERVA, Israel
  40. GIF, Israel
  41. I-CORE, Israel
  42. Benoziyo Center, Israel
  43. INFN, Italy
  44. MEXT, Japan
  45. JSPS, Japan
  46. CNRST, Morocco
  47. FOM, Netherlands
  48. NWO, Netherlands
  49. BRF, Norway
  50. RCN, Norway
  51. MNiSW, Poland
  52. NCN, Poland
  53. GRICES, Portugal
  54. FCT, Portugal
  55. MNE/IFA, Romania
  56. MES of Russia, Russian Federation
  57. ROSATOM, Russian Federation
  58. MSTD, Serbia
  59. JINR
  60. MSSR, Slovakia
  61. ARRS, Slovenia
  62. MIZS, Slovenia
  63. DST/NRF, South Africa
  64. MINECO, Spain
  65. SRC, Sweden
  66. Wallenberg Foundation, Sweden
  67. SER, Switzerland
  68. SNSF, Switzerland
  69. Canton of Bern, Switzerland
  70. Canton of Geneva, Switzerland
  71. NSC, Taiwan
  72. TAEK, Turkey
  73. STFC, United Kingdom
  74. Royal Society, United Kingdom
  75. Leverhulme Trust, United Kingdom
  76. DOE, United States of America
  77. NSF, United States of America
  78. Fundação para a Ciência e a Tecnologia [CERN/FIS-NUC/0005/2015] Funding Source: FCT
  79. Direct For Mathematical & Physical Scien
  80. Division Of Physics [1119200, 1404362, 1506173] Funding Source: National Science Foundation
  81. Science and Technology Facilities Council [ST/J501074/1, ST/M503575/1, ST/K50208X/1, ST/K001388/1, ST/M000664/1] Funding Source: researchfish
  82. STFC [ST/I000186/1, PP/E003087/1, ST/I005803/1, ST/N000277/1, ST/L000970/1, ST/M000664/1, ST/J005576/1, ST/M503575/1, ST/M002306/1, ST/L003511/1, ST/K001302/1, ST/L003325/1, ST/J004944/1, ST/M003213/1, ST/N000420/1, ST/M001504/1, ST/J00474X/1, ST/K00137X/1, ST/I006056/1, ST/L006480/1, ST/J501074/1, ST/M006980/1, ST/M001407/1, ST/K000705/1, ST/J005525/1, ST/J005487/1, ST/N000307/1, ST/L006464/1, ST/L001195/1, ST/I006080/1, ST/G502320/1, ST/L003414/1, ST/L001179/1, ST/K003658/1, ST/I00372X/1, ST/J004928/1, PP/E002846/1, PP/E000355/1, PP/D002915/1, ST/M004821/1, ST/K50208X/1, ST/L003112/1, ST/I000178/1, ST/K001388/1, ST/K001248/1, ST/G50228X/1, ST/K001329/1, ST/M001733/1, ST/H00100X/1, ST/H00100X/2] Funding Source: UKRI
  83. ICREA Funding Source: Custom

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This article reports on a search for dark matter pair production in association with bottom or top quarks in 20.3 fb(-1) of pp collisions collected at root s = 8 TeV by the ATLAS detector at the LHC. Events with large missing transverse momentum are selected when produced in association with high-momentum jets of which one or more are identified as jets containing b-quarks. Final states with top quarks are selected by requiring a high jet multiplicity and in some cases a single lepton. The data are found to be consistent with the Standard Model expectations and limits are set on the mass scale of effective field theories that describe scalar and tensor interactions between dark matter and Standard Model particles. Limits on the dark-matter-nucleon cross-section for spin-independent and spin-dependent interactions are also provided. These limits are particularly strong for low-mass dark matter. Using a simplified model, constraints are set on the mass of dark matter and of a coloured mediator suitable to explain a possible signal of annihilating dark matter.

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