4.4 Article

Search for resonant production of strongly coupled dark matter in proton-proton collisions at 13 TeV

Journal

JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 6, Pages -

Publisher

SPRINGER
DOI: 10.1007/JHEP06(2022)156

Keywords

Beyond Standard Model; Dark Matter; Hadron-Hadron Scattering

Funding

  1. BMBWF (Austria)
  2. FWF (Austria)
  3. FNRS (Belgium)
  4. FWO (Belgium)
  5. CNPq (Brazil)
  6. CAPES (Brazil)
  7. FAPERJ (Brazil)
  8. FAPERGS (Brazil)
  9. FAPESP (Brazil)
  10. MES (Bulgaria)
  11. BNSF (Bulgaria)
  12. CERN
  13. CAS (China)
  14. MoST (China)
  15. NSFC (China)
  16. MINCIENCIAS (Colombia)
  17. MSES (Croatia)
  18. CSF (Croatia)
  19. RIF (Cyprus)
  20. SENESCYT (Ecuador)
  21. MoER (Estonia)
  22. ERC PUT (Estonia)
  23. ERDF (Estonia)
  24. Academy of Finland (Finland)
  25. MEC (Finland)
  26. HIP (Finland)
  27. CEA (France)
  28. CNRS/IN2P3 (France)
  29. BMBF (Germany)
  30. DFG (Germany)
  31. HGF (Germany)
  32. GSRI (Greece)
  33. NKFIA (Hungary)
  34. DAE (India)
  35. DST (India)
  36. IPM (Iran)
  37. SFI (Ireland)
  38. INFN (Italy)
  39. MSIP (Republic of Korea)
  40. NRF (Republic of Korea)
  41. MES (Latvia)
  42. LAS (Lithuania)
  43. MOE (Malaysia)
  44. UM (Malaysia)
  45. BUAP (Mexico)
  46. CINVESTAV (Mexico)
  47. CONACYT (Mexico)
  48. LNS (Mexico)
  49. SEP (Mexico)
  50. UASLP-FAI (Mexico)
  51. MOS (Montenegro)
  52. MBIE (New Zealand)
  53. PAEC (Pakistan)
  54. MSHE (Poland)
  55. NSC (Poland)
  56. FCT (Portugal)
  57. JINR (Dubna)
  58. MON (Russia)
  59. RosAtom (Russia)
  60. RAS (Russia)
  61. RFBR (Russia)
  62. NRC KI (Russia)
  63. MESTD (Serbia)
  64. MCIN/AEI (Spain)
  65. PCTI (Spain)
  66. MOSTR (Sri Lanka)
  67. Swiss Funding Agencies (Switzerland)
  68. MST (Taipei)
  69. ThEPCenter (Thailand)
  70. IPST (Thailand)
  71. STAR (Thailand)
  72. NSTDA (Thailand)
  73. TUBITAK (Turkey)
  74. TAEK (Turkey)
  75. NASU (Ukraine)
  76. STFC (United Kingdom)
  77. DOE (U.S.A.)
  78. NSF (U.S.A.)
  79. Marie-Curie program (European Union)
  80. European Research Council (European Union)
  81. Horizon 2020 (European Union) [675440, 724704, 752730, 758316, 765710, 824093, 884104]
  82. COST Action (European Union) [CA16108]
  83. Leventis Foundation
  84. Alfred P. Sloan Foundation
  85. Alexander von Humboldt Foundation
  86. Belgian Federal Science Policy Office
  87. Fonds pour la Formation a la Recherche dans l'Industrie et dans l'Agriculture (FRIA-Belgium)
  88. Agentschap voor Innovatie door Wetenschap en Technologie (IWT-Belgium)
  89. F.R.S.-FNRS (Belgium) under the Excellence of Science -EOS -be.h project [30820817]
  90. FWO (Belgium) under the Excellence of Science -EOS -be.h project [30820817]
  91. Beijing Municipal Science & Technology Commission [Z191100007219010]
  92. Ministry of Education, Youth and Sports (MEYS) of the Czech Republic
  93. Deutsche Forschungsgemeinschaft (DFG) [EXC 2121, 390833306, 400140256 -GRK2497]
  94. Lendulet (Momentum) Program of the Hungarian Academy of Sciences
  95. Janos Bolyai Research Scholarship of the Hungarian Academy of Sciences
  96. New National Excellence Program UNKP
  97. NKFIA research grants (Hungary) [123842, 123959, 124845, 124850, 125105, 128713, 128786, 129058]
  98. Council of Science and Industrial Research, India
  99. Latvian Council of Science
  100. Ministry of Science and Higher Education (Poland)
  101. National Science Center [Opus 2014/15/B/ST2/03998, 2015/19/B/ST2/02861]
  102. Fundacao para a Ciencia e a Tecnologia (Portugal) [CEECIND/01334/2018]
  103. National Priorities Research Program by Qatar National Research Fund
  104. Ministry of Science and Higher Education (Russia) [14.W03.31.0026, FSWW-2020-0008]
  105. Russian Foundation for Basic Research (Russia) [19-42-703014]
  106. MCIN/AEI, ERDF a way of making Europe
  107. Programa Estatal de Fomento de la Investigacion Cientifica y Tecnica de Excelencia Maria de Maeztu (Spain) [MDM-2017-0765]
  108. Programa Severo Ochoa del Principado de Asturias (Spain)
  109. Stavros Niarchos Foundation (Greece)
  110. Rachadapisek Sompot Fund for Postdoctoral Fellowship, Chulalongkorn University (Thailand)
  111. Chulalongkorn Academic into Its 2nd Century Project Advancement Project (Thailand)
  112. Nvidia Corporation
  113. SuperMicro Corporation
  114. Welch Foundation [C-1845]
  115. Weston Havens Foundation (U.S.A.)

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The first collider search for dark matter from a strongly coupled hidden sector is presented. The study used a data sample corresponding to 138 fb(-1) collected with the CMS detector at the CERN LHC. No structure in the dijet transverse mass spectra compatible with the signal is observed.
The first collider search for dark matter arising from a strongly coupled hidden sector is presented and uses a data sample corresponding to 138 fb(-1), collected with the CMS detector at the CERN LHC, at root s = 13 TeV. The hidden sector is hypothesized to couple to the standard model (SM) via a heavy leptophobic Z' mediator produced as a resonance in proton-proton collisions. The mediator decay results in two semivisible jets, containing both visible matter and invisible dark matter. The final state therefore includes moderate missing energy aligned with one of the jets, a signature ignored by most dark matter searches. No structure in the dijet transverse mass spectra compatible with the signal is observed. Assuming the Z' boson has a universal coupling of 0.25 to the SM quarks, an inclusive search, relevant to any model that exhibits this kinematic behavior, excludes mediator masses of 1.5-4.0 TeV at 95% confidence level, depending on the other signal model parameters. To enhance the sensitivity of the search for this particular class of hidden sector models, a boosted decision tree (BDT) is trained using jet substructure variables to distinguish between semivisible jets and SM jets from background processes. When the BDT is employed to identify each jet in the dijet system as semivisible, the mediator mass exclusion increases to 5.1 TeV, for wider ranges of the other signal model parameters. These limits exclude a wide range of strongly coupled hidden sector models for the first time.

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