4.4 Article

Search for dark matter produced with an energetic jet or a hadronically decaying W or Z boson at √S=13 TeV

Journal

JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 7, Pages -

Publisher

SPRINGER
DOI: 10.1007/JHEP07(2017)014

Keywords

Jet substructure; Dark matter; Hadron-Hadron scattering (experiments); Exotics; Higgs physics

Funding

  1. Austrian Federal Ministry of Science, Research and Economy
  2. Austrian Science Fund
  3. Belgian Fonds de la Recherche Scientifique
  4. Fonds voor Wetenschappelijk Onderzoek
  5. CNPq
  6. CAPES
  7. FAPERJ
  8. FAPESP
  9. Bulgarian Ministry of Education and Science
  10. CERN
  11. Chinese Academy of Sciences
  12. Ministry of Science and Technology
  13. National Natural Science Foundation of China
  14. Colombian Funding Agency (COLCIENCIAS)
  15. Croatian Ministry of Science, Education and Sport
  16. Croatian Science Foundation
  17. Research Promotion Foundation, Cyprus
  18. Secretariat for Higher Education, Science, Technology and Innovation, Ecuador
  19. Ministry of Education and Research
  20. Estonian Research Council [IUT23-4, IUT23-6]
  21. European Regional Development Fund, Estonia
  22. Academy of Finland, Finnish Ministry of Education and Culture
  23. Helsinki Institute of Physics
  24. Institut National de Physique Nucleaire et de Physique des Particules / CNRS
  25. Commissariat a l'Energie Atomique et aux Energies Alternatives / CEA, France
  26. Bundesministerium fur Bildung und Forschung, Germany
  27. Deutsche Forschungsgemeinschaft, Germany
  28. Helmholtz-Gemeinschaft Deutscher Forschungszentren, Germany
  29. General Secretariat for Research and Technology, Greece
  30. National Scientific Research Foundation
  31. National Innovation Office, Hungary
  32. Department of Atomic Energy, India
  33. Department of Science and Technology, India
  34. Institute for Studies in Theoretical Physics and Mathematics, Iran
  35. Science Foundation, Ireland
  36. Istituto Nazionale di Fisica Nucleare, Italy
  37. Ministry of Science, ICT and Future Planning, Republic of Korea
  38. National Research Foundation (NRF), Republic of Korea
  39. Lithuanian Academy of Sciences
  40. Ministry of Education (Malaysia)
  41. University of Malaya (Malaysia)
  42. BUAP
  43. CINVESTAV
  44. CONACYT
  45. LNS
  46. SEP
  47. UASLP-FAI
  48. Ministry of Business, Innovation and Employment, New Zealand
  49. Pakistan Atomic Energy Commission
  50. Ministry of Science and Higher Education, Poland
  51. National Science Centre, Poland
  52. Fundacao para a Ciencia e a Tecnologia, Portugal
  53. JINR, Dubna
  54. Ministry of Education and Science of the Russian Federation
  55. Federal Agency of Atomic Energy of the Russian Federation
  56. Russian Academy of Sciences
  57. Russian Foundation for Basic Research
  58. Russian Competitiveness Program of NRNU MEPhI
  59. Ministry of Education, Science and Technological Development of Serbia
  60. Secretaria de Estado de Investigacion, Desarrollo e Innovacion, Programa Consolider-Ingenio, Plan de Ciencia, Tecnologia a e Innovacion del Principado de Asturias, Spain
  61. Fondo Europeo de Desarrollo Regional, Spain
  62. ETH Board
  63. ETH Zurich
  64. PSI
  65. SNF
  66. UniZH
  67. Canton Zurich
  68. SER
  69. Ministry of Science and Technology, Taipei
  70. Thailand Center of Excellence in Physics
  71. Institute for the Promotion of Teaching Science and Technology of Thailand
  72. Special Task Force for Activating Research
  73. National Science and Technology Development Agency of Thailand
  74. Scientific and Technical Research Council of Turkey
  75. Turkish Atomic Energy Authority
  76. National Academy of Sciences of Ukraine, Ukraine
  77. State Fund for Fundamental Researches, Ukraine
  78. Science and Technology Facilities Council, U.K.
  79. U.S. Department of Energy
  80. U.S. National Science Foundation
  81. Marie-Curie programme
  82. European Research Council
  83. EPLANET (European Union)
  84. Leventis Foundation
  85. A. P. Sloan Foundation
  86. Alexander von Humboldt Foundation
  87. Belgian Federal Science Policy Office
  88. Fonds pour la Formation a a la Recherche dans l'Industrie et dans l'Agriculture (FRIA-Belgium)
  89. Agentschap voor Innovatie door Wetenschap en Technologie (IWT-Belgium)
  90. Ministry of Education
  91. Youth and Sports (MEYS) of the Czech Republic
  92. Council of Scientific and Industrial Research, India
  93. HOMING PLUS programme of the Foundation for Polish Science
  94. European Union
  95. Regional Development Fund
  96. Mobility Plus programme of the Ministry of Science and Higher Education
  97. National Science Center (Poland)
  98. National Priorities Research Program by Qatar National Research Fund
  99. Programa Clarin-COFUND del Principado de Asturias
  100. Thalis and Aristeia programmes
  101. EU-ESF
  102. Greek NSRF
  103. Rachadapisek Sompot Fund for Postdoctoral Fellowship
  104. Chulalongkorn University
  105. Chulalongkorn Academic into Its 2nd Century Project Advancement Project (Thailand)
  106. Welch Foundation [C-1845]
  107. [2014/14/M/ST2/00428]
  108. [2014/13/B/ST2/02543]
  109. [2014/15/B/ST2/03998]
  110. [2015/19/B/ST2/02861]
  111. [2012/07/E/ST2/01406]
  112. Division Of Physics
  113. Direct For Mathematical & Physical Scien [1151640, 1506168] Funding Source: National Science Foundation
  114. Division Of Physics
  115. Direct For Mathematical & Physical Scien [1211067, 1624356, 1606321, 1506130] Funding Source: National Science Foundation
  116. Science and Technology Facilities Council [ST/H000925/1, GRIDPP, PP/E000479/1, ST/N003985/1, CMS] Funding Source: researchfish
  117. STFC [ST/H000925/1, ST/N003985/1, PP/E000479/1] Funding Source: UKRI

Ask authors/readers for more resources

A search for dark matter particles is performed using events with large missing transverse momentum, at least one energetic jet, and no leptons, in proton-proton collisions at root S = 13TeV collected with the CMS detector at the LHC. The data sample corresponds to an integrated luminosity of 12.9 fb(-1). The search includes events with jets from the hadronic decays of a W or Z boson. The data are found to be in agreement with the predicted background contributions from standard model processes. The results are presented in terms of simpli fi ed models in which dark matter particles are produced through interactions involving a vector, axial-vector, scalar, or pseudoscalar mediator. Vector and axial-vector mediator particles with masses up to 1.95TeV, and scalar and pseudoscalar mediator particles with masses up to 100 and 430 GeV respectively, are excluded at 95% con fi dence level. The results are also interpreted in terms of the invisible decays of the Higgs boson, yielding an observed (expected) 95% con fi dence level upper limit of 0.44 (0.56) on the corresponding branching fraction. The results of this search provide the strongest constraints on the dark matter pair production cross section through vector and axial-vector mediators at a particle collider. When compared to the direct detection experiments, the limits obtained from this search provide stronger constraints for dark matter masses less than 5, 9, and 550 GeV, assuming vector, scalar, and axial-vector mediators, respectively. The search yields stronger constraints for dark matter masses less than 200 GeV, assuming a pseudoscalar mediator, when compared to the indirect detection results from Fermi-LAT.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.4
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available