4.7 Article

Search for invisible decays of Higgs bosons in the vector boson fusion and associated ZH production modes

Journal

EUROPEAN PHYSICAL JOURNAL C
Volume 74, Issue 8, Pages -

Publisher

SPRINGER
DOI: 10.1140/epjc/s10052-014-2980-6

Keywords

-

Funding

  1. Austrian Federal Ministry of Science and Research
  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, Ministry of Science and Technology
  12. National Natural Science Foundation of China
  13. Colombian Funding Agency (COLCIENCIAS)
  14. Croatian Ministry of Science, Education and Sport
  15. Croatian Science Foundation
  16. Research Promotion Foundation, Cyprus
  17. Ministry of Education and Research [SF0690030s09]
  18. European Regional Development Fund, Estonia
  19. Academy of Finland, Finnish Ministry of Education and Culture
  20. Helsinki Institute of Physics
  21. Institut National de Physique Nucleaire et de Physique des Particules / CNRS
  22. Commissariat a l'Energie Atomique et aux Energies Alternatives / CEA, France
  23. Bundesministerium fur Bildung und Forschung
  24. Deutsche Forschungsgemeinschaft
  25. Helmholtz-Gemeinschaft Deutscher Forschungszentren, Germany
  26. General Secretariat for Research and Technology, Greece
  27. National Scientific Research Foundation
  28. National Innovation Office, Hungary
  29. Department of Atomic Energy, India
  30. Department of Science and Technology, India
  31. Institute for Studies in Theoretical Physics and Mathematics, Iran
  32. Science Foundation, Ireland
  33. Istituto Nazionale di Fisica Nucleare, Italy
  34. Korean Ministry of Education, Science and Technology
  35. World Class University program of NRF, Republic of Korea
  36. Lithuanian Academy of Sciences
  37. Ministry of Education and University of Malaya (Malaysia)
  38. CINVESTAV
  39. CONACYT
  40. SEP
  41. UASLP-FAI
  42. Ministry of Business, Innovation and Employment, New Zealand
  43. Pakistan Atomic Energy Commission
  44. Ministry of Science and Higher Education
  45. National Science Centre, Poland
  46. Fundacao para a Ciencia e a Tecnologia, Portugal
  47. JINR, Dubna
  48. Ministry of Education and Science of the Russian Federation
  49. Federal Agency of Atomic Energy of the Russian Federation
  50. Russian Academy of Sciences
  51. Russian Foundation for Basic Research
  52. Ministry of Education, Science and Technological Development of Serbia
  53. Secretaria de Estado de Investigacion, Desarrollo e Innovacion and Programa Consolider-Ingenio, Spain
  54. ETH Board
  55. ETH Zurich
  56. PSI
  57. SNF
  58. UniZH
  59. Canton Zurich
  60. SER
  61. National Science Council, Taipei
  62. Thailand Center of Excellence in Physics
  63. Institute for the Promotion of Teaching Science and Technology of Thailand
  64. Special Task Force for Activating Research
  65. National Science and Technology Development Agency of Thailand
  66. Scientific and Technical Research Council of Turkey
  67. Turkish Atomic Energy Authority
  68. National Academy of Sciences of Ukraine
  69. State Fund for Fundamental Researches, Ukraine
  70. Science and Technology Facilities Council, UK
  71. US Department of Energy
  72. US National Science Foundation
  73. Marie-Curie programme
  74. European Research Council
  75. EPLANET (European Union)
  76. Leventis Foundation
  77. A. P. Sloan Foundation
  78. Alexander von Humboldt Foundation
  79. Belgian Federal Science Policy Office
  80. Fonds pour la Formation la Recherche dans l'Industrie et dans l'Agriculture (FRIA-Belgium)
  81. Agentschap voor Innovatie door Wetenschap en Technologie (IWT-Belgium)
  82. Ministry of Education, Youth and Sports (MEYS) of Czech Republic
  83. Council of Science and Industrial Research, India
  84. Compagnia di San Paolo (Torino)
  85. HOMING PLUS programme of Foundation for Polish Science by EU, Regional Development Fund
  86. EU-ESF
  87. Greek NSRF
  88. Direct For Mathematical & Physical Scien
  89. Division Of Physics [0906479, 1120138, 1066578, 1205960] Funding Source: National Science Foundation
  90. Direct For Mathematical & Physical Scien
  91. Division Of Physics [1306951, 1314131, 1401984, 1151640] Funding Source: National Science Foundation
  92. Science and Technology Facilities Council [ST/K001604/1] Funding Source: researchfish
  93. STFC [ST/I002200/1, ST/J005479/1, ST/I505572/1, ST/K003844/1, ST/K001531/1, ST/K001604/1, ST/H00081X/2, ST/I000410/1, PP/E002803/1, ST/F006748/1, ST/K001639/1, ST/M002020/1, ST/L00609X/1, ST/G502347/1, ST/H000925/1, ST/L005603/1, ST/H000925/2, ST/L006340/1, ST/I003622/1, ST/I000305/1, ST/K003542/1, ST/J004901/1, ST/F007094/1, ST/J004871/1, ST/J005665/1, ST/I005912/1] Funding Source: UKRI

Ask authors/readers for more resources

A search for invisible decays of Higgs bosons is performed using the vector boson fusion and associated ZH production modes. In the ZH mode, the Z boson is required to decay to a pair of charged leptons or a bb quark pair. The searches use the 8TeV pp collision dataset collected by the CMS detector at the LHC, corresponding to an integrated luminosity of up to 19.7 fb(-1). Certain channels include data from 7TeV collisions corresponding to an integrated luminosity of 4.9 fb(-1).The searches are sensitive to non-standardmodel invisible decays of the recently observed Higgs boson, as well as additional Higgs bosons with similar production modes and large invisible branching fractions. In all channels, the observed data are consistent with the expected standard model backgrounds. Limits are set on the production cross section times invisible branching fraction, as a function of the Higgs boson mass, for the vector boson fusion and ZH production modes. By combining all channels, and assuming standard model Higgs boson cross sections and acceptances, the observed (expected) upper limit on the invisible branching fraction at m(H) = 125GeV is found to be 0.58 (0.44) at 95% confidence level. We interpret this limit in terms of a Higgs-portal model of dark matter interactions.

Authors

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

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available