4.4 Article

Search for disappearing tracks in proton-proton collisions at √s=8 TeV

Journal

JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 1, Pages -

Publisher

SPRINGER
DOI: 10.1007/JHEP01(2015)096

Keywords

Hadron-Hadron Scattering; Supersymmetry; Exotics

Funding

  1. BMWFW (Austria)
  2. FWF (Austria)
  3. FNRS (Belgium)
  4. FWO (Belgium)
  5. CNPq (Brazil)
  6. CAPES (Brazil)
  7. FAPERJ (Brazil)
  8. FAPESP (Brazil)
  9. MES (Bulgaria)
  10. CERN
  11. CAS (China)
  12. MoST (China)
  13. NSFC (China)
  14. COL-CIENCIAS (Colombia)
  15. MSES (Croatia)
  16. CSF (Croatia)
  17. RPF (Cyprus)
  18. MoER (Estonia)
  19. ERC IUT (Estonia)
  20. ERDF (Estonia)
  21. Academy of Finland (Finland)
  22. MEC (Finland)
  23. HIP (Finland)
  24. CEA (France)
  25. CNRS/IN2P3 (France)
  26. BMBF (Germany)
  27. DFG (Germany)
  28. HGF (Germany)
  29. GSRT (Greece)
  30. OTKA (Hungary)
  31. NIH (Hungary)
  32. DAE (India)
  33. DST (India)
  34. IPM (Iran)
  35. SFI (Ireland)
  36. INFN (Italy)
  37. NRF (Republic of Korea)
  38. WCU (Republic of Korea)
  39. LAS (Lithuania)
  40. MOE (Malaysia)
  41. UM (Malaysia)
  42. CINVESTAV (Mexico)
  43. CONACYT (Mexico)
  44. SEP (Mexico)
  45. UASLP-FAI (Mexico)
  46. MBIE (New Zealand)
  47. PAEC (Pakistan)
  48. MSHE (Poland)
  49. NSC (Poland)
  50. FCT (Portugal)
  51. JINR (Dubna)
  52. MON (Russia)
  53. RosAtom (Russia)
  54. RAS (Russia)
  55. RFBR (Russia)
  56. MESTD (Serbia)
  57. SEIDI (Spain)
  58. CPAN (Spain)
  59. Swiss Funding Agencies (Switzerland)
  60. MST (Taipei)
  61. ThEPCenter (Thailand)
  62. IPST (Thailand)
  63. STAR (Thailand)
  64. NSTDA (Thailand)
  65. TUBITAK (Turkey)
  66. TAEK (Turkey)
  67. NASU (Ukraine)
  68. SFFR (Ukraine)
  69. STFC (United Kingdom)
  70. DOE (U.S.A.)
  71. NSF (U.S.A.)
  72. Marie-Curie program
  73. European Research Council
  74. EPLANET (European Union)
  75. Leventis Foundation
  76. A.P. Sloan Foundation
  77. Alexander von Humboldt Foundation
  78. Belgian Federal Science Policy Office
  79. Fonds pour la Formation a la Recherche dans l'Industrie et dans l'Agriculture (FRIA-Belgium)
  80. Agentschap voor Innovatie door Wetenschap en Technologie (IWT-Belgium)
  81. Ministry of Education, Youth and Sports (MEYS) of the Czech Republic
  82. Council of Science and Industrial Research, India
  83. HOMING PLUS program of Foundation for Polish Science
  84. European Union, Regional Development Fund
  85. Compagnia di San Paolo (Torino)
  86. Consorzio per la Fisica (Trieste)
  87. MIUR project (Italy) [20108T4XTM]
  88. Thalis program
  89. Aristeia program
  90. EU-ESF
  91. Greek NSRF
  92. National Priorities Research Program by Qatar National Research Fund
  93. Science and Technology Facilities Council [ST/I005912/1 GRIDPP, ST/L00609X/1 GRIDPP, ST/M004775/1, ST/I005912/1, ST/M005356/1, ST/J50094X/1, ST/K001604/1, ST/J005479/1, ST/M004775/1 GRIDPP, ST/K003844/1, ST/J004901/1, ST/M005356/1 GRIDPP, ST/N000250/1, ST/L00609X/1, ST/J005665/1, ST/K003542/1 GRID PP, ST/K001256/1, ST/J004871/1, ST/K003542/1 GRIDPP, ST/K001639/1, ST/K001531/1, CMS, ST/K003844/1 GRIDPP, GRIDPP] Funding Source: researchfish
  94. STFC [ST/K003844/1, ST/K001531/1, ST/J004871/1, ST/M004775/1, ST/J004901/1, ST/J005479/1, ST/M005356/1, ST/L00609X/1, ST/K001639/1, ST/J50094X/1, ST/I005912/1, ST/J005665/1, ST/K001604/1, ST/H00081X/2] Funding Source: UKRI
  95. Direct For Mathematical & Physical Scien
  96. Division Of Physics [1211067, 1314131, 1205960] Funding Source: National Science Foundation
  97. Division Of Physics
  98. Direct For Mathematical & Physical Scien [1151640, 1120138, 1306951] Funding Source: National Science Foundation

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A search is presented for long-lived charged particles that decay within the CMS detector and produce the signature of a disappearing track. Disappearing tracks are identified as those with little or no associated calorimeter energy deposits and with missing hits in the outer layers of the tracker. The search uses proton-proton collision data recorded at root s = 8 TeV that corresponds to an integrated luminosity of 19.5 fb(-1). The results of the search are interpreted in the context of the anomaly-mediated supersymmetry breaking (AMSB) model. The number of observed events is in agreement with the background expectation, and limits are set on the cross section of direct electroweak chargino production in terms of the chargino mass and mean proper lifetime. At 95% confidence level, AMSB models with a chargino mass less than 260 GeV, corresponding to a mean proper lifetime of 0.2 ns, are excluded.

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