4.8 Article

Measurement of the W+W- Production Cross Section and Search for Anomalous WWγ and WWZ Couplings in p(p)over-bar Collisions at √s 1.96 TeV

Journal

PHYSICAL REVIEW LETTERS
Volume 104, Issue 20, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.104.201801

Keywords

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Funding

  1. U.S. Department of Energy
  2. Italian Istituto Nazionale di Fisica Nucleare
  3. Ministry of Education, Culture, Sports, Science and Technology of Japan
  4. Natural Sciences and Engineering Research Council of Canada
  5. National Science Council of the Republic of China
  6. Swiss National Science Foundation
  7. A.P. Sloan Foundation
  8. Bundesministerium fur Bildung und Forschung, Germany
  9. World Class University Program
  10. Science and Technology Facilities Council
  11. Institut National de Physique Nucleaire et Physique des Particules/CNRS
  12. Russian Foundation for Basic Research
  13. Ministerio de Ciencia e Innovacion, and Programa Consolider-Ingenio 2010, Spain
  14. Slovak RD Agency
  15. Academy of Finland
  16. National Science Foundation
  17. National Research Foundation of Korea
  18. Royal Society, UK
  19. STFC [ST/H001077/1, ST/H001026/2, ST/H001069/1, PP/D003199/1, ST/H001026/1] Funding Source: UKRI
  20. Science and Technology Facilities Council [PP/D003199/1, PP/E000444/1, ST/H001077/1, ST/H001026/1, ST/H001026/2] Funding Source: researchfish

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This Letter describes the current most precise measurement of the W boson pair production cross section and most sensitive test of anomalous WW gamma and WWZ couplings in p (p) over bar collisions at a center-of-mass energy of 1.96 TeV. The WW candidates are reconstructed from decays containing two charged leptons and two neutrinos. Using data collected by the CDF II detector from 3: 6 fb(-1) of integrated luminosity, a total of 654 candidate events are observed with an expected background of 320 +/- 47 events. The measured cross section is sigma(p (p) over bar -> W+W- +X) = 12.1 +/- 0.9(stat)(-1.4)(+1.6)(syst) pb, which is in good agreement with the standard model prediction. The same data sample is used to place constraints on anomalous WW gamma and WWZ couplings.

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