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Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV

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Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV. / Collaboration, D0; Bertram, Iain; Borissov, Guennadi et al.
In: Physical review letters, Vol. 107, No. 1, 011801, 29.06.2011.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Collaboration, D, Bertram, I, Borissov, G, Fox, H, Ross, A, Williams, M & Ratoff, P 2011, 'Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV', Physical review letters, vol. 107, no. 1, 011801. https://doi.org/10.1103/PhysRevLett.107.011801

APA

Collaboration, D., Bertram, I., Borissov, G., Fox, H., Ross, A., Williams, M., & Ratoff, P. (2011). Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV. Physical review letters, 107(1), Article 011801. https://doi.org/10.1103/PhysRevLett.107.011801

Vancouver

Collaboration D, Bertram I, Borissov G, Fox H, Ross A, Williams M et al. Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV. Physical review letters. 2011 Jun 29;107(1):011801. doi: 10.1103/PhysRevLett.107.011801

Author

Collaboration, D0 ; Bertram, Iain ; Borissov, Guennadi et al. / Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV. In: Physical review letters. 2011 ; Vol. 107, No. 1.

Bibtex

@article{43e69f51aba94b3e81dcce244a5dcbef,
title = "Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV",
abstract = "We search for resonant WW or WZ production using up to 5.4 fb-1 of integrated luminosity collected by the D0 experiment in Run II of the Fermilab Tevatron Collider. The data are consistent with the standard model background expectation, and we set limits on a resonance mass using the sequential standard model (SSM) W' boson and the Randall-Sundrum model graviton G as benchmarks. We exclude an SSM W' boson in the mass range 180 - 690 GeV and a Randall-Sundrum graviton in the range 300 - 754 GeV at 95% CL.",
author = "D0 Collaboration and Iain Bertram and Guennadi Borissov and Harald Fox and Anthony Ross and Mark Williams and Peter Ratoff",
note = "{\textcopyright} 2011 American Physical Society submitted to Phys. Rev. Letters",
year = "2011",
month = jun,
day = "29",
doi = "10.1103/PhysRevLett.107.011801",
language = "English",
volume = "107",
journal = "Physical review letters",
issn = "1079-7114",
publisher = "American Physical Society",
number = "1",

}

RIS

TY - JOUR

T1 - Search for resonant WW and WZ production in ppbar collisions at ?s = 1.96 TeV

AU - Collaboration, D0

AU - Bertram, Iain

AU - Borissov, Guennadi

AU - Fox, Harald

AU - Ross, Anthony

AU - Williams, Mark

AU - Ratoff, Peter

N1 - © 2011 American Physical Society submitted to Phys. Rev. Letters

PY - 2011/6/29

Y1 - 2011/6/29

N2 - We search for resonant WW or WZ production using up to 5.4 fb-1 of integrated luminosity collected by the D0 experiment in Run II of the Fermilab Tevatron Collider. The data are consistent with the standard model background expectation, and we set limits on a resonance mass using the sequential standard model (SSM) W' boson and the Randall-Sundrum model graviton G as benchmarks. We exclude an SSM W' boson in the mass range 180 - 690 GeV and a Randall-Sundrum graviton in the range 300 - 754 GeV at 95% CL.

AB - We search for resonant WW or WZ production using up to 5.4 fb-1 of integrated luminosity collected by the D0 experiment in Run II of the Fermilab Tevatron Collider. The data are consistent with the standard model background expectation, and we set limits on a resonance mass using the sequential standard model (SSM) W' boson and the Randall-Sundrum model graviton G as benchmarks. We exclude an SSM W' boson in the mass range 180 - 690 GeV and a Randall-Sundrum graviton in the range 300 - 754 GeV at 95% CL.

U2 - 10.1103/PhysRevLett.107.011801

DO - 10.1103/PhysRevLett.107.011801

M3 - Journal article

VL - 107

JO - Physical review letters

JF - Physical review letters

SN - 1079-7114

IS - 1

M1 - 011801

ER -