- Access by Xinjiang University
Combining next-to-leading order QCD and electroweak radiative corrections to -boson production at hadron colliders in the powheg framework
Phys. Rev. D 85, 093003 – Published 7 May, 2012
DOI: https://doi.org/10.1103/PhysRevD.85.093003
Abstract
The precision measurement of the mass of the boson is an important goal of the Fermilab Tevatron and the CERN Large Hadron Collider (LHC). It requires accurate theoretical calculations which incorporate both higher-order QCD and electroweak corrections, and also provide an interface to parton-shower Monte Carlo programs which make it possible to realistically simulate experimental data. In this paper, we present a combination of the full electroweak corrections of wgrad2, and the next-to-leading order QCD radiative corrections to production in hadronic collisions in a single event generator based on the powheg framework, which is able to interface with the parton-shower Monte Carlo programs pythia and herwig. Using this new combined QCD + EW Monte Carlo program for production, we provide numerical results for total cross sections and kinematic distributions of relevance to the mass measurement at the Tevatron and the LHC for the processes , . In particular, we discuss the impact of EW corrections in the presence of QCD effects when including detector resolution effects.
Article Text
References (54)
- T. Aaltonen et al. (CDF Collaboration), Phys. Rev. Lett. 99, 151801 (2007); Phys. Rev. D 77, 112001 (2008); arXiv:1203.0275.
- V. M. Abazov et al. (D0 Collaboration), Phys. Rev. Lett. 103, 141801 (2009).
- TEV-EWWG Group CDF and D0 Collaboration, arXiv:1204.0042.
- H. Flacher, M. Goebel, J. Haller, A. Hocker, K. Monig, and J. Stelzer, Eur. Phys. J. C 60, 543 (2009); D. Ludwig, Proc. Sci. ICHEP2010 (2010) 404.
- M. Baak, M. Goebel, J. Haller, A. Hoecker, D. Ludwig, K. Moenig, and M. Schott, arXiv:1107.0975.
- J. Alcaraz, arXiv:0911.2604.
- TEVNPH (Tevatron New Phenomena and Higgs Working Group), CDF, and DO Collaborations, arXiv:1107.5518.
- S. Chatrchyan et al. (CMS Collaboration), Phys. Lett. B 699, 25 (2011).
- G. Aad et al. (ATLAS Collaboration), Eur. Phys. J. C 71, 1728 (2011).
- A. V. Kotwal and J. Stark, Annu. Rev. Nucl. Part. Sci. 58, 147 (2008).
- N. Besson, M. Boonekamp, E. Klinkby, T. Petersen, and S. Mehlhase (ATLAS Collaboration), Eur. Phys. J. C 57, 627 (2008).
- V. Buge, C. Jung, G. Quast, A. Ghezzi, M. Malberti, and T. Tabarelli de Fatis, J. Phys. G 34, N193 (2007).
- M. W. Krasny, F. Dydak, F. Fayette, W. Placzek, and A. Siodmok, Eur. Phys. J. C 69, 379 (2010).
- C. Balazs and C. P. Yuan, Phys. Rev. D 56, 5558 (1997); R. K. Ellis and S. Veseli, Nucl. Phys. B511, 649 (1998).
- F. Landry, R. Brock, G. Ladinsky, and C. P. Yuan, Phys. Rev. D 63, 013004 (2000).
- S. Frixione and B. R. Webber, J. High Energy Phys. 06 (2002) 029; S. Frixione, F. Stoeckli, P. Torrielli, B. R. Webber, and C. D. White, arXiv:1010.0819.
- S. Alioli, P. Nason, C. Oleari, and E. Re, J. High Energy Phys. 07 (2008) 060.
- K. Hamilton, P. Richardson, and J. Tully, J. High Energy Phys. 10 (2008) 015
- C. Anastasiou, L. J. Dixon, K. Melnikov, and F. Petriello, Phys. Rev. D 69, 094008 (2004).
- K. Melnikov and F. Petriello, Phys. Rev. Lett. 96, 231803 (2006).
- S. Catani, L. Cieri, G. Ferrera, D. de Florian, and M. Grazzini, Phys. Rev. Lett. 103, 082001 (2009).
- W. B. Kilgore and C. Sturm, Phys. Rev. D 85, 033005 (2012).
- F. Abe et al. (CDF Collaboration), Phys. Rev. Lett. 75, 11 (1995); Phys. Rev. D 52, 4784 (1995); T. Affolder et al. (CDF Collaboration), 64, 052001 (2001).
- S. Abachi et al. (D0 Collaboration), Phys. Rev. Lett. 77, 3309 (1996); B. Abbott et al. (D0 Collaboration), Phys. Rev. D 58, 012002 (1998); 58, 092003 (1998); Phys. Rev. Lett. 80, 3008 (1998); 84, 222 (2000); Phys. Rev. D 62, 092006 (2000); V. M. Abazov et al. (D0 Collaboration), 66, 012001 (2002).
- W. Ashmanskas et al. (TEV-EWWG Collaboration), Phys. Rev. D 70, 092008 (2004) and references therein.
- F. Abe et al. (CDF Collaboration), Phys. Rev. Lett. 74, 341 (1995).
- T. Affolder et al. (CDF Collaboration), Phys. Rev. Lett. 85, 3347 (2000).
- V. M. Abazov et al. (D0 Collaboration), Phys. Rev. D 66, 032008 (2002).
- D. Wackeroth and W. Hollik, Phys. Rev. D 55, 6788 (1997).
- U. Baur, S. Keller, and D. Wackeroth, Phys. Rev. D 59, 013002 (1998).
- S. Dittmaier and M. Krämer, Phys. Rev. D 65, 073007 (2002).
- U. Baur and D. Wackeroth, Phys. Rev. D 70, 073015 (2004).
- A. Arbuzov, D. Bardin, S. Bondarenko, P. Christova, L. Kalinovskaya, G. Nanava, and R. Sadykov, Eur. Phys. J. C 46, 407 (2006); 50, 505(E) (2007).
- C. M. Carloni Calame, G. Montagna, O. Nicrosini, and A. Vicini, J. High Energy Phys. 12 (2006) 016.
- V. A. Zykunov, Phys. At. Nucl. 71, 732 (2008); Eur. Phys. J. direct C 3, 1 (2001).
- C. Buttar et al., arXiv:hep-ph/0604120.
- C. E. Gerber et al. TeV4LHC-Top and Electroweak Working Group, arXiv:0705.3251.
- C. M. Carloni Calame, G. Montagna, O. Nicrosini, and M. Treccani, Phys. Rev. D 69, 037301 (2004).
- W. Placzek and S. Jadach, Eur. Phys. J. C 29, 325 (2003).
- P. Golonka and Z. Was, Eur. Phys. J. C 45, 97 (2006).
- K. Hamilton and P. Richardson, J. High Energy Phys. 07 (2006) 010.
- S. Brensing, S. Dittmaier, M. Krämer, and A. Muck, Phys. Rev. D 77, 073006 (2008).
- E. Laenen and D. Wackeroth, Annu. Rev. Nucl. Part. Sci. 59, 367 (2009).
- Q. H. Cao and C. P. Yuan, Phys. Rev. Lett. 93, 042001 (2004).
- G. Balossini et al., J. High Energy Phys. 01 (2010) 013.
- G. Corcella, I. G. Knowles, G. Marchesisni, S. Moretti, K. Odagiri, P. Richardson, M. H. Seymour, and B. R. Webber, J. High Energy Phys. 01 (2001) 010.
- T. Sjostrand, S. Mrenna, and P. Z. Skands, J. High Energy Phys. 05 (2006) 026.
- P. Richardson, R. R. Sadykov, A. A. Sapronov, M. H. Seymour, and P. Z. Skands, arXiv:1011.5444.
- P. Nason, J. High Energy Phys. 11 (2004) 040.
- S. Frixione, P. Nason, and C. Oleari, J. High Energy Phys. 11 (2007) 070.
- S. Alioli, P. Nason, C. Oleari, and E. Re, J. High Energy Phys. 06 (2010) 043.
- http://powhegbox.mib.infn.it/
- B. W. Harris and J. F. Owens, Phys. Rev. D 65, 094032 (2002).
- H. -L. Lai et al., Phys. Rev. D 82, 074024 (2010).