- Access by Xinjiang University
Leptoquarks decaying to a top quark and a charged lepton at hadron colliders
Phys. Rev. D 83, 115016 – Published 17 June, 2011
DOI: https://doi.org/10.1103/PhysRevD.83.115016
Abstract
We study the sensitivity of the Tevatron and the 7 TeV LHC to a leptoquark coupling to a top quark and a charged lepton (, , or ). For the Tevatron, we focus on the case , where the leptoquark pair production cross section is large, and the decay is three-body: . We argue that existing Tevatron observations could exclude . For , we show that the LHC experiments with low integrated luminosity could be sensitive to such leptoquarks decaying to with or .
Article Text
References (44)
- Some earlier discussions are (see, e.g., references and citations thereof): S. Davidson, D. C. Bailey, and B. A. Campbell, Z. Phys. C 61, 613 (1994); J. L. Hewett and T. G. Rizzo, Phys. Rev. D 56, 5709 (1997).
- P. Langacker, Phys. Rep. 72, 185 (1981).
- E. Farhi and L. Susskind, Phys. Rep. 74, 277 (1981).
- R. Barbier et al., Phys. Rep. 420, 1 (2005).
- S. S. Gershtein, A. A. Likhoded, and A. I. Onishchenko, Phys. Rep. 320, 159 (1999); I. Dorsner and P. Fileviez Perez, Nucl. Phys. B723, 53 (2005).
- B. Gripaios, J. High Energy Phys. 02 (2010) 045.
- P. Fileviez Perez, T. Han, T. Li, and M. J. Ramsey-Musolf, Nucl. Phys. B819, 139 (2009); D. Aristizabal Sierra, M. Hirsch, and S. G. Kovalenko, Phys. Rev. D 77, 055011 (2008); P. Y. Popov, A. V. Povarov, and A. D. Smirnov, Mod. Phys. Lett. A 20, 755 (2005).
- W. Buchmuller, R. Ruckl, and D. Wyler, Phys. Lett. B 191, 442 (1987).
- P. Fileviez Perez, T. Han, T. Li, and M. J. Ramsey-Musolf, Nucl. Phys. B819, 139 (2009).
- M. Hirsch, H. V. Klapdor-Kleingrothaus, and S. G. Kovalenko, Phys. Lett. B 378, 17 (1996); U. Mahanta, Phys. Rev. D 62, 073009 (2000); K. S. Babu and J. Julio, Nucl. Phys. B841, 130 (2010).
- T. P. Cheng and M. Sher, Phys. Rev. D 35, 3484 (1987).
- M. Carpentier and S. Davidson, Eur. Phys. J. C 70, 1071 (2010).
- A. J. Buras, P. Gambino, M. Gorbahn, S. Jager, and L. Silvestrini, Phys. Lett. B 500, 161 (2001); R. S. Chivukula and H. Georgi, 188, 99 (1987).
- G. D’Ambrosio, G. F. Giudice, G. Isidori, and A. Strumia, Nucl. Phys. B645, 155 (2002).
- S. Davidson and S. Descotes-Genon, J. High Energy Phys. 11 (2010) 073.
- E. Nikolidakis and C. Smith, Phys. Rev. D 77, 015021 (2008).
- V. M. Abazov et al. (D0 Collaboration), Phys. Lett. B 681, 224 (2009); D0 Collaboration671, 224 (2009); D0 CollaborationPhys. Rev. Lett. 101, 241802 (2008). D0 CollaborationPhys. Lett. B 693, 95 (2010). D0 Collaboration668, 357 (2008).
- G. Grenier, Proc. Sci. (ICHEP2010) 391.
- S. Chekanov et al. (ZEUS Collaboration), Phys. Rev. D 68, 052004 (2003); A. Aktas et al. (H1 Collaboration), Phys. Lett. B 629, 9 (2005); R. Ciesielski (H1 and ZEUS Collaborations), Proc. Sci., EPS-HEP2009 (2009) 269.
- K. S. McFarland et al. (CCFR/NuTeV Collaboration), Eur. Phys. J. C 1, 509 (1998); S. Schael et al. (ALEPH Collaboration), 49, 411 (2007), D0 Collaboration, D0 note 4922-CONF; http://www-d0.fnal.gov/Run2Physics/WWW/results/np.htm D0 CollaborationD0 note 4552-CONF, http://www-d0.fnal.gov/Run2Physics/WWW/results/np.htm; R. Ciesielski (H1 and ZEUS Collaborations), Proc. Sci., EPS-HEP2009 (2009) 269.
- K. m. Cheung, Phys. Lett. B 517, 167 (2001).
- O. J. P. Eboli, R. Zukanovich Funchal, and T. L. Lungov, Phys. Rev. D 57, 1715 (1998); C. Boulahouache (ATLAS Collaboration), AIP Conf. Proc. 1078, 584 (2009).
- J. P. Saha, B. Misra, and A. Kundu, Phys. Rev. D 81, 095011 (2010).
- J. K. Mizukoshi, O. J. P. Eboli, and M. C. Gonzalez-Garcia, Nucl. Phys. B443, 20 (1995); G. Bhattacharyya, J. R. Ellis, and K. Sridhar, Phys. Lett. B 336, 100 (1994); 338, 522(E) (1994).
- O. J. P. Eboli, R. Zukanovich Funchal, and T. L. Lungov, Phys. Rev. D 59, 035002 (1998).
- B. Gripaios, A. Papaefstathiou, K. Sakurai, and B. Webber, J. High Energy Phys. 01 (2011) 156.
- A. Belyaev, C. Leroy, R. Mehdiyev, and A. Pukhov, J. High Energy Phys. 09 (2005) 005.
- M. Kramer, T. Plehn, M. Spira, and P. M. Zerwas, Phys. Rev. Lett. 79, 341 (1997); Phys. Rev. D 71, 057503 (2005); W. Beenakker, M. Kramer, T. Plehn, M. Spira, and P. M. Zerwas, Nucl. Phys. B515, 3 (1998).
- D0 Collaboration, D0 Note 6037-CONF, http://www-d0.fnal.gov/Run2Physics/WWW/results/prelim/TOP/T88/T88.pdf.
- D0 Collaboration, D0 Note 6038-CONF, http://www-d0.fnal.gov/Run2Physics/WWW/results/prelim/TOP/T86/T86.pdf.
- K. Nakamura et al. (Particle Data Group), J. Phys. G 37, 075021 (2010).
- T. Sjostrand, S. Mrenna, and P. Z. Skands, J. High Energy Phys. 05 (2006) 026.
- P. Golonka, B. Kersevan, T. Pierzchala, E. Richter-Was, Z. Was, and M. Worek, Comput. Phys. Commun. 174, 818 (2006).
We modified the tauola-pythia interface so that it finds and assigns polarisation to ’s from leptoquark decay.
- M. Cacciari and G. P. Salam, Phys. Lett. B 641, 57 (2006).
The various scalar leptoquarks of Eq. (1) have recently been included in herwig [26], which would avoid this limitation that pythia only knows one chiral structure for leptoquark interactions.
We checked that changing the polarisation makes a relatively insignificant change to the bounds.
- T. Junk, Nucl. Instrum. Methods Phys. Res., Sect. A 434, 435 (1999); A. Read, CERN Report No. CERN-2000-005, 2000.
The numbers are extracted from a histogram.
- V. Khachatryan et al. (CMS Collaboration), Phys. Lett. B 695, 424 (2011).
- G. Aad et al. (Atlas Collaboration), Eur. Phys. J. C 71, 1577 (2011).
This means, for instance, that our simulation now includes events with two leptonic ’s, which could pass cuts if there are additional QCD jets (this accounts for of our events at ).
- CMS Collaboration, CMS Report No. CMS-PAS-TOP-10-004.
This factor arises from kinematics and counting degrees of freedom. At Tevatron energies, and are subdominant, so can be neglected in the following. It is simple to show, at leading order, that . The 4 may be understood from the cancellation of quadratic divergences in the gluon propagator in supersymmetry models, where the top bubble compensates the two scalar bubbles (in and on the gluon line) of two complex scalars and . Whereas the production cross section corresponds to a scalar bubble in the gluon line for a single complex scalar, there is a relative factor of 4. The accounts for the remaining factor of suppressing leptoquark production relative to for masses at Tevatron energies.