New signature for color octet pseudoscalars at the CERN LHC Alfonso R. Zerwekh* Centro de Estudios Subatómicos and Instituto de Fı́sica, Facultad de Ciencias, Universidad Austral de Chile, Casilla 567, Valdivia, Chile Claudio O. Dib+ Centro de Estudios Subatómicos and Departamento de Fı́sica, Universidad Técnica Federico Santa Marı́a, Valparaı́so, Chile Rogerio Rosenfeld‡ Instituto de Fı́sica Teórica - UNESP, Rua Pamplona, 145, 01405-900, São Paulo, SP, Brazil (Received 11 March 2008; published 29 May 2008) Color octet (pseudo)scalars, if they exist, will be copiously produced at the CERN Large Hadron Collider (LHC). However, their detection can become a very challenging task. In particular, if their decay into a pair of top quarks is kinematically forbidden, the main decay channel would be into two jets, with a very large background. In this brief report we explore the possibility of using anomaly-induced decays of the color octet pseudoscalars into gauge bosons to find them at the LHC. DOI: 10.1103/PhysRevD.77.097703 PACS numbers: 12.60.Nz, 13.85.Qk I. INTRODUCTION In spite of its great experimental successes [1], the standard model (SM) of the electroweak interactions is still widely regarded as an incomplete theory. The reasons are manifold, including the existence of nonbaryonic dark matter and nonzero neutrino masses in addition to the theoretical problems of triviality and naturalness related to the scalar Higgs sector responsible for the mechanism of electroweak symmetry breaking. There are many extensions of the SM that require the existence of color octet scalar particles, such as the extra component of the gluon field in models with extra dimen- sions [2], supersymmetric models with an adjoint chiral supermultiplet [3], or models with an extended color sym- metry [4]. The existence of color octet scalars has also been used to explain the accelerated expansion of the Universe [5]. Extended scalar sectors of the SM with color octet scalars that respect the principle of minimal flavor viola- tion were also recently considered [6,7]. Color octet scalars may also have important effects in the Higgs boson pro- duction via gluon fusion [8]. Early studies on the existence of color octet scalars were done in the context of one-family technicolor models [9]. Both electroweak triplets (P�;0 8 ) and singlets (P00 8 , some- times denoted also as technieta �T8, a notation which we will adopt in this paper) are present in the spectrum of the pseudo-Nambu-Goldstone boson (PNGB) arising from the global SUð8ÞL � SUð8ÞR ! SUð8ÞV spontaneous symme- try breaking [10]. The masses of the color octet PNGB arise mainly from QCD contributions and are expected to be of the order of 300 GeV [11]. The cross section for pair production of the color octet scalars is dominated by gluon fusion, which in turn is determined by gauge invariance [12] and consequently, except for the gluon parton densities, is mostly model independent, being fixed by the masses of the particles. There could also be a model dependent enhancement due to the coupling of the scalars to color octet vector reso- nances such as a technirho �T8 [13], which in turn couples to quarks and gluons. However, as shown by two of the present authors [12], a proper gauge invariant treatment of the �T8 results in a vanishing �T8- g- g coupling [14]. Hence, only the quark initial state can cause this enhancement. While models of a strongly interacting sector respon- sible for electroweak symmetry breaking fell in disfavor in the mid-1990’s due to tight bounds from electroweak precision measurements, they have experienced a recent resurrection due to the correspondence with weakly inter- acting models in extra dimensions [15]. In this case, the �T8 could be interpreted as the Kaluza-Klein excitation of the gluon. Tevatron searches have excluded the existence of a �T8 in the mass range 260 80 GeV; (7) PTj > 80 GeV; (8) jM�j �Mjjj< 0:15M�; (9) jM�j �M�T8 j< 20 GeV: (10) In Fig. 1, we show the reconstructed technieta mass obtained by summing up the M�j and Mjj distributions after the cuts were applied. The dashed line represents the direct background, while the double-dotted-dashed line is the result obtained when a jet is misidentified as a photon. Our signal is shown by the dotted-dashed line. Assuming an integrated luminosity of L ¼ 10 fb�1, we expect to observe about 21 400 events with 4200 of them corresponding to our signal. That would correspond to a deviation from the SM with a statistical significance of 32�. In this analysis, we have used some cuts that depend on the technieta mass. This procedure may be uncomfortable from the experimental point of view since the mass of the searched particle is not known a priori and the whole possible range must be scanned. Fortunately, in our case the mass interval is limited because, due to QCD contri- butions, the technieta cannot be lighter than 300 GeV and we do not expect the channel considered in this work to be useful for discovery if the technieta is heavier than 350 GeV. However, it is possible to devise a search strategy which is independent of the technieta mass. Consider the follow- ing set of cuts: PT� > 80 GeV; (11) PTj > 80 GeV; (12) jM�j �Mjjj< 10 GeV; (13) jminðcos �jÞj< 0:6; (14) where �j is the angle formed by a photon and a jet. The last cut comes from the fact that the technieta is a spin 0 particle and its decay is isotropic in its rest system, while the background tends to have peaks at cos �j ¼ �1. Figure 2 shows the invariant mass distribution obtained with the new set of cuts. We expect to observe, integrating over the whole mass range, 12 600 background events and 1100 events coming from the technietas with L ¼ 10 fb�1, corresponding to a 10� signal. Invariant Mass (GeV) 260 280 300 320 340 360 380 E ve n ts /b in 1000 2000 3000 4000 5000 FIG. 1 (color online). Reconstructed technieta invariant mass distribution The dashed line represents the direct background, while the double-dotted-dashed line is the result obtained when a jet is misidentified as a photon. Our signal is shown by the dotted-dashed line. Invariant Mass (GeV) 300 305 310 315 320 325 330 335 340 345 350 E ve n ts /b in 200 250 300 350 400 450 500 550 600 650 FIG. 2 (color online). Reconstructed technieta invariant mass distribution using a set of cuts independent of the technieta mass. The dashed line represents the direct background (we neglect the small indirect background due to misidentification). Our signal is shown by the dotted-dashed line. BRIEF REPORTS PHYSICAL REVIEW D 77, 097703 (2008) 097703-3 IV. CONCLUSIONS We studied the pair production and detection of color octet pseudoscalar bosons at the LHC, which could be present in models of electroweak symmetry breaking in- duced by new strong interactions. We restricted our analy- sis to m�T8 (the color octet pseudoscalar mass) below 2mt, in which case the decay into t- �t is forbidden and conse- quently the detection is more challenging. In such cases, the color octet pseudoscalar decays mainly into two glu- ons, induced by the anomaly, while the direct decay into b- �b has a fraction less than 20%. We perform simulations for the production and decay of pseudoscalar pairs, including background. We did not look for the dominant 4-jet mode, but for the suppressed 3-jetþ photon mode, which has a much lower background. We used two different methods of analysis. In one method we assume m�T8 to be known in our cuts, and obtain a number of events 32� above the expected background, for an integrated luminosity of 10 fb�1. In our second method, we did not include any value of m�T8 in our cuts, but relied only on the invariant mass reconstruction of the two decaying pseudoscalars, in which case the number of events resulted in a statistical significance of 10� above the expected background. These results show that the LHC has the potential to detect or exclude the existence of such pseudoscalar colored bosons. ACKNOWLEDGMENTS The work of A. R. Z. is partially supported by Grant No. DID-UACH S-2006-28 and by Fondecyt Grant No. 1070880; C. O.D. is partially supported by Fondecyt, Chile, Grant No. 1070227; R. R. is partially supported by a CNPq, Brazil, Research Grant No. 309158/2006-0. C. D. and R. R. also acknowledge the support of Fondecyt, Chile, Grant No. 7070098 for international cooperation. This work is also supported by the CNPq PROSUL Program No. 490157/2006-8 and Conicyt Grant No. PBCT- ACT028. [1] For an updated overview, see LEP Electroweak Working Group, lepewwg.web.cern.ch/LEPEWWG/. [2] See, e.g., G. Burdman, B. A. Dobrescu, and E. Ponton, Phys. Rev. D 74, 075008 (2006). [3] Y. Cui, Phys. Rev. D 74, 075010 (2006). [4] P. Yu. Popov, A.V. Povarov, and A.D. Smirnov, Mod. Phys. Lett. A 20, 3003 (2005). [5] D. Stojkovic, G. Starkman, and R. Matsuo, Phys. Rev. D 77, 063006 (2008). [6] A. V. Manohar and M. B. Wise, Phys. Rev. D 74, 035009 (2006). [7] M. I. Gresham and M.B. Wise, Phys. Rev. D 76, 075003 (2007). [8] R. Bonciani, G. Degrassi, and A. Vicini, J. High Energy Phys. 11 (2007) 095. [9] E. Farhi and L. Susskind, Phys. Rev. D 20, 3404 (1979); S. Dimopoulos, Nucl. Phys. B168, 69 (1980). [10] For reviews see, e.g., R. S. Chivukula, R. Rosenfeld, E. H. Simmons, and J. Terning, in Electroweak Symmetry Breaking and New Physics at the TeV Scale, edited by T. L. Barklow, S. Dawson, H. E. Haber, and J. L. Siegrist (World Scientific, Singapore, 1996); C. T. Hill and E.H. Simmons, Phys. Rep. 381, 235 (2003); 390, 553(E) (2004). [11] M. E. Peskin, Nucl. Phys. B175, 197 (1980); J. Preskill, Nucl. Phys. B177, 21 (1981). [12] A. R. Zerwekh and R. Rosenfeld, Phys. Lett. B 503, 325 (2001). [13] E. Eichten, I. Hinchliffe, K. D. Lane, and C. Quigg, Rev. Mod. Phys. 56, 579 (1984); 58, 1065 (1986). [14] In this sense, our work reproduces the colored sector of the model by R. Casalbuoni, S. De Curtis, A. Deandrea, N. Di Bartolomeo, R. Gatto, D. Dominici, and F. Feruglio, Nucl. Phys. B409, 257 (1993). [15] See, e.g., K. Agashe, R. Contino, and A. Pomarol, Nucl. Phys. B719, 165 (2005). [16] F. Abe et al. (CDF Collaboration), Phys. Rev. D 55, R5263 (1997). [17] R. S. Chivukula, A. Grant, and E.H. Simmons, Phys. Lett. B 521, 239 (2001). [18] A. R. Zerwekh, Int. J. Mod. Phys. A 19, 4387 (2004). [19] A. R. Zerwekh, Eur. Phys. J. C 49, 1077 (2007). [20] B. A. Dobrescu, K. Kong, and R. Mahbubani, arXiv:0709.2378. [21] M. Gerbush, T. J. Khoo, D. J. Phalen, A. Pierce, and D. Tucker-Smith, arXiv:0710.3133 [Phys. Rev. D (to be pub- lished)]. [22] B. Lillie, J. Shu, and T.M. P. Tait, arXiv:0712.3057. [23] C. Kilic, T. Okui, and R. Sundrum, arXiv:0802.2568. [24] J. Ellis, M. K. Gaillard, D.V. Nanopoulos, and P. Sikivie, Nucl. Phys. B182, 529 (1981). [25] E. Boos et al. (CompHEP Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 534, 250 (2004). [26] A. Semenov, Nucl. Instrum. Methods Phys. Res., Sect. A 389, 293 (1997); arXiv:hep-ph/0208011; arXiv:0805. 0555. 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