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arXiv:1001.0022v2 [hep-ph] 17 Mar 2010Preprint typeset in JHEP style - HYPER VERSION MADPH–09-1552 |
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µτProduction at Hadron Colliders |
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Tao Han∗, Ian Lewis† |
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Department of Physics, University of Wisconsin, Madison, W I 53706, U.S.A. |
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Marc Sher‡ |
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Particle Theory Group, College of William and Mary, William sburg, Virginia 23187 |
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Abstract: Motivated by large νµ−ντflavor mixing, we consider µτproduction at hadron |
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colliders via dimension-6 effective operators, which can be a ttributed to new physics in the |
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flavor sector at a higher scale Λ. Current bounds on many of the se operators from low energy |
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experiments are very weak or nonexistent, and they may lead t o cleanµ+τ−andµ−τ+signals |
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at hadron colliders. At the Tevatron with 8 fb−1, one can exceed current bounds for most |
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operators, with most 2 σsensitivities being in the 6 −24 TeV range. We find that at the LHC |
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with 1 fb−1(100 fb−1) integrated luminosity, one can reach a2 σsensitivity for Λ ∼3−10 TeV |
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(Λ∼6−21 TeV), depending on the Lorentz structure of the operator. For some operators, |
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an improvement of several orders of magnitude in sensitivit y can be obtained with only a few |
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tens of pb−1at the LHC. |
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Keywords: Lepton flavor physics; Hadron collider phenomenology.. |
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∗[email protected] |
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†[email protected] |
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‡[email protected] |
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1. Introduction 1 |
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2.µτProduction at Hadron Colliders 3 |
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3. Signal Identification and Backgrounds 4 |
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3.1τDecay to Electrons 5 |
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3.1.1 Signal Reconstruction 5 |
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3.1.2 Backgrounds and their Suppression 6 |
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3.2τDecay to Hadrons 9 |
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3.3 Sensitivity Reach at the Tevatron 10 |
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3.4 Sensitivity Reach at the LHC 10 |
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4. Discussions and Conclusions 13 |
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A. New Physics Bounds 14 |
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B. Partial Wave Unitarity Bounds 14 |
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1. Introduction |
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The most important discovery in particle physics in the past decade has only deepened the |
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mystery of “flavor” of quarks and leptons. The fact that the mi xing angles in the leptonic |
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sector are large [1, 2] stands in sharp contrast with the obse rved small mixing angles in the |
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quarksector. Inparticular, mixingbetweenthesecondandt hirdgeneration neutrinosappears |
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to be maximal. Of course, this large mixing could occur from d iagonalizing the neutrino mass |
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matrix, the charged lepton mass matrix, or both. At present, the source of this large mixing |
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is a mystery. |
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In view of this, it is tempting to explore other interactions which change lepton flavor |
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between the second and third generations. Several years ago , two of us (TH, MS), along with |
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Black and He (BHHS) [3], performed a comprehensive analysis of constraints on these inter- |
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actions based on low energy meson physics. BHHS chose an effect ive field theory approach, |
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in which all dimension-6 operators of the form |
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(¯µΓτ)(¯qαΓqβ), (1.1) |
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– 1 –were studied, where Γ contains possible Dirac γ-matrices. With six flavors of quarks, there |
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were 12 possible combinations of qaandqb(assuming Hermiticity), six diagonal and six off- |
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diagonal, and four choices S,P,V,A of the gamma matrices were considered. All of these |
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operators were considered, and most were bounded by conside ringτ,K,Bandtdecays. |
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In particular, BHHS considered operators of the form |
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∆L= ∆L(6) |
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τµ=/summationdisplay |
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j,α,βCj |
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αβ |
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Λ2(µΓjτ)/parenleftBig |
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qαΓjqβ/parenrightBig |
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+ H.c., (1.2) |
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where Γ j∈(1, γ5, γσ, γσγ5) denotes relevant Dirac matrices, specifying scalar, pseu doscalar, |
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vector and axial vector couplings, respectively. They did n ot consider tensor operators since |
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the hadronic matrix elements were not known and the bounds we re expected to be weak in |
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any event. They chose a value of |
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Cj |
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αβ= 4πO(1) (default) , (1.3) |
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which corresponds to an underlying theory with a strong gaug e coupling of αS=O(1). |
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Arguments can be made for multiplying or dividing this by 4 π, for naive dimensional analysis |
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or for weakly coupled theories, respectively. A discussion is found in BHHS; we simply choose |
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the above definition of Λ and other choices can be made by simpl e rescaling. |
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Besides the four fermion operators in Eq. (1.2), there may be other induced operators |
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involving the SM gauge bosons, such as the electroweak trans ition operator |
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∆L=κv |
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Λ2¯µσµντFµν, (1.4) |
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wherevis the vacuum expectation value of the Standard Model Higgs fi eld andFµνis the |
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electroweak field tensor. However, when these operators are compared to the underlying |
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new strong dynamics of the four fermion interaction in Eq. (1 .2), it is found that they are |
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suppressed by O(MW/Λ), where MWis the mass of the electroweak gauge boson. For new |
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physics scales of order 1 TeV or greater, this is at least an or der of magnitude suppression. |
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Thus, we ignore these operators. |
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BHHS found that operators involving the three lightest quar ks were strongly bounded, |
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with bounds ranging from 3 to 13 TeV on the related value of Λ. T hese bounds can be found |
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in Appendix A. Not surprisingly, operators involving the to p quark were either unbounded or |
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very weakly bounded, with only the tuoperator for vector and axial vector couplings being |
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bounded by Λ <650 GeV (the bound arises through a loop in B→µτdecay). Operators |
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involving the b-quark and a light quark also have bounds on Λ which were gener ally in |
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the several TeV range. However, there were some surprises. T he scalar and pseudoscalar |
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operators involving cuandccwere completely unbounded, and the bboperator was essentially |
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unbounded for all S,P,V,A operators. And, as noted above, noneof the tensor operators |
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were considered at all, for all quark combinations. |
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In this note, we point out that the operators in Eq. (1.1) (wit hout involving top quarks) |
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will contribute to µ−τproduction at hadron colliders. Given that many of the possi ble |
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– 2 –operators, as noted above, are completely unbounded or weak ly bounded from the current |
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low energy data, study of pp→µτat the LHC or pp→µτat the Tevatron will probe |
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unexplored territory. |
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There have been some previous discussions of µ−τproduction at hadron colliders. Han |
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and Marfatia [4] looked at the lepton-violating decay h→µτat hadron colliders, and a very |
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detailed analysis of signals and backgrounds was carried ou t by Assamagan et al. [5] after- |
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wards. Other work looking at Higgs decays focused on mirror f ermions [6], supersymmetric |
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models [7], seesaw neutrino models [8], and Randall-Sundru m models [9]. In addition to |
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Higgs decays, others have considered lepton-flavor violati on in the decays of supersymmetric |
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particles [10] and in horizontal gauge boson models [11]. Th ese analyses, however, were done |
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in the context of very specific models (often relying on the as sumption that the µandτare |
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emitted in the decay of a single particle). Here, we will use a much more general effective |
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field theory approach. |
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This paper is organized as follows. In the next section, we di scuss the cross sections |
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forµτproduction via the various operators. A detailed analysis o f the signal identification |
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and background subtraction is in Section 3, and Section 4 con tains some discussions and our |
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conclusions. Appendix A reiterates the bounds from BHHS for comparison, and Appendix B |
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outlines the calculation of partial-wave unitarity bounds . |
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2.µτProduction at Hadron Colliders |
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Dueto the absenceof appreciable µτproductionin theSM, their production can beestimated |
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via the effective operators in Eq. (1.1). On dimensional groun ds, the cross section for ¯ qiqj→ |
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µτgrows with center of mass energy, i.e., |
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σ(¯qiqj→µτ)∝s |
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Λ4, (2.1) |
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where√sis the center of mass energy for the partonic system. This gro wth of cross section |
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with energy will eventually violate unitarity bounds. Expa nding the scattering amplitudes in |
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partial waves, we find the unitarity bounds to be (see Appendi x B) |
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s≤/braceleftBigg |
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2Λ2for scalar ,pseudoscalar ,and tensor; |
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3Λ2vector and axial vector case .(2.2) |
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The total cross sections for µτproduction at the hadronic level after convoluting with |
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the parton distribution functions (pdfs) are |
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σScalar=π |
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3S |
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Λ4/integraldisplayτmax |
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τ0dτ(q⊗q)(τ)/parenleftbigg |
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1−τ0 |
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τ/parenrightbigg2 |
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τ (2.3) |
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σVector=4π |
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9S |
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Λ4/integraldisplayτmax |
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τ0dτ(q⊗q)(τ)/parenleftbigg |
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1−τ0 |
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τ/parenrightbigg2/parenleftbigg |
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1+τ0 |
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2τ/parenrightbigg |
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τ (2.4) |
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σTensor=8π |
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9S |
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Λ4/integraldisplayτmax |
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τ0dτ(q⊗q)(τ)/parenleftbigg |
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1−τ0 |
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τ/parenrightbigg2/parenleftbigg |
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1+2τ0 |
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τ/parenrightbigg |
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τ, (2.5) |
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– 3 –whereτ=s/S,τ0=m2 |
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τ/S,mτis the tau mass, and√ |
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Sis the center of mass energy in the |
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lab frame. The pseudoscalar cross section is of the same form as the scalar cross section, and |
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the axial vector cross section is of the same form as the vecto r cross section. Our perturbative |
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calculation will become invalid at the unitarity bound, hen ce there is a maximum on the τ |
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integration. It is given by τmax= 2Λ2/Sfor the scalar, pseudoscalar, and tensor cases, and |
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τmax= 3Λ2/Sfor the vector and axial-vector cases. Also, q(x) is the quark distribution |
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function with flavor sum suppressed, and ⊗denotes the convolution defined as |
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(g1⊗g2)(y) =/integraldisplay1 |
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0dx1/integraldisplay1 |
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0dx2g1(x1)g2(x2)δ(x1x2−y). (2.6) |
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The CTEQ6L parton distribution function set is used for all o f the results [12]. |
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Results for the cross sections for the scalar, pseudoscalar , vector, axial vector, and tensor |
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structures at the Tevatron, LHC at 10 TeV and 14 TeV are given i n Table 1. Thecross section |
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for the pseudoscalar (axial vector) current is the same as fo r the scalar (vector) current. For |
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all cases, Λ is set equal to 2 TeV and the unitarity bounds are t aken into consideration. At |
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this rather high scale, the production rates are dominated b y the valence quark contributions. |
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The cross sections at the LHC are larger than those at the Teva tron by roughly an order of |
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magnitude, reaching about 100 pb. |
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For some cases the bounds from BHHS are greater than 2 TeV, hen ce the cross section |
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needs to be scaled to determine a realistic cross section at h adron colliders. The partonic |
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cross sections scale at Λ−4, but at the hadronic level a complication arises since the un itarity |
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bounds introduce a dependence on the new physics scale in the integration over pdfs. If |
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the unitarity bounds are ignored ( τmax= 1), one finds that with Λ = 2 TeV neglecting the |
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unitarity bounds has at most a 10% effect on the cross sections a t the LHC for both 10 TeV |
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and 14 TeV and no effect at the Tevatron since the unitarity boun ds are greater than the lab |
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frame energy. Hence, if Λ is increased from 2 TeV, at the LHC it is a good approximation to |
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assume the cross section scales as Λ−4and at the Tevatron the cross section scales exactly as |
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Λ−4. For example, the lower bound on Λ for the vector u¯ucoupling from BHHS is 12 TeV, so |
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the maximum cross section at the 14 TeV LHC from this operator would be approximately |
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160×(2/12)4pb = 120 fb. On the other hand, there is no bound whatsoever for the vector |
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u¯ccoupling, and thus a cross section limit of 110 pb would yield a new limit of 2 TeV on the |
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scale of this operator. This would constitute an improvemen t of many orders of magnitude. |
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3. Signal Identification and Backgrounds |
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Upon production at hadron colliders, τ’s will promptly decay and are detected via their decay |
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products. About 35% of the time the τdecays to two neutrinos and an electron or muon, the |
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other 65% of the time the τdecays to a few hadrons plus a neutrino. We will consider the τ |
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decay to an electron as well as hadronic decays in this work. T he decay to a muon will result |
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in aµ+µ−final state that has a large Drell-Yan background. We will stu dy the signal reach |
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at the Tevatron and at the 14 TeV LHC. |
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– 4 –Table 1: Cross sections for all the scalar, pseudoscalar, vector, axial ve ctor, and tensor structures at |
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the Tevatron at 2 TeV, the LHC at 10 TeV, and the LHC at 14 TeV. Th e pseudoscalar (axial vector) |
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cross section is the same as the scalar (vector) cross section. All cross sections were evaluated with |
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the new physics scale Λ = 2 TeV and the unitarity bounds are taken int o consideration. |
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Tevatron 2 TeV ( p¯p)LHC 10 TeV ( pp) LHC 14 TeV ( pp) |
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σ(pb)1,γ5γµ,γµγ5σµν1,γ5γµ,γµγ5σµν1,γ5γµ,γµγ5σµν |
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u¯u8.4 11 22 63 85 170 120 160 310 |
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d¯d2.5 3.3 6.7 38 51 100 72 98 190 |
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s¯s0.18 0.24 0.49 5.5 7.4 15 11 15 30 |
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d¯s1.3 1.7 3.4 34 45 91 66 89 180 |
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d¯b0.50 0.67 1.3 17 22 45 34 46 90 |
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s¯b0.13 0.17 0.34 5.0 6.7 13 11 14 28 |
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u¯c1.5 2.0 3.9 41 55 110 80 110 210 |
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c¯c0.070 0.094 0.19 2.6 3.5 7.0 5.5 7.3 15 |
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b¯b0.021 0.028 0.056 1.1 1.5 2.9 2.4 3.2 6.4 |
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3.1τDecay to Electrons |
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3.1.1 Signal Reconstruction |
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Theτdecays to an electron plus two neutrinos about 18% of the time . We thus search for a |
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final state of an electron and muon |
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e+µ. (3.1) |
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The electromagnetic calorimeter resolution is simulated b y smearing the electron energies |
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according to a Gaussian distribution with a resolution para meterized by |
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σ(E) |
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E=a/radicalbig |
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E/GeV⊕b, (3.2) |
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where the constants are a= 10% and b= 0% at the Tevatron [13], a= 5% and b= 0.55% at |
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the LHC [14], and ⊕indicates addition in quadrature. For simplicity, we have u sed the same |
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form of smearing for the muons. |
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The decay of the τleaves us with some missing energy and we need to consider how to |
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effectively reconstructthe τmomentum. Forourprocessallthemissingtransversemoment um |
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is coming from the τ, hence |
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pτ |
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T=pe |
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T+pmiss |
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T. (3.3) |
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At hadron colliders, we have no information on the longitudi nal component of the missing |
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momentum on an event-by-event basis. However, the τwill be highly boosted and its decay |
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– 5 –products will be collimated. Hence, the missing momentum sh ould be aligned with the |
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electron momentum and the ratio pe |
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z/pmiss |
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zshould be the same as the ratio of the magnitudes |
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of the transverse momenta, pe |
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T/pmiss |
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T. Therefore, the longitudinal component of the τcan be |
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reconstructed as [4] |
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pτ |
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z=pe |
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z/parenleftbigg |
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1+pmiss |
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T |
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pe |
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T/parenrightbigg |
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. (3.4) |
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Once the three-momentum is reconstructed, we can solve for t heτenergy,E2 |
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τ=p2 |
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τ+m2 |
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τ. |
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Figure 1 illustrates the effectiveness of this method at the Te vatron. Figure 1(a) (Figure 1(b)) |
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shows the transverse momentum (longitudinal momentum) dis tribution for the theoretically |
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generated (solid) and kinematically reconstructed (dashe d)τmomenta. As can be seen, the |
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τmomentum is reconstructed effectively. |
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We first apply some basic cuts on the transverse momentum and t he pseudo rapidity |
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to simulate the detector acceptance and triggering, as well as to isolate the signal from the |
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background, |
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pµ |
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T>20 GeV,|ηµ|<2.5, |
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pe |
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T>20 GeV,|ηe|<2.5. (3.5) |
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Since the signal does not contain any jets, we also require a j et veto such that there are no |
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jets with pT>50 GeV and |η|<2.5. |
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There are several distinctive kinematic features of our sig nal. The decay products of the |
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τwill be highly collimated, and the electron transverse mome ntum will be traveling in the |
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same direction as the missing transverse momentum. Also, in the transverse plane the muon |
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and tau should be back to back. Since the electron will mostly be in the direction of the τ, |
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it will also be nearly back to back with the muon. Finally, the τandµhave equal transverse |
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momenta; hence, the decay products of the τhave less transverse momentum than the µ. We |
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can measure this discrepancy using the momentum imbalance |
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∆pT=pµ |
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T−pe |
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T. (3.6) |
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For the signal, this observable should be positive. Based on the kinematics of our signal, we |
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apply the further cuts [5] |
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δφ(pµ |
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T,pe |
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T)>2.75 rad, δφ(pmiss |
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T,pe |
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T)<0.6 rad, (3.7) |
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∆pT>0. |
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3.1.2 Backgrounds and their Suppression |
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Theleadingbackgrounds are W+W−pair production, Z0/γ⋆→τ+τ−, andt¯tpair production |
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[5]. The total rates for these backgrounds at the Tevatron an d the LHC are given in Table 2 |
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with consecutive cuts. We consider both of the final states wi thµ+andµ−. |
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– 6 –0 100 200 300 |
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pτ |
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T (GeV)10-410-310-210-1dσ/dpT (pb/GeV)Generated |
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Reconstructed |
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(a)-300 -200 -100 0 100 200 300 |
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pτ |
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z (GeV)10-310-210-1dσ/dpz (pb/GeV)Generated |
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Reconstructed |
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(b) |
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Figure 1: Distributions of the theoretically generated (solid line) and kinematic ally reconstructed |
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(dashed line) τmomentum at the Tevatron at 2 TeV with a u¯cinitial state, scalar coupling, and new |
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physics scale of 1 TeV. Fig. (a) is the τtransverse momentum distribution, and Fig. (b) is the τ |
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longitidunal momentum distribution. |
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Table 2: Leading backgrounds to the τ’s electronic decay before and after consecutive kinematic and |
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invariant mass cuts for (a) the Tevatron at 2 TeV and (b) the LHC a t 14 TeV. |
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Backgrounds (pb) No Cuts Cuts Eq. (3.5) + Eq. (3.7) + Eq. (3.8) |
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(a) Tevatron 2 TeV |
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W+W−→µ±νµτ∓ντ0.032 0.0046 0.0012 2.6×10−4 |
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W+W−→µ±νµe∓νe0.18 0.13 0.0060 9.8×10−4 |
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Z0/γ⋆→τ+τ−→µ±νµτ∓610 0.21 0.091 1.4×10−4 |
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t¯t→µ±νµbτ∓ντ¯b 0.020 6.5×10−47.4×10−54.4×10−5 |
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t¯t→µ±νµbe∓νe¯b 0.11 0.0099 7.3×10−42.7×10−4 |
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(b) LHC 14 TeV |
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W+W−→µ±νµτ∓ντ0.34 0.030 0.0088 0.0031 |
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W+W−→µ±νµe∓νe 1.9 0.99 0.051 0.014 |
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Z0/γ⋆→τ+τ−→µ±νµτ∓2300 1.1 0.49 0.0014 |
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t¯t→µ±νµbτ∓ντ¯b 1.9 0.070 0.010 0.0077 |
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t¯t→µ±νµbe∓νe¯b 11 1.5 0.10 0.050 |
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The partonic cross section of our signal increases with ener gy while the cross sections |
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of the backgrounds will decrease with energy. Hence, the inv ariant mass distribution of our |
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signal does not fall off as quickly as the backgrounds. |
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Figure 2(a) shows the invariant mass distributions of backg rounds and our signal at the |
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Tevatron with initial states c¯candu¯cwith various couplings and a new physics scale of |
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1 TeV after applying the cuts in Eqs. (3.5) and (3.7). The cros s section for the pseudoscalar |
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– 7 –0 200 400 600800 1000 |
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Mµτ (GeV)10-510-410-310-2dσ/dMµτ (pb/GeV)eµνν |
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τ+τ− |
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Tensor |
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Vector |
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Scalaru c-bar |
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c c-barTevatron |
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(a)0 200 400 600800 1000 |
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Mµτ (GeV)10-510-410-310-2dσ/dMµτ (pb/GeV)eµνν |
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τ+τ−1 TeV |
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2 TeV |
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3 TeVTevatron |
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(b) |
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Figure 2: The invariant mass distributions of the reconstructed τ−µsystem at the Tevatron at 2 |
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TeV. Fig. (a) shows the distributions of the leading backgrounds (d otted and dot-dot-dash) and of |
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our signal for the u¯candc¯cinitial states with coupling of various Lorentz structures and a new physics |
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scale of 1 TeV. Fig. (b) shows the distributions of the leading backgr ounds (dotted and dashed) and |
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of our signal (solid) for the u¯cinitial state with scalar coupling and various new physics scales. The |
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cuts in Eqs. (3.5) and (3.7) have been applied. |
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(axial-vector) couplings are the same as those for the scala r (vector) couplings. The decline |
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in the signal rates is due to a suppression of the pdfs at large x. Although the signal rates |
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steeply decline with invariant mass the background falls off faster. The u¯csignal is still clearly |
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above background due to a valence quark in the initial state, but thec¯csignal distribution is |
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much closer to the background distribution due to the steep f all with invariant mass and a |
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lack of an initial state valence quark. Figure 2(b) shows the invariant mass distributions of |
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backgroundsandoursignalattheTevatronwithinitial stat eu¯candscalarcouplingforvarious |
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new physics scales. The 3 TeV new physics scale invariant mas s distribution is approaching |
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the background distribution. A higher cutoff on the invarian t mass will be needed to separate |
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the weak signal from the backgrounds. Based on Fig. 2, we prop ose a selection cut on |
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Mµτ>250 GeV . (3.8) |
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Table 2 shows the effects of the invariant mass cut on the backgr ounds in the last column. |
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Similar analyses can be carried out for the LHC. Figure 3(a) s hows the invariant mass |
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distribution for our signal with the u¯candc¯cinitial states and various Lorentz structures, as |
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well as the backgroundsafter thecuts in Eqs. (3.5) and(3.7) . Thenewphysics scale was set to |
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1 TeV and the unitarity bound is imposed. Figure 3(b) shows th e invariant mass distribution |
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of theu¯cinitial state with various new physics scales. The cutoff on t he invariant mass |
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corresponds to the unitarity bound, the scale at which the pe rturbative calculation becomes |
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untrustworthy. In the lack of the knowledge for the new physi cs to show up at the scale Λ, |
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we simply impose a sharp cutoff at the unitarity bound. As comp ared with the Tevatron, |
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the LHC signal rates fall off much less quickly with invariant mass since the Tevatron’s lower |
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– 8 –0 500 1000 1500 |
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Mµτ (GeV)10-410-310-210-1dσ/dMµτ (pb/GeV)Tensor |
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Vector |
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Scalar |
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bbeµνντ+τ−u c-bar |
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c c-barLHC |
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(a)0 1 2 3 4 |
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Mµτ (TeV)10-510-410-310-210-1dσ/dMµτ (pb/GeV)bbeµνν |
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τ+τ−1 TeV |
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2 TeV |
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3 TeV |
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4 TeV |
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5 TeVLHC |
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(b) |
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Figure 3: The invariant mass distributions of the reconstructed τ−µsystem at the LHC at 14 TeV. |
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Fig. (a) shows the distributions of the leading backgrounds (dotte d and dot-dot-dash) and of our |
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signal for the u¯candc¯cinitial states with coupling of various Lorentz structures and a new physics |
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scale of 1 TeV. Fig. (b) shows the distributions of the leading backgr ounds (dotted and dashed) and |
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of our signal (solid) for the u¯cinitial state with scalar coupling and various new physics scales. The |
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cut offs in the distributions at high invariant mass are due to the unita rity bounds. The cuts in Eqs. |
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(3.5) and (3.7) have been applied. |
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energy leads to a suppression from the pdfs at large x. As can be seen, as the new physics |
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scale increases the cross section decreases and the backgro und becomes more problematic at |
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lower invariant mass. Also, as the new physics scale increas es the unitarity bound becomes |
|
less strict. Hence, although the backgrounds at the LHC are c onsiderably larger than at the |
|
Tevatron, for large new physics scales the LHC has an enhance ment in the signal cross section |
|
from the large invariant mass region. |
|
3.2τDecay to Hadrons |
|
Although with significantly larger backgrounds, the signal fromτhadronic decays can be |
|
very distinctive as well. We limit the hadronic τdecays to 1-prong decays to pions, i.e., |
|
τ±→π±ντ,τ±→π±π0ντ, andτ±→π±2π0ντ. Theτ’s have 1-prong decays to these final |
|
states about 50% of the time. We thus search for a final state of aτjet and a muon |
|
jτ+µ. (3.9) |
|
To simulate detector resolution effects, the energy is smeare d according to Eq. (3.2) with |
|
a= 80% and b= 0% for the jet at the Tevatron [13] and a= 100% and b= 5% at the LHC |
|
[14]. As in the electronic decay, the τis highly boosted and its decay products are collimated. |
|
Hence, all the missing energy in the event should be aligned w ith theτ. The signal is then |
|
reconstructed as described in Eqs. (3.3) and (3.4) with the e lectron momentum replaced by |
|
the momentum of the τ-jet. |
|
– 9 –The hadronic decay of the τalso has the backgrounds W+W−pair production, Z0/γ⋆→ |
|
τ+τ−, andt¯tpair production plus an additional background of W+jet, where the jet is |
|
misidentified as a τ-jet. At the Tevatron, we assume a τ-jet tagging efficiency of 67% and |
|
that a light jet is mistagged as a τ-jet 1.1% of the time [15] and at the LHC we assume a τ-jet |
|
tagging efficiency of 40% and a light jet misidentification rat e of 1% [14]. Even with a low |
|
rate of misidentification, the W+jet background is large. To suppress this background, we |
|
note that for hadronic decays most of the τtransverse momentum will be carried by the jet. |
|
Hence the τ-jet should be traveling in the same direction as the reconst ructedτmomentum. |
|
Motivated by this observation, we apply the same cuts as Eqs. (3.5), (3.7), and (3.8) with the |
|
electron momentum replaced by the τ-jet momentum and the additional cuts |
|
pτ−jet |
|
T |
|
pτ |
|
T>0.6 ∆ R(pτ−jet |
|
T,pτ |
|
T)<0.2 rad. (3.10) |
|
3.3 Sensitivity Reach at the Tevatron |
|
One can determine the sensitivity of the Tevatron to the new p hysics scale with 8 fb−1of |
|
data. Table 3 shows the sensitivity of the Tevatron for (a) el ectronic and (b) hadronic τ |
|
decays. The tables list the maximum new physics scale sensit ivity at 2 σand 5σlevel at the |
|
Tevatron. The reaches for scalar (vector) and pseudoscalar (axial-vector) are the same at the |
|
Tevatron, although the previous bounds from BHHS for the sca lar (vector) and pseudoscalar |
|
(axial-vector) couplings may not be the same. The bounds fro m BHHS can be found in |
|
Appendix A. If only one of the bounds for scalar (vector) or ps eudoscalar (axial-vector) |
|
coupling from BHHS is greater than the Tevatron reach one sta r is placed next to the new |
|
physics scale, if both bounds are greater than the Tevatron r each two stars are placed next |
|
to the new physics scale. Due to the larger backgrounds from W+jet, the Tevatron is much |
|
less sensitive to the τhadronic decays than the τelectronic decays. |
|
There were no bounds from BHHS for the tensor couplings, so th e Tevatron will be |
|
able to exlude some of the parameter space. Since the tensor c ross sections are generally at |
|
least twice as large as the scalar cross sections, the Tevatr on is more sensitive to the tensor |
|
couplings than it is to scalar couplings. Also, in general, t he Tevatron is more sensitive to |
|
processes with initial state valence quarks than those with out initial state quarks. With 8 |
|
fb−1of data most of the bounds can be increased, some quite string ently. |
|
Somewhat similar leptonic final states have been searched fo r in a model-independent |
|
way at the Tevatron [16], although these included substanti al missing energy and possible |
|
jets. We encourage the Tevatron experimenters to carry out t he analyses as suggested in this |
|
article. |
|
3.4 Sensitivity Reach at the LHC |
|
The LHC is also sensitive to flavor changing operators. For th e signal and background anal- |
|
ysis, we used the same kinematical cuts as we used at the Tevat ron, see Eqs. (3.5), (3.7), |
|
and (3.8). Table 4 shows the sensitivity of the LHC to all poss ible initial states and the |
|
– 10 –Table 3: Maximum new physics scales the Tevatron is sensitive to with 8 fb−1of data at the 2 σ |
|
and 5σlevels. The sensitivities are presented for both (a) electronic and ( b) hadronic τdecays with |
|
various initial states. One star indicates that the Tevatron reach is less than only one of the scalar |
|
(vector) or pseudoscalar (axial-vector) bounds from BHHS, and two stars indicates that the Tevatron |
|
reach is less than both bounds from BHHS. BHHS does not contain bo unds on the tensor coupling. |
|
(a)τ→e |
|
ΛNP(TeV) 2σsensitivity 5σdiscovery |
|
Coupling 1,γ5γµ,γµγ5σµν1,γ5γµ,γµγ5σµν |
|
u¯u20 21 24 14 15 17 |
|
d¯d17 18 21 12 13 15 |
|
s¯s9.9 10 12 7.2* 7.7** 8.7 |
|
d¯s15 16 18 10 11* 13 |
|
d¯b13 14 16 9.8 10* 11 |
|
s¯b9.5 10 11 6.9 7.3 8.3 |
|
u¯c17 18 20 12 13 14 |
|
c¯c7.9 8.3 9.5 5.7 6.0 6.9 |
|
b¯b6.4 6.8 7.7 4.6 4.9 5.6 |
|
(b)τ→h± |
|
ΛNP(TeV) 2σsensitivity 5σdiscovery |
|
Coupling 1,γ5γµ,γµγ5σµν1,γ5γµ,γµγ5σµν |
|
u¯u8.6** 9.2** 10 6.5** 6.9** 8.1 |
|
d¯d5.7** 6.1** 7.1 4.3** 4.6** 5.4 |
|
s¯s1.8* 1.9** 2.3 1.4** 1.4** 1.7 |
|
d¯s3.7 4.0* 4.6 2.8* 3.0** 3.5 |
|
d¯b2.7* 2.9* 3.4 2.0** 2.2 2.5 |
|
s¯b1.5** 1.6** 1.9 1.1** 1.2** 1.4 |
|
u¯c3.9 4.1 4.8 2.9 3.1 3.6 |
|
c¯c1.1 1.2 1.4 0.89 0.95** 1.1 |
|
b¯b0.91 0.97 1.1 0.68 0.73 0.86 |
|
couplings under consideration with 100 fb−1of data. The table contains the maximum new |
|
physics scales the LHC is sensitive to at the 2 σand 5σlevels. As with the Tevatron, the |
|
LHC reach for scalar (vector) couplings is the same as that fo r pseudoscalar (axial-vector) |
|
couplings, although the bounds from BHHS may be different. If o nly one of the bounds for |
|
scalar (vector) or pseudoscalar (axial-vector) coupling f rom BHHS is greater than the LHC |
|
reach one star is placed next to the new physics scale, if both bounds are greater than the |
|
LHC reach two stars are placed next to the new physics scale. D espite the larger backrounds |
|
for the hadronic τdecays, at the LHC the reaches for the hadronic and electroni cτdecays are |
|
– 11 –Table 4: Maximum new physics scales the LHC is sensitive to at 14 TeV with 100 fb−1of data at the |
|
2σand 5σlevels. The sensitivities are presented for both (a) electronic and ( b) hadronic τdecays with |
|
various initial states. One star indicates that the LHC reach is less t han only one of the scalar (vector) |
|
or pseudoscalar (axial-vector) bounds from BHHS, and two stars indicates that the LHC reach is less |
|
than both bounds from BHHS. BHHS does not contain bounds on the tensor coupling. |
|
(a)τ→e |
|
ΛNP(TeV) 2σsensitivity 5σdiscovery |
|
Coupling 1,γ5γµ,γµγ5σµν1,γ5γµ,γµγ5σµν |
|
u¯u18 19 21 14 15 17 |
|
d¯d16 17 19 12 13 15 |
|
s¯s9.0* 9.6* 11 7.1* 7.6** 8.6 |
|
d¯s13 14 16 10 11* 13 |
|
d¯b12 13 14 9.7 10 11 |
|
s¯b8.7 9.2 10 6.8 7.3 8.2 |
|
u¯c15 16 18 12 13 14 |
|
c¯c7.2 7.6 8.6 5.7 6.0 6.8 |
|
b¯b5.8 6.2 7.0 4.6 4.9 5.5 |
|
(b)τ→h± |
|
ΛNP(TeV) 2σsensitivity 5σdiscovery |
|
u¯u15 16 18 12 13 14 |
|
d¯d13 14 16 10* 11* 13 |
|
s¯s7.9* 8.4** 9.7 6.2* 6.7** 7.7 |
|
d¯s11 12* 14 9.3 9.9* 11 |
|
d¯b10 11 13 8.4* 8.9 10 |
|
s¯b7.6 8.1 9.3 6.0 6.4 7.4 |
|
u¯c13 14 16 10 11 12 |
|
c¯c6.3 6.7 7.8 5.0 5.3 6.2 |
|
b¯b5.1 5.5 6.3 4.1 4.3 5.0 |
|
much more similar than at the Tevatron since the LHC cross sec tion receives an enhancement |
|
from the large invariant mass region. For electronic (hadro nic)τdecays the LHC with 100 |
|
fb−1of data is less (more) sensitive than the Tevatron with 8 fb−1of data. |
|
Figure 4 shows the integrated luminosities needed for 2 σand 5σobservation at the LHC |
|
with various initial states and τdecay to electrons as a function of the new physics scale. |
|
For some initial states and Lorentz structures BHHS had a bou nd on the new physics scale |
|
larger than 1 TeV. In those cases the distribution does not be gin until the BHHS bound on |
|
the new physics scale. The sensitivity for the pseudoscalar (axial-vector) is the same as the |
|
scalar (vector) state, although the bounds from BHHS are diffe rent. Note that extraordinary |
|
– 12 –1 2 3 4 5 6 78 9 10 |
|
ΛNP (TeV)10-310-210-1100101102103L (fb-1)Scalar |
|
Vector |
|
Tensor |
|
2σu c-bar Initial State |
|
5σLHC 14 TeV |
|
(a)1 2 3 4 5 6 78 9 10 |
|
ΛNP (TeV)10-310-210-1100101102103L (fb-1) |
|
Scalar |
|
Vector |
|
Tensor |
|
2σc c-bar Initial State |
|
5σLHC 14 TeV |
|
(b) |
|
1 2 3 4 5 6 78 9 10 |
|
ΛNP (TeV)10-310-210-1100101102103L (fb-1)Scalar |
|
Vector |
|
Tensor |
|
2σd b-bar Initial State |
|
5σLHC 14 TeV |
|
(c)1 2 3 4 5 6 78 9 10 |
|
ΛNP (TeV)10-310-210-1100101102103L (fb-1) |
|
Scalar |
|
Vector |
|
Tensor |
|
2σs b-bar Initial State |
|
5σLHC 14 TeV |
|
(d) |
|
Figure 4: The luminosity at the 14 TeV LHC needed for 2 σand 5σobservation as a function of the |
|
new physics scales with couplings of various Lorentz structures an d electronic τdecay. The sensitivity |
|
for theu¯cinitial state is shown in (a), for the c¯cinitial state in (b), for the d¯binitial state in (c), and |
|
for thes¯binitial state in (d). The lower bounds on the new physics scale were ta ken from BHHS. |
|
improvementintheboundscouldbefound(oradiscoverymade )withrelatively lowintegrated |
|
luminosity. Consider, for example, the u¯cinitial state. There is currently no bound at all; |
|
in principle, Λ could be tens of GeV. The figure shows that a tot al integrated luminosity of |
|
an inverse picobarn would give a 5 σsensitivity for a Λ of 1 TeV. An integrated luminosity of |
|
an inverse femtobarn would give substantial improvements f or all of the operators shown in |
|
Fig. 4. |
|
4. Discussions and Conclusions |
|
In a previous article, motivated by discovery of large νµ−ντmixing in charged current |
|
interactions, bounds on the analogous mixing in neutral cur rent interactions were explored. |
|
A general formalism for dimension-6 fermionic effective oper ators involving τ−µmixing with |
|
– 13 –typical Lorentz structure ( µΓτ)(qαΓqβ) was presented, and the low-energy constraints on |
|
the new physics scale associated with each operator were der ived, mostly from experimental |
|
bounds on rare decays of τ, hadrons or heavy quarks. Tensor operators were not conside red, |
|
and some of the operators, such as cuµτ, were completely unbounded. |
|
Inthis article, weconsider µτproductionat hadroncolliders viatheseoperators. Tables 3 |
|
and4 list thenewphysics scales that are accessible at the Te vatron and theLHC, respectively. |
|
Duetomuchsmallerbackgrounds, boththeLHCandTevatronar emoresensitivetoelectronic |
|
τdecays than hadronic τdecays. For hadronic τdecays, the LHC receives an enhancement |
|
from the large invariant mass region and is more sensitive th an the Tevatron. Since the |
|
backgrounds to electronic τdecays at the Tevatron are much smaller than those at the LHC, |
|
the Tevatron is more sensitive than the LHC to electronic τdecays. We found that at the |
|
Tevatron with 8 fb−1, one can exceed current bounds for most operators, with most 2σ |
|
sensitivities being in the 6 −24 TeV range. We find that at the LHC with 1 fb−1(100 fb−1) |
|
integrated luminosity, one can reach a 2 σsensitivity for Λ ∼3−10 TeV (Λ ∼6−21 TeV), |
|
depending on the Lorentz structure of the operator. |
|
Acknowledgments |
|
We would like to thank Vernon Barger and Xerxes Tata for discu ssions. MS would like to |
|
thank the Wisconsin Phenomenology Institute, in particula r Linda Dolan, for hospitality |
|
during his visit. The work of TH and IL was supported by the US D OE under contract |
|
No. DE-FG02-95ER40896, and that of MS was supported in part b y the National Science |
|
Foundation PHY-0755262. |
|
A. New Physics Bounds |
|
The bounds from BHHS in units of TeV are presented in Table 5. T he *s indicate there are |
|
no bounds on the new physics scale. Also, there are no bounds f rom BHHS for the tensor |
|
coupling. |
|
B. Partial Wave Unitarity Bounds |
|
Since the cross section from our higher-dimensional operat ors increases as s, it is necessary |
|
to determine the unitarity bound for q¯q→µτ. The partial wave expansion for a+b→1+2 |
|
can be written as |
|
M(s,t) = 16π∞/summationdisplay |
|
J=M(2J+1)aJ(s)dJ |
|
µµ′(cosθ) |
|
where |
|
aJ(s) =1 |
|
32π/integraldisplay1 |
|
−1M(s,t)dJ |
|
µµ′(cosθ)dcosθ, |
|
µ=sa−sb,µ′=s1−s2andJ≤max(|µ|,|µ′|). The condition for unitarity is |ℜ(aJ)| ≤1/2. |
|
– 14 –Coupling type 1 γ5 γµ γµγ5 |
|
u¯u 2.6 12 12 11 |
|
d¯d 2.6 12 12 11 |
|
s¯s 1.5 9.9 14 9.5 |
|
d¯s 2.3 3.7 13 3.6 |
|
d¯b 2.2 9.3 2.2 8.2 |
|
s¯b 2.6 2.8 2.6 2.5 |
|
u¯c * * 0.55 0.55 |
|
c¯c * * 1.1 1.1 |
|
b¯b * * 0.18 * |
|
Table 5: Bounds on the new physics scales from BHHS in units of TeV for variou s operators and the |
|
scalar, pseudoscalar, vector, and axial-vector couplings. The *s indicate there were no bounds. |
|
It is straightforward to calculate the coefficients for the S, V,T operators. For example, |
|
for the scalar operator |
|
M=4π |
|
Λ2¯vλ1(p1)uλ2(p2)¯uλ3(p3)vλ4(p4) |
|
one can just plug in the explicit expressions: |
|
uλ(p)≡/parenleftBigg/radicalbig |
|
E−λ|p|χλ(ˆp)/radicalbig |
|
E+λ|p|χλ(ˆp)/parenrightBigg |
|
vλ(p)≡/parenleftBigg |
|
−/radicalbig |
|
E+λ|p|χ−λ(ˆp)/radicalbig |
|
E−λ|p|χ−λ(ˆp)/parenrightBigg |
|
whereχ+(ˆz) =/parenleftbig1 |
|
0/parenrightbig |
|
,χ−(ˆz) =/parenleftbig0 |
|
1/parenrightbig |
|
. In the massless limit, this simply gives a0=s/(4Λ2) and |
|
so the unitarity bound gives s≤2Λ2. For the vector case, a0= 0 and a1=s/(6Λ2) giving |
|
the unitarity bound s≤3Λ2. The tensor case gets contributions from both a0anda1, and |
|
the stronger bound then applies. |
|
References |
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