Shedding light on the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ t\overline{t} $\end{document} asymmetry: the photon handle

We investigate a charge asymmetry in \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ t\overline{t}\gamma $\end{document} production at the LHC that provides complementary information to the measured asymmetries in \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ t\overline{t} $\end{document} production. We estimate the experimental uncertainty in its measurement at the LHC with 8 TeV and 14 TeV. We argue that, for new physics models that simultaneously reproduce the asymmetry excess in \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ t\overline{t} $\end{document} production at the Tevatron and the SM-like asymmetry at the LHC, the measurement in \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ t\overline{t}\gamma $\end{document} production at the LHC is likely to deviate from the SM prediction. In two new physics models studied in detail we find that the deviations could be significant and observable at the 14 TeV run.


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2. A cancellation between qq → tt (with q = u, d) and qg → ttj contributions, as for example in Z ′ models [22][23][24]. The qg processes are irrelevant at the Tevatron but not at the LHC. There, a negative asymmetry in ug → ttj could compensate a positive asymmetry in uū → tt, if one considers not only tt production but also including additional jets. This model is disfavoured by the measurement of the high-m tt tail at the LHC and may eventually be excluded with more precise measurements, but serves as a good benchmark for our discussion.
Thus, the small SM-like asymmetry observed at the LHC may in principle result from two asymmetries of opposite sign (the naturalness of this mechanism is a different issue). But the addition of a final state photon completely changes this. An asymmetry can be defined in ttγ production with ∆|y| = |y t | − |yt| the difference between the moduli of the rapidities of the top and antitop. That is, the same definition for the charge asymmetry as in tt production. In the SM, this asymmetry arises already at the tree level in qq → ttγ due to the interference between diagrams where the photon is emitted from initial quarks and diagrams where it is emitted from final state quarks. At a centre-of-mass (CM) energy of √ s = 8 TeV the tree-level value is A ttγ C = −0.058, and at √ s = 14 TeV it is A ttγ C = −0.038. Comparing to tt alone, the effect of the extra photon is twofold. First, it increases the total qq fraction of events F u + F d , F u ≡ σ(uū)/σ, F d ≡ σ(dd)/σ, thus reducing the washout due to symmetric gg fusion. (For simplicity we ignore here ss and cc initial states, which are irrelevant for the discussion.) Second, and even more importantly, if there is a cancellation between new physics contributions to turn A C small, the addition of a photon is likely to break it in A ttγ C . This is expected to be a general fact, and indeed is confirmed in this paper for the two aforementioned mechanisms.
In the first case, namely a cancellation between uū and dd contributions at the LHC, such cancellation is broken mainly because the photon couples differently to up and down quarks, and uū → ttγ is enhanced with respect to dd → ttγ. The effect can be clearly seen in figure 1 (left), where we plot the qq fraction F u + F d against the ratio F d /F u for the SM processes. (See section 2 for details of the simulations used to obtain these numbers.) Kinematical cuts on the tt velocity β [25] and the tt invariant mass m tt lead to small shifts in F d /F u and F u + F d towards the Tevatron point. But, clearly, requiring a final state photon is much more effective: it renders F d /F u very close to the Tevatron value (thus breaking a possible cancellation) and also increases the qq fraction by a factor of two, leading to larger asymmetries. For new physics contributions -such as an s-channel colour octet -that do not significantly alter the kinematics of tt and ttγ production, the behaviour is the same. Note also that F d /F u is nearly the same at the LHC with √ s = 8 TeV and √ s = 14 TeV (as well as with 7 TeV), hence the possible cancellation will also operate at 14 TeV and the measurement of A C at this energy is expected to show good consistency with the SM.  Figure 1. Left: Ratio F d /F u = σ(dd)/σ(uū) and total qq fraction F u +F d for tt and ttγ production in the SM. Right: F g /F u = σ(ug)/σ(uū) and uū fraction F u in tt(j) and ttγ(j), in the SM and for the production and decay of a Z ′ .
In the second case, the cancellation is broken due to two effects. First, there is a decrease in F g /F u = σ(ug)/σ(uū) in ttγ(j) with respect to tt(j) merely due to kinematics, which already happens in the SM. Secondly, there is a further decrease in the new physics Z ′ contribution because in uū → tt it is more likely to emit a photon than in ug → tZ ′ , since in the former there are more charged particles. We can observe this clearly in figure 1 (right), where the solid points correspond to the SM, and the hashed points are the ones for the Z ′ model, 1 as described in section 3. Notice also that F g /F u is larger at 14 TeV, increasing the negative component of A C , but the washout due to gg fusion increases too, and generically one does not expect to have visible asymmetries in tt production at 14 TeV if a cancellation of this type takes place.
As the main consequence of this simplified analysis, one can say that the requirement of an extra photon in tt production at the LHC "reweights" the new physics asymmetries in the different subprocesses, if present, recovering to a large extent the situation at the Tevatron. This is expected to be a rather general feature, and the exact numerical calculations carried out in this paper for two benchmark models confirm this semi-quantitative argument.
The remainder of this paper is organised as follows. In section 2 we present the simulation details and event selection to suppress radiative top decays, and we estimate the expected uncertainty in A ttγ C . In section 3 we study A ttγ C for two different new physics models that explain the excess in A FB and the absence of an excess in A C . Our conclusions and final remarks are given in section 4.

JHEP04(2014)188 2 Simulation details
In order to estimate the experimental uncertainty in the measurement of A ttγ C , we focus on the semileptonic tt decay channel, which constitutes the golden mode for this measurement owing to the relatively large branching ratio (∼ 30%), manageable background after b tagging requirements, and the ability to fully reconstruct the tt event kinematics. A complication arises from the fact that any realistic estimate should in principle take into consideration the full 2 → 7 calculation for the process pp → ℓνbqq ′b γ + X, since only a fraction of the cross section for this final state originates from photon radiation off the initial state quarks or the top/antitop quarks (referred to as "radiative top production"), that is, pp → ttγ + X with subsequent decay of the tt pair. As we will see in the following, the cross section is actually dominated by photon radiation off the top decay products (b quark, W boson and its charged decay products), referred to here as "radiative top decay". Therefore, it is necessary to design an event selection capable of effectively suppressing the contribution from radiative top decays, which would dilute the sensitivity of A ttγ C to new physics in the production process.
We use MadGraph 5 [27,28] to generate SM samples for the 2 → 3 process pp → ttγ + X, as well as the following two 2 → 7 processes: pp → ttγ + X with tt → ℓνbqq ′b and ℓ = e, µ (i.e. restricted to radiative top production), and pp → ℓνbqq ′b γ + X (i.e. including both radiative top production and decay). In the latter case we consider only resonant Feynman diagrams with two on-shell top quarks and two on-shell W bosons. The samples are generated for √ s = 8 TeV and 14 TeV using the CTEQ6L1 parton distribution set [29] and the event-by-event renormalisation and factorisation scale as implemented by default in MadGraph 5. A top quark mass of m t = 173 GeV is assumed throughout this study. All samples are generated requiring for the photon transverse momentum p T (γ) > 20 GeV and pseudo-rapidity |η(γ)| < 2.5. In the case of the 2 → 7 samples, additional requirements are made on final-state partons: • p T (j) > 20 GeV, |η(j)| < 5.0 (in the following we will use j to denote q or b), We perform our studies at the parton level but attempt to obtain reasonable estimates for the event selection efficiency and dilution in the measurement of A ttγ C . We do not include backgrounds, although experimental studies of ttγ production at the LHC [30,31] find that the overall background can be comparable to the signal, and dominated by tt production with an electron or jet being misidentified as a photon. Although such background contribution is large, its associated asymmetry can be precisely measured in dedicated data control samples. Estimating the effect of the background on the statistical and systematic uncertainty on A ttγ C is beyond the scope of this exploratory work and should be done in the context of the actual experimental analyses.

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Events are required to fulfill basic preselection requirements aimed at selecting the semileptonic signature: • exactly one lepton (electron or muon) with transverse momentum p T > 20 GeV and pseudorapidity |η| < 2.5; • missing transverse momentum / p T > 20 GeV; • four quarks with p T > 25 GeV and |η| < 4.5; • exactly one photon with p T > 20 GeV and |η| < 2.5; With these requirements, the leading-order (LO) effective cross section at √ s = 14 TeV is 0.13 pb in the case of the 2 → 7 calculation without radiative top decays, while it is 0.23 pb for the full 2 → 7 calculation, clearly showing the need to have additional cuts to suppress the large contribution from radiative top decays. This can be accomplished by a combination of cuts [32]: • tighter ∆R requirements between the photon and charged top quark decay products: is the invariant mass of the jjγ system and m T (ℓγ; / p T ) is the cluster transverse mass defined as with analogous definitions for particles other than the photon and the charged lepton; • veto radiative top decays: reject events satisfying either of the following conditions: • consistency with radiative top production: After all requirements, the effective cross section at √ s = 14 TeV becomes 0.083 pb in the case of the 2 → 7 calculation without radiative top decays, while it is also 0.083 pb for the full 2 → 7 calculation, demonstrating that the contribution from radiative top decays has been effectively eliminated. The effect of the sequential application of these cuts in some of the relevant kinematic distribution can be visualised in figure 2, where it is shown that after all requirements there is good agreement in both normalisation and shape between the full 2 → 7 calculation and the 2 → 7 calculation without radiative top decays. As a final  check, we have compared A ttγ C between the 2 → 3 calculation with just the photon cuts, and the full 2 → 7 calculation including all selection cuts. The inclusive asymmetries are A ttγ C = −0.039 (2) and A ttγ C = −0.035 (2), respectively, where the numbers in parentheses represent the uncertainty from limited Monte Carlo statistics. Reasonable agreement is also found for A ttγ C differentially as a function of m tt and |η(γ)|, as shown in figure 3. Therefore, in the remainder of this paper we will only consider the simpler 2 → 3 calculation for the ttγ process together with the selection efficiency estimated from the above study and summarised below. For a more realistic estimate, the LO cross section for the 2 → 3 calculation is multiplied by a k-factor of 1.75, in order to reproduce the NLO cross section of ref. [33]. Therefore, the total ttγ cross section for √ s = 8 TeV is 0.68 pb, and for √ s = 14 TeV it is 2.73 pb, corresponding to the requirements of p T (γ) > 20 GeV and |η(γ)| < 2.5. The semileptonic branching ratio is taken to be 30%. The total selection efficiency for semileptonic decays, including the effect of the preselection cuts as well the additional cuts to veto radiative top decay, is estimated to be ∼ 20% using a sample for the 2 → 7 process without radiative top decays, including only generator-level cuts on the photon of p T (γ) > 20 GeV and |η(γ)| < 2.5. We also assume a total efficiency for lepton triggering and identification of 70%, a photon identification efficiency of 85% and a per-jet b tagging JHEP04(2014)188 efficiency of 70%, resulting in an efficiency for a requirement of at least one b-tagged jet of 90%. The product of the above numbers results in a total efficiency times branching ratio of 3.2%. Therefore, the expected number of selected events for a total integrated luminosity of 20 fb −1 at √ s = 8 TeV is ∼ 440, resulting in an expected statistical uncertainty on A ttγ C of ±0.045. At a CM energy of √ s = 14 TeV with 100 fb −1 the expected number of events is ∼ 8800, giving a statistical uncertainty on A ttγ C of ±0.01. In the next section we will compute A ttγ C (see eq. (1.1)) from y t and yt at the parton level using the 2 → 3 calculation for the pp → ttγ + X process in the presence of new physics. Experimentally, the charge asymmetry would be computed after a kinematic reconstruction of the tt system in ttγ events similar to that used for the measurement of A tt C in tt production [6,7]. In the case of experimental measurements of A tt C , the fraction of events with the sign of ∆|y| correctly reconstructed is ∼ 75%. Using the simplified tt event reconstruction of ref. [25], we have verified that the fraction of events with the sign of ∆|y| correctly reconstructed is in fact ∼ 5% higher in absolute term for ttγ compared to tt production, possibly related to the higher longitudinal boost of the tt system in the case of ttγ events from the higher fraction of qq-initiated production. Nevertheless, we will conservatively assume the same fraction of 75%, which corresponds to a "dilution" factor D = 2 × 0.75 − 1 = 0.5. Such dilution results in a reduction by a factor of two of the measured A ttγ C which would effectively be corrected for by the unfolding procedure used in the experimental analyses, and can be taken into account here by an increase by a factor of two of the statistical uncertainty. Then, for √ s = 8 TeV and an integrated luminosity of 20 fb −1 , the resulting expected statistical uncertainty is ±0.09, and at √ s = 14 TeV with integrated luminosities of 100 fb −1 (400 fb −1 ) it is ±0.02 (±0.01). Our estimates do not include systematic uncertainties since, based on the present experience with the A C measurements, those are expected to be small (≤ 0.005). In any case, a careful assessment of systematic uncertainties would require a detailed analysis involving experimental simulations that are beyond the scope of this work.

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3 Asymmetries in ttγ and tt The importance of A ttγ C to provide a complementary probe of asymmetric tt production at the Tevatron is shown here with two benchmark examples. They correspond to the two types of cancellations between new physics contributions that may yield a small A C at the LHC. For our Monte Carlo calculations of tt with a colour octet we use Protos [34]. For ttγ(j) production in the colour octet and with an extra Z ′ we use MadGraph 5 [27,28] coupled to Pythia [35] in its default tune with a MLM matching scheme [36] implemented to avoid double counting in the extra jet between the matrix element calculation and the parton shower. In both models the asymmetries A ttγ C are calculated at leading order. For the comparison with experimental data, especially at √ s = 14 TeV, next-to-leading order (NLO) computations would be required, at least for the SM asymmetries. (The asymmetries including new physics contributions could be approximated, as usual, by summing the SM asymmetries at NLO and the new physics contributions at LO.) In any case, our leading-order calculations are sufficient to demonstrate the importance of this asymmetry and its potential to exhibit deviations from the SM predictions.

A ttγ C for a colour octet
We scan the parameter space of couplings of a light colour octet [37][38][39][40][41], with a fixed mass M = 250 GeV and a large width Γ/M = 0.2, that is assumed in order to comply with dijet pair constraints [42,43]. (This width may originate from additional decays to non-SM particles.) This scan is a particular subset of a more general parameter space scan to be presented and discussed elsewhere [44]. For simplicity, here we take the vector couplings of the up and down quarks to zero. The parameter space points considered here have a global agreement with tt experimental data at the level of 1σ or better, including several observables such as cross sections and asymmetries. The details of the fit are not essential here for our purposes, and it is sufficient to mention that the resulting points comprise high as well as low values of A FB , that might -or not -explain the Tevatron anomaly. Analogously, the resulting values of A C span a ±2σ range above and below the SM predictions for 7 and 8 TeV. For these points, we present in figure 4 the asymmetry A C at 8 TeV versus A ttγ C at 8 TeV (left) and 14 TeV (right). The shaded horizontal area corresponds to the CMS measurement A C = 0.005 ± 0.009 [7] and its 1σ uncertainty. The vertical lines represent the SM value of A ttγ C and its expected uncertainty, estimated in section 2. The points are coloured according to the value of the Tevatron asymmetry A FB . From left to right: red points have A FB below −2σ of the naive Tevatron average A exp FB = 0.187 ± 0.036; orange points have A FB between −2σ and −1σ; green points have A FB between −1σ and 1σ; blue points have asymmetries above 1σ. In all cases the SM contribution to the asymmetries [11] is summed to the ones resulting from new physics. The difference found between 8 TeV and 14 TeV is given by the much better statistics at the latter CM energy, which by far compensates the slightly smaller A ttγ C due to the increased gg cross section. (As pointed out before, the ratio F d /F u is nearly the same at these two energies.) Interestingly, for the parameter space points (in green) that predict an asymmetry A FB within ±1σ of the Tevatron average, the asymmetry in ttγ departs 1σ or more above the SM value. This happens irrespectively of the value of the asymmetry in tt production A C , that may even have the SM value. We also note that for all points the increase in A ttγ C with respect to the SM value is positive. This is expected from the behaviour shown in figure 1 (left), and is clearly because the increase in A FB with respect to the SM value is also positive, as preferred by the fit to the Tevatron measurements.

A ttγ
C for a Z ′ We have chosen a reference point in the extra Z ′ model that represents the region of parameter space compatible with the relevant observables as stated in the study in ref. [45]. We have set M Z ′ = 275 GeV, g utZ ′ = 0.7 and an invisible Z ′ branching ratio B(Z ′ → invisible) = 3/4. This model predicts a charge asymmetry at the LHC of A C = 0.015 at 8 TeV, which is compatible with CMS measurement [7] and SM prediction. However, when an extra photon is required, its prediction yields A ttγ C = −0.048 and A ttγ C = −0.018 at 8 TeV and 14 TeV, respectively, which again is an excess over the SM expected asymmetry (compare to the SM prediction in figure 4). We see that also in this case, the 8 TeV measurement of A ttγ C would not differentiate this model from the SM, but we can expect that 400 fb −1 at 14 TeV could be able to do it.

A C at 14 TeV
Finally, in order to stress the importance of A ttγ C , we have checked that in both models the prediction of A C in tt production at 14 TeV is always consistent with the SM, assuming an experimental uncertainty of ±0.005. This is expected from the arguments given in the introduction. If a cancellation between uū and dd contributions takes place to render the LHC asymmetry small at 7 and 8 TeV, it should also operate at 14 TeV, where F d /F u is similar. Or, if there exists a cancellation between uū and gu, at 14 TeV this cancellation is relaxed by the larger F g /F u but the resulting asymmetry is small anyway.

JHEP04(2014)188 4 Conclusions
After several years of measurements with increasing precision, the excess asymmetry A FB in tt production at the Tevatron and the SM-like charge asymmetry A C in tt production at the LHC continue to be puzzling. If new data confirm the current central values and reduce their uncertainties, it is unlikely that both can be explained within the SM (also with additional isospin-conserving contributions yet unaccounted for) and simple extensions. Barring the possibility of unknown systematic uncertainties, the only way to explain these measurements is by means of some cancellation of new physics contributions at the LHC, to give approximately the SM value.
A previous attempt to solve this puzzle has been the introduction of the colliderindependent asymmetries [12,46] A u , A d that are the same at the Tevatron and the LHC, and whose measurement -quite demanding from the experimental point of view -could settle the issue. Also, the determination of ratios of differential asymmetries [47,48] would be useful to uncover possible anomalies. In this paper we have pointed out that, if the pattern of large A FB and SM-like A C corresponds to some cancellation, such cancellation should not occur in ttγ production at the LHC, where the additional photon alters the balance between new physics contributions compared to the case of tt production. This fact turns extremely interesting the measurement of a charge asymmetry in ttγ production. Moreover, even if the Tevatron excess is not due to new physics, the measurement of A ttγ C could shed light into the nature of the Tevatron anomaly.
We have studied the feasibility of this measurement and we have shown that the unwanted contributions to the final state of interest, where the photon is radiated off the top quark decay products, can be effectively suppressed with a judicious set of kinematical cuts. We have then estimated the experimental uncertainty on the measurement of A ttγ C , to investigate the potential to observe deviations from the SM. Our estimations are conservative, partly because the correct reconstruction of |∆y| is better in ttγ than in tt, and we have assumed the same performance. In addition, we expect that optimised experimental analyses could potentially achieve higher selection efficiencies than those assumed in this study. Finally, the measurements from ATLAS and CMS can be combined, which brings an advantage for a statistics-dominated measurement as in our case.
At 7 and 8 TeV, the statistics is likely not enough to reach a conclusive statement. At 14 TeV, we have shown that there are good chances of observing a deviation from the SM prediction in the case of a colour octet and in the extra Z ′ model. In both cases we do find an excess in A ttγ C with respect to the SM -and we argue that this should be in general expected for new physics models that yield an excess in A FB . On the other hand, the predictions for the charge asymmetry A C in tt production at 14 TeV are close to the SM expectation. Therefore -aside more demanding doubly-differential studies of the β and m tt dependence of A C [12] or ratios of differential asymmetries [47,48] -the measurement of a charge asymmetry in ttγ seems the best avenue to explore FB-asymmetric tt production in the upcoming LHC run.