Spin polarisation of \(t\bar{t}\gamma \gamma \) production at NLO+PS with GoSam interfaced to MadGraph5_aMC@NLO

The European Physical Journal C, Apr 2016

We present an interface between the multipurpose Monte Carlo tool MadGraph5_aMC@NLO and the automated amplitude generator GoSam. As a first application of this novel framework, we compute the NLO corrections to \(pp \rightarrow \) \(t\bar{t}H\) and \(pp \rightarrow \) \(t\bar{t}\gamma \gamma \) matched to a parton shower. In the phenomenological analyses of these processes, we focus our attention on observables which are sensitive to the polarisation of the top quarks.

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Spin polarisation of \(t\bar{t}\gamma \gamma \) production at NLO+PS with GoSam interfaced to MadGraph5_aMC@NLO

Eur. Phys. J. C Spin polarisation of t t¯γ γ production at NLO+PS with GOSAM interfaced to MADGRAPH5_AMC@NLO Hans van Deurzen 2 Rikkert Frederix 1 Valentin Hirschi 0 Gionata Luisoni 2 Pierpaolo Mastrolia 2 5 Giovanni Ossola 3 4 0 SLAC, National Accelerator Laboratory , 2575 Sand Hill Road, Menlo Park, CA 94025-7090 , USA 1 Physik Department T31, Technische Universität München , James-Franck-Str. 1, 85748 Garching , Germany 2 Max-Planck-Institut für Physik , Föhringer Ring 6, 80805 Munich , Germany 3 The Graduate School and University Center, City University of New York , 365 Fifth Avenue, New York, NY 10016 , USA 4 New York City College of Technology, City University of New York , 300 Jay Street, Brooklyn, NY 11201 , USA 5 Dipartimento di Fisica e Astronomia, Università di Padova and INFN Sezione di Padova , via Marzolo 8, 35131 Padua , Italy We present an interface between the multipurpose Monte Carlo tool MadGraph5_aMC@NLO and the automated amplitude generator GoSam. As a first application of this novel framework, we compute the NLO corrections to pp → t t¯H and pp → t t¯γ γ matched to a parton shower. In the phenomenological analyses of these processes, we focus our attention on observables which are sensitive to the polarisation of the top quarks. 1 Introduction The development of automated tools for precise calculations of total cross sections and differential distributions in high-energy collisions has undergone a dramatic acceleration in the last decade. While Leading-Order (LO) tools, based on automated tree-level calculations, have been available for a long time [ 1–11 ], the needs of the experimental analyses at the Large Hadron Collider (LHC) and a deeper understanding of the structure of scattering amplitudes [ 12– 14 ] at one loop led to the development of several computer frameworks for the automated computation of loop matrix elements [ 15–20 ] and physical observables at Nextto-leading-Order (NLO) accuracy [ 21–27 ]. Moreover, techniques to properly deal with the merging of different multiplicities in the final states and the matching [ 28,29 ] to parton shower were successfully developed [ 30–34 ] and are nowadays available. Advanced automated calculations have been performed by embedding the codes for generating virtual corrections at NLO precision, the so called One Loop Providers (OLPs), within a Monte Carlo program (MC). The interplay between MCs programs and OLPs is controlled by means of interfaces, which allow the user to get direct access to the main features of the MC code, bypassing the need of knowing the technical details of the OLP, which is ideally an inner engine within the MC generator. Many of such interfaces are based on the standards settled by the Binoth Les Houches Accord (BLHA) [ 35,36 ], which defines specifications of the communication between MCs and OLPs. The LHC has recently started Run II, collecting data at an energy scale never explored before. Within this activities automated multipurpose tools for particle collisions simulation are of fundamental importance for comparing theoretical predictions with experimental data, thereby extracting important information as regards the Standard Model (SM) and exploring all traces of deviations from it. The need for flexible tools which at the same time can provide accurate predictions, both in the SM and Beyond (BSM), may become of primary relevance in the near future. It is therefore important to be able to connect different tools to increase the reliability of the results. With these goals in mind, we present the interface between the multipurpose NLO Monte Carlo tool MadGraph5_aMC@NLO(MG5_aMC) [ 27 ] and the automated one-loop amplitude generator GoSam [ 20 ]. The advantage of this combination is twofold. On the one hand, this tandem allows the user of MG5_aMC to switch between two options of OLPs, namely between the inhouse code MadLoop [ 23 ] fully integrated directly in the MC distribution package, and GoSam. Thus, the user can experience the evaluation of NLO virtual corrections by means of two alternative solutions corresponding to different algorithms and methods of generation and evaluation of Feynman amplitudes. On the other hand, GoSam is interfaced to several MCs codes, like Sherpa [ 21 ], Herwig++ [ 26 ], Powheg [ 25 ], beside MG5_aMC, therefore the user of the MCs can explore and compare the different features of the event generators, without being biased by the performances of the OLPs, since they all can be run using GoSam. As an illustration of the novel framework MG5_aMC + GoSam, we present its application to the NLO corrections to pp → t t¯H , H → γ γ and the continuum pp → t t¯γ γ matched to a parton shower. The production of a Higgs boson in association with a pair of top anti-top quarks is an important process to directly study the Yukawa coupling of the Higgs boson with massive fermions. Such a channel, and its corresponding backgrounds, were recently the subject of detailed studies, both at LO [ 37–39 ] and NLO [ 40 ] precision. Very recently, new analyses have appeared which further extend these studies including the decay of the top and anti-top quark into bottom quarks and leptons [ 41 ], considering the production of a top-quark pair in conjunction with up to two vector bosons [ 42 ], and exploring the CP-structure of the top-Higgs coupling [ 43 ]. In the phenomenological analysis contained in this paper, we focus our attention on observables sensible to the polarisation of the top quarks, such as angular variables which involve the decay of the top quark. The paper is organised as follows: in Sect. 2, after a general introduction to the GoSam and MG5_aMC codes, we will discuss the interface between the two frameworks and its validation. In Sect. 3, we will present an application of the GoSam+ MG5_aMC interface, namely the study of NLO corrections to pp → t t¯H , H → γ γ and pp → t t¯γ γ matched to a parton shower. Finally in Sect. 4, we will draw our conclusions. 2 Computational setup For the computations contained in this paper, the automated one-loop amplitude generator GoSam has been fully interfaced to the MG5_aMC Monte Carlo framework. In this section, we briefly review the main characteristics of each of these tools and describe the details of the interface between them, which allows one to use one-loop amplitudes generated by GoSam within MG5_aMC. Finally we discuss the validation of the interface by means of a comparison with an independent framework. 2.1 GoSam The main idea that distinguishes the GoSam framework [ 20 ] from other codes for the automated generation of one-loop amplitudes is the combined use of automated diagrammatic generation and algebraic manipulation in d = 4 − 2 dimensions, thus providing analytic expressions for the integrands, with d-dimensional integrand-level reduction techniques, or tensorial reduction. Amplitudes are automatically generated via Feynman diagrams and, according to the reduction algorithm selected by the user, are algebraically manipulated and cast in the most appropriate output [ 44–49 ]. The individual program tasks are controlled by means of a python code, while the user only needs to prepare an input card to specify the details of the process to be calculated without worrying about internal details of the code generation. After the generation of all contributing diagrams, the virtual corrections are evaluated using the integrand reduction via Laurent expansion [ 50 ], provided by Ninja [ 51,52 ], or the d-dimensional integrand-level reduction method [ 53–55 ], as implemented in Samurai [ 56,57 ]. Alternatively, the tensorial decomposition provided by Golem95C [ 58–61 ] is also available. The scalar loop integrals can be evaluated using Golem95C, OneLOop [62], or QCDLoop [63,64]. The GoSam framework can be used to generate and evaluate one-loop corrections in both QCD and electroweak theory [ 65 ]. Model files for Beyond Standard Model (BSM) applications generated from a Universal FeynRules Output (UFO) [ 66,67 ] or with LanHEP [68] are also supported. A model file which contains the effective Higgs–gluon couplings that arise in the infinite top-mass limit is also available in the current distribution and it was successfully used to compute the virtual corrections for the production of a Higgs boson in association with 2 and 3 jets [ 69,70 ]. The computation of physical observables at NLO accuracy, such as cross sections and differential distributions, requires one to combine the one-loop results for the virtual amplitudes obtained with GoSam, with other parts of the calculations, namely the computation of the real emission contributions and of the subtraction terms, needed to control the cancellation of IR singularities. In some of the earlier calculations performed with GoSam [ 71–75 ], the problem was solved by means of an ad hoc adaptation of the MadDipoleMadgraph4- MadEvent framework [ 1,9,76,77 ]. Far more efficiently, this task can be performed by embedding the calculation of virtual corrections within a multipurpose Monte Carlo program (MC), that can also provide the phase-space integration, which is what is pursued in this work. In this case, the MC takes control over the different stages of the calculation, in particular the phase-space integration and the event generation, and calls GoSam at runtime to obtain the corresponding value of the one-loop amplitude at the given phase-space points. This approach has the great advantage of making available to the user all the advanced features that the MC generator provides, for example to allow for parton showering, further decays of the final-state hard particles retaining spin correlation and merging of different final state multiplicities. While in the present paper we will focus on the interface between GoSam and MG5_aMC, it is worth mentioning that a number of phenomenological results can be found in the literature which were obtained by combining GoSam with other MC programs, in particular with Sherpa [ 21,78–81 ], Herwig++ [ 26,82 ], and Powheg [ 25,83,84 ]. 2.2 MadGraph5_aMC@NLO The MG5_aMC framework [ 27 ] has been developed to be able to generate events and compute differential cross sections with a high-level of automation. The central idea behind the code is that the structure of cross sections is essentially independent of the process under consideration. Therefore, once this structure has been set up, any cross section can be computed within the framework. For example, even though the matrix elements are process and theory dependent, they can be computed from a very limited set of instructions based on the Feynman rules. The core of the MG5_aMC framework is based on treelevel amplitude generation, since in this code the matrix elements used in both LO and NLO computations are constructed from tree-level Feynman diagrams. The generation of these amplitudes is based on three elements which are key to taming the complexity of the computation as the number of external particles increases: colour decomposition, helicity amplitudes and recycling of identical substructures between diagrams. The internal algorithms used have been described extensively in Ref. [ 85 ] and Ref. [ 18,23,27,53,86,87 ] for the generation of tree-level and one-loop matrix elements, respectively. Beyond the lowest order in perturbation theory, intermediate contributions to the computation of (differential) cross sections are plagued by divergences. In particular the soft/collinear divergences in the numerical phase-space integration over the real-emission (Bremsstrahlung) corrections are non-trivial to deal with. In MG5_aMC, the FKS subtraction method [ 88,89 ] is used to factor out the singularities in order to cancel them analytically with singularities present in the virtual corrections. The FKS subtraction is based on partitioning the phase space, in which each phasespace region has at most one collinear and one soft singularity. These singularities are subtracted before performing the numerical phase-space integration by using a straightforward plus-description. The subtraction terms have been integrated analytically, using dimensional regularisation, once and for all, resulting in explicit poles in 1/ and 1/ 2, which cancel similar poles in the virtual corrections and the PDFs. Independently of which code one uses for the computation of the virtual corrections, for example MadLoop [ 23 ] or GoSam [ 20 ], optimisations in the phase-space integration of these contributions are used, as described in Ref. [ 27 ]. That is, during the phase-space integration an approximation of the virtual corrections based on the born matrix elements is created dynamically. These approximate virtual matrix elements are very fast to evaluate and can therefore be efficiently integrated numerically with high statistics. The small difference between the approximate and the exact virtual corrections is relatively slow to evaluate for a given phasespace point, but given that this is a very small contribution to the final result, the requirement on the relative precision with which it needs to be computed can be relaxed. Therefore, using low statistics for this complicated contribution suffices, greatly reducing the overall computational time. To match the short-distance matrix elements to a parton shower, the framework of MG5_aMC employs the MC@NLO technique [ 28 ] available for Pythia 6 [ 90 ], Herwig 6 [ 91 ], Pythia 8 [ 92 ] and Herwig++ [ 93 ]. In this method, the possible double counting between the NLO corrections and the parton shower is accounted for by explicitly subtracting the parton shower approximation for the emission of a hard parton from the real-emission contributions, and the parton shower approximation of a non-emitting parton from the virtual corrections. To consistently merge various multiplicities at NLO accuracy and match them to the parton shower, the FxFx merging method [ 33 ] is available. 2.3 Interface The interface between GoSam and MG5_aMC is based on the standards of the first BLHA defined in [ 35 ]. When running the MG5_aMC interactive session, the command $ set OLP GoSam changes the employed OLP from its default MadLoop to GoSam. Alternatively, the file input/mg5_configuration.txt can be directly edited to include the line OLP = GoSam. The BLHA order and contract file system allows for a basic communication between the two codes to exchange the most fundamental information about the number and type of subprocesses, the powers of the couplings involved in the specific process, the schemes in which the computation should be performed and also the value of parameters like masses and widths. For static parameters, which do not change at each phase-space point, but stay constant during the MC integration and event generation, the information is passed via a SUSY Les Houches Accord (SLHA) parameter file. This is created by MG5_aMC and read by GoSam. The #OLE_order written by MadGraph5_aMC@NLO path to this SLHA file is specified in the order file with the key word ModelFile. An example generated for the computation of t t¯γ γ is shown in Fig. 1. For parameters which instead may change at each phase-space point, the BLHA 1 interface defines an array to pass the numerical value of dynamical variables. The definition and order of the parameters passed through this array is set in the order file using the keyword Parameters. Although in principle extensible to up to ten parameters, at present only the first entry is used, to communicate the value of αS. Further customisation of the one-loop amplitudes which need to be generated can be achieved by editing a separate input file for GoSam. In the file gosam.rc, additional information can be specified, i.e. the model, the particle content of the loop diagrams, and the number of active flavours. Here it is also possible to define ad hoc filters to remove unwanted diagrams or loop contributions which are known to be negligible or vanishing, which may, however, if kept in the calculation, introduce numerical instabilities or slow down the evaluation. Some settings are present by default, but many more can be introduced by the user. We refer to the appendix for a more extensive list of possible options. The GoSam input file needs to be edited by hand and can be found at Template/loop_material/OLP_specifics/GoSam/ gosam.rc, in the MG5_aMC repository, or at OLP_virtuals/gosam.rc, in the folder that is generated by MG5_aMC automatically when a new process is started. After the input file is ready, any NLO process can be generated following the general MG5_aMC procedure. The interface between MG5_aMC and GoSam is available starting from MG5_aMC version The two codes can be downloaded from the following URL: MG5_aMC: https://launchpad.net/mg5amcnlo GoSam: http://gosam.hepforge.org/ 2.4 NLO predictions and validation To validate the interface, and consequently the results we present in Sect. 3, several cross checks were performed. The loop amplitudes of GoSam and MadLoop were compared for single phase-space points and also at the level of the total cross section for a number of different processes, as presented in a dedicated table in [ 94 ]. Furthermore, for pp → t t¯γ γ , a fully independent check was also performed by computing the same cross section using GoSam interfaced to Sherpa. The comparison between the results obtained with MG5_aMC+GoSam, Sherpa+GoSam, and MG5_aMC+MadLoop is presented Table 1, where we report the total integrated cross sections for LO and NLO at a centre-of-mass energy √s = 8 TeV. The results shown in this and the following sections are computed using the following setup. The mass of the Higgs was set to m H = 125 GeV, the mass of the top quark to mt = 173.2 GeV. We work in the N f = 5 model. The value of the electroweak coupling is set to its low energy limit α−EW1 = 137.0. The mass of the Z boson was set to m Z = 91.1876 GeV and the value of the Fermi constant to G F = 1.16639 · 10−5 GeV−2, which fixes the electroweak scheme. For the photons, we used the isolation procedure introduced by Frixione [ 95 ] with minimal transverse momentum pγ T min = 20 GeV, radius of isolation Rγ < 0.4 and Frixione parameters n = 1.0 and γ = 1.0. Furthermore, we applied an isolation radius between the two photons Rγ γ = 0.4. In leading order calculations, we used the PDF set cteq6L1 [ 96 ]. At next-to-leading order, we instead used the PDF set CT10. The renormalisation and factorisa)V10−5 e G / b p (,t T dp10−6 / σ d 1.6 LO 1.4 ¯/LNOttγγ 100...1286 0 )V10−5 e G / b p (,t T dp10−6 / σ d n 34σσ iitao 102σσσ evD ----4321σσσσ ) 10−5 V e G / b p (γγ10−6 m d / σ d 10−7 1.6 LO 1.4 ¯/LNOttγγ 001...1682 0 ) 10−5 V e G / b p (γγ10−6 m d / σ d 10−7 n 34σσ iitao 012σσσ evD ----4321σσσσ σtt¯γ γ , √s = 8 TeV LO (pb) NLO (pb) MG5_aMC + MadLoop MG5_aMC + GoSam Sherpa+GoSam tion scales are set to μR = μF = μ0 with 3 Results μ0 = HˆT 1 2 = 2 final state i m T,i In Fig. 2, above, we compare LO and NLO predictions for the transverse momentum of the top quark obtained with GoSam+MG5_aMC, while below we compare the same NLO predictions with results obtained using GoSam+Sherpa. In Fig. 3 we do the same for the photon pair invariant mass. All predictions are computed for a centre-of-mass energy of 8 TeV. (1) In this section we present results at NLO+PS level for the LHC at 13 TeV and compare the background process t t¯γ γ , where the photons are directly radiated from the quarks, with the signal process t t¯H in which the Higgs boson decays to two photons. We will refer to the latter simply as “t t¯H ”; it should be understood that we consider only the process with the photonic Higgs decay t t¯H , H → γ γ . As a reference, we also include results for the total cross sections and a selection of distributions obtained at 8 TeV. The study is performed using NLO predictions for t t¯H and continuum t t¯γ γ production. The top and anti-top quarks are √s = 8 TeV LO (pb) NLO (pb) K -factor √s = 13 TeV LO (pb) NLO (pb) K -factor NLO ratio 13TeV/8TeV subsequently decayed semi-leptonically t → W +(→ l¯ νl )b, t¯ → W −(→ l, ν¯l )b¯ with MadSpin [ 97,98 ], taking into account spin correlation effects, and then showered and hadronised by means of Pythia 8.2, using its default parameters, but with underlying event turned off. The short-distance events were generated and compared with two slightly different sets of cuts in order to verify that they had no impact on the results at the level of the analysis. Apart from the kinematical requirements on the reconstructed objects, which we will describe below, we use identical model parameters, renormalisation and factorisation scales, PDFs and photon isolation as described in Sect. 2.4. Note that for the background process we neglect effects of photon bremsstrahlung from the charged top decay products, which can at least partially be reduced by applying proper kinematical cuts. For the spin correlation observables, on which we will focus our attention in the last part of this section, a LO study [ 37 ] showed that the impact of neglecting these contributions is present but not dramatic. The analysis cuts are designed to increase the signal over the background, but are by no means optimised to maximise the enhancement. The two photons from the Higgs decay (or the two hard photons in the t t¯γ γ process) are required to be isolated and fulfill pT,γ > 20 GeV, |ηγ | < 2.5, 123 GeV < mγ γ < 129 GeV, where the invariant mass requirement selects a window around the Higgs boson mass, which reduces the background significantly without altering the signal strength. Furthermore, we require the events to have two oppositely charged leptons and two b-jets coming from the top and anti-top decays. The leptons are selected requiring following the cross section correspond to the scale and PDF variations, respectively. We also report the ratio between the cross sections at the two centre-of-mass energies pT,l± > 10 GeV, |ηl± | < 2.7. 2.90(1) · 10−7 +30 % +14 % 3.71(1) · 10−7 +−−4821%%%−+−115615%%% 1.28(1) pp → tt¯H , H → γ γ The b-jets are defined to be jets containing at least one lowest lying B meson. The jets themselves are defined by clustering all stable hadrons and photons, but excluding the two photons selected using Eq. (2), using the anti-kT algorithm as implemented in the code FastJet [ 99–101 ], with We use MC truth information to select the photons from the Higgs decay (signal) or hard events (background) as well as the leptons and b-jets coming from the top and anti-top decays. As reconstructed (anti-)top quark, we use the fourmomentum of the (anti-)top quark just before it decays, as provided in the Pythia 8 event record. In the presence of these analysis cuts, we obtain the cross sections reported in Table 2. In the next section we focus our attention on some relevant observables related to a single particle, whereas in Sect. 3.2 we will concentrate on observables which can directly probe correlation effects due to the top quark polarisation. In the following, unless specified otherwise, the plots will always consist of four distributions. The top curves show the differential cross sections for a given observable and for both the signal and the background process. The two middle insets display the relative uncertainty of the t t¯H and t t¯γ γ predictions, respectively. The scale dependence (transparent band) is estimated by taking the envelope of the nine predictions obtained by the separate variation of renormalisation and factorisation scales by factors of 0.5 and 2 around the central scale μ0 defined in Eq. (1). For estimating the PDF uncertainty (dotted lines), we use the Hessian method. Finally, the bottom inset highlights the differential signal-to-background ratio. 3.1 Single particle observables We start comparing the transverse momentum distribution of the reconstructed top and anti-top quarks, which is shown in Top quark transverse momentum Top quark transverse momentum Figs. 4 and 5, for a centre-of-mass energy of 8 and 13 TeV, respectively. For either the signal or background process, the shapes of the top and anti-top quark pT distributions are very similar, as expected, and therefore the same is true for the signalto-background ratio. In both cases, it reaches a maximum between 50 and 100 GeV and than decreases slightly in the high transverse momentum tail. Increasing the centreof-mass energy from 8 to 13 TeV does not lead to significant changes. Since this is true also for the other distributions that we studied, in the following we will only report and comment on the 13 TeV scenario. It is worth noting, by looking at Fig. 5, that the uncertainty due to the PDF variation is larger in t t¯H , due to the dominant gluon-channel production, and is increasing for larger transverse momenta. At pT ≈ 400 GeV the PDF uncertainty for t t¯H is around 20 %, whereas it stays below 15 % for t t¯γ γ . LHC 13 TeV Reconstructed Higgs boson transverse momentum NLO tt¯H PDF variation NLO tt¯γγ PDF variation Figure 6 shows the transverse momentum and the rapidity of the photon pair, which for the signal process corresponds to the one of the reconstructed Higgs boson. Since in t t¯γ γ the photon pair does not originate from a massive particle decay, its transverse momentum is softer and the spectrum falls off faster for large pT . The signal-to-background rapidity curve shows that photons coming from the decay of the Higgs boson are generally produced more centrally. This is not surprising given that such a decay does not feature a collinear enhancement, contrary to the case of t t¯γ γ . The transverse momentum distribution for the single photons (ordered according to their pT ) is shown in Fig. 7. The shoulder in the t t¯H signal distribution stemming from the presence of the Higgs boson resonance is also visible in the background shape, albeit less pronounced, given the invariant mass cut on the photon pair. As expected, the shoulder 300 350 400 20 40 60 80 100 120 140 160 180 200 pT, γ1 Second leading photon transverse momentum NLO tt¯H PDF variation NLO tt¯γγ PDF variation -2 -1 1 2 0 yγ2 Top quark rapidity 10−7 is shifted towards lower transverse momenta for the case of t t¯γ γ , because of the initial state collinear enhancement. It is particularly interesting to compare the rapidities of the top and anti-top quarks (Fig. 8) and of their decay products. This highlights the well known difference between the broadness of the respective top and anti-top quark rapidity distribution and it can be used to improve on background discrimination. This difference is known as the charge asymmetry and is usually quantified by the following observable: (5) AC σ ( |y| > 0) − σ ( |y| < 0) , t¯t = σ ( |y| > 0) + σ ( |y| < 0) where |y| = |yt| − |y¯t|. This observable has been measured at the LHC by both the ATLAS [ 102,103 ] and the CMS [ 104– 106 ] collaboration in the context of top-quark studies. For top-pair production at the LHC AtC¯t is positive, i.e. top quarks are produced at larger rapidities compared to anti-top quarks [ 107 ]. It is, however, known that the presence of a photon reverses the sign of AtC¯t already at tree-level [ 108 ]. This change in the rapidity distributions of the top and antitop quarks, due to additional photon radiation, can clearly be seen in the plots of Fig. 9, which compare yt and y¯t individually for t t¯H and t t¯γ γ . In the signal process the additional presence of a Higgs boson in the final state does not change the qualitative result, as compared to simple t t¯-production. This can be seen in the upper portion of the top plot in Fig. 9, which shows that top quarks are produced at slightly higher rapidities, as compared to anti-tops, which are more central, leading to a positive AtC¯t. In the lower left plot, instead, the effect is reversed. The presence of the additional photons causes the top quarks to be more central compared to the anti-tops. This effect is even more visible when comparing directly the distributions for t t¯H with the ones for t t¯γ γ . To better appreciate the change in the shape, which is only marginally visible in Fig. 8, we plot the same distribution normalised to the inclusive t t¯H cross section on the right hand side of Fig. 9. From the upper plot it becomes clear that the top quark rapidities have very similar shape in both the signal and the background process, although in the latter the tops are produced at slightly higher rapidities. This means that despite the top being produced at higher rapidities as compared to the anti-top in t t¯H , overall, they are still slightly more central than in t t¯γ γ . The opposite is true for the anti-top quark rapidity, and, therefore, the difference is even more visible in the lower right plot of Fig. 9. Analogous conclusions can be derived by looking at the rapidities of the top decay products. They are shown in Figs. 10 and 11, where the rapidities of the b- and b¯-jets and the charged leptons are shown, respectively. In Fig. 12 we compare the rapidities of the leading and second leading photon. Not surprisingly, the photon coming form the Higgs boson decay are produced more centrally as compared to the ones radiated from the partons. 3.2 Spin polarisation observables In this section we focus on observables that allow for investigating polarisation effects of the top and anti-top quarks as well as in their decay products. This can be done by studying angular variables which involve the decay products of t and ¯t rapidity for tt¯H and tt¯γγ b-jet rapidity top tt¯H anti-top tt¯H Fig. 9 Upper plot the rapidity distribution comparison between the top and anti-top quark for t t¯H (above) and t t¯γ γ (below). Lower plot normalised top (above) and anti-top (below) rapidity distribution for signal and background the top and anti-top quarks; both top quarks are considered to decay semi-leptonically (same as in the previous section). We stress that a similar analysis was already performed at LO in Ref. [ 37 ]. 10−7 Typically, for hadronic t t¯-production, very specific kinematic frames are defined [ 109–111 ]. In the following we will consider the three-dimensional opening angle θll between the leptonic decay products of the top (l+) and anti-top quarks (l−), defined in three different frames. The most straightforward possibility is to define θll in the laboratory frame (referred to as lab frame in the following). The results for this case are shown in Fig. 13. The definition of two other frames, Positively charged lepton rapidity Leading photon rapidity Fig. 11 Rapidity distribution of the lepton (top) and anti-lepton (bottom) produced in the decay of the top and anti-top quark, respectively introduced for the first time in [ 110 ], became customary in polarisation studies, since they capture particularly well spin correlation effects. For these particular frames, we define θll to be the angle between the direction of flight of l+, measured in frame where the top quark is at rest, and the direction of flight of l−, measured in the frame where the anti-top quark is at -2 -1 1 2 0 yγ2 Fig. 12 Rapidity distribution of the leading (top) and second leading photon (bottom) rest. Since two rest frames are involved in this definition, a common initial frame needs to be specified, from which the (rotation-free) Lorentz boost can be applied in order to transform the system to the t and t¯ rest frames. We choose two possible starting points, which we label as frame-1 and frame-2, defined as follows: Cosine θl+l− in the laboratory frame Cosine θl+l− in the frame-1 Fig. 13 cos θll distribution for the signal (t t¯H ) and background (t t¯γ γ ) processes in the laboratory frame. The exact definition of the angle θ is given in the text. The t t¯γ γ prediction is normalised to the t t¯H inclusive cross section. In the upper plot, we compare LO with NLO predictions and show their K -factor separately for t t¯H and t t¯γ γ in bottom insets. In the lower plot, we show NLO relative uncertainties with the signalto-background ratio as the last bottom inset – frame-1 the Lorentz boosts to bring t and t¯ separately at rest are defined with respect to the t t¯-pair centre-of-mass frame, – frame-2 the Lorentz boosts to bring t and t¯ separately at rest are defined with respect to the lab frame. These two frames are designed to be maximally sensitive to the different polarisation structures of the top-pair Relative uncertainties Relative uncertainties -0.5 0 cos θl+l− in frame-1 0.5 Fig. 14 Same as Fig. 13, but for reference frame-1 in the final state. Furthermore, as already demonstrated at LO [ 37 ], considering the spin information in the decay of the top and anti-top quark is crucial to disentangle the two different final states, which otherwise look identical, being characterised by a completely flat distribution in both cases. In Fig. 13 we show the behaviour of cos θll in the lab frame. To highlight shape differences, the background predictions have been normalised to the inclusive t t¯H cross section. The upper portions of Figs. 13, 14 and 15 presents the comparison of the LO and NLO predictions for t t¯H and t t¯γ γ Cosine θl+l− in the frame-2 ] b p [ n i b r e p γ γ ¯t t σ to tto t , ,H γγ σ¯tt σ¯tt 1.2e-07 ]b 1e-07 p i[n 8e-08 b r 6e-08 e p ¯tH 4e-08 t σ 2e-08 Fig. 15 Same as Fig. 13, but for reference frame-2 separately and shows their respective differential K -factors. The histograms in the lower portion of the figures compare results for the signal and background processes, with their ratio and respective relative uncertainty in the bottom insets. This is to be compared with the plots in Figs. 14 and 15, where the same observable is shown in frame-1 and frame-2. In the two latter frames a difference in the sign of the slope emerges, while in the lab frame, despite a clear difference in the slopes, the curves have an analogous trend. By comparing the two ratio plots at the bottom of the right plots in Figs. 14 and 15, we conclude that the frame-1 offers the best signalto-background ratio. It is also worth stressing that, while in the lab frame the K -factors tend to decrease slightly when cos θll → 1, in frame-1 and frame-2, the NLO corrections feature an almost perfectly flat K -factor which agrees with the inclusive cross section K -factor reported in Table 1. A comparison of the LO and NLO predictions reveals the anticipated reduction of the scale uncertainties. Let us finally remark that the results shown here for the background, only consider photon radiation from the initial state and from the top and anti-top quark, but not from their decay products. This is opposite to the case of the signal, where photons always originate from the decay of the Higgs boson. By considering more general cases and using top tagging techniques without relying on MC truth is expected to decrease the purity of the signal. A more quantitative analysis of these effects is beyond the scope of the present work. 4 Conclusions The event generator MG5_aMC and the one-loop amplitudes provider GoSam have been interfaced to provide the user with a framework implenting the most advanced techniques for the evaluation of cross sections and differential distributions at next-to-leading order (NLO) accuracy. In this work, the integration of the two codes has been applied for the first time to the NLO corrections to the production of a Higgs Boson in association with a pair of top– anti-top quarks, as well as to the background process where two hard photons are produced directly. We compared several key distributions to disentangle the two processes and focussed in particular on observables designed to study spin correlation effects. We found that NLO corrections give a sizeable contribution, which, however, distorts the shape of the distributions only very mildly. Moreover, we observed a clear reduction of the theoretical uncertainties. The high-level of flexibility and reliability of the joined technologies of the two codes make of the combination of MG5_aMC and GoSam an ideal tool for the high-precision studies and the hunt for deviations from known-physics signals which characterise the Run II programme at the LHC. Acknowledgments We thank German Rodrigo and Jan Winter for valuable discussions. The work of H.v.D., R.F., G.L. and P.M. is supported by the Alexander von Humboldt Foundation, in the framework of the Sofja Kovaleskaja Award Projects “Advanced Mathematical Methods for Particle Physics” (H.v.D., G.L. and P.M.) and “Event Simulation for the Large Hadron Collider at High Precision” (R.F.), endowed by the German Federal Ministry of Education and Research. The work of G.O. is supported in part by the NSF under Grants PHY-1068550 and PHY-1417354. V.H. is supported by the Swiss National Fund for Science (SNSF) under grant number P300P2_161050. This research made use of the CTP computational cluster of the New York City College of Technology. We thank the CP3 IT team for their constant support and the availability of the cluster hosted by the Université Catholique de Louvain. Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecomm ons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. Funded by SCOAP3. Appendix A: The GoSam input card We report here a copy of the default GoSam input card with a brief explanation of the different options. For a more detailed overview we refer to the GoSam papers [ 17,20 ] and the GoSam manual which can be found online (http://gosam. hepforge.org) and is continuously updated. The default gosam.rc file is the following: ############################################### # Copy this file to setup.in in order to set # some common options for all examples. ################### # physics options # ################### # Model specs.: model=smdiag_mad model.options=GF: 0.0000116639, mZ: 91.188, mW: 80.419, Nf: 4 # Parameters set to zero algebraically: zero=me,mmu,mU,mD,mC,mS,wB,wT # Symmetries: symmetries=family,generation # Filter for scale-less loop integrals: filter.nlo=lambda d: (not (d.isScaleless())) ################### # program options # ################### form.bin=tform form.threads=4 form.tempdir=/tmp fc.bin=gfortran -O2 ############################################### This input file needs to be modified if the computation is performed within the 5-flavour scheme. The b-quark mass can be set algebraically to zero by adding mB to the list zero: zero=me,mmu,mU,mD,mC,mS,mB,wB,wT. Furthermore the number of light quarks Nf has to be set equal to 5. The tag symmetries specifies some further symmetries in the calculation of the amplitudes. The information is used when the list of helicities is generated. Possible options are: – flavour: does not allow for flavour-changing interactions. When this option is set, fermion lines are assumed not to mix. – family: allows for flavour-changing interactions only within the same family. When this option is set, fermion lines 1-6 are assumed to mix only within families. This means that e.g. a quark line connecting an up with down quark would be considered, while a up-bottom one would not. – lepton: means for leptons what “flavour” means for quarks. – generation: means for leptons what “family” means for quarks. Furthermore it is possible to fix the helicity of particles. 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Hans van Deurzen, Rikkert Frederix, Valentin Hirschi, Gionata Luisoni, Pierpaolo Mastrolia, Giovanni Ossola. Spin polarisation of \(t\bar{t}\gamma \gamma \) production at NLO+PS with GoSam interfaced to MadGraph5_aMC@NLO, The European Physical Journal C, 2016, DOI: 10.1140/epjc/s10052-016-4048-2