CERN-PH-2015-163 \AtlasJournalEur. Phys. J. C
Study of the and decays with the ATLAS detector
Abstract
The decays and are studied with the ATLAS detector at the LHC using a dataset corresponding to integrated luminosities of 4.9 fb-1 and 20.6 fb-1 of collisions collected at centre-of-mass energies TeV and TeV, respectively. Signal candidates are identified through and decays. With a two-dimensional likelihood fit involving the reconstructed invariant mass and an angle between the and candidate momenta in the muon pair rest frame, the yields of and , and the transverse polarisation fraction in decay are measured. The transverse polarisation fraction is determined to be , and the derived ratio of the branching fractions of the two modes is , where the first error is statistical and the second is systematic. Finally, a sample of decays is used to derive the ratios of branching fractions and , where the third error corresponds to the uncertainty of the branching fraction of decay. The available theoretical predictions are generally consistent with the measurement.
1 Introduction
The meson11 1 Charge conjugate states are implied throughout the paper unless otherwise stated. is the only known weakly decaying particle consisting of two heavy quarks. The ground state was first observed by CDF [1] via its semileptonic decay . An excited state has been observed recently by ATLAS [2] using the decay mode . The presence of two heavy quarks, each of which can decay weakly, affects theoretical calculations of the decay properties of the meson. In the case of processes, decays to charmonium and a or a meson are predicted to occur via colour-suppressed and colour-favoured spectator diagrams as well as via the weak annihilation diagram (see Fig. 1). The latter, in contrast to decays of other mesons, is not Cabibbo-suppressed and can contribute significantly to the decay amplitudes. The decay properties are addressed in various theoretical calculations [3, 4, 5, 6, 7, 8, 9] and can also be compared to the analogous properties in the lighter meson systems such as or . The decays and , which have been observed recently by the LHCb experiment [10], provide a means to test these theoretical predictions.
This paper presents a measurement of the branching fractions of and decays, normalised to that of decay, and polarisation in decay performed with the ATLAS detector [11]. The meson is reconstructed via the decay with the meson decaying into a pair of charged kaons. The meson decays into a meson and a soft photon or . Detecting such soft neutral particles is very challenging, thus no attempt to reconstruct them is made in the analysis. The meson is reconstructed via its decay into a muon pair.
The measurement presented in this paper allows an independent verification of the results of Ref. [10] with comparable statistical and systematic uncertainties. The following ratios are measured: , , and , where denotes the branching fraction of the decay. The decay is a transition of a pseudoscalar meson into a pair of vector states and is thus described by the three helicity amplitudes, , , and , where the subscripts correspond to the helicities of and mesons. The contribution of the and amplitudes, referred to as the component, corresponds to the and transverse polarisation. The fraction of transverse polarisation, , is also measured. From a naive prediction by spin counting, one would expect this fraction to be , while calculations [8, 9] predict values of 0.41–0.48.
This analysis is based on a combined sample of collision data collected by the ATLAS experiment at the LHC at centre-of-mass energies TeV and TeV corresponding to integrated luminosities of 4.9 fb-1 and 20.6 fb-1, respectively.
2 The ATLAS detector, trigger selection and Monte Carlo samples
ATLAS is a general-purpose detector consisting of several subsystems including the inner detector (ID), calorimeters and the muon spectrometer (MS). Muon reconstruction makes use of both the ID and the MS. The ID comprises three types of detectors: a silicon pixel detector, a silicon microstrip semiconductor tracker (SCT) and a transition radiation tracker. The ID provides a pseudorapidity22 2 ATLAS uses a right-handed coordinate system with its origin at the nominal interaction point (IP) in the centre of the detector and the -axis along the beam pipe. The -axis points from the IP to the centre of the LHC ring, and the -axis points upward. Cylindrical coordinates are used in the transverse plane, being the azimuthal angle around the beam pipe. The pseudorapidity is defined in terms of the polar angle as . coverage up to . Muons pass through the calorimeters and reach the MS if their transverse momentum, , is above approximately 3 GeV.33 3 Using a system of units with is implied throughout the paper. Muon candidates are formed either from a stand-alone MS track matched to an ID track or, in case the MS stand-alone track is not reconstructed, from an ID track extrapolated to the MS and matched to track segments in the MS. Candidates of the latter type are referred to as segment-tagged muons while the former are called combined muons. Muon track parameters are taken from the ID measurement alone in this analysis, since the precision of the measured track parameters for muons in the range of interest is dominated by the ID track reconstruction.
The ATLAS trigger system consists of a hardware-based Level-1 trigger and a two-stage High Level Trigger (HLT). At Level-1, the muon trigger uses dedicated MS chambers to search for patterns of hits satisfying different thresholds. The region-of-interest around these hit patterns then serves as a seed for the HLT muon reconstruction, in which dedicated algorithms are used to incorporate information from both the MS and the ID, achieving a position and momentum resolution close to that provided by the offline muon reconstruction. Muons are efficiently triggered in the pseudorapidity range .
Triggers based on single-muon, dimuon, and three-muon signatures are used to select decays for the analysis. The third muon can be produced in the signal events in semileptonic decays of the two other heavy-flavour hadrons. The majority of events are collected by dimuon triggers requiring a vertex of two oppositely charged muons with an invariant mass between 2.5 GeV and 4.3 GeV. During the data taking, the threshold for muons in these triggers was either 4 GeV or 6 GeV. Single-muon triggers additionally increase the acceptance for asymmetric decays where one muon has GeV. Finally, three-muon triggers had a threshold of 4 GeV, thus enhancing the acceptance during the periods of high luminosity when the threshold for at least one muon in the dimuon triggers was 6 GeV.
Monte Carlo (MC) simulation is used for the event selection criteria optimisation and the calculation of the acceptance for the considered decay modes. The MC samples of the decays were generated with Pythia 6.4 [12] along with a dedicated extension for the production based on calculations from Refs. [13, 14, 15, 16]. The decays of are then simulated with EvtGen [17]. The generated events were passed through a full simulation of the detector using the ATLAS simulation framework [18] based on Geant 4 [19, 20] and processed with the same reconstruction algorithms as were used for the data.
3 Reconstruction and event selection
The candidates are reconstructed from pairs of oppositely charged muons. At least one of the two muons is required to be a combined muon. Each pair is fitted to a common vertex [21]. The quality of the vertex fit must satisfy , where the stands for the number of degrees of freedom. The candidates in the invariant mass window MeV are retained.
For the reconstruction, tracks of particles with opposite charges are assigned kaon mass hypotheses and combined in pairs to form candidates. An additional track is assigned a pion mass and combined with the candidate to form a candidate. To ensure good momentum resolution, all three tracks are required to have at least two hits in the silicon pixel detector and at least six hits in the SCT. Only three-track combinations successfully fitted to a common vertex with are kept. The candidate invariant mass, , and the candidate invariant mass, , are calculated using the track momenta refitted to the common vertex. Only candidates with within MeV around the mass, MeV [22], and with MeV are retained.
The candidates are built by combining the five tracks of the and candidates. The meson decays instantly at the same point as the does (secondary vertex) while the lives long enough to form a displaced tertiary vertex. Therefore the five-track combinations are refitted assuming this cascade topology [21]. The invariant mass of the muon pair is constrained to the mass, MeV [22]. The three daughter tracks are constrained to a tertiary vertex and their invariant mass is fixed to the mass of , MeV [22]. The combined momentum of the refitted decay tracks is constrained to point to the dimuon vertex. The quality of the cascade fit must satisfy .
The meson is reconstructed within the kinematic range GeV and , where the detector acceptance is high and depends weakly on and .
The refitted tracks of the daughter hadrons are required to have and GeV, while the muons must have and GeV. To further discriminate the sample of candidates from a large combinatorial background, the following requirements are applied:
- •
, where is the angle between the pion momentum in the rest frame and the combined momentum in the laboratory frame;
- •
, where is the angle between one of the kaons and the pion in the rest frame. The decay of the pseudoscalar meson to the (vector) plus (pseudoscalar) final state results in an alignment of the spin of the meson perpendicularly to the direction of motion of the relative to . Consequently, the distribution of follows a shape, implying a uniform distribution for . In contrast, the distribution of the combinatorial background is uniform and its distribution peaks at zero. The cut suppresses the background significantly while reducing the signal by 15%.
The candidate is required to point back to a primary vertex such that mm and mm, where and are respectively the transverse and longitudinal impact parameters with respect to the primary vertex. All primary vertices in the event are considered. If there is more than one primary vertex satisfying these requirements (% events both in data and MC simulation), the one with the largest sum of squared transverse momenta of the tracks originating from it is chosen.
The transverse decay length44 4 The transverse decay length of a particle is defined as the transverse distance between the production (primary) vertex and the particle decay (secondary) vertex projected along its transverse momentum. of the candidate is required to satisfy mm. The transverse decay length of the measured from the vertex must be mm. In order to remove fake candidates, both and are required not to exceed 10 mm.
Taking into account the characteristic hard fragmentation of -quarks, a requirement is applied, where the sum in the denominator is taken over all tracks originating from the primary vertex (tracks of the candidate are included in the sum if they are associated with the primary vertex). The requirement reduces a sizeable fraction of combinatorial background while having almost no effect on the signal.
The following angular selection requirements are introduced to further suppress the combinatorial background:
- •
, where is the angle between the candidate momentum in the rest frame of the candidate, and the candidate line of flight in the laboratory frame. The distribution of is uniform for the decays of pseudoscalar meson before any kinematic selection while it tends to increase for negative values of for the background.
- •
, where is the angle between the candidate momentum and the pion momentum in the rest frame. Its distribution is nearly uniform for the signal processes but peaks towards for the background.
Distributions of these two variables after applying all other selection requirements described in this section are shown in Fig. 2. They are shown for the simulated signal samples, as well as for sidebands of the mass spectrum in data, defined as the regions MeV (left sideband) and MeV (right sideband). A dip in the distribution for the signal is caused by rejection of candidates discussed below.
Various possible contributions of partially reconstructed decays were studied. The only significant one was found from the decay process. This contribution arises when the combination of the tracks from a true decay with a fifth random track results in a fake candidate. For each reconstructed candidate, an additional vertex fit is performed. The two muon tracks and the two kaon tracks are fitted to a common vertex, where the kaon tracks are assumed to be from and the muon pair is constrained to have the nominal mass. The mass of the candidate, , is then calculated from the refitted track parameters. Candidates with MeV are rejected. This requirement suppresses the bulk of the events while rejecting only % of the signal.
After applying the selection requirements described above, 1547 candidates are selected in the mass range 5640–6760 MeV.
4 candidate fit
The mass distribution of the selected candidates is shown in Fig. 3. The peak near the mass, MeV [22], is attributed to the signal of decay while a wider structure between 5900 MeV and 6200 MeV corresponds to with subsequent or decays where the neutral particle is not reconstructed.
Mass distributions of the and candidates corresponding to the mass region of the observed signals are shown in Fig. 4. To obtain these plots, the candidates are built without the mass constraints in the cascade fit, with the mass of the candidate calculated as , where and are the nominal masses of the respective particles. The mass of the candidate is required to be MeV while the mass windows for the corresponding intermediate resonances are widened to the plotting ranges. The and mass distributions are fitted with a sum of an exponential function describing the background and a modified Gaussian function [23, 24] describing the corresponding signal peak. The modified Gaussian function is defined as
| (1) |
where with the mean mass and width being free parameters. The fitted masses of ( MeV) and ( MeV) agree with their nominal masses, the widths are consistent with those in the simulated samples, and the signal yields are found to be and .
The information about the helicity in decay is encoded both in the mass distribution of the system and in the distribution of the helicity angle, , which is defined in the rest frame of the muon pair as the angle between the and the candidate momenta. Thus, a two-dimensional extended unbinned maximum-likelihood fit of the and distributions is performed. The and helicity amplitude contributions are described by the same mass and angular shapes because of the parity symmetry of the and decays. This is confirmed by the MC simulation. Thus these components are treated together as the component, while the shape of the component is different and is therefore treated separately. A simultaneous fit to the mass and angular distributions significantly improves the sensitivity to the contributions of the helicity amplitudes in decay with respect to a one-dimensional mass fit.
Four two-dimensional probability density functions (PDFs) are defined to describe the signal, the and components of the signal, and the background. The signal PDFs are factorised into mass and angular components. The effect of correlations between their mass and angular shapes is found to be small and is accounted for as a systematic uncertainty.
The mass distribution of the signal is described by a modified Gaussian function. For the signal components, the mass shape templates obtained from the simulation with the kernel estimation technique [25] are used. The branching fractions of and decays for the simulation are set to the world average values [22]. The position of the templates along the mass axis is varied in the fit simultaneously with the position of the signal peak. The background mass shape is described with a two-parameter exponential function, .
To describe the shapes, templates from the kernel estimation are used. The templates for the signal angular PDFs are extracted from the simulated samples. Although their shapes are calculable analytically, using the templates allows the fit to account for detector effects. The background angular description is based on the shape of the candidates in the sidebands of mass spectra. Two templates are produced from the angular distributions of the candidates in the left and right mass sidebands as defined in Sect. 3. The angular PDF for the background is defined as a conditional PDF of given the per-candidate . For the candidates in the lower half of the left sideband (5640–5770 MeV), the template from the left sideband is used. Similarly, the template from the right sideband is used for the upper half of the right sideband (6560–6760 MeV). For the candidates in the middle part of the mass spectrum (5770–6560 MeV), a linear interpolation between the two templates is used.
The fit has seven free parameters: the mass of the meson, ; the relative contribution of the component to the total decay rate in the selected sample, ; the two parameters of the exponential background; the yields of the two signal modes, and , and the background yield. The width of the modified Gaussian function, , is fixed to the value obtained from the fit to the simulated signal, MeV. Leaving this parameter free in the data fit results in the value MeV, consistent with the simulation in the range of statistical uncertainty.
It was checked that the fit procedure provides unbiased values and correct statistical uncertainties for the extracted parameters using pseudo-experiments. The values of the relevant parameters obtained from the fit are given in Table 1. The fitted mass agrees with the world average value [22]. The mass and angular projections of the fit on the selected candidate dataset are also shown in Figs. 3 and 5, respectively. In order to illustrate the effect of the angular part of the fit in separating the helicity amplitudes, the projection for the subset of candidates with the masses MeV corresponding to the region of the observed signal is shown in Fig. 5.
| Parameter | Value | |
|---|---|---|
| [MeV] | ||
The statistical significance for the observed signal estimated from toy MC studies is 4.9 standard deviations.
5 candidate reconstruction and fit
candidates are reconstructed by fitting a common vertex of a pion candidate track and the two muons from a candidate, selected as described in Sect. 3. For the pion candidate, tracks identified as muons are vetoed in order to suppress the substantial background from decays. The invariant mass of the two muons in the vertex fit is constrained to the nominal mass. The quality of the fit must satisfy . The following selection requirements applied to the candidates are analogous to those for candidates described in Sect. 3: the candidates must be within the kinematic range GeV, ; the refitted values of the transverse momenta and pseudorapidities of the muons are required to satisfy GeV, ; the same requirements on pointing to the primary vertex and the ratio are applied. The refitted pion track kinematics must satisfy GeV and . The transverse decay length is required to be mm, and not to exceed 10 mm.
To further suppress combinatorial background, the following selection is applied:
- •
, where is the angle between the pion momentum in the rest frame and the candidate line of flight in laboratory frame. This angular variable behaviour for the signal and the background is the same as that of used for candidates selection.
- •
, where is the angle between the and momenta in the muon pair rest frame. The signal distribution follows a shape, while the background is flat.
After applying the above-mentioned requirements, 38542 candidates are selected in the mass range 5640–6760 MeV. Figure 6 shows the mass distribution of the selected candidates. An extended unbinned maximum-likelihood fit of the mass spectrum is performed to evaluate the signal yield. The signal contribution is described with the modified Gaussian function while an exponential function is used for the background. The mass, , the width of the modified Gaussian function, , the yields of the signal, , and the background, and the slope of the exponential background are free parameters of the fit. The fit results are summarised in Table 2, and the fit projection is also shown in Fig. 6. The extracted mass value is consistent with the world average [22], and the signal peak width agrees with the simulation (37.4 MeV).
| Parameter | Value | |
|---|---|---|
| [MeV] | ||
| [MeV] | ||
6 Branching fractions and polarisation measurement
The ratios of the branching fractions and are calculated as
| (2) |
where and are the total acceptance and the yield of the corresponding mode. For , the CLEO measurement [26] of the partial branching fractions, with a kaon-pair mass within various intervals around the nominal meson mass, is used. An interpolation between the partial branching fractions, measured for MeV and MeV intervals, using a relativistic Breit–Wigner shape of the resonance yields the value % for the MeV interval which is used in the analysis. The effect of admixture of other decay modes with final state which are not present in the MC simulation is studied separately and accounted for as a systematic uncertainty.
The acceptance for the decay mode is different for the and components, thus the full acceptance for the mode is
| (3) |
where the subscripts indicate the helicity state and is the value extracted from the fit (Table 1). The acceptances are determined from the simulation and shown in Table 3.
| Mode | [%] |
|---|---|
| , | |
| , |
The ratio is calculated as
| (4) |
where the ratio of the yields and its uncertainty is extracted from the fit as a parameter in order to account for correlations between the yields.
The fraction of the component contribution in decay is calculated from the value quoted in Table 1 by applying a correction to account for the different acceptances for the two component contributions:
| (5) |
7 Systematic uncertainties
The systematic uncertainties of the measured values are determined by varying the analysis procedure and repeating all calculations. Although some sources can have rather large effects on the individual decay rate measurements, they largely cancel in the ratios of the branching fractions due to correlation between the effects on the different decay modes. The following groups of systematic uncertainties are considered.
The first group of sources of systematic uncertainty relates to possible differences between the data and simulation affecting the acceptances for the decay modes. Thus, an effect of the production model is evaluated by varying the simulated and spectra while preserving agreement with the data distributions obtained using the abundant channel. These variations have very similar effects on the acceptances for the different decay modes, thus giving rather moderate estimates of the uncertainties, not exceeding 3% in total, on the ratios of branching fractions. The effect of presence of other decay modes with final state on the calculated acceptances is studied with a separate MC simulation. Its conservative estimate yields 0.4% which is assigned as and uncertainties. An uncertainty on the tracking efficiency is dominated by the uncertainty of the detector material description in the MC simulation. Samples generated with distorted geometries and with increased material are used to estimate the effect on track reconstruction efficiencies. When propagated to the ratios of branching fractions, these estimates give 0.5% uncertainty for and due to the two extra tracks in modes. Limited knowledge of the and lifetimes leads to an additional systematic uncertainty. The simulated proper decay times are varied within one standard deviation from the world average values [22] resulting in uncertainties of % assigned to and due to the lifetime, and 0.3% due to the lifetime. Removing the requirement on is found to produce no noticeable effect on the measured values.
The next group of uncertainties originates from the signal extraction procedure. These uncertainties are evaluated separately for and candidate fits. For the former, the following variations of the fit model are applied and the difference is treated as a systematic uncertainty:
- •
different background mass shape parametrisations (three-parameter exponential, second- and third-order polynomials), different fitted mass range (reduced by up to 40 MeV from each side independently);
- •
- •
variation of the smoothness of the signal mass templates, which is controlled by a parameter of the kernel estimation procedure [25];
- •
similar variation of the smoothness of the signal angular templates;
- •
variation of the smoothness of the sideband templates used for the background angular PDF construction; different ranges of the sidebands; different sideband interpolation procedure;
- •
modelling of the correlation between the mass and angular parts of the signal PDFs. This correlation takes place only at the detector level and manifests itself in degradation of the mass resolution for higher values of . A dedicated fit model accounting for this effect is used for the data fit. The impact on the result is found to be negligible compared to the total uncertainty.
The first two items give the dominant contributions to the uncertainties of the ratios of branching fractions while the transverse polarisation fraction measurement is mostly affected by the background angular modelling variations. For the normalisation channel fit model, the similar variations of the background and signal mass shape parametrisation are applied. The deviations produced by the variations of the fits reach values as high as 10–15% thus making them the dominant sources of systematic uncertainty.
The branching fractions of [22] are varied in simulation within their uncertainties to estimate their effect on the measured quantities. Very small uncertainties are obtained for the and , while for , the estimate is %.
The statistical uncertainties on the acceptance values due to the MC sample sizes are also treated as a separate source of systematic uncertainty and estimated to be 2–3%.
In order to check for a possible bias from using three-muon triggers, vetoing the meson daughter tracks identified as muons is tested and found not to affect the measurement.
Finally, since enters Eq. (2), its uncertainty, evaluated from Ref. [26] as 5.9%, is propagated to the final values of the relative branching fractions.
The systematic uncertainties on the measured quantities are summarised in Table 4.
| Source | Uncertainty [%] | |||
| Simulated spectrum | ||||
| Simulated spectrum | ||||
| Other decay modes contribution | – | – | ||
| Tracking efficiency | ||||
| lifetime | ||||
| lifetime | ||||
| signal extraction | ||||
| signal extraction | – | – | ||
| branching fractions | ||||
| MC sample sizes | ||||
| Total | ||||
| – | – | |||
8 Results
The following ratios of the branching fractions are measured:
| (6) | ||||
| (7) | ||||
| (8) |
where the BF uncertainty corresponds to the knowledge of . The relative contribution of the component in decay is measured to be
| (9) |
These results are compared with those of the LHCb measurement [10] and to the expectations from various theoretical calculations in Table 5 and Fig. 7. The measurement agrees with the LHCb result. All ratios are well described by the recent perturbative QCD predictions [8]. The expectations from models in Refs. [3, 5, 7] as well as the sum-rules prediction [4] for the ratio are consistent with the measurement. The QCD relativistic potential model predictions [3] are consistent with the measured ratio while the expectations from the sum rules [4] and models in Refs. [5, 6, 7] are somewhat smaller than the measured value. The predictions in Refs. [3, 4, 5, 7] are also generally smaller than the measured ratio ; however, the discrepancies do not exceed two standard deviations when taking into account only the experimental uncertainty.
| Ref. | ||||
| ATLAS | ||||
| – | LHCb [10] | |||
| – | QCD potential model [3] | |||
| – | QCD sum rules [4] | |||
| – | RCQM [5] | |||
| – | – | – | BSW [6] | |
| – | – | LFQM [7] | ||
| – | pQCD [8] | |||
| – | – | – | RIQM [9] |
9 Conclusion
A study of and decays has been performed. The ratios of the branching fractions , , and the transverse polarisation fraction of decay have been measured by the ATLAS experiment at the LHC using collision data corresponding to an integrated luminosity of 4.9 fb-1 at 7 TeV centre-of-mass energy and 20.6 fb-1 at 8 TeV. The polarisation is found to be well described by the available theoretical approaches. The measured ratios of the branching fraction are generally described by perturbative QCD, sum rules, and relativistic quark models. There is an indication of underestimation of the decay rates for the decays by some models, although the discrepancies do not exceed two standard deviations when taking into account only the experimental uncertainty. The measurement results agree with those published by the LHCb experiment.
Acknowledgements
We thank CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated efficiently.
We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; RGC, Hong Kong SAR, China; ISF, MINERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and NRC KI, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZŠ, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America.
The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN and the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA) and in the Tier-2 facilities worldwide.
References
- [1] CDF and F. Abe “Observation of the meson in collisions at TeV” In Phys. Rev. Lett. 81, 1998, pp. 2432–2437 DOI: 10.1103/PhysRevLett.81.2432
- [2] ATLAS “Observation of an Excited Meson State with the ATLAS Detector” In Phys. Rev. Lett. 113, 2014, pp. 212004 DOI: 10.1103/PhysRevLett.113.212004
- [3] Pietro Colangelo and Fulvia De “Using heavy quark spin symmetry in semileptonic decays” In Phys. Rev. D 61, 2000, pp. 034012 DOI: 10.1103/PhysRevD.61.034012
- [4] V.V. Kiselev “Exclusive decays and lifetime of meson in QCD sum rules”, 2002 arXiv:hep-ph/0211021 [hep-ph]
- [5] Mikhail Ivanov, Jurgen Korner and Pietro Santorelli “Exclusive semileptonic and nonleptonic decays of the meson” In Phys. Rev. D 73, 2006, pp. 054024 DOI: 10.1103/PhysRevD.73.054024
- [6] Rohit Dhir and R.C. Verma “ Meson Form-factors and Decays Involving Flavor Dependence of Transverse Quark Momentum” In Phys. Rev. D 79, 2009, pp. 034004 DOI: 10.1103/PhysRevD.79.034004
- [7] Hong-Wei Ke, Tan Liu and Xue-Qian Li “Transitions of and the modified harmonic oscillator wave function in LFQM” In Phys. Rev. D 89, 2014, pp. 017501 DOI: 10.1103/PhysRevD.89.017501
- [8] Zhou Rui and Zhi-Tian Zou “S-wave ground state charmonium decays of mesons in the perturbative QCD approach” In Phys. Rev. D 90, 2014, pp. 114030 DOI: 10.1103/PhysRevD.90.114030
- [9] Susmita Kar et al. “Nonleptonic decays” In Phys. Rev. D 88, 2013, pp. 094014 DOI: 10.1103/PhysRevD.88.094014
- [10] LHCb and R Aaij “Observation of and decays” In Phys. Rev. D 87, 2013, pp. 112012 DOI: 10.1103/PhysRevD.87.112012
- [11] ATLAS “The ATLAS Experiment at the CERN Large Hadron Collider” In JINST 3, 2008, pp. S08003 DOI: 10.1088/1748-0221/3/08/S08003
- [12] Torbjorn Sjostrand, Stephen Mrenna and Peter Skands “PYTHIA 6.4 Physics and Manual” In JHEP 0605, 2006, pp. 026 DOI: 10.1088/1126-6708/2006/05/026
- [13] A.V. Berezhnoy, A.K. Likhoded and O.P. Yushchenko “Some features of the hadronic meson production at large ” In Phys. Atom. Nucl. 59, 1996, pp. 709–713 arXiv:hep-ph/9504302 [hep-ph]
- [14] A.V. Berezhnoy, V.V. Kiselev and A.K. Likhoded “Hadronic production of - and -wave states of -quarkonium” In Z. Phys. A 356, 1996, pp. 79–87 DOI: 10.1007/s002180050151
- [15] A.V. Berezhnoy, V.V. Kiselev, A.K. Likhoded and A.I. Onishchenko “ meson at LHC” In Phys. Atom. Nucl. 60, 1997, pp. 1729–1740 arXiv:hep-ph/9703341 [hep-ph]
- [16] A.V. Berezhnoy “Color flows for the process ” In Phys. Atom. Nucl. 68, 2005, pp. 1866–1872 DOI: 10.1134/1.2131116
- [17] D.J. Lange “The EvtGen particle decay simulation package” In Nucl. Instrum. Meth. A 462, 2001, pp. 152–155 DOI: 10.1016/S0168-9002(01)00089-4
- [18] ATLAS “The ATLAS Simulation Infrastructure” In Eur. Phys. J. C 70, 2010, pp. 823–874 DOI: 10.1140/epjc/s10052-010-1429-9
- [19] GEANT4 and S. Agostinelli “GEANT4: A Simulation toolkit” In Nucl. Instrum. Meth. A 506, 2003, pp. 250–303 DOI: 10.1016/S0168-9002(03)01368-8
- [20] John Allison et al. “Geant4 developments and applications” In IEEE Trans. Nucl. Sci. 53, 2006, pp. 270 DOI: 10.1109/TNS.2006.869826
- [21] V. Kostyukhin “VKalVrt - package for vertex reconstruction in ATLAS”, ATL-PHYS-2003-031, 2003 URL: http://cds.cern.ch/record/685551
- [22] K…(Particle) “Review of Particle Physics” In Chin. Phys. C 38, 2014, pp. 090001 DOI: 10.1088/1674-1137/38/9/090001
- [23] ZEUS and S. Chekanov “Measurement of inelastic production in deep inelastic scattering at HERA” In Eur. Phys. J. C 44, 2005, pp. 13–25 DOI: 10.1140/epjc/s2005-02346-2
- [24] Georges Aad “Measurement of the b-hadron production cross section using decays to final states in collisions at TeV with the ATLAS detector” In Nucl. Phys. B 864, 2012, pp. 341–381 DOI: 10.1016/j.nuclphysb.2012.07.009
- [25] Kyle Cranmer “Kernel estimation in high-energy physics” In Comput. Phys. Commun. 136, 2001, pp. 198–207 DOI: 10.1016/S0010-4655(00)00243-5
- [26] CLEO and J.P. Alexander “Absolute Measurement of Hadronic Branching Fractions of the D(s)+ Meson” In Phys. Rev. Lett. 100, 2008, pp. 161804 DOI: 10.1103/PhysRevLett.100.161804
- [27] M. Oreglia “A Study of the Reactions ”, PhD thesis, SLAC-R-236, 1980 URL: http://www.slac.stanford.edu/pubs/slacreports/slac-r-236.html
- [28] J. Gaiser “Charmonium Spectroscopy From Radiative Decays of the and ”, PhD thesis, SLAC-R-255, 1982 URL: http://www.slac.stanford.edu/pubs/slacreports/slac-r-255.html
- [29] Tomasz Skwarnicki “A study of the radiative cascade transitions between the and resonances”, PhD thesis, DESY-F31-86-02, 1986 URL: http://inspirehep.net/record/230779/
The ATLAS Collaboration
G. Aad85, B. Abbott113, J. Abdallah151, O. Abdinov11, R. Aben107, M. Abolins90, O.S. AbouZeid158, H. Abramowicz153, H. Abreu152, R. Abreu30, Y. Abulaiti146a,146b, B.S. Acharya164a,164b,a, L. Adamczyk38a, D.L. Adams25, J. Adelman108, S. Adomeit100, T. Adye131, A.A. Affolder74, T. Agatonovic-Jovin13, J.A. Aguilar-Saavedra126a,126f, S.P. Ahlen22, F. Ahmadov65,b, G. Aielli133a,133b, H. Akerstedt146a,146b, T.P.A. Åkesson81, G. Akimoto155, A.V. Akimov96, G.L. Alberghi20a,20b, J. Albert169, S. Albrand55, M.J. Alconada Verzini71, M. Aleksa30, I.N. Aleksandrov65, C. Alexa26a, G. Alexander153, T. Alexopoulos10, M. Alhroob113, G. Alimonti91a, L. Alio85, J. Alison31, S.P. Alkire35, B.M.M. Allbrooke18, P.P. Allport74, A. Aloisio104a,104b, A. Alonso36, F. Alonso71, C. Alpigiani76, A. Altheimer35, B. Alvarez Gonzalez30, D. Álvarez Piqueras167, M.G. Alviggi104a,104b, B.T. Amadio15, K. Amako66, Y. Amaral Coutinho24a, C. Amelung23, D. Amidei89, S.P. Amor Dos Santos126a,126c, A. Amorim126a,126b, S. Amoroso48, N. Amram153, G. Amundsen23, C. Anastopoulos139, L.S. Ancu49, N. Andari30, T. Andeen35, C.F. Anders58b, G. Anders30, J.K. Anders74, K.J. Anderson31, A. Andreazza91a,91b, V. Andrei58a, S. Angelidakis9, I. Angelozzi107, P. Anger44, A. Angerami35, F. Anghinolfi30, A.V. Anisenkov109,c, N. Anjos12, A. Annovi124a,124b, M. Antonelli47, A. Antonov98, J. Antos144b, F. Anulli132a, M. Aoki66, L. Aperio Bella18, G. Arabidze90, Y. Arai66, J.P. Araque126a, A.T.H. Arce45, F.A. Arduh71, J-F. Arguin95, S. Argyropoulos42, M. Arik19a, A.J. Armbruster30, O. Arnaez30, V. Arnal82, H. Arnold48, M. Arratia28, O. Arslan21, A. Artamonov97, G. Artoni23, S. Asai155, N. Asbah42, A. Ashkenazi153, B. Åsman146a,146b, L. Asquith149, K. Assamagan25, R. Astalos144a, M. Atkinson165, N.B. Atlay141, B. Auerbach6, K. Augsten128, M. Aurousseau145b, G. Avolio30, B. Axen15, M.K. Ayoub117, G. Azuelos95,d, M.A. Baak30, A.E. Baas58a, C. Bacci134a,134b, H. Bachacou136, K. Bachas154, M. Backes30, M. Backhaus30, P. Bagiacchi132a,132b, P. Bagnaia132a,132b, Y. Bai33a, T. Bain35, J.T. Baines131, O.K. Baker176, P. Balek129, T. Balestri148, F. Balli84, E. Banas39, Sw. Banerjee173, A.A.E. Bannoura175, H.S. Bansil18, L. Barak30, E.L. Barberio88, D. Barberis50a,50b, M. Barbero85, T. Barillari101, M. Barisonzi164a,164b, T. Barklow143, N. Barlow28, S.L. Barnes84, B.M. Barnett131, R.M. Barnett15, Z. Barnovska5, A. Baroncelli134a, G. Barone49, A.J. Barr120, F. Barreiro82, J. Barreiro Guimarães da Costa57, R. Bartoldus143, A.E. Barton72, P. Bartos144a, A. Basalaev123, A. Bassalat117, A. Basye165, R.L. Bates53, S.J. Batista158, J.R. Batley28, M. Battaglia137, M. Bauce132a,132b, F. Bauer136, H.S. Bawa143,e, J.B. Beacham111, M.D. Beattie72, T. Beau80, P.H. Beauchemin161, R. Beccherle124a,124b, P. Bechtle21, H.P. Beck17,f, K. Becker120, M. Becker83, S. Becker100, M. Beckingham170, C. Becot117, A.J. Beddall19b, A. Beddall19b, V.A. Bednyakov65, C.P. Bee148, L.J. Beemster107, T.A. Beermann175, M. Begel25, J.K. Behr120, C. Belanger-Champagne87, W.H. Bell49, G. Bella153, L. Bellagamba20a, A. Bellerive29, M. Bellomo86, K. Belotskiy98, O. Beltramello30, O. Benary153, D. Benchekroun135a, M. Bender100, K. Bendtz146a,146b, N. Benekos10, Y. Benhammou153, E. Benhar Noccioli49, J.A. Benitez Garcia159b, D.P. Benjamin45, J.R. Bensinger23, S. Bentvelsen107, L. Beresford120, M. Beretta47, D. Berge107, E. Bergeaas Kuutmann166, N. Berger5, F. Berghaus169, J. Beringer15, C. Bernard22, N.R. Bernard86, C. Bernius110, F.U. Bernlochner21, T. Berry77, P. Berta129, C. Bertella83, G. Bertoli146a,146b, F. Bertolucci124a,124b, C. Bertsche113, D. Bertsche113, M.I. Besana91a, G.J. Besjes106, O. Bessidskaia Bylund146a,146b, M. Bessner42, N. Besson136, C. Betancourt48, S. Bethke101, A.J. Bevan76, W. Bhimji46, R.M. Bianchi125, L. Bianchini23, M. Bianco30, O. Biebel100, S.P. Bieniek78, M. Biglietti134a, J. Bilbao De Mendizabal49, H. Bilokon47, M. Bindi54, S. Binet117, A. Bingul19b, C. Bini132a,132b, C.W. Black150, J.E. Black143, K.M. Black22, D. Blackburn138, R.E. Blair6, J.-B. Blanchard136, J.E. Blanco77, T. Blazek144a, I. Bloch42, C. Blocker23, W. Blum83,∗, U. Blumenschein54, G.J. Bobbink107, V.S. Bobrovnikov109,c, S.S. Bocchetta81, A. Bocci45, C. Bock100, M. Boehler48, J.A. Bogaerts30, D. Bogavac13, A.G. Bogdanchikov109, C. Bohm146a, V. Boisvert77, T. Bold38a, V. Boldea26a, A.S. Boldyrev99, M. Bomben80, M. Bona76, M. Boonekamp136, A. Borisov130, G. Borissov72, S. Borroni42, J. Bortfeldt100, V. Bortolotto60a,60b,60c, K. Bos107, D. Boscherini20a, M. Bosman12, J. Boudreau125, J. Bouffard2, E.V. Bouhova-Thacker72, D. Boumediene34, C. Bourdarios117, N. Bousson114, A. Boveia30, J. Boyd30, I.R. Boyko65, I. Bozic13, J. Bracinik18, A. Brandt8, G. Brandt54, O. Brandt58a, U. Bratzler156, B. Brau86, J.E. Brau116, H.M. Braun175,∗, S.F. Brazzale164a,164c, W.D. Breaden Madden53, K. Brendlinger122, A.J. Brennan88, L. Brenner107, R. Brenner166, S. Bressler172, K. Bristow145c, T.M. Bristow46, D. Britton53, D. Britzger42, F.M. Brochu28, I. Brock21, R. Brock90, J. Bronner101, G. Brooijmans35, T. Brooks77, W.K. Brooks32b, J. Brosamer15, E. Brost116, J. Brown55, P.A. Bruckman de Renstrom39, D. Bruncko144b, R. Bruneliere48, A. Bruni20a, G. Bruni20a, M. Bruschi20a, N. Bruscino21, L. Bryngemark81, T. Buanes14, Q. Buat142, P. Buchholz141, A.G. Buckley53, S.I. Buda26a, I.A. Budagov65, F. Buehrer48, L. Bugge119, M.K. Bugge119, O. Bulekov98, D. Bullock8, H. Burckhart30, S. Burdin74, B. Burghgrave108, S. Burke131, I. Burmeister43, E. Busato34, D. Büscher48, V. Büscher83, P. Bussey53, J.M. Butler22, A.I. Butt3, C.M. Buttar53, J.M. Butterworth78, P. Butti107, W. Buttinger25, A. Buzatu53, A.R. Buzykaev109,c, S. Cabrera Urbán167, D. Caforio128, V.M. Cairo37a,37b, O. Cakir4a, P. Calafiura15, A. Calandri136, G. Calderini80, P. Calfayan100, L.P. Caloba24a, D. Calvet34, S. Calvet34, R. Camacho Toro31, S. Camarda42, P. Camarri133a,133b, D. Cameron119, L.M. Caminada15, R. Caminal Armadans165, S. Campana30, M. Campanelli78, A. Campoverde148, V. Canale104a,104b, A. Canepa159a, M. Cano Bret76, J. Cantero82, R. Cantrill126a, T. Cao40, M.D.M. Capeans Garrido30, I. Caprini26a, M. Caprini26a, M. Capua37a,37b, R. Caputo83, R. Cardarelli133a, F. Cardillo48, T. Carli30, G. Carlino104a, L. Carminati91a,91b, S. Caron106, E. Carquin32a, G.D. Carrillo-Montoya8, J.R. Carter28, J. Carvalho126a,126c, D. Casadei78, M.P. Casado12, M. Casolino12, E. Castaneda-Miranda145b, A. Castelli107, V. Castillo Gimenez167, N.F. Castro126a,g, P. Catastini57, A. Catinaccio30, J.R. Catmore119, A. Cattai30, J. Caudron83, V. Cavaliere165, D. Cavalli91a, M. Cavalli-Sforza12, V. Cavasinni124a,124b, F. Ceradini134a,134b, B.C. Cerio45, K. Cerny129, A.S. Cerqueira24b, A. Cerri149, L. Cerrito76, F. Cerutti15, M. Cerv30, A. Cervelli17, S.A. Cetin19c, A. Chafaq135a, D. Chakraborty108, I. Chalupkova129, P. Chang165, B. Chapleau87, J.D. Chapman28, D.G. Charlton18, C.C. Chau158, C.A. Chavez Barajas149, S. Cheatham152, A. Chegwidden90, S. Chekanov6, S.V. Chekulaev159a, G.A. Chelkov65,h, M.A. Chelstowska89, C. Chen64, H. Chen25, K. Chen148, L. Chen33d,i, S. Chen33c, X. Chen33f, Y. Chen67, H.C. Cheng89, Y. Cheng31, A. Cheplakov65, E. Cheremushkina130, R. Cherkaoui El Moursli135e, V. Chernyatin25,∗, E. Cheu7, L. Chevalier136, V. Chiarella47, J.T. Childers6, G. Chiodini73a, A.S. Chisholm18, R.T. Chislett78, A. Chitan26a, M.V. Chizhov65, K. Choi61, S. Chouridou9, B.K.B. Chow100, V. Christodoulou78, D. Chromek-Burckhart30, J. Chudoba127, A.J. Chuinard87, J.J. Chwastowski39, L. Chytka115, G. Ciapetti132a,132b, A.K. Ciftci4a, D. Cinca53, V. Cindro75, I.A. Cioara21, A. Ciocio15, Z.H. Citron172, M. Ciubancan26a, A. Clark49, B.L. Clark57, P.J. Clark46, R.N. Clarke15, W. Cleland125, C. Clement146a,146b, Y. Coadou85, M. Cobal164a,164c, A. Coccaro138, J. Cochran64, L. Coffey23, J.G. Cogan143, B. Cole35, S. Cole108, A.P. Colijn107, J. Collot55, T. Colombo58c, G. Compostella101, P. Conde Muiño126a,126b, E. Coniavitis48, S.H. Connell145b, I.A. Connelly77, S.M. Consonni91a,91b, V. Consorti48, S. Constantinescu26a, C. Conta121a,121b, G. Conti30, F. Conventi104a,j, M. Cooke15, B.D. Cooper78, A.M. Cooper-Sarkar120, T. Cornelissen175, M. Corradi20a, F. Corriveau87,k, A. Corso-Radu163, A. Cortes-Gonzalez12, G. Cortiana101, G. Costa91a, M.J. Costa167, D. Costanzo139, D. Côté8, G. Cottin28, G. Cowan77, B.E. Cox84, K. Cranmer110, G. Cree29, S. Crépé-Renaudin55, F. Crescioli80, W.A. Cribbs146a,146b, M. Crispin Ortuzar120, M. Cristinziani21, V. Croft106, G. Crosetti37a,37b, T. Cuhadar Donszelmann139, J. Cummings176, M. Curatolo47, C. Cuthbert150, H. Czirr141, P. Czodrowski3, S. D’Auria53, M. D’Onofrio74, M.J. Da Cunha Sargedas De Sousa126a,126b, C. Da Via84, W. Dabrowski38a, A. Dafinca120, T. Dai89, O. Dale14, F. Dallaire95, C. Dallapiccola86, M. Dam36, J.R. Dandoy31, N.P. Dang48, A.C. Daniells18, M. Danninger168, M. Dano Hoffmann136, V. Dao48, G. Darbo50a, S. Darmora8, J. Dassoulas3, A. Dattagupta61, W. Davey21, C. David169, T. Davidek129, E. Davies120,l, M. Davies153, P. Davison78, Y. Davygora58a, E. Dawe88, I. Dawson139, R.K. Daya-Ishmukhametova86, K. De8, R. de Asmundis104a, S. De Castro20a,20b, S. De Cecco80, N. De Groot106, P. de Jong107, H. De la Torre82, F. De Lorenzi64, L. De Nooij107, D. De Pedis132a, A. De Salvo132a, U. De Sanctis149, A. De Santo149, J.B. De Vivie De Regie117, W.J. Dearnaley72, R. Debbe25, C. Debenedetti137, D.V. Dedovich65, I. Deigaard107, J. Del Peso82, T. Del Prete124a,124b, D. Delgove117, F. Deliot136, C.M. Delitzsch49, M. Deliyergiyev75, A. Dell’Acqua30, L. Dell’Asta22, M. Dell’Orso124a,124b, M. Della Pietra104a,j, D. della Volpe49, M. Delmastro5, P.A. Delsart55, C. Deluca107, D.A. DeMarco158, S. Demers176, M. Demichev65, A. Demilly80, S.P. Denisov130, D. Derendarz39, J.E. Derkaoui135d, F. Derue80, P. Dervan74, K. Desch21, C. Deterre42, P.O. Deviveiros30, A. Dewhurst131, S. Dhaliwal23, A. Di Ciaccio133a,133b, L. Di Ciaccio5, A. Di Domenico132a,132b, C. Di Donato104a,104b, A. Di Girolamo30, B. Di Girolamo30, A. Di Mattia152, B. Di Micco134a,134b, R. Di Nardo47, A. Di Simone48, R. Di Sipio158, D. Di Valentino29, C. Diaconu85, M. Diamond158, F.A. Dias46, M.A. Diaz32a, E.B. Diehl89, J. Dietrich16, S. Diglio85, A. Dimitrievska13, J. Dingfelder21, P. Dita26a, S. Dita26a, F. Dittus30, F. Djama85, T. Djobava51b, J.I. Djuvsland58a, M.A.B. do Vale24c, D. Dobos30, M. Dobre26a, C. Doglioni49, T. Dohmae155, J. Dolejsi129, Z. Dolezal129, B.A. Dolgoshein98,∗, M. Donadelli24d, S. Donati124a,124b, P. Dondero121a,121b, J. Donini34, J. Dopke131, A. Doria104a, M.T. Dova71, A.T. Doyle53, E. Drechsler54, M. Dris10, E. Dubreuil34, E. Duchovni172, G. Duckeck100, O.A. Ducu26a,85, D. Duda175, A. Dudarev30, L. Duflot117, L. Duguid77, M. Dührssen30, M. Dunford58a, H. Duran Yildiz4a, M. Düren52, A. Durglishvili51b, D. Duschinger44, M. Dyndal38a, C. Eckardt42, K.M. Ecker101, R.C. Edgar89, W. Edson2, N.C. Edwards46, W. Ehrenfeld21, T. Eifert30, G. Eigen14, K. Einsweiler15, T. Ekelof166, M. El Kacimi135c, M. Ellert166, S. Elles5, F. Ellinghaus83, A.A. Elliot169, N. Ellis30, J. Elmsheuser100, M. Elsing30, D. Emeliyanov131, Y. Enari155, O.C. Endner83, M. Endo118, J. Erdmann43, A. Ereditato17, G. Ernis175, J. Ernst2, M. Ernst25, S. Errede165, E. Ertel83, M. Escalier117, H. Esch43, C. Escobar125, B. Esposito47, A.I. Etienvre136, E. Etzion153, H. Evans61, A. Ezhilov123, L. Fabbri20a,20b, G. Facini31, R.M. Fakhrutdinov130, S. Falciano132a, R.J. Falla78, J. Faltova129, Y. Fang33a, M. Fanti91a,91b, A. Farbin8, A. Farilla134a, T. Farooque12, S. Farrell15, S.M. Farrington170, P. Farthouat30, F. Fassi135e, P. Fassnacht30, D. Fassouliotis9, M. Faucci Giannelli77, A. Favareto50a,50b, L. Fayard117, P. Federic144a, O.L. Fedin123,m, W. Fedorko168, S. Feigl30, L. Feligioni85, C. Feng33d, E.J. Feng6, H. Feng89, A.B. Fenyuk130, L. Feremenga8, P. Fernandez Martinez167, S. Fernandez Perez30, J. Ferrando53, A. Ferrari166, P. Ferrari107, R. Ferrari121a, D.E. Ferreira de Lima53, A. Ferrer167, D. Ferrere49, C. Ferretti89, A. Ferretto Parodi50a,50b, M. Fiascaris31, F. Fiedler83, A. Filipčič75, M. Filipuzzi42, F. Filthaut106, M. Fincke-Keeler169, K.D. Finelli150, M.C.N. Fiolhais126a,126c, L. Fiorini167, A. Firan40, A. Fischer2, C. Fischer12, J. Fischer175, W.C. Fisher90, E.A. Fitzgerald23, I. Fleck141, P. Fleischmann89, S. Fleischmann175, G.T. Fletcher139, G. Fletcher76, R.R.M. Fletcher122, T. Flick175, A. Floderus81, L.R. Flores Castillo60a, M.J. Flowerdew101, A. Formica136, A. Forti84, D. Fournier117, H. Fox72, S. Fracchia12, P. Francavilla80, M. Franchini20a,20b, D. Francis30, L. Franconi119, M. Franklin57, M. Frate163, M. Fraternali121a,121b, D. Freeborn78, S.T. French28, F. Friedrich44, D. Froidevaux30, J.A. Frost120, C. Fukunaga156, E. Fullana Torregrosa83, B.G. Fulsom143, J. Fuster167, C. Gabaldon55, O. Gabizon175, A. Gabrielli20a,20b, A. Gabrielli132a,132b, S. Gadatsch107, S. Gadomski49, G. Gagliardi50a,50b, P. Gagnon61, C. Galea106, B. Galhardo126a,126c, E.J. Gallas120, B.J. Gallop131, P. Gallus128, G. Galster36, K.K. Gan111, J. Gao33b,85, Y. Gao46, Y.S. Gao143,e, F.M. Garay Walls46, F. Garberson176, C. García167, J.E. García Navarro167, M. Garcia-Sciveres15, R.W. Gardner31, N. Garelli143, V. Garonne119, C. Gatti47, A. Gaudiello50a,50b, G. Gaudio121a, B. Gaur141, L. Gauthier95, P. Gauzzi132a,132b, I.L. Gavrilenko96, C. Gay168, G. Gaycken21, E.N. Gazis10, P. Ge33d, Z. Gecse168, C.N.P. Gee131, D.A.A. Geerts107, Ch. Geich-Gimbel21, M.P. Geisler58a, C. Gemme50a, M.H. Genest55, S. Gentile132a,132b, M. George54, S. George77, D. Gerbaudo163, A. Gershon153, H. Ghazlane135b, B. Giacobbe20a, S. Giagu132a,132b, V. Giangiobbe12, P. Giannetti124a,124b, B. Gibbard25, S.M. Gibson77, M. Gilchriese15, T.P.S. Gillam28, D. Gillberg30, G. Gilles34, D.M. Gingrich3,d, N. Giokaris9, M.P. Giordani164a,164c, F.M. Giorgi20a, F.M. Giorgi16, P.F. Giraud136, P. Giromini47, D. Giugni91a, C. Giuliani48, M. Giulini58b, B.K. Gjelsten119, S. Gkaitatzis154, I. Gkialas154, E.L. Gkougkousis117, L.K. Gladilin99, C. Glasman82, J. Glatzer30, P.C.F. Glaysher46, A. Glazov42, M. Goblirsch-Kolb101, J.R. Goddard76, J. Godlewski39, S. Goldfarb89, T. Golling49, D. Golubkov130, A. Gomes126a,126b,126d, R. Gonçalo126a, J. Goncalves Pinto Firmino Da Costa136, L. Gonella21, S. González de la Hoz167, G. Gonzalez Parra12, S. Gonzalez-Sevilla49, L. Goossens30, P.A. Gorbounov97, H.A. Gordon25, I. Gorelov105, B. Gorini30, E. Gorini73a,73b, A. Gorišek75, E. Gornicki39, A.T. Goshaw45, C. Gössling43, M.I. Gostkin65, D. Goujdami135c, A.G. Goussiou138, N. Govender145b, E. Gozani152, H.M.X. Grabas137, L. Graber54, I. Grabowska-Bold38a, P. Grafström20a,20b, K-J. Grahn42, J. Gramling49, E. Gramstad119, S. Grancagnolo16, V. Grassi148, V. Gratchev123, H.M. Gray30, E. Graziani134a, Z.D. Greenwood79,n, K. Gregersen78, I.M. Gregor42, P. Grenier143, J. Griffiths8, A.A. Grillo137, K. Grimm72, S. Grinstein12,o, Ph. Gris34, J.-F. Grivaz117, J.P. Grohs44, A. Grohsjean42, E. Gross172, J. Grosse-Knetter54, G.C. Grossi79, Z.J. Grout149, L. Guan33b, J. Guenther128, F. Guescini49, D. Guest176, O. Gueta153, E. Guido50a,50b, T. Guillemin117, S. Guindon2, U. Gul53, C. Gumpert44, J. Guo33e, S. Gupta120, G. Gustavino132a,132b, P. Gutierrez113, N.G. Gutierrez Ortiz53, C. Gutschow44, C. Guyot136, C. Gwenlan120, C.B. Gwilliam74, A. Haas110, C. Haber15, H.K. Hadavand8, N. Haddad135e, P. Haefner21, S. Hageböck21, Z. Hajduk39, H. Hakobyan177, M. Haleem42, J. Haley114, D. Hall120, G. Halladjian90, G.D. Hallewell85, K. Hamacher175, P. Hamal115, K. Hamano169, M. Hamer54, A. Hamilton145a, G.N. Hamity145c, P.G. Hamnett42, L. Han33b, K. Hanagaki118, K. Hanawa155, M. Hance15, P. Hanke58a, R. Hanna136, J.B. Hansen36, J.D. Hansen36, M.C. Hansen21, P.H. Hansen36, K. Hara160, A.S. Hard173, T. Harenberg175, F. Hariri117, S. Harkusha92, R.D. Harrington46, P.F. Harrison170, F. Hartjes107, M. Hasegawa67, S. Hasegawa103, Y. Hasegawa140, A. Hasib113, S. Hassani136, S. Haug17, R. Hauser90, L. Hauswald44, M. Havranek127, C.M. Hawkes18, R.J. Hawkings30, A.D. Hawkins81, T. Hayashi160, D. Hayden90, C.P. Hays120, J.M. Hays76, H.S. Hayward74, S.J. Haywood131, S.J. Head18, T. Heck83, V. Hedberg81, L. Heelan8, S. Heim122, T. Heim175, B. Heinemann15, L. Heinrich110, J. Hejbal127, L. Helary22, S. Hellman146a,146b, D. Hellmich21, C. Helsens30, J. Henderson120, R.C.W. Henderson72, Y. Heng173, C. Hengler42, A. Henrichs176, A.M. Henriques Correia30, S. Henrot-Versille117, G.H. Herbert16, Y. Hernández Jiménez167, R. Herrberg-Schubert16, G. Herten48, R. Hertenberger100, L. Hervas30, G.G. Hesketh78, N.P. Hessey107, J.W. Hetherly40, R. Hickling76, E. Higón-Rodriguez167, E. Hill169, J.C. Hill28, K.H. Hiller42, S.J. Hillier18, I. Hinchliffe15, E. Hines122, R.R. Hinman15, M. Hirose157, D. Hirschbuehl175, J. Hobbs148, N. Hod107, M.C. Hodgkinson139, P. Hodgson139, A. Hoecker30, M.R. Hoeferkamp105, F. Hoenig100, M. Hohlfeld83, D. Hohn21, T.R. Holmes15, M. Homann43, T.M. Hong125, L. Hooft van Huysduynen110, W.H. Hopkins116, Y. Horii103, A.J. Horton142, J-Y. Hostachy55, S. Hou151, A. Hoummada135a, J. Howard120, J. Howarth42, M. Hrabovsky115, I. Hristova16, J. Hrivnac117, T. Hryn’ova5, A. Hrynevich93, C. Hsu145c, P.J. Hsu151,p, S.-C. Hsu138, D. Hu35, Q. Hu33b, X. Hu89, Y. Huang42, Z. Hubacek30, F. Hubaut85, F. Huegging21, T.B. Huffman120, E.W. Hughes35, G. Hughes72, M. Huhtinen30, T.A. Hülsing83, N. Huseynov65,b, J. Huston90, J. Huth57, G. Iacobucci49, G. Iakovidis25, I. Ibragimov141, L. Iconomidou-Fayard117, E. Ideal176, Z. Idrissi135e, P. Iengo30, O. Igonkina107, T. Iizawa171, Y. Ikegami66, K. Ikematsu141, M. Ikeno66, Y. Ilchenko31,q, D. Iliadis154, N. Ilic143, Y. Inamaru67, T. Ince101, P. Ioannou9, M. Iodice134a, K. Iordanidou35, V. Ippolito57, A. Irles Quiles167, C. Isaksson166, M. Ishino68, M. Ishitsuka157, R. Ishmukhametov111, C. Issever120, S. Istin19a, J.M. Iturbe Ponce84, R. Iuppa133a,133b, J. Ivarsson81, W. Iwanski39, H. Iwasaki66, J.M. Izen41, V. Izzo104a, S. Jabbar3, B. Jackson122, M. Jackson74, P. Jackson1, M.R. Jaekel30, V. Jain2, K. Jakobs48, S. Jakobsen30, T. Jakoubek127, J. Jakubek128, D.O. Jamin151, D.K. Jana79, E. Jansen78, R. Jansky62, J. Janssen21, M. Janus170, G. Jarlskog81, N. Javadov65,b, T. Javůrek48, L. Jeanty15, J. Jejelava51a,r, G.-Y. Jeng150, D. Jennens88, P. Jenni48,s, J. Jentzsch43, C. Jeske170, S. Jézéquel5, H. Ji173, J. Jia148, Y. Jiang33b, S. Jiggins78, J. Jimenez Pena167, S. Jin33a, A. Jinaru26a, O. Jinnouchi157, M.D. Joergensen36, P. Johansson139, K.A. Johns7, K. Jon-And146a,146b, G. Jones170, R.W.L. Jones72, T.J. Jones74, J. Jongmanns58a, P.M. Jorge126a,126b, K.D. Joshi84, J. Jovicevic159a, X. Ju173, C.A. Jung43, P. Jussel62, A. Juste Rozas12,o, M. Kaci167, A. Kaczmarska39, M. Kado117, H. Kagan111, M. Kagan143, S.J. Kahn85, E. Kajomovitz45, C.W. Kalderon120, S. Kama40, A. Kamenshchikov130, N. Kanaya155, M. Kaneda30, S. Kaneti28, V.A. Kantserov98, J. Kanzaki66, B. Kaplan110, A. Kapliy31, D. Kar53, K. Karakostas10, A. Karamaoun3, N. Karastathis10,107, M.J. Kareem54, M. Karnevskiy83, S.N. Karpov65, Z.M. Karpova65, K. Karthik110, V. Kartvelishvili72, A.N. Karyukhin130, L. Kashif173, R.D. Kass111, A. Kastanas14, Y. Kataoka155, A. Katre49, J. Katzy42, K. Kawagoe70, T. Kawamoto155, G. Kawamura54, S. Kazama155, V.F. Kazanin109,c, M.Y. Kazarinov65, R. Keeler169, R. Kehoe40, J.S. Keller42, J.J. Kempster77, H. Keoshkerian84, O. Kepka127, B.P. Kerševan75, S. Kersten175, R.A. Keyes87, F. Khalil-zada11, H. Khandanyan146a,146b, A. Khanov114, A.G. Kharlamov109,c, T.J. Khoo28, V. Khovanskiy97, E. Khramov65, J. Khubua51b,t, H.Y. Kim8, H. Kim146a,146b, S.H. Kim160, Y.K. Kim31, N. Kimura154, O.M. Kind16, B.T. King74, M. King167, S.B. King168, J. Kirk131, A.E. Kiryunin101, T. Kishimoto67, D. Kisielewska38a, F. Kiss48, K. Kiuchi160, O. Kivernyk136, E. Kladiva144b, M.H. Klein35, M. Klein74, U. Klein74, K. Kleinknecht83, P. Klimek146a,146b, A. Klimentov25, R. Klingenberg43, J.A. Klinger139, T. Klioutchnikova30, E.-E. Kluge58a, P. Kluit107, S. Kluth101, E. Kneringer62, E.B.F.G. Knoops85, A. Knue53, A. Kobayashi155, D. Kobayashi157, T. Kobayashi155, M. Kobel44, M. Kocian143, P. Kodys129, T. Koffas29, E. Koffeman107, L.A. Kogan120, S. Kohlmann175, Z. Kohout128, T. Kohriki66, T. Koi143, H. Kolanoski16, I. Koletsou5, A.A. Komar96,∗, Y. Komori155, T. Kondo66, N. Kondrashova42, K. Köneke48, A.C. König106, S. König83, T. Kono66,u, R. Konoplich110,v, N. Konstantinidis78, R. Kopeliansky152, S. Koperny38a, L. Köpke83, A.K. Kopp48, K. Korcyl39, K. Kordas154, A. Korn78, A.A. Korol109,c, I. Korolkov12, E.V. Korolkova139, O. Kortner101, S. Kortner101, T. Kosek129, V.V. Kostyukhin21, V.M. Kotov65, A. Kotwal45, A. Kourkoumeli-Charalampidi154, C. Kourkoumelis9, V. Kouskoura25, A. Koutsman159a, R. Kowalewski169, T.Z. Kowalski38a, W. Kozanecki136, A.S. Kozhin130, V.A. Kramarenko99, G. Kramberger75, D. Krasnopevtsev98, M.W. Krasny80, A. Krasznahorkay30, J.K. Kraus21, A. Kravchenko25, S. Kreiss110, M. Kretz58c, J. Kretzschmar74, K. Kreutzfeldt52, P. Krieger158, K. Krizka31, K. Kroeninger43, H. Kroha101, J. Kroll122, J. Kroseberg21, J. Krstic13, U. Kruchonak65, H. Krüger21, N. Krumnack64, Z.V. Krumshteyn65, A. Kruse173, M.C. Kruse45, M. Kruskal22, T. Kubota88, H. Kucuk78, S. Kuday4b, S. Kuehn48, A. Kugel58c, F. Kuger174, A. Kuhl137, T. Kuhl42, V. Kukhtin65, Y. Kulchitsky92, S. Kuleshov32b, M. Kuna132a,132b, T. Kunigo68, A. Kupco127, H. Kurashige67, Y.A. Kurochkin92, R. Kurumida67, V. Kus127, E.S. Kuwertz169, M. Kuze157, J. Kvita115, T. Kwan169, D. Kyriazopoulos139, A. La Rosa49, J.L. La Rosa Navarro24d, L. La Rotonda37a,37b, C. Lacasta167, F. Lacava132a,132b, J. Lacey29, H. Lacker16, D. Lacour80, V.R. Lacuesta167, E. Ladygin65, R. Lafaye5, B. Laforge80, T. Lagouri176, S. Lai48, L. Lambourne78, S. Lammers61, C.L. Lampen7, W. Lampl7, E. Lançon136, U. Landgraf48, M.P.J. Landon76, V.S. Lang58a, J.C. Lange12, A.J. Lankford163, F. Lanni25, K. Lantzsch30, S. Laplace80, C. Lapoire30, J.F. Laporte136, T. Lari91a, F. Lasagni Manghi20a,20b, M. Lassnig30, P. Laurelli47, W. Lavrijsen15, A.T. Law137, P. Laycock74, T. Lazovich57, O. Le Dortz80, E. Le Guirriec85, E. Le Menedeu12, M. LeBlanc169, T. LeCompte6, F. Ledroit-Guillon55, C.A. Lee145b, S.C. Lee151, L. Lee1, G. Lefebvre80, M. Lefebvre169, F. Legger100, C. Leggett15, A. Lehan74, G. Lehmann Miotto30, X. Lei7, W.A. Leight29, A. Leisos154,w, A.G. Leister176, M.A.L. Leite24d, R. Leitner129, D. Lellouch172, B. Lemmer54, K.J.C. Leney78, T. Lenz21, B. Lenzi30, R. Leone7, S. Leone124a,124b, C. Leonidopoulos46, S. Leontsinis10, C. Leroy95, C.G. Lester28, M. Levchenko123, J. Levêque5, D. Levin89, L.J. Levinson172, M. Levy18, A. Lewis120, A.M. Leyko21, M. Leyton41, B. Li33b,x, H. Li148, H.L. Li31, L. Li45, L. Li33e, S. Li45, Y. Li33c,y, Z. Liang137, H. Liao34, B. Liberti133a, A. Liblong158, P. Lichard30, K. Lie165, J. Liebal21, W. Liebig14, C. Limbach21, A. Limosani150, S.C. Lin151,z, T.H. Lin83, F. Linde107, B.E. Lindquist148, J.T. Linnemann90, E. Lipeles122, A. Lipniacka14, M. Lisovyi58b, T.M. Liss165, D. Lissauer25, A. Lister168, A.M. Litke137, B. Liu151,aa, D. Liu151, H. Liu89, J. Liu85, J.B. Liu33b, K. Liu85, L. Liu165, M. Liu45, M. Liu33b, Y. Liu33b, M. Livan121a,121b, A. Lleres55, J. Llorente Merino82, S.L. Lloyd76, F. Lo Sterzo151, E. Lobodzinska42, P. Loch7, W.S. Lockman137, F.K. Loebinger84, A.E. Loevschall-Jensen36, A. Loginov176, T. Lohse16, K. Lohwasser42, M. Lokajicek127, B.A. Long22, J.D. Long89, R.E. Long72, K.A. Looper111, L. Lopes126a, D. Lopez Mateos57, B. Lopez Paredes139, I. Lopez Paz12, J. Lorenz100, N. Lorenzo Martinez61, M. Losada162, P. Loscutoff15, P.J. Lösel100, X. Lou33a, A. Lounis117, J. Love6, P.A. Love72, N. Lu89, H.J. Lubatti138, C. Luci132a,132b, A. Lucotte55, F. Luehring61, W. Lukas62, L. Luminari132a, O. Lundberg146a,146b, B. Lund-Jensen147, D. Lynn25, R. Lysak127, E. Lytken81, H. Ma25, L.L. Ma33d, G. Maccarrone47, A. Macchiolo101, C.M. Macdonald139, J. Machado Miguens122,126b, D. Macina30, D. Madaffari85, R. Madar34, H.J. Maddocks72, W.F. Mader44, A. Madsen166, S. Maeland14, T. Maeno25, A. Maevskiy99, E. Magradze54, K. Mahboubi48, J. Mahlstedt107, C. Maiani136, C. Maidantchik24a, A.A. Maier101, T. Maier100, A. Maio126a,126b,126d, S. Majewski116, Y. Makida66, N. Makovec117, B. Malaescu80, Pa. Malecki39, V.P. Maleev123, F. Malek55, U. Mallik63, D. Malon6, C. Malone143, S. Maltezos10, V.M. Malyshev109, S. Malyukov30, J. Mamuzic42, G. Mancini47, B. Mandelli30, L. Mandelli91a, I. Mandić75, R. Mandrysch63, J. Maneira126a,126b, A. Manfredini101, L. Manhaes de Andrade Filho24b, J. Manjarres Ramos159b, A. Mann100, P.M. Manning137, A. Manousakis-Katsikakis9, B. Mansoulie136, R. Mantifel87, M. Mantoani54, L. Mapelli30, L. March145c, G. Marchiori80, M. Marcisovsky127, C.P. Marino169, M. Marjanovic13, D.E. Marley89, F. Marroquim24a, S.P. Marsden84, Z. Marshall15, L.F. Marti17, S. Marti-Garcia167, B. Martin90, T.A. Martin170, V.J. Martin46, B. Martin dit Latour14, M. Martinez12,o, S. Martin-Haugh131, V.S. Martoiu26a, A.C. Martyniuk78, M. Marx138, F. Marzano132a, A. Marzin30, L. Masetti83, T. Mashimo155, R. Mashinistov96, J. Masik84, A.L. Maslennikov109,c, I. Massa20a,20b, L. Massa20a,20b, N. Massol5, P. Mastrandrea148, A. Mastroberardino37a,37b, T. Masubuchi155, P. Mättig175, J. Mattmann83, J. Maurer26a, S.J. Maxfield74, D.A. Maximov109,c, R. Mazini151, S.M. Mazza91a,91b, L. Mazzaferro133a,133b, G. Mc Goldrick158, S.P. Mc Kee89, A. McCarn89, R.L. McCarthy148, T.G. McCarthy29, N.A. McCubbin131, K.W. McFarlane56,∗, J.A. Mcfayden78, G. Mchedlidze54, S.J. McMahon131, R.A. McPherson169,k, M. Medinnis42, S. Meehan145a, S. Mehlhase100, A. Mehta74, K. Meier58a, C. Meineck100, B. Meirose41, B.R. Mellado Garcia145c, F. Meloni17, A. Mengarelli20a,20b, S. Menke101, E. Meoni161, K.M. Mercurio57, S. Mergelmeyer21, P. Mermod49, L. Merola104a,104b, C. Meroni91a, F.S. Merritt31, A. Messina132a,132b, J. Metcalfe25, A.S. Mete163, C. Meyer83, C. Meyer122, J-P. Meyer136, J. Meyer107, R.P. Middleton131, S. Miglioranzi164a,164c, L. Mijović21, G. Mikenberg172, M. Mikestikova127, M. Mikuž75, M. Milesi88, A. Milic30, D.W. Miller31, C. Mills46, A. Milov172, D.A. Milstead146a,146b, A.A. Minaenko130, Y. Minami155, I.A. Minashvili65, A.I. Mincer110, B. Mindur38a, M. Mineev65, Y. Ming173, L.M. Mir12, T. Mitani171, J. Mitrevski100, V.A. Mitsou167, A. Miucci49, P.S. Miyagawa139, J.U. Mjörnmark81, T. Moa146a,146b, K. Mochizuki85, S. Mohapatra35, W. Mohr48, S. Molander146a,146b, R. Moles-Valls167, K. Mönig42, C. Monini55, J. Monk36, E. Monnier85, J. Montejo Berlingen12, F. Monticelli71, S. Monzani132a,132b, R.W. Moore3, N. Morange117, D. Moreno162, M. Moreno Llácer54, P. Morettini50a, M. Morgenstern44, M. Morii57, M. Morinaga155, V. Morisbak119, S. Moritz83, A.K. Morley147, G. Mornacchi30, J.D. Morris76, S.S. Mortensen36, A. Morton53, L. Morvaj103, M. Mosidze51b, J. Moss111, K. Motohashi157, R. Mount143, E. Mountricha25, S.V. Mouraviev96,∗, E.J.W. Moyse86, S. Muanza85, R.D. Mudd18, F. Mueller101, J. Mueller125, K. Mueller21, R.S.P. Mueller100, T. Mueller28, D. Muenstermann49, P. Mullen53, G.A. Mullier17, Y. Munwes153, J.A. Murillo Quijada18, W.J. Murray170,131, H. Musheghyan54, E. Musto152, A.G. Myagkov130,ab, M. Myska128, O. Nackenhorst54, J. Nadal54, K. Nagai120, R. Nagai157, Y. Nagai85, K. Nagano66, A. Nagarkar111, Y. Nagasaka59, K. Nagata160, M. Nagel101, E. Nagy85, A.M. Nairz30, Y. Nakahama30, K. Nakamura66, T. Nakamura155, I. Nakano112, H. Namasivayam41, R.F. Naranjo Garcia42, R. Narayan31, T. Naumann42, G. Navarro162, R. Nayyar7, H.A. Neal89, P.Yu. Nechaeva96, T.J. Neep84, P.D. Nef143, A. Negri121a,121b, M. Negrini20a, S. Nektarijevic106, C. Nellist117, A. Nelson163, S. Nemecek127, P. Nemethy110, A.A. Nepomuceno24a, M. Nessi30,ac, M.S. Neubauer165, M. Neumann175, R.M. Neves110, P. Nevski25, P.R. Newman18, D.H. Nguyen6, R.B. Nickerson120, R. Nicolaidou136, B. Nicquevert30, J. Nielsen137, N. Nikiforou35, A. Nikiforov16, V. Nikolaenko130,ab, I. Nikolic-Audit80, K. Nikolopoulos18, J.K. Nilsen119, P. Nilsson25, Y. Ninomiya155, A. Nisati132a, R. Nisius101, T. Nobe157, M. Nomachi118, I. Nomidis29, T. Nooney76, S. Norberg113, M. Nordberg30, O. Novgorodova44, S. Nowak101, M. Nozaki66, L. Nozka115, K. Ntekas10, G. Nunes Hanninger88, T. Nunnemann100, E. Nurse78, F. Nuti88, B.J. O’Brien46, F. O’grady7, D.C. O’Neil142, V. O’Shea53, F.G. Oakham29,d, H. Oberlack101, T. Obermann21, J. Ocariz80, A. Ochi67, I. Ochoa78, J.P. Ochoa-Ricoux32a, S. Oda70, S. Odaka66, H. Ogren61, A. Oh84, S.H. Oh45, C.C. Ohm15, H. Ohman166, H. Oide30, W. Okamura118, H. Okawa160, Y. Okumura31, T. Okuyama155, A. Olariu26a, S.A. Olivares Pino46, D. Oliveira Damazio25, E. Oliver Garcia167, A. Olszewski39, J. Olszowska39, A. Onofre126a,126e, P.U.E. Onyisi31,q, C.J. Oram159a, M.J. Oreglia31, Y. Oren153, D. Orestano134a,134b, N. Orlando154, C. Oropeza Barrera53, R.S. Orr158, B. Osculati50a,50b, R. Ospanov84, G. Otero y Garzon27, H. Otono70, M. Ouchrif135d, E.A. Ouellette169, F. Ould-Saada119, A. Ouraou136, K.P. Oussoren107, Q. Ouyang33a, A. Ovcharova15, M. Owen53, R.E. Owen18, V.E. Ozcan19a, N. Ozturk8, K. Pachal142, A. Pacheco Pages12, C. Padilla Aranda12, M. Pagáčová48, S. Pagan Griso15, E. Paganis139, C. Pahl101, F. Paige25, P. Pais86, K. Pajchel119, G. Palacino159b, S. Palestini30, M. Palka38b, D. Pallin34, A. Palma126a,126b, Y.B. Pan173, E. Panagiotopoulou10, C.E. Pandini80, J.G. Panduro Vazquez77, P. Pani146a,146b, S. Panitkin25, D. Pantea26a, L. Paolozzi49, Th.D. Papadopoulou10, K. Papageorgiou154, A. Paramonov6, D. Paredes Hernandez154, M.A. Parker28, K.A. Parker139, F. Parodi50a,50b, J.A. Parsons35, U. Parzefall48, E. Pasqualucci132a, S. Passaggio50a, F. Pastore134a,134b,∗, Fr. Pastore77, G. Pásztor29, S. Pataraia175, N.D. Patel150, J.R. Pater84, T. Pauly30, J. Pearce169, B. Pearson113, L.E. Pedersen36, M. Pedersen119, S. Pedraza Lopez167, R. Pedro126a,126b, S.V. Peleganchuk109,c, D. Pelikan166, H. Peng33b, B. Penning31, J. Penwell61, D.V. Perepelitsa25, E. Perez Codina159a, M.T. Pérez García-Estañ167, L. Perini91a,91b, H. Pernegger30, S. Perrella104a,104b, R. Peschke42, V.D. Peshekhonov65, K. Peters30, R.F.Y. Peters84, B.A. Petersen30, T.C. Petersen36, E. Petit42, A. Petridis146a,146b, C. Petridou154, E. Petrolo132a, F. Petrucci134a,134b, N.E. Pettersson157, R. Pezoa32b, P.W. Phillips131, G. Piacquadio143, E. Pianori170, A. Picazio49, E. Piccaro76, M. Piccinini20a,20b, M.A. Pickering120, R. Piegaia27, D.T. Pignotti111, J.E. Pilcher31, A.D. Pilkington84, J. Pina126a,126b,126d, M. Pinamonti164a,164c,ad, J.L. Pinfold3, A. Pingel36, B. Pinto126a, S. Pires80, M. Pitt172, C. Pizio91a,91b, L. Plazak144a, M.-A. Pleier25, V. Pleskot129, E. Plotnikova65, P. Plucinski146a,146b, D. Pluth64, R. Poettgen146a,146b, L. Poggioli117, D. Pohl21, G. Polesello121a, A. Poley42, A. Policicchio37a,37b, R. Polifka158, A. Polini20a, C.S. Pollard53, V. Polychronakos25, K. Pommès30, L. Pontecorvo132a, B.G. Pope90, G.A. Popeneciu26b, D.S. Popovic13, A. Poppleton30, S. Pospisil128, K. Potamianos15, I.N. Potrap65, C.J. Potter149, C.T. Potter116, G. Poulard30, J. Poveda30, V. Pozdnyakov65, P. Pralavorio85, A. Pranko15, S. Prasad30, S. Prell64, D. Price84, L.E. Price6, M. Primavera73a, S. Prince87, M. Proissl46, K. Prokofiev60c, F. Prokoshin32b, E. Protopapadaki136, S. Protopopescu25, J. Proudfoot6, M. Przybycien38a, E. Ptacek116, D. Puddu134a,134b, E. Pueschel86, D. Puldon148, M. Purohit25,ae, P. Puzo117, J. Qian89, G. Qin53, Y. Qin84, A. Quadt54, D.R. Quarrie15, W.B. Quayle164a,164b, M. Queitsch-Maitland84, D. Quilty53, S. Raddum119, V. Radeka25, V. Radescu42, S.K. Radhakrishnan148, P. Radloff116, P. Rados88, F. Ragusa91a,91b, G. Rahal178, S. Rajagopalan25, M. Rammensee30, C. Rangel-Smith166, F. Rauscher100, S. Rave83, T. Ravenscroft53, M. Raymond30, A.L. Read119, N.P. Readioff74, D.M. Rebuzzi121a,121b, A. Redelbach174, G. Redlinger25, R. Reece137, K. Reeves41, L. Rehnisch16, H. Reisin27, M. Relich163, C. Rembser30, H. Ren33a, A. Renaud117, M. Rescigno132a, S. Resconi91a, O.L. Rezanova109,c, P. Reznicek129, R. Rezvani95, R. Richter101, S. Richter78, E. Richter-Was38b, O. Ricken21, M. Ridel80, P. Rieck16, C.J. Riegel175, J. Rieger54, M. Rijssenbeek148, A. Rimoldi121a,121b, L. Rinaldi20a, B. Ristić49, E. Ritsch30, I. Riu12, F. Rizatdinova114, E. Rizvi76, S.H. Robertson87,k, A. Robichaud-Veronneau87, D. Robinson28, J.E.M. Robinson84, A. Robson53, C. Roda124a,124b, S. Roe30, O. Røhne119, S. Rolli161, A. Romaniouk98, M. Romano20a,20b, S.M. Romano Saez34, E. Romero Adam167, N. Rompotis138, M. Ronzani48, L. Roos80, E. Ros167, S. Rosati132a, K. Rosbach48, P. Rose137, P.L. Rosendahl14, O. Rosenthal141, V. Rossetti146a,146b, E. Rossi104a,104b, L.P. Rossi50a, R. Rosten138, M. Rotaru26a, I. Roth172, J. Rothberg138, D. Rousseau117, C.R. Royon136, A. Rozanov85, Y. Rozen152, X. Ruan145c, F. Rubbo143, I. Rubinskiy42, V.I. Rud99, C. Rudolph44, M.S. Rudolph158, F. Rühr48, A. Ruiz-Martinez30, Z. Rurikova48, N.A. Rusakovich65, A. Ruschke100, H.L. Russell138, J.P. Rutherfoord7, N. Ruthmann48, Y.F. Ryabov123, M. Rybar165, G. Rybkin117, N.C. Ryder120, A.F. Saavedra150, G. Sabato107, S. Sacerdoti27, A. Saddique3, H.F-W. Sadrozinski137, R. Sadykov65, F. Safai Tehrani132a, M. Saimpert136, H. Sakamoto155, Y. Sakurai171, G. Salamanna134a,134b, A. Salamon133a, M. Saleem113, D. Salek107, P.H. Sales De Bruin138, D. Salihagic101, A. Salnikov143, J. Salt167, D. Salvatore37a,37b, F. Salvatore149, A. Salvucci106, A. Salzburger30, D. Sampsonidis154, A. Sanchez104a,104b, J. Sánchez167, V. Sanchez Martinez167, H. Sandaker119, R.L. Sandbach76, H.G. Sander83, M.P. Sanders100, M. Sandhoff175, C. Sandoval162, R. Sandstroem101, D.P.C. Sankey131, M. Sannino50a,50b, A. Sansoni47, C. Santoni34, R. Santonico133a,133b, H. Santos126a, I. Santoyo Castillo149, K. Sapp125, A. Sapronov65, J.G. Saraiva126a,126d, B. Sarrazin21, O. Sasaki66, Y. Sasaki155, K. Sato160, G. Sauvage5,∗, E. Sauvan5, G. Savage77, P. Savard158,d, C. Sawyer131, L. Sawyer79,n, J. Saxon31, C. Sbarra20a, A. Sbrizzi20a,20b, T. Scanlon78, D.A. Scannicchio163, M. Scarcella150, V. Scarfone37a,37b, J. Schaarschmidt172, P. Schacht101, D. Schaefer30, R. Schaefer42, J. Schaeffer83, S. Schaepe21, S. Schaetzel58b, U. Schäfer83, A.C. Schaffer117, D. Schaile100, R.D. Schamberger148, V. Scharf58a, V.A. Schegelsky123, D. Scheirich129, M. Schernau163, C. Schiavi50a,50b, C. Schillo48, M. Schioppa37a,37b, S. Schlenker30, E. Schmidt48, K. Schmieden30, C. Schmitt83, S. Schmitt58b, S. Schmitt42, B. Schneider159a, Y.J. Schnellbach74, U. Schnoor44, L. Schoeffel136, A. Schoening58b, B.D. Schoenrock90, E. Schopf21, A.L.S. Schorlemmer54, M. Schott83, D. Schouten159a, J. Schovancova8, S. Schramm49, M. Schreyer174, C. Schroeder83, N. Schuh83, M.J. Schultens21, H.-C. Schultz-Coulon58a, H. Schulz16, M. Schumacher48, B.A. Schumm137, Ph. Schune136, C. Schwanenberger84, A. Schwartzman143, T.A. Schwarz89, Ph. Schwegler101, H. Schweiger84, Ph. Schwemling136, R. Schwienhorst90, J. Schwindling136, T. Schwindt21, F.G. Sciacca17, E. Scifo117, G. Sciolla23, F. Scuri124a,124b, F. Scutti21, J. Searcy89, G. Sedov42, E. Sedykh123, P. Seema21, S.C. Seidel105, A. Seiden137, F. Seifert128, J.M. Seixas24a, G. Sekhniaidze104a, K. Sekhon89, S.J. Sekula40, D.M. Seliverstov123,∗, N. Semprini-Cesari20a,20b, C. Serfon30, L. Serin117, L. Serkin164a,164b, T. Serre85, M. Sessa134a,134b, R. Seuster159a, H. Severini113, T. Sfiligoj75, F. Sforza30, A. Sfyrla30, E. Shabalina54, M. Shamim116, L.Y. Shan33a, R. Shang165, J.T. Shank22, M. Shapiro15, P.B. Shatalov97, K. Shaw164a,164b, S.M. Shaw84, A. Shcherbakova146a,146b, C.Y. Shehu149, P. Sherwood78, L. Shi151,af, S. Shimizu67, C.O. Shimmin163, M. Shimojima102, M. Shiyakova65, A. Shmeleva96, D. Shoaleh Saadi95, M.J. Shochet31, S. Shojaii91a,91b, S. Shrestha111, E. Shulga98, M.A. Shupe7, S. Shushkevich42, P. Sicho127, O. Sidiropoulou174, D. Sidorov114, A. Sidoti20a,20b, F. Siegert44, Dj. Sijacki13, J. Silva126a,126d, Y. Silver153, S.B. Silverstein146a, V. Simak128, O. Simard5, Lj. Simic13, S. Simion117, E. Simioni83, B. Simmons78, D. Simon34, R. Simoniello91a,91b, P. Sinervo158, N.B. Sinev116, G. Siragusa174, A.N. Sisakyan65,∗, S.Yu. Sivoklokov99, J. Sjölin146a,146b, T.B. Sjursen14, M.B. Skinner72, H.P. Skottowe57, P. Skubic113, M. Slater18, T. Slavicek128, M. Slawinska107, K. Sliwa161, V. Smakhtin172, B.H. Smart46, L. Smestad14, S.Yu. Smirnov98, Y. Smirnov98, L.N. Smirnova99,ag, O. Smirnova81, M.N.K. Smith35, R.W. Smith35, M. Smizanska72, K. Smolek128, A.A. Snesarev96, G. Snidero76, S. Snyder25, R. Sobie169,k, F. Socher44, A. Soffer153, D.A. Soh151,af, C.A. Solans30, M. Solar128, J. Solc128, E.Yu. Soldatov98, U. Soldevila167, A.A. Solodkov130, A. Soloshenko65, O.V. Solovyanov130, V. Solovyev123, P. Sommer48, H.Y. Song33b, N. Soni1, A. Sood15, A. Sopczak128, B. Sopko128, V. Sopko128, V. Sorin12, D. Sosa58b, M. Sosebee8, C.L. Sotiropoulou124a,124b, R. Soualah164a,164c, A.M. Soukharev109,c, D. South42, B.C. Sowden77, S. Spagnolo73a,73b, M. Spalla124a,124b, F. Spanò77, W.R. Spearman57, F. Spettel101, R. Spighi20a, G. Spigo30, L.A. Spiller88, M. Spousta129, T. Spreitzer158, R.D. St. Denis53,∗, S. Staerz44, J. Stahlman122, R. Stamen58a, S. Stamm16, E. Stanecka39, C. Stanescu134a, M. Stanescu-Bellu42, M.M. Stanitzki42, S. Stapnes119, E.A. Starchenko130, J. Stark55, P. Staroba127, P. Starovoitov42, R. Staszewski39, P. Stavina144a,∗, P. Steinberg25, B. Stelzer142, H.J. Stelzer30, O. Stelzer-Chilton159a, H. Stenzel52, S. Stern101, G.A. Stewart53, J.A. Stillings21, M.C. Stockton87, M. Stoebe87, G. Stoicea26a, P. Stolte54, S. Stonjek101, A.R. Stradling8, A. Straessner44, M.E. Stramaglia17, J. Strandberg147, S. Strandberg146a,146b, A. Strandlie119, E. Strauss143, M. Strauss113, P. Strizenec144b, R. Ströhmer174, D.M. Strom116, R. Stroynowski40, A. Strubig106, S.A. Stucci17, B. Stugu14, N.A. Styles42, D. Su143, J. Su125, R. Subramaniam79, A. Succurro12, Y. Sugaya118, C. Suhr108, M. Suk128, V.V. Sulin96, S. Sultansoy4c, T. Sumida68, S. Sun57, X. Sun33a, J.E. Sundermann48, K. Suruliz149, G. Susinno37a,37b, M.R. Sutton149, S. Suzuki66, Y. Suzuki66, M. Svatos127, S. Swedish168, M. Swiatlowski143, I. Sykora144a, T. Sykora129, D. Ta90, C. Taccini134a,134b, K. Tackmann42, J. Taenzer158, A. Taffard163, R. Tafirout159a, N. Taiblum153, H. Takai25, R. Takashima69, H. Takeda67, T. Takeshita140, Y. Takubo66, M. Talby85, A.A. Talyshev109,c, J.Y.C. Tam174, K.G. Tan88, J. Tanaka155, R. Tanaka117, S. Tanaka66, B.B. Tannenwald111, N. Tannoury21, S. Tapprogge83, S. Tarem152, F. Tarrade29, G.F. Tartarelli91a, P. Tas129, M. Tasevsky127, T. Tashiro68, E. Tassi37a,37b, A. Tavares Delgado126a,126b, Y. Tayalati135d, F.E. Taylor94, G.N. Taylor88, W. Taylor159b, F.A. Teischinger30, M. Teixeira Dias Castanheira76, P. Teixeira-Dias77, K.K. Temming48, H. Ten Kate30, P.K. Teng151, J.J. Teoh118, F. Tepel175, S. Terada66, K. Terashi155, J. Terron82, S. Terzo101, M. Testa47, R.J. Teuscher158,k, J. Therhaag21, T. Theveneaux-Pelzer34, J.P. Thomas18, J. Thomas-Wilsker77, E.N. Thompson35, P.D. Thompson18, R.J. Thompson84, A.S. Thompson53, L.A. Thomsen176, E. Thomson122, M. Thomson28, R.P. Thun89,∗, M.J. Tibbetts15, R.E. Ticse Torres85, V.O. Tikhomirov96,ah, Yu.A. Tikhonov109,c, S. Timoshenko98, E. Tiouchichine85, P. Tipton176, S. Tisserant85, T. Todorov5, S. Todorova-Nova129, J. Tojo70, S. Tokár144a, K. Tokushuku66, K. Tollefson90, E. Tolley57, L. Tomlinson84, M. Tomoto103, L. Tompkins143,ai, K. Toms105, E. Torrence116, H. Torres142, E. Torró Pastor167, J. Toth85,aj, F. Touchard85, D.R. Tovey139, T. Trefzger174, L. Tremblet30, A. Tricoli30, I.M. Trigger159a, S. Trincaz-Duvoid80, M.F. Tripiana12, W. Trischuk158, B. Trocmé55, C. Troncon91a, M. Trottier-McDonald15, M. Trovatelli169, P. True90, L. Truong164a,164c, M. Trzebinski39, A. Trzupek39, C. Tsarouchas30, J.C-L. Tseng120, P.V. Tsiareshka92, D. Tsionou154, G. Tsipolitis10, N. Tsirintanis9, S. Tsiskaridze12, V. Tsiskaridze48, E.G. Tskhadadze51a, I.I. Tsukerman97, V. Tsulaia15, S. Tsuno66, D. Tsybychev148, A. Tudorache26a, V. Tudorache26a, A.N. Tuna122, S.A. Tupputi20a,20b, S. Turchikhin99,ag, D. Turecek128, R. Turra91a,91b, A.J. Turvey40, P.M. Tuts35, A. Tykhonov49, M. Tylmad146a,146b, M. Tyndel131, I. Ueda155, R. Ueno29, M. Ughetto146a,146b, M. Ugland14, M. Uhlenbrock21, F. Ukegawa160, G. Unal30, A. Undrus25, G. Unel163, F.C. Ungaro48, Y. Unno66, C. Unverdorben100, J. Urban144b, P. Urquijo88, P. Urrejola83, G. Usai8, A. Usanova62, L. Vacavant85, V. Vacek128, B. Vachon87, C. Valderanis83, N. Valencic107, S. Valentinetti20a,20b, A. Valero167, L. Valery12, S. Valkar129, E. Valladolid Gallego167, S. Vallecorsa49, J.A. Valls Ferrer167, W. Van Den Wollenberg107, P.C. Van Der Deijl107, R. van der Geer107, H. van der Graaf107, R. Van Der Leeuw107, N. van Eldik152, P. van Gemmeren6, J. Van Nieuwkoop142, I. van Vulpen107, M.C. van Woerden30, M. Vanadia132a,132b, W. Vandelli30, R. Vanguri122, A. Vaniachine6, F. Vannucci80, G. Vardanyan177, R. Vari132a, E.W. Varnes7, T. Varol40, D. Varouchas80, A. Vartapetian8, K.E. Varvell150, V.I. Vassilakopoulos56, F. Vazeille34, T. Vazquez Schroeder87, J. Veatch7, L.M. Veloce158, F. Veloso126a,126c, T. Velz21, S. Veneziano132a, A. Ventura73a,73b, D. Ventura86, M. Venturi169, N. Venturi158, A. Venturini23, V. Vercesi121a, M. Verducci132a,132b, W. Verkerke107, J.C. Vermeulen107, A. Vest44, M.C. Vetterli142,d, O. Viazlo81, I. Vichou165, T. Vickey139, O.E. Vickey Boeriu139, G.H.A. Viehhauser120, S. Viel15, R. Vigne62, M. Villa20a,20b, M. Villaplana Perez91a,91b, E. Vilucchi47, M.G. Vincter29, V.B. Vinogradov65, I. Vivarelli149, F. Vives Vaque3, S. Vlachos10, D. Vladoiu100, M. Vlasak128, M. Vogel32a, P. Vokac128, G. Volpi124a,124b, M. Volpi88, H. von der Schmitt101, H. von Radziewski48, E. von Toerne21, V. Vorobel129, K. Vorobev98, M. Vos167, R. Voss30, J.H. Vossebeld74, N. Vranjes13, M. Vranjes Milosavljevic13, V. Vrba127, M. Vreeswijk107, R. Vuillermet30, I. Vukotic31, Z. Vykydal128, P. Wagner21, W. Wagner175, H. Wahlberg71, S. Wahrmund44, J. Wakabayashi103, J. Walder72, R. Walker100, W. Walkowiak141, C. Wang151, F. Wang173, H. Wang15, H. Wang40, J. Wang42, J. Wang33a, K. Wang87, R. Wang6, S.M. Wang151, T. Wang21, X. Wang176, C. Wanotayaroj116, A. Warburton87, C.P. Ward28, D.R. Wardrope78, M. Warsinsky48, A. Washbrook46, C. Wasicki42, P.M. Watkins18, A.T. Watson18, I.J. Watson150, M.F. Watson18, G. Watts138, S. Watts84, B.M. Waugh78, S. Webb84, M.S. Weber17, S.W. Weber174, J.S. Webster31, A.R. Weidberg120, B. Weinert61, J. Weingarten54, C. Weiser48, H. Weits107, P.S. Wells30, T. Wenaus25, T. Wengler30, S. Wenig30, N. Wermes21, M. Werner48, P. Werner30, M. Wessels58a, J. Wetter161, K. Whalen116, A.M. Wharton72, A. White8, M.J. White1, R. White32b, S. White124a,124b, D. Whiteson163, F.J. Wickens131, W. Wiedenmann173, M. Wielers131, P. Wienemann21, C. Wiglesworth36, L.A.M. Wiik-Fuchs21, A. Wildauer101, H.G. Wilkens30, H.H. Williams122, S. Williams107, C. Willis90, S. Willocq86, A. Wilson89, J.A. Wilson18, I. Wingerter-Seez5, F. Winklmeier116, B.T. Winter21, M. Wittgen143, J. Wittkowski100, S.J. Wollstadt83, M.W. Wolter39, H. Wolters126a,126c, B.K. Wosiek39, J. Wotschack30, M.J. Woudstra84, K.W. Wozniak39, M. Wu55, M. Wu31, S.L. Wu173, X. Wu49, Y. Wu89, T.R. Wyatt84, B.M. Wynne46, S. Xella36, D. Xu33a, L. Xu33b,ak, B. Yabsley150, S. Yacoob145b,al, R. Yakabe67, M. Yamada66, Y. Yamaguchi118, A. Yamamoto66, S. Yamamoto155, T. Yamanaka155, K. Yamauchi103, Y. Yamazaki67, Z. Yan22, H. Yang33e, H. Yang173, Y. Yang151, W-M. Yao15, Y. Yasu66, E. Yatsenko5, K.H. Yau Wong21, J. Ye40, S. Ye25, I. Yeletskikh65, A.L. Yen57, E. Yildirim42, K. Yorita171, R. Yoshida6, K. Yoshihara122, C. Young143, C.J.S. Young30, S. Youssef22, D.R. Yu15, J. Yu8, J.M. Yu89, J. Yu114, L. Yuan67, A. Yurkewicz108, I. Yusuff28,am, B. Zabinski39, R. Zaidan63, A.M. Zaitsev130,ab, J. Zalieckas14, A. Zaman148, S. Zambito57, L. Zanello132a,132b, D. Zanzi88, C. Zeitnitz175, M. Zeman128, A. Zemla38a, K. Zengel23, O. Zenin130, T. Ženiš144a, D. Zerwas117, D. Zhang89, F. Zhang173, H. Zhang33c, J. Zhang6, L. Zhang48, R. Zhang33b, X. Zhang33d, Z. Zhang117, X. Zhao40, Y. Zhao33d,117, Z. Zhao33b, A. Zhemchugov65, J. Zhong120, B. Zhou89, C. Zhou45, L. Zhou35, L. Zhou40, N. Zhou163, C.G. Zhu33d, H. Zhu33a, J. Zhu89, Y. Zhu33b, X. Zhuang33a, K. Zhukov96, A. Zibell174, D. Zieminska61, N.I. Zimine65, C. Zimmermann83, S. Zimmermann48, Z. Zinonos54, M. Zinser83, M. Ziolkowski141, L. Živković13, G. Zobernig173, A. Zoccoli20a,20b, M. zur Nedden16, G. Zurzolo104a,104b, L. Zwalinski30.
1 Department of Physics, University of Adelaide, Adelaide, Australia
2 Physics Department, SUNY Albany, Albany NY, United States of America
3 Department of Physics, University of Alberta, Edmonton AB, Canada
4 (a) Department of Physics, Ankara University, Ankara; (b) Istanbul Aydin University, Istanbul; (c) Division of Physics, TOBB University of Economics and Technology, Ankara, Turkey
5 LAPP, CNRS/IN2P3 and Université Savoie Mont Blanc, Annecy-le-Vieux, France
6 High Energy Physics Division, Argonne National Laboratory, Argonne IL, United States of America
7 Department of Physics, University of Arizona, Tucson AZ, United States of America
8 Department of Physics, The University of Texas at Arlington, Arlington TX, United States of America
9 Physics Department, University of Athens, Athens, Greece
10 Physics Department, National Technical University of Athens, Zografou, Greece
11 Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan
12 Institut de Física d’Altes Energies and Departament de Física de la Universitat Autònoma de Barcelona, Barcelona, Spain
13 Institute of Physics, University of Belgrade, Belgrade, Serbia
14 Department for Physics and Technology, University of Bergen, Bergen, Norway
15 Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley CA, United States of America
16 Department of Physics, Humboldt University, Berlin, Germany
17 Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland
18 School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
19 (a) Department of Physics, Bogazici University, Istanbul; (b) Department of Physics Engineering, Gaziantep University, Gaziantep; (c) Department of Physics, Dogus University, Istanbul, Turkey
20 (a) INFN Sezione di Bologna; (b) Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy
21 Physikalisches Institut, University of Bonn, Bonn, Germany
22 Department of Physics, Boston University, Boston MA, United States of America
23 Department of Physics, Brandeis University, Waltham MA, United States of America
24 (a) Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro; (b) Electrical Circuits Department, Federal University of Juiz de Fora (UFJF), Juiz de Fora; (c) Federal University of Sao Joao del Rei (UFSJ), Sao Joao del Rei; (d) Instituto de Fisica, Universidade de Sao Paulo, Sao Paulo, Brazil
25 Physics Department, Brookhaven National Laboratory, Upton NY, United States of America
26 (a) National Institute of Physics and Nuclear Engineering, Bucharest; (b) National Institute for Research and Development of Isotopic and Molecular Technologies, Physics Department, Cluj Napoca; (c) University Politehnica Bucharest, Bucharest; (d) West University in Timisoara, Timisoara, Romania
27 Departamento de Física, Universidad de Buenos Aires, Buenos Aires, Argentina
28 Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom
29 Department of Physics, Carleton University, Ottawa ON, Canada
30 CERN, Geneva, Switzerland
31 Enrico Fermi Institute, University of Chicago, Chicago IL, United States of America
32 (a) Departamento de Física, Pontificia Universidad Católica de Chile, Santiago; (b) Departamento de Física, Universidad Técnica Federico Santa María, Valparaíso, Chile
33 (a) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; (b) Department of Modern Physics, University of Science and Technology of China, Anhui; (c) Department of Physics, Nanjing University, Jiangsu; (d) School of Physics, Shandong University, Shandong; (e) Department of Physics and Astronomy, Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University, Shanghai; (f) Physics Department, Tsinghua University, Beijing 100084, China
34 Laboratoire de Physique Corpusculaire, Clermont Université and Université Blaise Pascal and CNRS/IN2P3, Clermont-Ferrand, France
35 Nevis Laboratory, Columbia University, Irvington NY, United States of America
36 Niels Bohr Institute, University of Copenhagen, Kobenhavn, Denmark
37 (a) INFN Gruppo Collegato di Cosenza, Laboratori Nazionali di Frascati; (b) Dipartimento di Fisica, Università della Calabria, Rende, Italy
38 (a) AGH University of Science and Technology, Faculty of Physics and Applied Computer Science, Krakow; (b) Marian Smoluchowski Institute of Physics, Jagiellonian University, Krakow, Poland
39 Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland
40 Physics Department, Southern Methodist University, Dallas TX, United States of America
41 Physics Department, University of Texas at Dallas, Richardson TX, United States of America
42 DESY, Hamburg and Zeuthen, Germany
43 Institut für Experimentelle Physik IV, Technische Universität Dortmund, Dortmund, Germany
44 Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany
45 Department of Physics, Duke University, Durham NC, United States of America
46 SUPA - School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
47 INFN Laboratori Nazionali di Frascati, Frascati, Italy
48 Fakultät für Mathematik und Physik, Albert-Ludwigs-Universität, Freiburg, Germany
49 Section de Physique, Université de Genève, Geneva, Switzerland
50 (a) INFN Sezione di Genova; (b) Dipartimento di Fisica, Università di Genova, Genova, Italy
51 (a) E. Andronikashvili Institute of Physics, Iv. Javakhishvili Tbilisi State University, Tbilisi; (b) High Energy Physics Institute, Tbilisi State University, Tbilisi, Georgia
52 II Physikalisches Institut, Justus-Liebig-Universität Giessen, Giessen, Germany
53 SUPA - School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom
54 II Physikalisches Institut, Georg-August-Universität, Göttingen, Germany
55 Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
56 Department of Physics, Hampton University, Hampton VA, United States of America
57 Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge MA, United States of America
58 (a) Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg; (b) Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg; (c) ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany
59 Faculty of Applied Information Science, Hiroshima Institute of Technology, Hiroshima, Japan
60 (a) Department of Physics, The Chinese University of Hong Kong, Shatin, N.T., Hong Kong; (b) Department of Physics, The University of Hong Kong, Hong Kong; (c) Department of Physics, The Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, China
61 Department of Physics, Indiana University, Bloomington IN, United States of America
62 Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität, Innsbruck, Austria
63 University of Iowa, Iowa City IA, United States of America
64 Department of Physics and Astronomy, Iowa State University, Ames IA, United States of America
65 Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia
66 KEK, High Energy Accelerator Research Organization, Tsukuba, Japan
67 Graduate School of Science, Kobe University, Kobe, Japan
68 Faculty of Science, Kyoto University, Kyoto, Japan
69 Kyoto University of Education, Kyoto, Japan
70 Department of Physics, Kyushu University, Fukuoka, Japan
71 Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
72 Physics Department, Lancaster University, Lancaster, United Kingdom
73 (a) INFN Sezione di Lecce; (b) Dipartimento di Matematica e Fisica, Università del Salento, Lecce, Italy
74 Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom
75 Department of Physics, Jožef Stefan Institute and University of Ljubljana, Ljubljana, Slovenia
76 School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
77 Department of Physics, Royal Holloway University of London, Surrey, United Kingdom
78 Department of Physics and Astronomy, University College London, London, United Kingdom
79 Louisiana Tech University, Ruston LA, United States of America
80 Laboratoire de Physique Nucléaire et de Hautes Energies, UPMC and Université Paris-Diderot and CNRS/IN2P3, Paris, France
81 Fysiska institutionen, Lunds universitet, Lund, Sweden
82 Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain
83 Institut für Physik, Universität Mainz, Mainz, Germany
84 School of Physics and Astronomy, University of Manchester, Manchester, United Kingdom
85 CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France
86 Department of Physics, University of Massachusetts, Amherst MA, United States of America
87 Department of Physics, McGill University, Montreal QC, Canada
88 School of Physics, University of Melbourne, Victoria, Australia
89 Department of Physics, The University of Michigan, Ann Arbor MI, United States of America
90 Department of Physics and Astronomy, Michigan State University, East Lansing MI, United States of America
91 (a) INFN Sezione di Milano; (b) Dipartimento di Fisica, Università di Milano, Milano, Italy
92 B.I. Stepanov Institute of Physics, National Academy of Sciences of Belarus, Minsk, Republic of Belarus
93 National Scientific and Educational Centre for Particle and High Energy Physics, Minsk, Republic of Belarus
94 Department of Physics, Massachusetts Institute of Technology, Cambridge MA, United States of America
95 Group of Particle Physics, University of Montreal, Montreal QC, Canada
96 P.N. Lebedev Institute of Physics, Academy of Sciences, Moscow, Russia
97 Institute for Theoretical and Experimental Physics (ITEP), Moscow, Russia
98 National Research Nuclear University MEPhI, Moscow, Russia
99 D.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University, Moscow, Russia
100 Fakultät für Physik, Ludwig-Maximilians-Universität München, München, Germany
101 Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), München, Germany
102 Nagasaki Institute of Applied Science, Nagasaki, Japan
103 Graduate School of Science and Kobayashi-Maskawa Institute, Nagoya University, Nagoya, Japan
104 (a) INFN Sezione di Napoli; (b) Dipartimento di Fisica, Università di Napoli, Napoli, Italy
105 Department of Physics and Astronomy, University of New Mexico, Albuquerque NM, United States of America
106 Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen, Netherlands
107 Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, Netherlands
108 Department of Physics, Northern Illinois University, DeKalb IL, United States of America
109 Budker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia
110 Department of Physics, New York University, New York NY, United States of America
111 Ohio State University, Columbus OH, United States of America
112 Faculty of Science, Okayama University, Okayama, Japan
113 Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman OK, United States of America
114 Department of Physics, Oklahoma State University, Stillwater OK, United States of America
115 Palacký University, RCPTM, Olomouc, Czech Republic
116 Center for High Energy Physics, University of Oregon, Eugene OR, United States of America
117 LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France
118 Graduate School of Science, Osaka University, Osaka, Japan
119 Department of Physics, University of Oslo, Oslo, Norway
120 Department of Physics, Oxford University, Oxford, United Kingdom
121 (a) INFN Sezione di Pavia; (b) Dipartimento di Fisica, Università di Pavia, Pavia, Italy
122 Department of Physics, University of Pennsylvania, Philadelphia PA, United States of America
123 National Research Centre ”Kurchatov Institute” B.P.Konstantinov Petersburg Nuclear Physics Institute, St. Petersburg, Russia
124 (a) INFN Sezione di Pisa; (b) Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy
125 Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh PA, United States of America
126 (a) Laboratório de Instrumentação e Física Experimental de Partículas - LIP, Lisboa; (b) Faculdade de Ciências, Universidade de Lisboa, Lisboa; (c) Department of Physics, University of Coimbra, Coimbra; (d) Centro de Física Nuclear da Universidade de Lisboa, Lisboa; (e) Departamento de Fisica, Universidade do Minho, Braga; (f) Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada (Spain); (g) Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal
127 Institute of Physics, Academy of Sciences of the Czech Republic, Praha, Czech Republic
128 Czech Technical University in Prague, Praha, Czech Republic
129 Faculty of Mathematics and Physics, Charles University in Prague, Praha, Czech Republic
130 State Research Center Institute for High Energy Physics, Protvino, Russia
131 Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom
132 (a) INFN Sezione di Roma; (b) Dipartimento di Fisica, Sapienza Università di Roma, Roma, Italy
133 (a) INFN Sezione di Roma Tor Vergata; (b) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy
134 (a) INFN Sezione di Roma Tre; (b) Dipartimento di Matematica e Fisica, Università Roma Tre, Roma, Italy
135 (a) Faculté des Sciences Ain Chock, Réseau Universitaire de Physique des Hautes Energies - Université Hassan II, Casablanca; (b) Centre National de l’Energie des Sciences Techniques Nucleaires, Rabat; (c) Faculté des Sciences Semlalia, Université Cadi Ayyad, LPHEA-Marrakech; (d) Faculté des Sciences, Université Mohamed Premier and LPTPM, Oujda; (e) Faculté des sciences, Université Mohammed V-Agdal, Rabat, Morocco
136 DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France
137 Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz CA, United States of America
138 Department of Physics, University of Washington, Seattle WA, United States of America
139 Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
140 Department of Physics, Shinshu University, Nagano, Japan
141 Fachbereich Physik, Universität Siegen, Siegen, Germany
142 Department of Physics, Simon Fraser University, Burnaby BC, Canada
143 SLAC National Accelerator Laboratory, Stanford CA, United States of America
144 (a) Faculty of Mathematics, Physics & Informatics, Comenius University, Bratislava; (b) Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic
145 (a) Department of Physics, University of Cape Town, Cape Town; (b) Department of Physics, University of Johannesburg, Johannesburg; (c) School of Physics, University of the Witwatersrand, Johannesburg, South Africa
146 (a) Department of Physics, Stockholm University; (b) The Oskar Klein Centre, Stockholm, Sweden
147 Physics Department, Royal Institute of Technology, Stockholm, Sweden
148 Departments of Physics & Astronomy and Chemistry, Stony Brook University, Stony Brook NY, United States of America
149 Department of Physics and Astronomy, University of Sussex, Brighton, United Kingdom
150 School of Physics, University of Sydney, Sydney, Australia
151 Institute of Physics, Academia Sinica, Taipei, Taiwan
152 Department of Physics, Technion: Israel Institute of Technology, Haifa, Israel
153 Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel
154 Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece
155 International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan
156 Graduate School of Science and Technology, Tokyo Metropolitan University, Tokyo, Japan
157 Department of Physics, Tokyo Institute of Technology, Tokyo, Japan
158 Department of Physics, University of Toronto, Toronto ON, Canada
159 (a) TRIUMF, Vancouver BC; (b) Department of Physics and Astronomy, York University, Toronto ON, Canada
160 Faculty of Pure and Applied Sciences, University of Tsukuba, Tsukuba, Japan
161 Department of Physics and Astronomy, Tufts University, Medford MA, United States of America
162 Centro de Investigaciones, Universidad Antonio Narino, Bogota, Colombia
163 Department of Physics and Astronomy, University of California Irvine, Irvine CA, United States of America
164 (a) INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine; (b) ICTP, Trieste; (c) Dipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy
165 Department of Physics, University of Illinois, Urbana IL, United States of America
166 Department of Physics and Astronomy, University of Uppsala, Uppsala, Sweden
167 Instituto de Física Corpuscular (IFIC) and Departamento de Física Atómica, Molecular y Nuclear and Departamento de Ingeniería Electrónica and Instituto de Microelectrónica de Barcelona (IMB-CNM), University of Valencia and CSIC, Valencia, Spain
168 Department of Physics, University of British Columbia, Vancouver BC, Canada
169 Department of Physics and Astronomy, University of Victoria, Victoria BC, Canada
170 Department of Physics, University of Warwick, Coventry, United Kingdom
171 Waseda University, Tokyo, Japan
172 Department of Particle Physics, The Weizmann Institute of Science, Rehovot, Israel
173 Department of Physics, University of Wisconsin, Madison WI, United States of America
174 Fakultät für Physik und Astronomie, Julius-Maximilians-Universität, Würzburg, Germany
175 Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany
176 Department of Physics, Yale University, New Haven CT, United States of America
177 Yerevan Physics Institute, Yerevan, Armenia
178 Centre de Calcul de l’Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Villeurbanne, France
a Also at Department of Physics, King’s College London, London, United Kingdom
b Also at Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan
c Also at Novosibirsk State University, Novosibirsk, Russia
d Also at TRIUMF, Vancouver BC, Canada
e Also at Department of Physics, California State University, Fresno CA, United States of America
f Also at Department of Physics, University of Fribourg, Fribourg, Switzerland
g Also at Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Portugal
h Also at Tomsk State University, Tomsk, Russia
i Also at CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France
j Also at Universita di Napoli Parthenope, Napoli, Italy
k Also at Institute of Particle Physics (IPP), Canada
l Also at Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom
m Also at Department of Physics, St. Petersburg State Polytechnical University, St. Petersburg, Russia
n Also at Louisiana Tech University, Ruston LA, United States of America
o Also at Institucio Catalana de Recerca i Estudis Avancats, ICREA, Barcelona, Spain
p Also at Department of Physics, National Tsing Hua University, Taiwan
q Also at Department of Physics, The University of Texas at Austin, Austin TX, United States of America
r Also at Institute of Theoretical Physics, Ilia State University, Tbilisi, Georgia
s Also at CERN, Geneva, Switzerland
t Also at Georgian Technical University (GTU),Tbilisi, Georgia
u Also at Ochadai Academic Production, Ochanomizu University, Tokyo, Japan
v Also at Manhattan College, New York NY, United States of America
w Also at Hellenic Open University, Patras, Greece
x Also at Institute of Physics, Academia Sinica, Taipei, Taiwan
y Also at LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France
z Also at Academia Sinica Grid Computing, Institute of Physics, Academia Sinica, Taipei, Taiwan
aa Also at School of Physics, Shandong University, Shandong, China
ab Also at Moscow Institute of Physics and Technology State University, Dolgoprudny, Russia
ac Also at Section de Physique, Université de Genève, Geneva, Switzerland
ad Also at International School for Advanced Studies (SISSA), Trieste, Italy
ae Also at Department of Physics and Astronomy, University of South Carolina, Columbia SC, United States of America
af Also at School of Physics and Engineering, Sun Yat-sen University, Guangzhou, China
ag Also at Faculty of Physics, M.V.Lomonosov Moscow State University, Moscow, Russia
ah Also at National Research Nuclear University MEPhI, Moscow, Russia
ai Also at Department of Physics, Stanford University, Stanford CA, United States of America
aj Also at Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Budapest, Hungary
ak Also at Department of Physics, The University of Michigan, Ann Arbor MI, United States of America
al Also at Discipline of Physics, University of KwaZulu-Natal, Durban, South Africa
am Also at University of Malaya, Department of Physics, Kuala Lumpur, Malaysia
∗ Deceased