Search for the Standard Model Higgs boson decay to $\mu^{+}\mu^{-}$ with the ATLAS detector

EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH (CERN)

CERN-PH-EP-2014-131

Submitted to: Physics Letters B

Search for the Standard Model Higgs boson decay to µ

+

µ

−

with

the ATLAS detector

The ATLAS Collaboration

Abstract

A search is reported for Higgs boson decay to µ

+

µ

−

_{using data with an integrated luminosity of}

24.8 fb

−1

collected with the ATLAS detector in pp collisions at

√

s

=7 and 8 TeV at the CERN Large

Hadron Collider. The observed dimuon invariant mass distribution is consistent with the Standard

Model background-only hypothesis in the 120–150 GeV search range. For a Higgs boson with a mass

of 125.5 GeV, the observed (expected) upper limit at the 95% confidence level is 7.0 (7.2) times the

Standard Model expectation. This corresponds to an upper limit on the branching ratio BR(H → µ

+

µ

−

)

of 1.5 × 10

−3

_.

c

2014 CERN for the benefit of the ATLAS Collaboration.

Search for the Standard Model Higgs boson decay to µ

+

µ

−

with the ATLAS

detector

Abstract

A search is reported for Higgs boson decay to µ+µ−_{using data with an integrated luminosity of 24.8 fb}−1_collected

with the ATLAS detector in pp collisions at √s =7 and 8 TeV at the CERN Large Hadron Collider. The observed dimuon invariant mass distribution is consistent with the Standard Model background-only hypothesis in the 120– 150 GeV search range. For a Higgs boson with a mass of 125.5 GeV, the observed (expected) upper limit at the 95% confidence level is 7.0 (7.2) times the Standard Model expectation. This corresponds to an upper limit on the branching ratio BR(H → µ+µ−) of 1.5 × 10−3.

1. Introduction

The Standard Model (SM) describes a wide range of particle physics phenomena to a high degree of pre-cision. In the SM, the Brout–Englert–Higgs (BEH) mechanism [1–3] spontaneously breaks the electroweak (EW) gauge symmetry and generates masses for the W and Z gauge bosons as well as for the charged fermions via Yukawa couplings [4–6]. In searches for the Higgs boson predicted by the BEH mechanism, the ATLAS and CMS collaborations have discovered a new parti-cle, via decays into gauge bosons [7, 8], with a mass of approximately 125.5 GeV and measured properties consistent with those predicted by the SM [9–12].

Higgs boson decays to b¯b, τ+τ− _{and µ}+_µ− _{can be}

measured at the LHC with their SM branching ratios proportional to the squares of the fermion masses. The SM branching ratio for the H → µ+µ−decay is 21.9 × 10−5for a Higgs boson mass (mH) of 125 GeV [13, 14].

The H → µ+µ− decay has a clean final state signa-ture that allows a measurement of the Higgs boson cou-pling to second-generation fermions. The dominant ir-reducible background is the Z/γ∗ _{→ µ}+_µ− _process,

which has an approximately three orders of magnitude higher production rate compared to that of the expected signal.

In this Letter a search for the H → µ+µ− _{decay of}

the SM Higgs boson is presented. This search for the presence of a narrow H → µ+µ− _{resonance, with a}

signal width determined by experimental resolution, is performed by fitting the invariant mass distribution in the 110–160 GeV region. This range allows determin-ing background shape and normalisation and settdetermin-ing a

limit on the dimuon decay of the SM Higgs boson with a mass of 125.5 GeV. Section 2 gives a description of the experimental setup and summarises the data sam-ple and Monte Carlo (MC) simulation samsam-ples used to model the signal process and to develop an analytical model for the background processes. Sections 3 and 4 describe the event selections and categorisation. Ana-lytical models used to describe invariant mass distribu-tions for signal and background processes are discussed in Section 5, and systematic uncertainties are detailed in Section 6. The results are presented in Section 7.

2. Experimental setup, data and simulated samples This search is performed on the data sample recorded in 2011 and 2012 by the ATLAS detector in pp col-lisions at the LHC at √s =7 and 8 TeV, respectively. ATLAS [15] is a general-purpose particle detector with a cylindrical geometry and consists of several subdetec-tors surrounding the interaction point and covering al-most the full solid angle.1_{The trajectories and momenta}

of charged particles are measured within the pseudo-rapidity range of |η| < 2.5 by multi-layer silicon pixel and microstrip detectors as well as a transition radia-tion tracker. The tracking system is immersed in a 2 T magnetic field produced by a superconducting solenoid,

1_{ATLAS uses a right-handed coordinate system with its origin at} the nominal interaction point (IP) in the centre of the detector and the z-axis along the beam pipe. The x-axis points from the IP to the centre of the LHC ring, and the y-axis points upward. Cylindrical co-ordinates (r, φ) are used in the transverse plane, φ being the azimuthal angle around the beam pipe. The pseudorapidity is defined in terms of the polar angle θ as η= − ln tan(θ/2).

and is surrounded by a high-granularity liquid-argon (LAr) electromagnetic sampling calorimeter covering |η| < 3.2. An iron and scintillator tile hadronic calorime-ter provides coverage in the range |η| < 1.7. The LAr calorimeters also provide measurements of elec-tromagnetic and hadronic energy deposits in the region 1.5 < |η| < 4.9. The muon spectrometer surrounds the calorimeters and consists of three large air-core super-conducting magnets with a torodial field of 0.5 T in the barrel region and 1 T in the forward regions, and a sys-tem of precision tracking chambers; it provides cover-age for |η| < 2.7. The muon spectrometer also includes fast detectors for triggering covering |η| < 2.4.

Events were recorded with a trigger [16] requiring at least one muon candidate with transverse momen-tum pT > 18 GeV for 7 TeV data and pT > 24 GeV

for 8 TeV data. This trigger is approximately 70% ef-ficient for muons with |η| < 1.05 and approximately 90% efficient for muons with |η| > 1.05. The differ-ences in the efficiency are mostly due to the different geometrical acceptance of the muon trigger system in these regions. For 8 TeV data, events were also recorded with a dimuon trigger requiring at least two muon can-didates with transverse momenta of pT > 18 GeV and

pT > 8 GeV. After applying data quality requirements,

the total integrated luminosity of the selected data sam-ple is 4.5 ± 0.1 fb−1for 7 TeV data and 20.3 ± 0.6 fb−1 for 8 TeV data. The associated systematic uncertainties are summarised in Section 6.

At the LHC, SM Higgs boson production is domi-nated by the gluon fusion (ggF) process with the next two most important contributions arising from the vec-tor boson fusion (VBF) process and production in asso-ciation with vector bosons (VH). The signal MC sam-ples are generated in 5 GeV steps of the Higgs boson mass from 120 GeV to 150 GeV. The ggF and VBF samples are generated at next-to-leading-order (NLO) in QCD with Powheg [17, 18] with the parton shower-ing modelled by Pythia8 [19] for the 8 TeV samples and Pythia [20] for the 7 TeV samples. The CT10 [21] par-ton distribution functions (PDFs) are used in Powheg, with the ATLAS Underlying Event Tune, AU2 [22]. The ggF Higgs boson pTspectrum in Powheg is tuned to

agree with the prediction from HRES [23, 24]; this pro-cedure shifts the Higgs boson pT spectrum to slightly

smaller values. The VH samples are generated with Pythia8, using AU2 and the CTEQ6 [25] PDFs.

The predicted SM Higgs boson cross-sections and branching ratios are compiled in Refs. [13, 14, 26]. The cross section for the ggF process is calculated at next-to-next-to-leading-order (NNLO) [27–32] in QCD and NLO electroweak (EW) corrections are applied [33, 34],

assuming that the QCD and EW corrections factorise. The cross section for the VBF process is calculated with full NLO QCD and EW corrections [35–37] and ap-proximate NNLO QCD corrections [38]. The cross sec-tion for the VH process is calculated at NNLO [39, 40] in QCD, and NLO EW radiative corrections [41] are ap-plied. The branching ratios for H → µ+µ−decays as a function of mHare calculated using Hdecay [42].

The following MC event generators are used to simu-late background processes: Alpgen [43]+Herwig [44] for W+jets, MC@NLO [45]+Herwig for t¯t, tW and tb, AcerMC [46]+Pythia for tqb, Powheg+Pythia8 for Z/γ∗_{and q ¯q → WW, gg2WW [47]+Herwig for gg →}

WW, Powheg [48]+Pythia for WZ and ZZ and Mad-Graph [49, 50]+Pythia for Wγ∗_{. WW, WZ, ZZ and}

Wγ∗ _{production are referred to as diboson production}

later in the text. In addition, contributions from W boson production in association with one or more jets (W+jets), where one of the jets is misidentified as a muon, are estimated using a data control region contain-ing same-sign dimuon events as described in Ref. [9].

The signal and background MC samples are pro-cessed through the ATLAS detector simulation [51] based on Geant4 [52], followed by the same reconstruc-tion algorithms that are used for collision data. The effects arising from multiple collisions in the same or neighbouring bunch crossings (pile-up) are included in the MC simulation, matching the pile-up conditions of the selected data sample.

3. Event selection

Events are required to contain at least one recon-structed pp collision vertex candidate with at least three associated tracks each with pT > 0.4 GeV. The vertex

with the largest sum of p2

Tof tracks is considered to be

the primary vertex. Muon candidates are reconstructed by matching tracks in the inner detector to tracks re-constructed in the muon spectrometer. In addition to stringent track quality requirements imposed for muon identification, the muon tracks must be consistent with having originated from the primary vertex. All selected muon candidates are required to be within |η| < 2.5. Muon candidates must pass track and calorimeter iso-lation requirements that scale with the pT of the muon

track. The isolation is calculated as the scalar sum of the pT of additional tracks or the ETof calorimeter energy

deposits within cone of radius∆R = p(∆φ)2+ (∆η2₎=

0.3 around the muon track, normalised by pµ_T. For 8 TeV data, each muon with pµ_T > 20 (15) GeV is re-quired to have a normalised track isolation smaller than

0.12 (0.08) and a normalised calorimetric isolation less than 0.30 (0.18). For 7 TeV data, equivalent values for pµ_T > 15 GeV are 0.15 and 0.2 for track and calorimetric isolation, respectively. Due to different pile-up condi-tions, different isolation criteria are used for 7 TeV and 8 TeV data.

Jets are reconstructed from clusters of calorimeter cells using the anti-kt algorithm [53, 54] with a

ra-dius parameter of 0.4. The selected jets must satisfy ET > 25 GeV for |η| < 2.4 and ET > 30 GeV for

2.4 ≤ |η| < 4.5. Muon candidates overlapping with the selected jets within a cone of radius∆R = 0.4 are re-moved from the analysis. In the pseudorapidity range |η| < 2.5, jets originating from b-quarks are identi-fied using a b-tagging algorithm [55, 56] with an e ffi-ciency of approximately 80%, determined from t¯t MC events, and with a misidentification rate for selecting light-quark or gluon jets of less than 1%. The missing transverse momentum [57], Emiss

T , is the magnitude of

the vector sum of the pTof muons, electrons, photons,

jets and clusters of calorimeter cells with |η| < 4.9 not associated with these objects.

Corrections are applied to simulated MC samples in order to account for differences between data and MC simulation for the trigger and identification e ffi-ciency and for the muon momentum scale and resolu-tion. The trigger and reconstruction efficiency correc-tions are measured using Z → µ+µ− _{events and are}

found to be within 2% of unity. The muon momen-tum corrections are determined by comparing the recon-structed invariant mass distribution of Z → µ+µ−events in data with that from simulated events; these correc-tions are within 0.1% of unity.

H → µ+µ− candidate events are selected by requir-ing exactly two oppositely charged muons with trans-verse momentum pµ1

T > 25 GeV and p µ2

T > 15 GeV

for the leading and subleading muon, respectively. Se-lected events must contain at least one muon identified by the trigger system within a cone of radius∆R = 0.15 centred on the reconstructed muon candidate. The dom-inant background in this search is Z/γ∗→µ+µ− produc-tion, followed by smaller backgrounds from single and pair production of top quarks and diboson processes. To suppress backgrounds from top quark pair produc-tion and diboson processes, events are required to have Emiss_T < 80 GeV. The dimuon invariant mass distribu-tion mµ+_µ−and the dimuon transverse momentum pµ

+_µ−

T

for data and MC events passing all the selection require-ments so far are shown in Fig. 1. The number of ex-pected signal events for mH = 125 GeV, the expected

background contributions, and the number of observed

data events in the mµ+µ−region from 122.5 to 127.5 GeV are shown in Table 1. The MC background yields are given to illustrate the expected background composi-tion. The selection efficiency times acceptance for sig-nal events with mH= 125 GeV after all selection criteria

described thus far is approximately 55%.

[GeV] -µ + µ m 80 100 120 140 160 180 200 220 240 260 Events / 2 GeV -1 10 1 10 2 10 3 10 4 10 5 10 6 10 7 10 8 10 9 10 10 10 ATLAS -1 Ldt = 24.8 fb ∫ = 8 TeV s = 7 TeV s -µ + µ → H Data MC (stat) * γ Z/ WZ/ZZ/Wγ t t WW

Single Top W+jet

H [125 GeV] [GeV] -µ + µ T p 0 20 40 60 80 100 120 140 160 Events / 5 GeV -1 10 1 10 2 10 3 10 4 10 5 10 6 10 7 10 8 10 9 10 10 10 ATLAS -1 Ldt = 24.8 fb ∫ = 8 TeV s = 7 TeV s -µ + µ → H Data MC (stat) * γ Z/ WZ/ZZ/Wγ t t WW

Single Top W+jet

H [125 GeV]

Figure 1: The distribution of the dimuon invariant mass (top) and dimuon momentum (bottom) for 7 TeV and 8 TeV data with all the selection requirements described in Section 3. The expected signal is shown for mH= 125 GeV.

The expected background processes produce smooth mµ+µ− distributions in the search window, allowing the total background normalisation and shape in each cat-egory to be derived from fitting the data as described in Section 5. The mµ+µ− distribution is examined in the range 110–160 GeV. This range is larger than the 120–150 GeV search window in order to account for signal resolution effects and to allow sufficient side-bands for background normalisation.

4. Event categorisation

To increase sensitivity to the Higgs boson signal, the selected events are separated into seven mutually ex-clusive categories with different signal-to-background ratios based on their muon pseudorapidity (ηµ), pµ_T+µ−, and VBF dijet signature. Events produced in the VBF

Table 1: Number of expected signal events for mH= 125 GeV, num-ber of expected background events from MC simulation, and numnum-ber of observed data events within a window of |mH− mµ+µ−| ≤ 2.5 GeV after all selection criteria are applied. Only statistical uncertainties are given. The theoretical systematic uncertainty on the dominant Z/γ∗ background is about 4%. The MC background yields are given to illustrate the expected background composition.

7 TeV 8 TeV Signal (125 GeV) 5.6 ± 0.1 32.7 ± 0.2 Z/γ∗ 3110 ± 40 16660 ± 270 WZ/ZZ/Wγ 2.2 ± 0.2 12.3 ± 0.7 t¯t 75.6 ± 1.8 509.2 ± 2.7 WW 23.2 ± 0.5 123.3 ± 1.6 Single top 7.2 ± 0.9 54.5 ± 0.6 W+jets 3.2 ± 1.5 38 ± 4 Total Bkg. 3220 ± 40 17390 ± 270 Observed 3344 17745

process are characterised by two forward jets with lit-tle hadronic activity between them. The VBF category is thus defined by requiring the events to have at least two jets with an invariant mass greater than 500 GeV, |ηjet₁−ηjet₂| > 3 and ηjet₁ ×ηjet₂ < 0. In events with

more than two jets, those with the highest pT are used

in the selection. Events with at least one jet identified as originating from a b-quark are excluded from the VBF category.

The events that are not selected for the VBF category are classified using pµ+µ

−

T . Signal events have on

av-erage larger values of pµ_T+µ− than the Z/γ∗ _background

events. Therefore, the remaining events are separated into three pµ_T+µ− categories: low (< 15 GeV), medium (15–50 GeV) and high (> 50 GeV). To further improve the search sensitivity, each of these three categories is also subdivided into a central category with |ηµ1| < 1 and |ηµ2| < 1 and a non-central category containing all remaining events. This value for the ηµ boundary has been chosen by scanning a range of ηµvalues and select-ing a value with the highest signal sensitivity. The muon momentum measurement for the central muons is more precise, producing a narrower mµ+µ−distribution for sig-nal events in the central category and thus resulting in a higher overall signal sensitivity. Table 2 shows the signal event yields, NS/

√

NBratios, approximate signal

width and results of the fits to the data, described in Sec-tion 5, for all analysis categories.

5. Signal and background models

Analytical models are used to describe the mµ+µ− dis-tributions for signal and background processes. The

Table 2: Expected signal yields (NS) for mH= 125 GeV and the ratio NS/

√

NBusing the simulated MC background yields (NB) within a window of |mH− mµ+µ−| ≤ 2.5 GeV for each of the event categories under study. In addition, the full width at half maximum (FWHM) of the signal mµ+µ−distribution, modelled as described in Section 5, is given. Also shown are χ2_{/ndof of the fits to the m}

µ+µ−distribution described in Section 5. √ s Category NS NS √ NB FWHM χ 2_/ndof [TeV] [GeV] 8 non-cen. low pµ_T+µ− 6.1 0.07 6.6 49.8/48 8 cen. low pµT+µ− 2.6 0.06 5.5 52.8/48 8 non-cen. medium pµ_T+µ− 10.4 0.15 6.6 45.1/48 8 cen. medium pµ+µ − T 4.7 0.13 5.6 36.7/48 8 non-cen. high pµT+µ− 5.5 0.13 7.2 26.7/48 8 cen. high pµ_T+µ− 2.6 0.10 6.0 32.3/48 8 VBF 0.8 0.09 7.0 18.6/19 7 non-cen. low pµT+µ− 1.0 0.03 6.8 42.0/48 7 cen. low pµ_T+µ− 0.5 0.03 5.3 43.5/48 7 non-cen. medium pµ_T+µ− 1.8 0.06 6.9 41.2/48 7 cen. medium pµT+µ− 0.8 0.05 5.5 34.4/48 7 non-cen. high pµ_T+µ− 0.9 0.05 7.5 60.0/48 7 cen. high pµ+µ − T 0.5 0.05 5.9 56.2/48 7 VBF 0.1 0.05 6.9 6.2/19

simulated samples detailed in Section 2 are used to velop background models which are designed to de-scribe essential features of the background mµ+µ− dis-tributions, dominated by Z/γ∗, while having sufficient flexibility to describe different categories and to absorb potential differences between data and MC simulation.

The background model selected for the pµ_T+µ− cate-gories is the sum of a Breit–Wigner (BW) function con-volved with a Gaussian function (GS), and an exponen-tial function divided by x3_:

PB(x)= f · [BW(MBW, ΓBW) ∗ GS(σBGS)](x)

+ (1 − f ) · C · eA·x_/x3_, (1)

where x represents mµ+µ− and f represents the fraction of the BW component when each individual component is normalised to unity. C is an overall normalisation coefficient. The σB

GS parameters in each category are

fixed to the average mµ+µ− resolution in that category as determined from the MC simulation of Z/γ∗_{. The}

background model for the VBF category is the product of a Breit–Wigner and an exponential function:

PB(x)= BW(MBW, ΓBW, x) · eA·x. (2)

For all categories, the BW parameters are fixed to MBW = 91.2 GeV and ΓBW = 2.49 GeV. The

determined from fits to the data, as shown in Fig. 2 for the central medium pµ_T+µ−category. Similar fit quality is observed for all other categories.

mll Entries / GeV 0 20 40 60 80 100 120 140 160 -µ + µ T Central medium p /ndof = 32.4/48 2 χ s = 7 TeV -1 Ldt = 4.5 fb

∫

ATLAS Data Background model 50 × Signal [125] [GeV] -µ + µ m 110 115 120 125 130 135 140 145 150 155 160 Pull -4 -2 0 2 4 mll Entries / GeV 0 100 200 300 400 500 600 700 800 900 -µ + µ T Central medium p /ndof = 36.7/48 2 χ s = 8 TeV -1 Ldt = 20.3 fb

∫

ATLAS Data Background model 50 × Signal [125] [GeV] -µ + µ m 110 115 120 125 130 135 140 145 150 155 160 Pull -4 -2 0 2 4

Figure 2: The background model fits to the mµ+µ−distribution for the central medium pµ_T+µ−category for 7 TeV (top) and 8 TeV (bottom) data. The statistical uncertainties are given for the data points. The expected signal is shown for mH= 125 GeV and is scaled by a factor of 50.

The signal model is obtained from simulated Higgs boson signal samples, where contributions from the ggF, VBF and VH Higgs boson production processes are added together. This model is the sum of a Crystal Ball (CB)2_{and a Gaussian function:}

PS(x)= fCB· CB(x, m, σCB, α, n) + (1 − fCB) · GS  x, m, σS GS , (3)

where x represents mµ+µ−and f_CBrepresents the fraction of the CB contribution when each individual component

2_{A Gaussian function with a power-law tail.}

is normalised to unity. The parameters α and n define the power-law tail of the CB distribution. The parame-ters σCBand σSGS denote the widths of the CB and GS

distributions, respectively. The parameters m, σCB and

σS

GSare determined from the fits to the simulated Higgs

boson samples. In order to improve stability of the fits, the remaining parameters fCB, α and n are fixed to

val-ues determined from empirical tests where a range of possible values have been tested.

Fig. 3 shows how the signal model reproduces the simulation for the medium pµ+µ

−

T category for the

ex-pected signal dimuon mass distributions. Similar fit quality is obtained for all other categories. The signal model parameters are linearly interpolated in steps of 1 GeV between the generated signal samples. These signal model parameters are then fixed in the fit to data.

[GeV] -µ + µ m 105 110 115 120 125 130 135 Events / 0.5 GeV 0 0.2 0.4 0.6 ATLAS Simulation =125 GeV H m CB+Gaussian fit -µ + µ T Central medium p m=124.5 GeV =2.3 GeV CB σ FWHM=5.6 GeV -µ + µ → H = 8 TeV s [GeV] -µ + µ m 105 110 115 120 125 130 135 Events / 0.5 GeV 0 0.5 1 ATLAS Simulation =125 GeV H m CB+Gaussian fit -µ + µ T Non-central medium p m=124.6 GeV =2.7 GeV CB σ FWHM=6.6 GeV -µ + µ → H = 8 TeV s

Figure 3: The signal model fit to the mµ+µ−_{distribution for the} cen-tral (top) and non-cencen-tral (bottom) simulated Higgs boson events for mH= 125 GeV in the medium pµ

+µ−

T category for √

s= 8 TeV.

To derive the results presented in Section 7, a binned maximum likelihood fit to the observed mµ+µ− distribu-tions in the range 110–160 GeV is performed using the sum of the signal and background model. The fit is done simultaneously in all seven categories with sep-arate distributions for 7 TeV and 8 TeV data. In addi-tion to the background model parameters described ear-lier, a background normalisation in each category and the H → µ+µ−_{signal strength µ}

S are free parameters

of the fit, where µSis defined such that µS = 0

corre-sponds to the background-only hypothesis and µS = 1

6. Systematic uncertainties

The main theoretical and experimental sources of un-certainty on the number of expected signal events are shown in Table 3. The uncertainty on the integrated lu-minosity is ±1.8% for 7 TeV data [58] and ±2.8% for 8 TeV data; it is obtained following the same method-ology as that detailed in Ref. [58], from a preliminary calibration of the luminosity scale derived from beam-separation scans performed in November 2012.

Sources of experimental uncertainty include the ef-ficiency of the muon trigger, reconstruction, identifica-tion, and isolation requirements, as well as the muon momentum scale and resolution. Uncertainties on the jet energy scale and resolution affect the selection of jets used in the VBF category definitions. Smaller un-certainties arise from pile-up and the primary vertex se-lection.

The theoretical uncertainties on the production and H → µ+µ−decay of a SM Higgs boson of mass mH =

125 GeV are taken from Refs. [13, 14]. The uncer-tainty on the relative populations of the pµ+µ

−

T categories,

due to the uncertainty on the description of the Higgs boson pT spectrum arising from missing higher-order

corrections, is determined by varying the QCD renor-malisation, factorisation and resummation scales used in the HRES program. To evaluate these uncertain-ties, the scales are independently varied up and down by a factor of two while keeping their ratio between 0.5 and 2.0. The ggF contribution to the VBF category has large uncertainties due to missing higher-order correc-tions; they are estimated using the method described in Ref. [26]. The uncertainties associated with the mod-elling of multi-parton interactions (MPI) are estimated by turning off the MPI modelling in the event genera-tion, according to the recommendations in Ref. [26].

In addition to the samples described in Section 2, samples of the dominant Z/γ∗ background are gener-ated with Powheg+Pythia8 and parameterised with a detector response measured using simulated MC events. These samples contain approximately 170 times more events than expected in the data and are used to val-idate the background models and to derive systematic uncertainties due to potential mismodelling bias. This bias is estimated by fitting the parametrised signal plus background model to the simulated mµ+µ− background distribution in the mass range 110–160 GeV where the signal strength µSis a free parameter. The bias is then

defined as the root mean square of the signal yield ob-tained from the fit for Higgs boson masses in the range 120–150 GeV. This uncertainty varies from 3% to 20% of the statistical uncertainty on the signal strength µS,

depending on the selection category and data-taking pe-riod.

Table 3: Main sources of experimental and theoretical uncertainty on the signal yield, excepting the error from mismodelling bias. “QCD scale” indicates the theoretical uncertainty on the Higgs boson pro-duction due to missing higher-order corrections estimated by varying the QCD renormalisation and factorisation scales, while “PDFs+ αs” indicates uncertainty due to parton distribution functions, as described in Ref. [13, 14]. The ranges for the uncertainties cover the variations among different categories and data-taking periods.

Source (experimental) Uncertainty (%)

Luminosity ±1.8 (7 TeV), ±2.8 (8 TeV) Muon efficiency ±1

Muon momentum res. ±1

Muon trigger ±1.5

Muon isolation ±1.1 Pile-up reweighting ±1 Jet energy scale +3.4_−4.5(VBF) Source (theory) Uncertainty (%)

Higgs boson branching ratio ±7

QCD scale ±8 (ggF), ±1 (VBF, VH) PDFs+ αs ±8 (ggF), ±4 (VBF, VH) ggF uncert. in VBF ±22

Multi-parton inter. in VBF ±9 (ggF), ±4 (VBF)

7. Results and conclusions

The statistical procedure used to interpret the data is summarised in Ref. [7]. The observed data is consis-tent with the expected backgrounds and no evidence for a signal is found. Upper limits are computed on the signal strength µSusing a modified frequentist CLs

method [59, 60] based on a Poisson log-likelihood ratio statistical test.

The observed and expected 95% confidence level (CL) limits on the H → µ+µ−_{signal strength are shown}

in Fig. 4. Table 4 summarises the observed and expected limits for different values of mH. Including the

system-atic uncertainties described in Section 6 changes the ex-pected limit by approximately 2% for mH = 125 GeV.

Table 4: Observed and expected 95% CL upper limits on the H → µ+_µ−_{signal strength µ}

Sfor different values of mH.

mH[GeV] 120 125 130 135 140 145 150 Obs. 9.5 7.1 6.5 8.3 14.7 16.5 16.8 Exp. 6.7 7.2 7.9 9.1 11.3 16.0 26.6

To conclude, a search for Higgs boson decay to µ+µ−

[GeV] H m 120 125 130 135 140 145 150 S µ 95% CL limit on 0 10 20 30 40 50 Observed CL Expected CL σ 1 ± σ 2 ± ATLAS _{H →µ}+_µ --1 =7 TeV 4.5 fb s -1 =8 TeV 20.3 fb s

Figure 4: Observed (solid) and expected (dashed) 95% CL upper lim-its on the H → µ+µ−_{signal strength as a function of m}

Hover the mass range 120–150 GeV. The dark- and light-shaded regions indicate the ±1σ and ±2σ uncertainty bands on the expected limit, respectively.

LHC has been performed with the ATLAS experiment. The observed data is consistent with the expected back-grounds. No evidence for a signal is observed and upper limits are set on the signal strength as a function of the Higgs boson mass. For a SM Higgs boson with a mass of 125.5 GeV, the observed (expected) limit on the sig-nal strength µSat the 95% CL is 7.0 (7.2) times the SM

prediction. Assuming a Higgs boson mass of 125.5 GeV and the SM production cross section, which is allowed to vary within its uncertainty, the 95% CL upper limit on the H → µ+µ−_{branching ratio is 1.5 × 10}−3_.

Acknowledgements

We thank CERN for the very successful operation of the LHC, as well as the support staff from our institu-tions without whom ATLAS could not be operated e ffi-ciently.

We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF 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; ISF, MINERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Nether-lands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Roma-nia; MES of Russia and ROSATOM, Russian

Federa-tion; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZ ˇS, 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 Soci-ety and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America.

The crucial computing support from all WLCG part-ners 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 (Tai-wan), RAL (UK) and BNL (USA) and in the Tier-2 fa-cilities worldwide.

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The ATLAS Collaboration

G. Aad84_{, B. Abbott}112_{, J. Abdallah}152_{, S. Abdel Khalek}116_{, O. Abdinov}11_{, R. Aben}106_{, B. Abi}113_{, M. Abolins}89_,

O.S. AbouZeid159_{, H. Abramowicz}154_{, H. Abreu}153_{, R. Abreu}30_{, Y. Abulaiti}147a,147b_{, B.S. Acharya}165a,165b,a_,

L. Adamczyk38a_{, D.L. Adams}25_{, J. Adelman}177_{, S. Adomeit}99_{, T. Adye}130_{, T. Agatonovic-Jovin}13a_,

J.A. Aguilar-Saavedra125a,125f_{, M. Agustoni}17_{, S.P. Ahlen}22_{, F. Ahmadov}64,b_{, G. Aielli}134a,134b_{, H. Akerstedt}147a,147b_,

T.P.A. Åkesson80_{, G. Akimoto}156_{, A.V. Akimov}95_{, G.L. Alberghi}20a,20b_{, J. Albert}170_{, S. Albrand}55_,

M.J. Alconada Verzini70_{, M. Aleksa}30_{, I.N. Aleksandrov}64_{, C. Alexa}26a_{, G. Alexander}154_{, G. Alexandre}49_,

T. Alexopoulos10, M. Alhroob165a,165c, G. Alimonti90a, L. Alio84, J. Alison31, B.M.M. Allbrooke18, L.J. Allison71, P.P. Allport73, J. Almond83, A. Aloisio103a,103b, A. Alonso36, F. Alonso70, C. Alpigiani75, A. Altheimer35,

B. Alvarez Gonzalez89, M.G. Alviggi103a,103b, K. Amako65, Y. Amaral Coutinho24a, C. Amelung23, D. Amidei88, S.P. Amor Dos Santos125a,125c, A. Amorim125a,125b, S. Amoroso48, N. Amram154, G. Amundsen23,

C. Anastopoulos140, L.S. Ancu49, N. Andari30, T. Andeen35, C.F. Anders58b, G. Anders30, K.J. Anderson31, A. Andreazza90a,90b, V. Andrei58a, X.S. Anduaga70, S. Angelidakis9, I. Angelozzi106, P. Anger44, A. Angerami35, F. Anghinolfi30_{, A.V. Anisenkov}108_{, N. Anjos}125a_{, A. Annovi}47_{, A. Antonaki}9_{, M. Antonelli}47_{, A. Antonov}97_,

J. Antos145b_{, F. Anulli}133a_{, M. Aoki}65_{, L. Aperio Bella}18_{, R. Apolle}119,c_{, G. Arabidze}89_{, I. Aracena}144_{, Y. Arai}65_,

J.P. Araque125a_{, A.T.H. Arce}45_{, J-F. Arguin}94_{, S. Argyropoulos}42_{, M. Arik}19a_{, A.J. Armbruster}30_{, O. Arnaez}30_,

V. Arnal81_{, H. Arnold}48_{, M. Arratia}28_{, O. Arslan}21_{, A. Artamonov}96_{, G. Artoni}23_{, S. Asai}156_{, N. Asbah}42_,

A. Ashkenazi154_{, B. Åsman}147a,147b_{, L. Asquith}6_{, K. Assamagan}25_{, R. Astalos}145a_{, M. Atkinson}166_{, N.B. Atlay}142_,

B. Auerbach6_{, K. Augsten}127_{, M. Aurousseau}146b_{, G. Avolio}30_{, G. Azuelos}94,d_{, Y. Azuma}156_{, M.A. Baak}30_,

A. Baas58a_{, C. Bacci}135a,135b_{, H. Bachacou}137_{, K. Bachas}155_{, M. Backes}30_{, M. Backhaus}30_{, J. Backus Mayes}144_,

E. Badescu26a_{, P. Bagiacchi}133a,133b_{, P. Bagnaia}133a,133b_{, Y. Bai}33a_{, T. Bain}35_{, J.T. Baines}130_{, O.K. Baker}177_,

P. Balek128_{, F. Balli}137_{, E. Banas}39_{, Sw. Banerjee}174_{, A.A.E. Bannoura}176_{, V. Bansal}170_{, H.S. Bansil}18_{, L. Barak}173_,

S.P. Baranov95, E.L. Barberio87, D. Barberis50a,50b, M. Barbero84, T. Barillari100, M. Barisonzi176, T. Barklow144, N. Barlow28, B.M. Barnett130, R.M. Barnett15, Z. Barnovska5, A. Baroncelli135a, G. Barone49, A.J. Barr119, F. Barreiro81, J. Barreiro Guimar˜aes da Costa57, R. Bartoldus144, A.E. Barton71, P. Bartos145a, V. Bartsch150, A. Bassalat116, A. Basye166, R.L. Bates53, J.R. Batley28, M. Battaglia138, M. Battistin30, F. Bauer137, H.S. Bawa144,e, M.D. Beattie71, T. Beau79, P.H. Beauchemin162, R. Beccherle123a,123b, P. Bechtle21, H.P. Beck17, K. Becker176, S. Becker99, M. Beckingham171, C. Becot116, A.J. Beddall19c, A. Beddall19c, S. Bedikian177, V.A. Bednyakov64, C.P. Bee149_{, L.J. Beemster}106_{, T.A. Beermann}176_{, M. Begel}25_{, K. Behr}119_{, C. Belanger-Champagne}86_{, P.J. Bell}49_,

W.H. Bell49_{, G. Bella}154_{, L. Bellagamba}20a_{, A. Bellerive}29_{, M. Bellomo}85_{, K. Belotskiy}97_{, O. Beltramello}30_,

O. Benary154_{, D. Benchekroun}136a_{, K. Bendtz}147a,147b_{, N. Benekos}166_{, Y. Benhammou}154_{, E. Benhar Noccioli}49_,

J.A. Benitez Garcia160b_{, D.P. Benjamin}45_{, J.R. Bensinger}23_{, K. Benslama}131_{, S. Bentvelsen}106_{, D. Berge}106_,

E. Bergeaas Kuutmann16_{, N. Berger}5_{, F. Berghaus}170_{, J. Beringer}15_{, C. Bernard}22_{, P. Bernat}77_{, C. Bernius}78_,

F.U. Bernlochner170_{, T. Berry}76_{, P. Berta}128_{, C. Bertella}84_{, G. Bertoli}147a,147b_{, F. Bertolucci}123a,123b_{, C. Bertsche}112_,

D. Bertsche112_{, M.I. Besana}90a_{, G.J. Besjes}105_{, O. Bessidskaia}147a,147b_{, M.F. Bessner}42_{, N. Besson}137_,

C. Betancourt48_{, S. Bethke}100_{, W. Bhimji}46_{, R.M. Bianchi}124_{, L. Bianchini}23_{, M. Bianco}30_{, O. Biebel}99_,

S.P. Bieniek77, K. Bierwagen54, J. Biesiada15, M. Biglietti135a, J. Bilbao De Mendizabal49, H. Bilokon47, M. Bindi54, S. Binet116, A. Bingul19c, C. Bini133a,133b, C.W. Black151, J.E. Black144, K.M. Black22, D. Blackburn139, R.E. Blair6, J.-B. Blanchard137, T. Blazek145a, I. Bloch42, C. Blocker23, W. Blum82,∗, U. Blumenschein54, G.J. Bobbink106, V.S. Bobrovnikov108, S.S. Bocchetta80, A. Bocci45, C. Bock99, C.R. Boddy119, M. Boehler48, T.T. Boek176, J.A. Bogaerts30, A.G. Bogdanchikov108, A. Bogouch91,∗, C. Bohm147a, J. Bohm126, V. Boisvert76, T. Bold38a, V. Boldea26a, A.S. Boldyrev98, M. Bomben79, M. Bona75, M. Boonekamp137, A. Borisov129, G. Borissov71, M. Borri83_{, S. Borroni}42_{, J. Bortfeldt}99_{, V. Bortolotto}135a,135b_{, K. Bos}106_{, D. Boscherini}20a_{, M. Bosman}12_,

H. Boterenbrood106_{, J. Boudreau}124_{, J. Bouffard}2_{, E.V. Bouhova-Thacker}71_{, D. Boumediene}34_{, C. Bourdarios}116_,

N. Bousson113_{, S. Boutouil}136d_{, A. Boveia}31_{, J. Boyd}30_{, I.R. Boyko}64_{, J. Bracinik}18_{, A. Brandt}8_{, G. Brandt}15_,

O. Brandt58a_{, U. Bratzler}157_{, B. Brau}85_{, J.E. Brau}115_{, H.M. Braun}176,∗_{, S.F. Brazzale}165a,165c_{, B. Brelier}159_,

K. Brendlinger121_{, A.J. Brennan}87_{, R. Brenner}167_{, S. Bressler}173_{, K. Bristow}146c_{, T.M. Bristow}46_{, D. Britton}53_,

F.M. Brochu28_{, I. Brock}21_{, R. Brock}89_{, C. Bromberg}89_{, J. Bronner}100_{, G. Brooijmans}35_{, T. Brooks}76_{, W.K. Brooks}32b_,

J. Brosamer15_{, E. Brost}115_{, J. Brown}55_{, P.A. Bruckman de Renstrom}39_{, D. Bruncko}145b_{, R. Bruneliere}48_{, S. Brunet}60_,

A. Bruni20a_{, G. Bruni}20a_{, M. Bruschi}20a_{, L. Bryngemark}80_{, T. Buanes}14_{, Q. Buat}143_{, F. Bucci}49_{, P. Buchholz}142_,

O. Bulekov97_{, A.C. Bundock}73_{, H. Burckhart}30_{, S. Burdin}73_{, B. Burghgrave}107_{, S. Burke}130_{, I. Burmeister}43_,

E. Busato34_{, D. B¨uscher}48_{, V. B¨uscher}82_{, P. Bussey}53_{, C.P. Buszello}167_{, B. Butler}57_{, J.M. Butler}22_{, A.I. Butt}3_,

C.M. Buttar53_{, J.M. Butterworth}77_{, P. Butti}106_{, W. Buttinger}28_{, A. Buzatu}53_{, M. Byszewski}10_{, S. Cabrera Urb´an}168_,

D. Caforio20a,20b_{, O. Cakir}4a_{, P. Calafiura}15_{, A. Calandri}137_{, G. Calderini}79_{, P. Calfayan}99_{, R. Calkins}107_,

L.P. Caloba24a_{, D. Calvet}34_{, S. Calvet}34_{, R. Camacho Toro}49_{, S. Camarda}42_{, D. Cameron}118_{, L.M. Caminada}15_,

R. Caminal Armadans12_{, S. Campana}30_{, M. Campanelli}77_{, A. Campoverde}149_{, V. Canale}103a,103b_{, A. Canepa}160a_,

M. Cano Bret75_{, J. Cantero}81_{, R. Cantrill}125a_{, T. Cao}40_{, M.D.M. Capeans Garrido}30_{, I. Caprini}26a_{, M. Caprini}26a_,

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M.A. Chelstowska88_{, C. Chen}63_{, H. Chen}25_{, K. Chen}149_{, L. Chen}33d,g_{, S. Chen}33c_{, X. Chen}146c_{, Y. Chen}66_{, Y. Chen}35_,

H.C. Cheng88_{, Y. Cheng}31_{, A. Cheplakov}64_{, R. Cherkaoui El Moursli}136e_{, V. Chernyatin}25,∗_{, E. Cheu}7_,

L. Chevalier137_{, V. Chiarella}47_{, G. Chiefari}103a,103b_{, J.T. Childers}6_{, A. Chilingarov}71_{, G. Chiodini}72a_{, A.S. Chisholm}18_,

R.T. Chislett77_{, A. Chitan}26a_{, M.V. Chizhov}64_{, S. Chouridou}9_{, B.K.B. Chow}99_{, D. Chromek-Burckhart}30_,

M.L. Chu152_{, J. Chudoba}126_{, J.J. Chwastowski}39_{, L. Chytka}114_{, G. Ciapetti}133a,133b_{, A.K. Ciftci}4a_{, R. Ciftci}4a_,

D. Cinca53_{, V. Cindro}74_{, A. Ciocio}15_{, P. Cirkovic}13b_{, Z.H. Citron}173_{, M. Citterio}90a_{, M. Ciubancan}26a_{, A. Clark}49_,

P.J. Clark46_{, R.N. Clarke}15_{, W. Cleland}124_{, J.C. Clemens}84_{, C. Clement}147a,147b_{, Y. Coadou}84_{, M. Cobal}165a,165c_,

A. Coccaro139_{, J. Cochran}63_{, L. Coffey}23_{, J.G. Cogan}144_{, J. Coggeshall}166_{, B. Cole}35_{, S. Cole}107_{, A.P. Colijn}106_,

J. Collot55, T. Colombo58c, G. Colon85, G. Compostella100, P. Conde Mui˜no125a,125b, E. Coniavitis48, M.C. Conidi12, S.H. Connell146b, I.A. Connelly76, S.M. Consonni90a,90b, V. Consorti48, S. Constantinescu26a, C. Conta120a,120b, G. Conti57, F. Conventi103a,h, M. Cooke15, B.D. Cooper77, A.M. Cooper-Sarkar119, N.J. Cooper-Smith76, K. Copic15, T. Cornelissen176, M. Corradi20a, F. Corriveau86,i, A. Corso-Radu164, A. Cortes-Gonzalez12, G. Cortiana100,

G. Costa90a, M.J. Costa168, D. Costanzo140, D. Cˆot´e8, G. Cottin28, G. Cowan76, B.E. Cox83, K. Cranmer109, G. Cree29, S. Cr´ep´e-Renaudin55, F. Crescioli79, W.A. Cribbs147a,147b, M. Crispin Ortuzar119, M. Cristinziani21, V. Croft105_{, G. Crosetti}37a,37b_{, C.-M. Cuciuc}26a_{, T. Cuhadar Donszelmann}140_{, J. Cummings}177_{, M. Curatolo}47_,

C. Cuthbert151_{, H. Czirr}142_{, P. Czodrowski}3_{, Z. Czyczula}177_{, S. D’Auria}53_{, M. D’Onofrio}73_,

M.J. Da Cunha Sargedas De Sousa125a,125b_{, C. Da Via}83_{, W. Dabrowski}38a_{, A. Dafinca}119_{, T. Dai}88_{, O. Dale}14_,

F. Dallaire94_{, C. Dallapiccola}85_{, M. Dam}36_{, A.C. Daniells}18_{, M. Dano Hoffmann}137_{, V. Dao}48_{, G. Darbo}50a_,

S. Darmora8_{, J.A. Dassoulas}42_{, A. Dattagupta}60_{, W. Davey}21_{, C. David}170_{, T. Davidek}128_{, E. Davies}119,c_,

M. Davies154_{, O. Davignon}79_{, A.R. Davison}77_{, P. Davison}77_{, Y. Davygora}58a_{, E. Dawe}143_{, I. Dawson}140_,

R.K. Daya-Ishmukhametova85_{, K. De}8_{, R. de Asmundis}103a_{, S. De Castro}20a,20b_{, S. De Cecco}79_{, N. De Groot}105_,

P. de Jong106_{, H. De la Torre}81_{, F. De Lorenzi}63_{, L. De Nooij}106_{, D. De Pedis}133a_{, A. De Salvo}133a_,

U. De Sanctis165a,165b, A. De Santo150, J.B. De Vivie De Regie116, W.J. Dearnaley71, R. Debbe25, C. Debenedetti138, B. Dechenaux55, D.V. Dedovich64, I. Deigaard106, J. Del Peso81, T. Del Prete123a,123b, F. Deliot137, C.M. Delitzsch49, M. Deliyergiyev74, A. Dell’Acqua30, L. Dell’Asta22, M. Dell’Orso123a,123b, M. Della Pietra103a,h, D. della Volpe49, M. Delmastro5, P.A. Delsart55, C. Deluca106, S. Demers177, M. Demichev64, A. Demilly79, S.P. Denisov129, D. Derendarz39, J.E. Derkaoui136d, F. Derue79, P. Dervan73, K. Desch21, C. Deterre42, P.O. Deviveiros106,

A. Dewhurst130, S. Dhaliwal106, A. Di Ciaccio134a,134b, L. Di Ciaccio5, A. Di Domenico133a,133b, C. Di Donato103a,103b, A. Di Girolamo30_{, B. Di Girolamo}30_{, A. Di Mattia}153_{, B. Di Micco}135a,135b_{, R. Di Nardo}47_{, A. Di Simone}48_,

R. Di Sipio20a,20b_{, D. Di Valentino}29_{, F.A. Dias}46_{, M.A. Diaz}32a_{, E.B. Diehl}88_{, J. Dietrich}42_{, T.A. Dietzsch}58a_,

S. Diglio84_{, A. Dimitrievska}13a_{, J. Dingfelder}21_{, C. Dionisi}133a,133b_{, P. Dita}26a_{, S. Dita}26a_{, F. Dittus}30_{, F. Djama}84_,

T. Djobava51b_{, M.A.B. do Vale}24c_{, A. Do Valle Wemans}125a,125g_{, T.K.O. Doan}5_{, D. Dobos}30_{, C. Doglioni}49_,

T. Doherty53_{, T. Dohmae}156_{, J. Dolejsi}128_{, Z. Dolezal}128_{, B.A. Dolgoshein}97,∗_{, M. Donadelli}24d_{, S. Donati}123a,123b_,

P. Dondero120a,120b_{, J. Donini}34_{, J. Dopke}130_{, A. Doria}103a_{, M.T. Dova}70_{, A.T. Doyle}53_{, M. Dris}10_{, J. Dubbert}88_,

S. Dube15_{, E. Dubreuil}34_{, E. Duchovni}173_{, G. Duckeck}99_{, O.A. Ducu}26a_{, D. Duda}176_{, A. Dudarev}30_{, F. Dudziak}63_,

L. Duflot116_{, L. Duguid}76_{, M. D¨uhrssen}30_{, M. Dunford}58a_{, H. Duran Yildiz}4a_{, M. D¨uren}52_{, A. Durglishvili}51b_,

K. Einsweiler15_{, T. Ekelof}167_{, M. El Kacimi}136c_{, M. Ellert}167_{, S. Elles}5_{, F. Ellinghaus}82_{, N. Ellis}30_{, J. Elmsheuser}99_,

M. Elsing30_{, D. Emeliyanov}130_{, Y. Enari}156_{, O.C. Endner}82_{, M. Endo}117_{, R. Engelmann}149_{, J. Erdmann}177_,

A. Ereditato17_{, D. Eriksson}147a_{, G. Ernis}176_{, J. Ernst}2_{, M. Ernst}25_{, J. Ernwein}137_{, D. Errede}166_{, S. Errede}166_,

E. Ertel82_{, M. Escalier}116_{, H. Esch}43_{, C. Escobar}124_{, B. Esposito}47_{, A.I. Etienvre}137_{, E. Etzion}154_{, H. Evans}60_,

A. Ezhilov122_{, L. Fabbri}20a,20b_{, G. Facini}31_{, R.M. Fakhrutdinov}129_{, S. Falciano}133a_{, R.J. Falla}77_{, J. Faltova}128_,

Y. Fang33a_{, M. Fanti}90a,90b_{, A. Farbin}8_{, A. Farilla}135a_{, T. Farooque}12_{, S. Farrell}15_{, S.M. Farrington}171_{, P. Farthouat}30_,

F. Fassi136e_{, P. Fassnacht}30_{, D. Fassouliotis}9_{, A. Favareto}50a,50b_{, L. Fayard}116_{, P. Federic}145a_{, O.L. Fedin}122, j_,

W. Fedorko169_{, M. Fehling-Kaschek}48_{, S. Feigl}30_{, L. Feligioni}84_{, C. Feng}33d_{, E.J. Feng}6_{, H. Feng}88_{, A.B. Fenyuk}129_,

S. Fernandez Perez30, S. Ferrag53, J. Ferrando53, A. Ferrari167, P. Ferrari106, R. Ferrari120a, D.E. Ferreira de Lima53, A. Ferrer168, D. Ferrere49, C. Ferretti88, A. Ferretto Parodi50a,50b, M. Fiascaris31, F. Fiedler82, A. Filipˇciˇc74,

M. Filipuzzi42, F. Filthaut105, M. Fincke-Keeler170, K.D. Finelli151, M.C.N. Fiolhais125a,125c, L. Fiorini168, A. Firan40, A. Fischer2, J. Fischer176, W.C. Fisher89, E.A. Fitzgerald23, M. Flechl48, I. Fleck142, P. Fleischmann88,

S. Fleischmann176, G.T. Fletcher140, G. Fletcher75, T. Flick176, A. Floderus80, L.R. Flores Castillo174,k, A.C. Florez Bustos160b, M.J. Flowerdew100, A. Formica137, A. Forti83, D. Fortin160a, D. Fournier116, H. Fox71, S. Fracchia12_{, P. Francavilla}79_{, M. Franchini}20a,20b_{, S. Franchino}30_{, D. Francis}30_{, L. Franconi}118_{, M. Franklin}57_,

S. Franz61_{, M. Fraternali}120a,120b_{, S.T. French}28_{, C. Friedrich}42_{, F. Friedrich}44_{, D. Froidevaux}30_{, J.A. Frost}28_,

C. Fukunaga157_{, E. Fullana Torregrosa}82_{, B.G. Fulsom}144_{, J. Fuster}168_{, C. Gabaldon}55_{, O. Gabizon}173_,

A. Gabrielli20a,20b_{, A. Gabrielli}133a,133b_{, S. Gadatsch}106_{, S. Gadomski}49_{, G. Gagliardi}50a,50b_{, P. Gagnon}60_{, C. Galea}105_,

B. Galhardo125a,125c_{, E.J. Gallas}119_{, V. Gallo}17_{, B.J. Gallop}130_{, P. Gallus}127_{, G. Galster}36_{, K.K. Gan}110_{, J. Gao}33b,g_,

Y.S. Gao144,e_{, F.M. Garay Walls}46_{, F. Garberson}177_{, C. Garc´ıa}168_{, J.E. Garc´ıa Navarro}168_{, M. Garcia-Sciveres}15_,

R.W. Gardner31_{, N. Garelli}144_{, V. Garonne}30_{, C. Gatti}47_{, G. Gaudio}120a_{, B. Gaur}142_{, L. Gauthier}94_{, P. Gauzzi}133a,133b_,

I.L. Gavrilenko95_{, C. Gay}169_{, G. Gaycken}21_{, E.N. Gazis}10_{, P. Ge}33d_{, Z. Gecse}169_{, C.N.P. Gee}130_{, D.A.A. Geerts}106_,

Ch. Geich-Gimbel21_{, K. Gellerstedt}147a,147b_{, C. Gemme}50a_{, A. Gemmell}53_{, M.H. Genest}55_{, S. Gentile}133a,133b_,

M. George54, S. George76, D. Gerbaudo164, A. Gershon154, H. Ghazlane136b, N. Ghodbane34, B. Giacobbe20a, S. Giagu133a,133b, V. Giangiobbe12, P. Giannetti123a,123b, F. Gianotti30, B. Gibbard25, S.M. Gibson76, M. Gilchriese15, T.P.S. Gillam28, D. Gillberg30, G. Gilles34, D.M. Gingrich3,d, N. Giokaris9, M.P. Giordani165a,165c,

R. Giordano103a,103b, F.M. Giorgi20a, F.M. Giorgi16, P.F. Giraud137, D. Giugni90a, C. Giuliani48, M. Giulini58b, B.K. Gjelsten118, S. Gkaitatzis155, I. Gkialas155,l, L.K. Gladilin98, C. Glasman81, J. Glatzer30, P.C.F. Glaysher46, A. Glazov42, G.L. Glonti64, M. Goblirsch-Kolb100, J.R. Goddard75, J. Godfrey143, J. Godlewski30, C. Goeringer82, S. Goldfarb88_{, T. Golling}177_{, D. Golubkov}129_{, A. Gomes}125a,125b,125d_{, L.S. Gomez Fajardo}42_{, R. Gonc¸alo}125a_,

J. Goncalves Pinto Firmino Da Costa137_{, L. Gonella}21_{, S. Gonz´alez de la Hoz}168_{, G. Gonzalez Parra}12_,

S. Gonzalez-Sevilla49_{, L. Goossens}30_{, P.A. Gorbounov}96_{, H.A. Gordon}25_{, I. Gorelov}104_{, B. Gorini}30_{, E. Gorini}72a,72b_,

A. Goriˇsek74_{, E. Gornicki}39_{, A.T. Goshaw}6_{, C. G¨ossling}43_{, M.I. Gostkin}64_{, M. Gouighri}136a_{, D. Goujdami}136c_,

M.P. Goulette49_{, A.G. Goussiou}139_{, C. Goy}5_{, S. Gozpinar}23_{, H.M.X. Grabas}137_{, L. Graber}54_{, I. Grabowska-Bold}38a_,

P. Grafstr¨om20a,20b_{, K-J. Grahn}42_{, J. Gramling}49_{, E. Gramstad}118_{, S. Grancagnolo}16_{, V. Grassi}149_{, V. Gratchev}122_,

H.M. Gray30_{, E. Graziani}135a_{, O.G. Grebenyuk}122_{, Z.D. Greenwood}78,m_{, K. Gregersen}77_{, I.M. Gregor}42_{, P. Grenier}144_,

J. Griffiths8_{, A.A. Grillo}138_{, K. Grimm}71_{, S. Grinstein}12,n_{, Ph. Gris}34_{, Y.V. Grishkevich}98_{, J.-F. Grivaz}116_,

J.P. Grohs44, A. Grohsjean42, E. Gross173, J. Grosse-Knetter54, G.C. Grossi134a,134b, J. Groth-Jensen173, Z.J. Grout150, L. Guan33b, F. Guescini49, D. Guest177, O. Gueta154, C. Guicheney34, E. Guido50a,50b, T. Guillemin116, S. Guindon2, U. Gul53, C. Gumpert44, J. Gunther127, J. Guo35, S. Gupta119, P. Gutierrez112, N.G. Gutierrez Ortiz53, C. Gutschow77, N. Guttman154, C. Guyot137, C. Gwenlan119, C.B. Gwilliam73, A. Haas109, C. Haber15, H.K. Hadavand8,

N. Haddad136e, P. Haefner21, S. Hageb¨ock21, Z. Hajduk39, H. Hakobyan178, M. Haleem42, D. Hall119, G. Halladjian89, K. Hamacher176, P. Hamal114, K. Hamano170, M. Hamer54, A. Hamilton146a, S. Hamilton162, G.N. Hamity146c, P.G. Hamnett42_{, L. Han}33b_{, K. Hanagaki}117_{, K. Hanawa}156_{, M. Hance}15_{, P. Hanke}58a_{, R. Hanna}137_{, J.B. Hansen}36_,

J.D. Hansen36_{, P.H. Hansen}36_{, K. Hara}161_{, A.S. Hard}174_{, T. Harenberg}176_{, F. Hariri}116_{, S. Harkusha}91_{, D. Harper}88_,

R.D. Harrington46_{, O.M. Harris}139_{, P.F. Harrison}171_{, F. Hartjes}106_{, M. Hasegawa}66_{, S. Hasegawa}102_{, Y. Hasegawa}141_,

A. Hasib112_{, S. Hassani}137_{, S. Haug}17_{, M. Hauschild}30_{, R. Hauser}89_{, M. Havranek}126_{, C.M. Hawkes}18_,

R.J. Hawkings30_{, A.D. Hawkins}80_{, T. Hayashi}161_{, D. Hayden}89_{, C.P. Hays}119_{, H.S. Hayward}73_{, S.J. Haywood}130_,

S.J. Head18_{, T. Heck}82_{, V. Hedberg}80_{, L. Heelan}8_{, S. Heim}121_{, T. Heim}176_{, B. Heinemann}15_{, L. Heinrich}109_,

J. Hejbal126_{, L. Helary}22_{, C. Heller}99_{, M. Heller}30_{, S. Hellman}147a,147b_{, D. Hellmich}21_{, C. Helsens}30_{, J. Henderson}119_,

R.C.W. Henderson71_{, Y. Heng}174_{, C. Hengler}42_{, A. Henrichs}177_{, A.M. Henriques Correia}30_{, S. Henrot-Versille}116_,

L. Hervas30_{, G.G. Hesketh}77_{, N.P. Hessey}106_{, R. Hickling}75_{, E. Hig´on-Rodriguez}168_{, E. Hill}170_{, J.C. Hill}28_,

K.H. Hiller42_{, S. Hillert}21_{, S.J. Hillier}18_{, I. Hinchliffe}15_{, E. Hines}121_{, M. Hirose}158_{, D. Hirschbuehl}176_{, J. Hobbs}149_,

N. Hod106_{, M.C. Hodgkinson}140_{, P. Hodgson}140_{, A. Hoecker}30_{, M.R. Hoeferkamp}104_{, F. Hoenig}99_{, J. Hoffman}40_,

D. Hoffmann84_{, J.I. Hofmann}58a_{, M. Hohlfeld}82_{, T.R. Holmes}15_{, T.M. Hong}121_{, L. Hooft van Huysduynen}109_,

Y. Horii102_{, J-Y. Hostachy}55_{, S. Hou}152_{, A. Hoummada}136a_{, J. Howard}119_{, J. Howarth}42_{, M. Hrabovsky}114_,

I. Hristova16_{, J. Hrivnac}116_{, T. Hryn’ova}5_{, C. Hsu}146c_{, P.J. Hsu}82_{, S.-C. Hsu}139_{, D. Hu}35_{, X. Hu}25_{, Y. Huang}42_,

Z. Hubacek30_{, F. Hubaut}84_{, F. Huegging}21_{, T.B. Huffman}119_{, E.W. Hughes}35_{, G. Hughes}71_{, M. Huhtinen}30_,

T.A. H¨ulsing82_{, M. Hurwitz}15_{, N. Huseynov}64,b_{, J. Huston}89_{, J. Huth}57_{, G. Iacobucci}49_{, G. Iakovidis}10_,

I. Ibragimov142, L. Iconomidou-Fayard116, E. Ideal177, P. Iengo103a, O. Igonkina106, T. Iizawa172, Y. Ikegami65, K. Ikematsu142, M. Ikeno65, Y. Ilchenko31, D. Iliadis155, N. Ilic159, Y. Inamaru66, T. Ince100, P. Ioannou9, M. Iodice135a, K. Iordanidou9, V. Ippolito57, A. Irles Quiles168, C. Isaksson167, M. Ishino67, M. Ishitsuka158, R. Ishmukhametov110, C. Issever119, S. Istin19a, J.M. Iturbe Ponce83, R. Iuppa134a,134b, J. Ivarsson80, W. Iwanski39, H. Iwasaki65, J.M. Izen41, V. Izzo103a, B. Jackson121, M. Jackson73, P. Jackson1, M.R. Jaekel30, V. Jain2, K. Jakobs48, S. Jakobsen30, T. Jakoubek126, J. Jakubek127, D.O. Jamin152, D.K. Jana78, E. Jansen77, H. Jansen30, J. Janssen21, M. Janus171_{, G. Jarlskog}80_{, N. Javadov}64,b_{, T. Jav˚urek}48_{, L. Jeanty}15_{, J. Jejelava}51a,o_{, G.-Y. Jeng}151_{, D. Jennens}87_,

P. Jenni48,p_{, J. Jentzsch}43_{, C. Jeske}171_{, S. J´ez´equel}5_{, H. Ji}174_{, J. Jia}149_{, Y. Jiang}33b_{, M. Jimenez Belenguer}42_{, S. Jin}33a_,

A. Jinaru26a_{, O. Jinnouchi}158_{, M.D. Joergensen}36_{, K.E. Johansson}147a,147b_{, P. Johansson}140_{, K.A. Johns}7_,

K. Jon-And147a,147b_{, G. Jones}171_{, R.W.L. Jones}71_{, T.J. Jones}73_{, J. Jongmanns}58a_{, P.M. Jorge}125a,125b_{, K.D. Joshi}83_,

J. Jovicevic148_{, X. Ju}174_{, C.A. Jung}43_{, R.M. Jungst}30_{, P. Jussel}61_{, A. Juste Rozas}12,n_{, M. Kaci}168_{, A. Kaczmarska}39_,

M. Kado116_{, H. Kagan}110_{, M. Kagan}144_{, E. Kajomovitz}45_{, C.W. Kalderon}119_{, S. Kama}40_{, A. Kamenshchikov}129_,

N. Kanaya156_{, M. Kaneda}30_{, S. Kaneti}28_{, V.A. Kantserov}97_{, J. Kanzaki}65_{, B. Kaplan}109_{, A. Kapliy}31_{, D. Kar}53_,

K. Karakostas10_{, N. Karastathis}10_{, M. Karnevskiy}82_{, S.N. Karpov}64_{, Z.M. Karpova}64_{, K. Karthik}109_,

V. Kartvelishvili71_{, A.N. Karyukhin}129_{, L. Kashif}174_{, G. Kasieczka}58b_{, R.D. Kass}110_{, A. Kastanas}14_{, Y. Kataoka}156_,

A. Katre49, J. Katzy42, V. Kaushik7, K. Kawagoe69, T. Kawamoto156, G. Kawamura54, S. Kazama156, V.F. Kazanin108, M.Y. Kazarinov64, R. Keeler170, R. Kehoe40, M. Keil54, J.S. Keller42, J.J. Kempster76, H. Keoshkerian5, O. Kepka126, B.P. Kerˇsevan74, S. Kersten176, K. Kessoku156, J. Keung159, F. Khalil-zada11, H. Khandanyan147a,147b, A. Khanov113, A. Khodinov97, A. Khomich58a, T.J. Khoo28, G. Khoriauli21, A. Khoroshilov176, V. Khovanskiy96, E. Khramov64, J. Khubua51b, H.Y. Kim8, H. Kim147a,147b, S.H. Kim161, N. Kimura172, O. Kind16, B.T. King73, M. King168, R.S.B. King119, S.B. King169, J. Kirk130, A.E. Kiryunin100, T. Kishimoto66, D. Kisielewska38a, F. Kiss48, T. Kittelmann124_{, K. Kiuchi}161_{, E. Kladiva}145b_{, M. Klein}73_{, U. Klein}73_{, K. Kleinknecht}82_{, P. Klimek}147a,147b_,

A. Klimentov25_{, R. Klingenberg}43_{, J.A. Klinger}83_{, T. Klioutchnikova}30_{, P.F. Klok}105_{, E.-E. Kluge}58a_{, P. Kluit}106_,

S. Kluth100_{, E. Kneringer}61_{, E.B.F.G. Knoops}84_{, A. Knue}53_{, D. Kobayashi}158_{, T. Kobayashi}156_{, M. Kobel}44_,

M. Kocian144_{, P. Kodys}128_{, P. Koevesarki}21_{, T. Koffas}29_{, E. Koffeman}106_{, L.A. Kogan}119_{, S. Kohlmann}176_,

Z. Kohout127_{, T. Kohriki}65_{, T. Koi}144_{, H. Kolanoski}16_{, I. Koletsou}5_{, J. Koll}89_{, A.A. Komar}95,∗_{, Y. Komori}156_,

T. Kondo65_{, N. Kondrashova}42_{, K. K¨oneke}48_{, A.C. K¨onig}105_{, S. K¨onig}82_{, T. Kono}65,q_{, R. Konoplich}109,r_,

N. Konstantinidis77_{, R. Kopeliansky}153_{, S. Koperny}38a_{, L. K¨opke}82_{, A.K. Kopp}48_{, K. Korcyl}39_{, K. Kordas}155_,

A. Korn77_{, A.A. Korol}108,s_{, I. Korolkov}12_{, E.V. Korolkova}140_{, V.A. Korotkov}129_{, O. Kortner}100_{, S. Kortner}100_,

V.V. Kostyukhin21, V.M. Kotov64, A. Kotwal45, C. Kourkoumelis9, V. Kouskoura155, A. Koutsman160a, R. Kowalewski170, T.Z. Kowalski38a, W. Kozanecki137, A.S. Kozhin129, V. Kral127, V.A. Kramarenko98, G. Kramberger74, D. Krasnopevtsev97, M.W. Krasny79, A. Krasznahorkay30, J.K. Kraus21, A. Kravchenko25,

S. Kreiss109, M. Kretz58c, J. Kretzschmar73, K. Kreutzfeldt52, P. Krieger159, K. Kroeninger54, H. Kroha100, J. Kroll121, J. Kroseberg21, J. Krstic13a, U. Kruchonak64, H. Kr¨uger21, T. Kruker17, N. Krumnack63, Z.V. Krumshteyn64,

A. Kruse174, M.C. Kruse45, M. Kruskal22, T. Kubota87, S. Kuday4a, S. Kuehn48, A. Kugel58c, A. Kuhl138, T. Kuhl42, V. Kukhtin64_{, Y. Kulchitsky}91_{, S. Kuleshov}32b_{, M. Kuna}133a,133b_{, J. Kunkle}121_{, A. Kupco}126_{, H. Kurashige}66_,

Y.A. Kurochkin91_{, R. Kurumida}66_{, V. Kus}126_{, E.S. Kuwertz}148_{, M. Kuze}158_{, J. Kvita}114_{, A. La Rosa}49_,

L. La Rotonda37a,37b_{, C. Lacasta}168_{, F. Lacava}133a,133b_{, J. Lacey}29_{, H. Lacker}16_{, D. Lacour}79_{, V.R. Lacuesta}168_,

E. Ladygin64_{, R. Lafaye}5_{, B. Laforge}79_{, T. Lagouri}177_{, S. Lai}48_{, H. Laier}58a_{, L. Lambourne}77_{, S. Lammers}60_,

C.L. Lampen7_{, W. Lampl}7_{, E. Lanc¸on}137_{, U. Landgraf}48_{, M.P.J. Landon}75_{, V.S. Lang}58a_{, A.J. Lankford}164_,

F. Lanni25_{, K. Lantzsch}30_{, S. Laplace}79_{, C. Lapoire}21_{, J.F. Laporte}137_{, T. Lari}90a_{, M. Lassnig}30_{, P. Laurelli}47_,

W. Lavrijsen15_{, A.T. Law}138_{, P. Laycock}73_{, O. Le Dortz}79_{, E. Le Guirriec}84_{, E. Le Menedeu}12_{, T. LeCompte}6_,

F. Ledroit-Guillon55_{, C.A. Lee}152_{, H. Lee}106_{, J.S.H. Lee}117_{, S.C. Lee}152_{, L. Lee}1_{, G. Lefebvre}79_{, M. Lefebvre}170_,