Search for top and bottom squarks from gluino pair production in final states with missing transverse energy and at least three b-jets with the ATLAS detector

arXiv:1207.4686v1 [hep-ex] 19 Jul 2012

EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH (CERN)

CERN-PH-EP-2012-194

Submitted to: European Physical Journal C

Search for top and bottom squarks from gluino pair production

in final states with missing transverse energy and at least three

b

_{-jets with the ATLAS detector}

The ATLAS Collaboration

Abstract

This letter reports the results of a search for top and bottom squarks from gluino pair production in

4.7

fb

of

pp

collisions at

√

s = 7 TeV

using the ATLAS detector at the LHC. The search is performed

in events with large missing transverse momentum and at least three jets identified as originating from

a

b

-quark. Exclusion limits are presented for a variety of gluino-mediated models with gluino masses

(will be inserted by the editor)

Search for top and bottom squarks from gluino pair production

in final states with missing transverse energy and at least three

b

_{-jets with the ATLAS detector}

The ATLAS Collaboration

July 19, 2012

Abstract This letter reports the results of a search for

top and bottom squarks from gluino pair production

in 4.7 fb−1 of pp collisions at √s = 7 TeV using the

ATLAS detector at the LHC. The search is performed in events with large missing transverse momentum and at least three jets identified as originating from a b-quark. Exclusion limits are presented for a variety of gluino-mediated models with gluino masses up to 1 TeV excluded.

Supersymmetry (SUSY) [1–9] provides an extension of the Standard Model (SM) which resolves the hi-erarchy problem [10–13] by introducing supersymmet-ric partners of the known bosons and fermions. In the framework of the R-parity conserving minimal super-symmetric extension of the SM (MSSM) [14–18], SUSY particles are produced in pairs and the lightest super-symmetric particle (LSP) is stable, providing a possible candidate for dark matter. In a large variety of models,

the LSP is the lightest neutralino ( ˜χ0

1). The coloured

superpartners of quarks and gluons, the squarks (˜q)

and gluinos (˜g), if not too heavy, would be produced in

strong interaction processes at the Large Hadron Col-lider (LHC) and decay via cascades ending with the LSP. The undetected LSP results in missing transverse

momentum – whose magnitude is referred to as Emiss

T

– while the rest of the cascade yields final states with multiple jets and possibly leptons. In the MSSM, the

right-handed and left-handed squarks, ˜qR and ˜qL, can

mix to form two mass eigenstates ˜q1and ˜q2. The mixing

effect is proportional to the masses of the SM fermion partners and can therefore be large for the third

gener-ation. This may lead to the lightest sbottom (˜b1) and

stop (˜t1) mass eigenstates being much lighter than the

other squarks. As a consequence, ˜b₁and ˜t₁could be

pro-duced with relatively large cross-sections at the LHC,

either directly in pairs, or through ˜g˜g production

fol-lowed by ˜g → ˜b1b or ˜g → ˜t1t decays.

This letter extends the search for gluino-mediated

˜b1 and ˜t1 production at ATLAS reported earlier [19],

which used 2.05 fb−1 _{of data collected in the first half}

of 2011 at a centre-of-mass energy of 7 TeV. The present

analysis comprises the full 2011 dataset of 4.7 fb−1_and

adopts an improved selection that requires large Emiss

T ,

no electron or muon and at least three jets identified as originating from b-quarks (b-jets) in the final state. Results are interpreted in four simplified models where sbottoms or stops are the only squarks produced in the gluino decays, leading to final states with four b-quarks. Searches in similar scenarios have also been reported by the CMS Collaboration [20].

The ATLAS detector [21] consists of inner track-ing devices surrounded by a superconducttrack-ing solenoid, electromagnetic and hadronic calorimeters and a muon spectrometer with a toroidal magnetic field. The inner detector provides precision tracking of charged particles

for |η| < 2.51_{. It is immersed in a 2 T magnetic field}

from the solenoid and consists of a silicon pixel detec-tor, a silicon strip detector and a straw tube tracker that also provides transition radiation measurements for electron identification. The calorimeter system cov-ers the pseudorapidity range |η| < 4.9. It is composed of sampling calorimeters with either liquid argon (LAr) or scintillating tiles as the active medium. The muon

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 coordinates (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).The distance ∆R in the η − φ space is defined as ∆R =p(∆η)2

+ (∆φ)2

spectrometer has separate trigger and high-precision tracking chambers which provide muon identification and momentum measurement for |η| < 2.7.

Samples of simulated events are used for the descrip-tion of the background and to model the SUSY signal. The dominant sources of background come from events with b-quarks in the final state. Monte Carlo (MC)

sam-ples of t¯t, W /Z and diboson events produced in

asso-ciation with light- and heavy-flavour jets are generated with ALPGEN [22] and the parton distribution function (PDF) set CTEQ6L1 [23]. These samples are generated with different maximum numbers of additional partons at the matrix-element level. Diboson samples are

gen-erated with up to three additional partons, t¯t+jet and

Z(→ ℓ+_ℓ−

)+jets (ℓ = e,µ,τ ) samples with up to five ad-ditional partons, and W (→ ℓν)+jets and Z(→ ¯νν)+jet samples with up to six additional partons. Single top quark production is simulated with MC@NLO [24] using the next-to-leading-order (NLO) PDF set CTEQ6.6 [25]. The fragmentation and hadronisation for the ALPGEN and MC@NLO samples are performed with HERWIG [26, 27], using JIMMY [28] for the underlying event.

Sam-ples of t¯t+W , t¯t+Z and t¯t+W W events are generated

with MADGRAPH [29] interfaced to PYTHIA [30]. The sig-nal samples are generated using Herwig++ [31]. The MC samples are processed through the ATLAS detector simulation [32] based on GEANT4 [33] taking into account the effect of multiple pp interactions per bunch cross-ing. For the comparison with data, all SM background cross-sections are normalised to the results of higher-order calculations when available, using the same values as in Ref. [19].

Jets are reconstructed from three-dimensional

calorime-ter energy cluscalorime-ters using the anti-kt jet algorithm [34,

35] with a radius parameter of 0.4. The measured jet energy is corrected for inhomogeneities and for the

non-compensating nature of the calorimeter by using pT

-and η-dependent correction factors, -and additional cor-rections for pile-up are applied [36]. Jets are required to

have pT> 20 GeV, and are reconstructed in the range

|η| < 4.9. Events are rejected if they include jets failing the quality criteria described in Ref. [36], or if there is any selected jet with |η| < 2 for which the scalar sum of the transverse momenta of its associated tracks is less

than 5% of the jet pT. A neural-network-based

algo-rithm [37] is used to identify jets containing a b-hadron decay. This uses as inputs the output weights of differ-ent algorithms exploiting the impact parameter of the inner detector tracks, the secondary vertex reconstruc-tion and the topology of b- and c-hadron decays inside the jet. Three operating points are used, corresponding to efficiencies of 60%, 70% and 75% for tagging b-jets in

a MC sample of t¯t events. In all cases the tagging rate

is less than 2% for light-quark and gluon jets, 10% for τ leptons decaying hadronically and 25% for c-quark jets. The b-jets are identified within the nominal acceptance of the inner detector (|η| < 2.5) and are required to

have pT > 30 GeV. To compensate for the differences

between the b-tagging efficiency and the mistag rates in data and MC simulation, b-tagging scale factors are applied to each jet in the simulations, as described in Refs. [37–39].

Electrons are reconstructed from energy clusters in the electromagnetic calorimeter matched to a track in the inner detector. Electron candidates are required to

have pT > 20 GeV and |η| < 2.47 and must satisfy

the “medium” selection criteria described in Ref. [40]. Muons candidates are identified using a match between an extrapolated inner detector track and one or more track segments in the muon spectrometer, and are

re-quired to have pT> 10 GeV and |η| < 2.4.

To resolve overlaps between reconstructed jets and leptons, jets within a distance of ∆R = 0.2 of an elec-tron candidate are rejected. Furthermore, any lepton candidate with a distance ∆R < 0.4 to the closest re-maining jet is discarded. Events containing any remain-ing electrons and muons are vetoed in the control and signal regions defined in Tables 1 and 2.

The measurement of the missing transverse

momen-tum two-dimensional vector (and its magnitude Emiss

T )

is based on the transverse momenta of all remaining jets with |η| < 4.9, all electron and muon candidates and all calorimeter clusters not associated to such objects.

Events are selected using triggers requiring one high

pTjet and ETmiss. Different trigger thresholds were used

to cope with the increasing luminosity. These triggers are fully efficient for this analysis, which requires one jet

with pT> 130 GeV and ETmiss> 160 GeV at the offline

reconstruction stage. Events must pass basic quality criteria to reject detector noise and non-collision back-grounds. They are also required to have a reconstructed primary vertex associated with five or more tracks with

pT> 0.4 GeV; when more than one such vertex is found,

the vertex with the largest summed p2

T of the

associ-ated tracks is chosen as the hard interaction vertex. Events are required to have at least three b-tagged jets,

and two jet-multiplicity regions (NJ ≥ 4 and NJ ≥ 6)

are considered by selecting jets with |η| < 2.8 and

pT> 50 GeV.

Two variables are calculated from the reconstructed

objects to further select the events: meff and ∆φmin.

The effective mass meff is defined as the scalar sum of

the Emiss

T and the pTof all selected jets in a given

jet-multiplicity region. The ∆φmin is defined as the

min-imum azimuthal separation between the selected jets and the missing transverse momentum direction.

Plac-Common criteria: lepton veto, pj1

T> 130 GeV,

≥3 b-jets, Emiss

T /meff > 0.2, ∆φmin> 0.4

SR NJ ETmiss meff b-tag OP

SR4-L ≥4j >160 GeV >500 GeV 60% SR4-M ≥4j >160 GeV >700 GeV 60% SR4-T ≥4j >160 GeV >900 GeV 70% SR6-L ≥6j >160 GeV >700 GeV 70% SR6-T ≥6j >200 GeV >900 GeV 75% Table 1 Definition of the five signal regions based on the number of jets (NJ), the ETmiss, meff requirements and the

b-tagging operating point (OP).

ing the requirements ∆φmin > 0.4 and ETmiss/meff >

0.2 reduces the amount of multi-jet background, where

Emiss

T results from mis-reconstructed jets or from

neu-trinos emitted close to the direction of the jet axis. Two sets of signal regions are defined which yield good signal sensitivity for the various models and pa-rameter values studied here. They are characterised by having at least four (SR4) or six (SR6) jet candidates, no electron or muon, and are further classified as loose

(L), medium (M) or tight (T) depending on the Emiss

T

and meffthresholds and on the b-tagging operating point.

The requirements that characterise each signal region are summarised in Table 1.

The main source of reducible background is the

pro-duction of t¯t events in association with additional jets

followed by the leptonic decay of one W boson, where the lepton is not reconstructed or is misidentified as a jet (mainly through the hadronic decays of a τ lepton). This background is estimated by normalising the MC event yield in the signal region to the extrapolated event

yield observed in a t¯t-dominated control region.

Sys-tematic uncertainties that are correlated between the control and the signal regions largely cancel out in this procedure. Additional sources of reducible background

are single top, t¯t+W /Z and W /Z+heavy-flavour jets.

Their contributions are taken from MC simulation and account for 10% to 20% of the total background depend-ing on the signal region. The irreducible background

t¯t+b¯b is also estimated from MC simulation and

ac-counts for about 10% of the total background in all sig-nal regions. The reducible contribution from multi-jet events is estimated with a data-driven method, based on a jet response smearing technique [41], and is found to account for less than 5% of the total background in all signal regions.

Four control regions where the t¯t+jets background

accounts for more than 80% of the total yield are de-fined by applying the same jet requirements and lep-ton veto as in the signal regions, but requiring exactly two b-jets instead of three or more. The requirements

meff > 500 GeV and ETmiss > 160 GeV are applied to

all control regions to make them kinematically similar

Common criteria: lepton veto, pj1

T > 130 GeV,

= 2 b-jets, Emiss

T /meff > 0.2, ∆φmin> 0.4,

Emiss

T > 160 GeV, meff > 500 GeV

CR NJ b-tag OP corresponding SR

CR4-60 ≥4j 60% SR4-L, SR4-M

CR4-70 ≥4j 70% SR4-T

CR6-70 ≥6j 70% SR6-L

CR6-75 ≥6j 75% SR6-T

Table 2 Definition of the four control regions used to esti-mate the t¯t+jets background.

to the signal regions, while reducing the contamination from possible SUSY signal events. The definition of the control regions is summarised in Table 2. The numbers of expected SM events in the four control regions, as predicted by the jet smearing technique for multi-jet events and by MC simulation for other processes, are compared to those observed in data in Table 3. The results agree within experimental errors.

CR t¯t+jets others SM data

CR4-60 330 ± 90 65 ± 25 395 ± 115 402 CR4-70 490 ± 125 100 ± 35 590 ± 160 515

CR6-70 38 ± 11 7 ± 3 45 ± 13 46

CR6-75 40 ± 12 10 ± 4 50 ± 15 52

Table 3 Expected numbers of SM events and observed data events in the four t¯t control regions. The contribution from t¯t+jets events is taken directly from MC simulation. The column “others” includes the contributions from single top, t¯t+b¯b, t¯t+W /Z and W /Z+jets processes, also estimated from MC simulation, and the contribution from multi-jet events which is estimated with the jet smearing technique and accounts for less than 5% of the total background. The column “SM” shows the total expected background and is the sum of the columns “t¯t+jets” and “others”. The uncertainties include all detector-related systematic uncertainties.

The dominant detector-related systematic effects are due to the jet energy scale (JES) and resolution (JER) uncertainties, and the uncertainty on the b-tagging ef-ficiency and mistag rates. The JES uncertainty is de-rived from a combination of simulations, test beam data and in-situ measurements [36], and includes additional uncertainties due to the jet flavour and nearby jets. Uncertainties on the JER are obtained with an in-situ measurement of the jet response asymmetry in di-jet events. These uncertainties on jets are propagated to

the Emiss

T measurement, and additional uncertainties

on Emiss

T arising from energy deposits not associated

with any reconstructed objects are also included. The

b-tagging uncertainty is evaluated by varying the η-, pT

-and flavour-dependent scale factors applied to each jet in the simulation within a range that reflects the sys-tematic uncertainty on the measured tagging efficiency and mistag rates.

The systematic uncertainties in the modelling of the

t¯t+jets background are assessed as follows: the

uncer-tainty due to the choice of the MC generator is esti-mated by comparing the leading-order ALPGEN gener-ator to the MC@NLO genergener-ator; the uncertainty due to the factorisation and matching scale ambiguities in

ALPGEN are estimated by independently varying their

nominal settings by factors of one half and two; the un-certainty due to the finite number of additional partons at the matrix-element level is assessed by comparing in-clusive ALPGEN samples generated with up to three and up to five extra partons. Finally the PDF uncertainties are estimated using the MSTW2008NNLO PDF set. Uncer-tainties of 100% are assumed for the multi-jet prediction

and for the cross-section of t¯t and W /Z production in

association with a b¯b pair. For t¯t+W /Z production, an

uncertainty of approximatively 70% has been derived from the variations of the factorisation and renormali-sation scales and from the PDF uncertainties [42].

The t¯t+jets yield in each signal region is

extrapo-lated from the measured number of events in the cor-responding control region (as per Table 2) using a fit based on the profile likelihood method [43]. Each pair of control and signal regions is fitted separately, assum-ing no signal events. The free parameter in each fit is

the t¯t+jets overall normalisation scale, while the

con-tributions from subdominant background processes are fixed at the expected value. Systematic uncertainties are treated as nuisance parameters constrained with a Gaussian function and correlations are taken into ac-count where appropriate. The results of the fits and the numbers of observed events for each signal region are summarised in Table 4. The fitted values of the

nor-malisation factors for t¯t+jets are compatible with one

and the main impact of the data-driven estimate is a reduction in the uncertainty by approximately a

fac-tor of two. Figure 1 shows the measured meff

distribu-tions and the MC predicdistribu-tions for the SM backgrounds in each signal region. Also shown are the prediction of two benchmark signal models described below.

The reliability of the MC extrapolation of the t¯t

background to larger b-jet multiplicities has been checked in validation regions defined with kinematic cuts similar to those used in the control and signal regions, except that exactly one isolated electron or muon is required.

The transverse mass of the lepton and the Emiss

T is

re-quired to be less than 100 GeV in all validation regions to minimise the possible contamination from stop pro-duction. The extrapolated event yield in the validation regions with at least three b-jets from the validation re-gions with exactly two b-jets is found to be consistent with the number of observed events for all b-tagging operating points.

SR t¯t+jets others SM data

(MC) SR4-L _{(32.6 ± 15.4)}33.3 ± 7.9 11.1 ± 4.9 44.4 ± 10.0 45 SR4-M _{(16.1 ± 8.4)}16.4 ± 4.1 6.6 ± 2.9 23.0 ± 5.4 14 SR4-T _{(11.4 ± 5.4)}9.6 ± 2.1 3.7 ± 1.6 13.3 ± 2.6 10 SR6-L 10.3 ± 3.3 2.4 ± 1.4 12.7 ± 3.6 12 (10.0 ± 6.2) SR6-T _{(7.9 ± 5.3)}8.3 ± 2.4 1.6 ± 1.1 9.9 ± 2.6 8 Table 4 Comparison between the results of the fits and the numbers of observed events in the five signal regions. The t¯t+jets event yield predicted by the MC simulation is quoted in parentheses. The column “others” includes the contribu-tions from single top, t¯t+b¯b, t¯t+W /Z, W /Z+jets and multi-jet processes. Multi-multi-jet events contribute less than 5% of the total background. The column “SM” shows the total expected background and is the sum of the columns “t¯t+jets” and “oth-ers”. The uncertainties include the statistical and systematic uncertainties.

The background predictions have been further vali-dated using a data-driven method that simultaneously estimates all SM background contributions with at least one misidentified b-jet. This method consists of predict-ing the number of jets originatpredict-ing from b-quarks in each event by solving a system of equations based on the number of b-tagged and non b-tagged jets in the event, along with the b-tagging efficiency and mistag rates. Consistent background predictions with respect to the fit results have been found in all signal regions.

Limits for non-SM signal at 95% confidence level (CL) are derived by testing the signal plus background

hypothesis in each signal region with the CLs

prescrip-tion [43]. These limits are obtained with fits similar to those used to estimate the background in each signal re-gion, except that the number of observed events in the signal region is added as an input to the fit and a sec-ond free parameter for the non-SM signal strength, con-strained to be non-negative, is adjusted in the likelihood maximisation. This additional free parameter ensures a proper treatment of the expected signal contamination in the control regions when the results are interpreted in the framework of specific SUSY scenarios. Model-independent upper limits at 95% CL on the number of signal events and on the visible cross-section (defined as the cross-section times kinematic acceptance times ex-perimental efficiency) for non-SM contributions derived for each signal region are given in Table 5.

These data have been used to derive limits in the parameter space of the following SUSY models:

Gluino-sbottom model: MSSM scenarios where

the ˜b₁is the lightest squark, all other squarks are

heav-ier than the gluino, and m_˜g > m˜b1

> m_χ˜0

[GeV] eff m Events / 100 GeV 1 10 2 10 3 10 Data 2011 SM Total +jets t t Others =50 GeV 1 0 χ∼ =950 GeV, m g ~ Gbb: m =400 GeV 1 0 χ∼ =700 GeV, m g ~ Gbb: m ATLAS = 7 TeV s , -1 L dt ~ 4.7 fb ∫ SR4-L [GeV] eff m 400 600 800 1000 1200 1400 1600 1800 2000 data / exp 0 1 2 meff [GeV] Events / 100 GeV 1 10 2 10 Data 2011 SM Total +jets t t Others =50 GeV 1 0 χ∼ =950 GeV, m g ~ Gbb: m =400 GeV 1 0 χ∼ =700 GeV, m g ~ Gbb: m ATLAS = 7 TeV s , -1 L dt ~ 4.7 fb ∫ SR4-T [GeV] eff m 400 600 800 1000 1200 1400 1600 1800 2000 data / exp 0 1 2 [GeV] eff m Events / 100 GeV 1 10 2 10 Data 2011 SM Total +jets t t Others =50 GeV 1 0 χ∼ =800 GeV, m g ~ Gtt: m =200 GeV 1 0 χ∼ =600 GeV, m g ~ Gtt: m ATLAS = 7 TeV s , -1 L dt ~ 4.7 fb ∫ SR6-L [GeV] eff m 400 600 800 1000 1200 1400 1600 1800 2000 data / exp 0 1 2 meff [GeV] Events / 100 GeV 1 10 2 10 Data 2011 SM Total +jets t t Others =50 GeV 1 0 χ∼ =800 GeV, m g ~ Gtt: m =200 GeV 1 0 χ∼ =600 GeV, m g ~ Gtt: m ATLAS = 7 TeV s , -1 L dt ~ 4.7 fb ∫ SR6-T [GeV] eff m 400 600 800 1000 1200 1400 1600 1800 2000 data / exp 0 1 2

Fig. 1 Distribution of meff for SR4-L and SR4-T (top) and SR6-L and SR6-T (bottom). The hatched band shows the

systematic uncertainty on the MC prediction, which includes both experimental uncertainties (among which JES and b-tagging uncertainties are dominant) and theoretical uncertainties on the background normalisation and shape. The label “others” includes the contributions from single top, t¯t+b¯b, t¯t+W /Z, W /Z+jets and multi-jet processes. The lower plot in each figure shows the ratio of the observed distribution to that expected for the SM background. Two signal points (with small and large mass splitting between the gluino and the LSP) for the Gbb and Gtt models described in the text are overlaid.

Obs (exp) 95% CL upper limit

SR N events σvis(fb) SR4-L 23.8 (23.4) 5.1 (5.0) SR4-M 8.6 (12.8) 1.8 (2.7) SR4-T 7.1 (9.2) 1.5 (2.0) SR6-L 9.6 (10.1) 2.0 (2.1) SR6-T 7.1 (8.3) 1.5 (1.8)

Table 5 Observed (expected) 95% CL upper limits on the non-SM contributions to all signal regions. Limits are given on numbers of events and in terms of visible cross-sections defined by cross-section times kinematic acceptance times experimental efficiency. Systematic uncertainties on the SM background estimation are included in the limits.

branching ratio for ˜g → ˜b1b decays is 100%. Sbottoms

are produced via ˜g˜g or by ˜b1˜b1 direct pair production

and are assumed to decay exclusively via ˜b1 → b ˜χ01,

where m_χ˜0

1 is set to 60 GeV. Exclusion limits are

pre-sented in the (mg_˜, m˜b1

) plane.

Gbb model: Simplified scenarios, where ˜b1 is the

lightest squark but m_˜g< m˜b1

. Pair production of gluinos is the only process taken into account since the masses

of all other sparticles apart from the ˜χ0

1 are set above

the TeV scale. A three-body decay via an off-shell sbot-tom is assumed for the gluino, yielding a 100% BR for

the decay ˜g → b¯b˜χ0

1. The sbottom mass has no impact

on the kinematics of the decay and the exclusion limits

are presented in the (m_˜g, mχ˜0

1) plane.

Gluino-stop model: MSSM scenarios where the

˜

t1 is the lightest squark, all other squarks are heavier

than the gluino, and m˜g> m˜t1+ mt, so the branching

ratio for ˜g → ˜t1t decays is 100%. Stops are produced

via ˜g˜g and ˜t1˜t1 and are assumed to decay exclusively

via ˜t1 → b ˜χ

±

1. The neutralino mass is set to 60 GeV,

the chargino mass to 120 GeV and the latter is assumed to decay through a virtual W boson. Exclusion limits

are presented in the (m˜g, m˜t1

) plane.

Gtt model: Simplified scenarios, where ˜t1 is the

lightest squark but mg˜< mt˜1. Pair production of gluinos

is the only process taken into account since the mass

of all other sparticles apart from the ˜χ0

1 are above the

TeV scale. A three-body decay via off-shell stop is as-sumed for the gluino, yielding a 100% BR for the decay ˜

g → t¯t˜χ0

[GeV] g ~ m 200 300 400 500 600 700 800 900 1000 1100 1200 [GeV] 1 b ~ m 200 400 600 800 1000 1200 -1 2.05 fb 1 b ~ 1 b ~ ATLAS -1 2.65 fb 1 b ~ 1 b ~ CDF -1 5.2 fb 1 b ~ 1 b ~ D0 -1 b 2.5 fb 1 b ~ → , g ~ g ~ CDF 0 1 χ∼ b+ → 1 b ~ production, 1 b ~ -1 b ~ + g ~ -g ~ ) g ~ ) >> m( 1,2 q ~ ) = 60 GeV, m( 0 1 χ∼ m( b forbidden 1 b ~ → g ~ = 7 TeV s , -1 = 4.7 fb int L

3 b-jets channel All limits at 95% CL ATLAS exp σ 1 ± Expected limit s CL Theory SUSY σ 1 ± Observed limit s CL -1 0-lepton + b-jets 2.0 fb [GeV] g ~ m 300 400 500 600 700 800 900 1000 [GeV]~t1 m 200 300 400 500 600 700 800 900 ± 1 χ∼ b+ → 1 t ~ production, 1 t ~ -1 t ~ + g ~ -g ~ ) g ~ ) >> m( 1,2 q ~ ) = 60 GeV, m( 0 1 χ∼ m( t forbidden 1 t ~ → g ~ = 7 TeV s , -1 = 4.7 fb int L 3 b-jets channel All limits at 95% CL ATLAS exp σ 1 ± Expected limit s CL Theory SUSY σ 1 ± Observed limit s CL -1 1-lepton + b-jets 2.0 fb -1 SS dilepton, 2.0 fb [GeV] g ~ m 200 300 400 500 600 700 800 900 1000 1100 1200 [GeV]0_χ∼1 m 0 200 400 600 800 1000 1200 forbidden 0 1 χ ∼ + b b → g ~ ) g ~ ) >> m( q ~ , m( 0 1 χ∼ + b b → g ~ production, g ~ -g ~ _Lint _{= 4.7 fb}-1_{, s = 7 TeV} 3 b-jets channel All limits at 95% CL ATLAS exp σ 1 ± Expected limit s CL Theory SUSY σ 1 ± Observed limit s CL -1 0-lepton + b-jets, 2.0 fb [GeV] g ~ m 400 500 600 700 800 900 1000 1100 [GeV] 0_χ∼1 m 0 100 200 300 400 500 600 700 800 forbidden 0 1 χ ∼ + t t → g ~ ) g ~ ) >> m( q ~ , m( 0 1 χ∼ + t t → g ~ production, g ~ -g ~ _Lint _{= 4.7 fb}-1_{, s = 7 TeV} 3 b-jets channel All limits at 95% CL ATLAS exp σ 1 ± Expected limit s CL Theory SUSY σ 1 ± Observed limit s CL -1 SS dilepton, 2.0 fb -1

1-lepton plus b-jets, 2.0 fb

-1 Multi-jet, 4.7 fb exp σ 1 ± Expected limit s CL Theory SUSY σ 1 ± Observed limit s CL -1 SS dilepton, 2.0 fb -1

1-lepton plus b-jets, 2.0 fb

-1

Multi-jet, 4.7 fb

Fig. 2 Exclusion limits in the (mg˜, m˜ b1

) plane for the gluino-sbottom model (top left), in the (mg˜, m˜_t

1

) plane for the gluino-stop model (top right) and in the (mg˜, mχ˜0

1) plane for the Gbb (bottom left) and Gtt (bottom right) models. The

dashed black and solid bold red lines show the 95% CL expected and observed limits respectively, including all uncertainties except the theoretical signal cross-section uncertainty. The shaded (yellow) bands around the expected limits show the impact of the experimental uncertainties while the dotted red lines show the impact on the observed limit of the variation of the nominal signal cross-section by 1σ theoretical uncertainty. Also shown for reference are the previous CDF [44, 45], D0 [46] and ATLAS [19, 42, 47, 48] analyses.

ics of the decay and the exclusion limits are presented

in the (mg˜, mχ˜0

1) plane.

The SR4 regions are mostly sensitive to the SUSY models where sbottom production dominates, whilst the SR6 regions are used to set exclusion limits in mod-els characterised by on-shell or off-shell stop produc-tion, where top-enriched final states are expected. The signal region with the best expected sensitivity at each point in the parameter space is used to derive the limits at 95% CL. Signal cross-sections are calculated to next-to-leading order in the strong coupling constant, includ-ing the resummation of soft gluon emission at next-to-leading-logarithmic accuracy (NLO+NLL) [49–53]. The

nominal cross-section and the uncertainty σSUSY

Theory are

taken from an envelope of cross-section predictions us-ing different PDF sets and factorisation and renormal-isation scales, as described in Ref. [54]. All detector-related systematic uncertainties are treated as fully cor-related between signal and backgrounds. In the Gbb scenario, the impact of initial-state radiation (ISR) is

expected to be large in the region with low mg˜− mχ˜0

1

due to the small signal acceptance. Therefore, an uncer-tainty on the modelling of ISR is assessed by comparing the signal acceptance obtained with the Herwig++ ples to the one obtained with dedicated MADGRAPH sam-ples generated with additional jets. This uncertainty

varies from 4% to 35% as a function of m˜g− mχ˜0

1 and

is included in the ±1σSUSY

Theory band.

The expected and observed 95% CL exclusion lim-its in the four models considered above are shown in Figure 2. In the gluino-sbottom model, gluino masses below 1000 GeV are excluded for sbottom masses up to

about 870 GeV using the most conservative −1σSUSY

Theory

hypothesis. This extends by approximatively 100 GeV the limits derived in the same scenario by the

previ-ous ATLAS analysis performed with 2 fb−1_{[19] and is}

complementary to the ATLAS search for direct

sbot-tom pair production, also carried out with 2 fb−1_[47].

The exclusion is less stringent in the region with low

m˜g− m˜b1, where softer jets are expected. Because of

the kinematic cuts applied, the limits depend on the neutralino mass assumption for low mass splitting

be-tween the sbottom and the neutralino as shown for the

Gbb _{model where gluino masses below 1020 GeV are}

excluded for neutralino masses up to about 400 GeV, improving the previous ATLAS limits [19] by approx-imatively 100 GeV. In the gluino-stop model, gluino masses below 820 GeV are excluded for stop masses up to 640 GeV, extending the previous ATLAS lim-its [19, 42] by approximatively 150 GeV. In the Gtt model, gluino masses below 940 GeV are excluded for

mχ˜0

1< 50 GeV while neutralino masses below 320 GeV

are excluded for m˜g = 800 GeV. This search extends

the exclusion limits on the gluino mass from the AT-LAS multi-jet analysis carried out with the same data set [48] and from the CMS same-sign dilepton analysis

performed with 5 fb−1[20] by approximatively 60 GeV

and 130 GeV, respectively, for neutralino masses below

100 GeV. In the region with low m˜g− mχ˜0

1, the limits

obtained with the CMS analysis are most stringent due to the softer kinematic cuts.

In summary, this letter presents results from a search for top and bottom squarks in the decay of gluino pairs

produced in pp collisions at √s = 7 TeV, based on

4.7 fb−1 _{of ATLAS data. The events are selected with}

large Emiss

T , four or six jets and at least three jets

orig-inating from b-quarks in the final state. The results are in agreement with the SM background prediction and translate into 95% CL upper limits on excluded masses for a variety of SUSY benchmark scenarios. Gluino masses up to 1 TeV are excluded, depending on the model, which significantly extends the previous results.

We thank CERN for the very successful operation of the LHC, as well as the support staff from our in-stitutions without whom ATLAS could not be oper-ated efficiently. We acknowledge the support of AN-PCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF, 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; ARTEMIS, Euro-pean Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNAS, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT, Greece; ISF, MINERVA, GIF, DIP and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; RCN, Norway; MNiSW, Poland; GRICES and FCT, Portugal; MERYS (MECTS), Ro-mania; MES of Russia and ROSATOM, Russian Fed-eration; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MVZT, Slovenia; DST/NRF, South Africa; MICINN, 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 comput-ing support from all WLCG partners is acknowledged gratefully, in particular from CERN and the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Den-mark, 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.

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J.A. Dassoulas41_{, W. Davey}20_{, T. Davidek}125_{, N. Davidson}85_{, R. Davidson}70_{, E. Davies}117,c_{, M. Davies}92_,

O. Davignon77_{, A.R. Davison}76_{, Y. Davygora}57a_{, E. Dawe}141_{, I. Dawson}138_{, R.K. Daya-Ishmukhametova}22_,

K. De7_{, R. de Asmundis}101a_{, S. De Castro}19a,19b_{, S. De Cecco}77_{, J. de Graat}97_{, N. De Groot}103_{, P. de Jong}104_,

C. De La Taille114_{, H. De la Torre}79_{, F. De Lorenzi}62_{, L. de Mora}70_{, L. De Nooij}104_{, D. De Pedis}131a_,

A. De Salvo131a_{, U. De Sanctis}163a,163c_{, A. De Santo}148_{, J.B. De Vivie De Regie}114_{, G. De Zorzi}131a,131b_,

W.J. Dearnaley70_{, R. Debbe}24_{, C. Debenedetti}45_{, B. Dechenaux}54_{, D.V. Dedovich}63_{, J. Degenhardt}119_,

C. Del Papa163a,163c_{, J. Del Peso}79_{, T. Del Prete}121a,121b_{, T. Delemontex}54_{, M. Deliyergiyev}73_{, A. Dell’Acqua}29_,

L. Dell’Asta21_{, M. Della Pietra}101a,j_{, D. della Volpe}101a,101b_{, M. Delmastro}4_{, P.A. Delsart}54_{, C. Deluca}104_,

S. Demers175_{, M. Demichev}63_{, B. Demirkoz}11,l_{, J. Deng}162_{, S.P. Denisov}127_{, D. Derendarz}38_{, J.E. Derkaoui}134d_,

F. Derue77_{, P. Dervan}72_{, K. Desch}20_{, E. Devetak}147_{, P.O. Deviveiros}104_{, A. Dewhurst}128_{, B. DeWilde}147_,

S. Dhaliwal157_{, R. Dhullipudi}24 ,m_{, A. Di Ciaccio}132a,132b_{, L. Di Ciaccio}4_{, A. Di Girolamo}29_{, B. Di Girolamo}29_,

S. Di Luise133a,133b_{, A. Di Mattia}172_{, B. Di Micco}29_{, R. Di Nardo}46_{, A. Di Simone}132a,132b_{, R. Di Sipio}19a,19b_,

M.A. Diaz31a_{, E.B. Diehl}86_{, J. Dietrich}41_{, T.A. Dietzsch}57a_{, S. Diglio}85_{, K. Dindar Yagci}39_{, J. Dingfelder}20_,

F. Dinut25a_{, C. Dionisi}131a,131b_{, P. Dita}25a_{, S. Dita}25a_{, F. Dittus}29_{, F. Djama}82_{, T. Djobava}50b_,

M.A.B. do Vale23c_{, A. Do Valle Wemans}123a,n_{, T.K.O. Doan}4_{, M. Dobbs}84_{, R. Dobinson}29,∗_{, D. Dobos}29_,

E. Dobson29,o_{, J. Dodd}34_{, C. Doglioni}48_{, T. Doherty}52_{, Y. Doi}64,∗_{, J. Dolejsi}125_{, I. Dolenc}73_{, Z. Dolezal}125_,

B.A. Dolgoshein95,∗_{, T. Dohmae}154_{, M. Donadelli}23d_{, J. Donini}33_{, J. Dopke}29_{, A. Doria}101a_{, A. Dos Anjos}172_,

A. Dotti121a,121b_{, M.T. Dova}69_{, A.D. Doxiadis}104_{, A.T. Doyle}52_{, M. Dris}9_{, J. Dubbert}98_{, S. Dube}14_,

M-A. Dufour84_{, L. Duguid}75_{, M. Dunford}29_{, H. Duran Yildiz}3a_{, R. Duxfield}138_{, M. Dwuznik}37_{, F. Dydak}29_,

M. D¨uren51_{, J. Ebke}97_{, S. Eckweiler}80_{, K. Edmonds}80_{, W. Edson}1_{, C.A. Edwards}75_{, N.C. Edwards}52_,

W. Ehrenfeld41_{, T. Eifert}142_{, G. Eigen}13_{, K. Einsweiler}14_{, E. Eisenhandler}74_{, T. Ekelof}165_{, M. El Kacimi}134c_,

M. Ellert165_{, S. Elles}4_{, F. Ellinghaus}80_{, K. Ellis}74_{, N. Ellis}29_{, J. Elmsheuser}97_{, M. Elsing}29_{, D. Emeliyanov}128_,

R. Engelmann147_{, A. Engl}97_{, B. Epp}60_{, J. Erdmann}53_{, A. Ereditato}16_{, D. Eriksson}145a_{, J. Ernst}1_{, M. Ernst}24_,

J. Ernwein135_{, D. Errede}164_{, S. Errede}164_{, E. Ertel}80_{, M. Escalier}114_{, H. Esch}42_{, C. Escobar}122_,

X. Espinal Curull11_{, B. Esposito}46_{, F. Etienne}82_{, A.I. Etienvre}135_{, E. Etzion}152_{, D. Evangelakou}53_{, H. Evans}59_,

L. Fabbri19a,19b_{, C. Fabre}29_{, R.M. Fakhrutdinov}127_{, S. Falciano}131a_{, Y. Fang}172_{, M. Fanti}88a,88b_{, A. Farbin}7_,

A. Farilla133a_{, J. Farley}147_{, T. Farooque}157_{, S. Farrell}162_{, S.M. Farrington}169_{, P. Farthouat}29_{, P. Fassnacht}29_,

D. Fassouliotis8_{, B. Fatholahzadeh}157_{, A. Favareto}88a,88b_{, L. Fayard}114_{, S. Fazio}36a,36b_{, R. Febbraro}33_,

P. Federic143a_{, O.L. Fedin}120_{, W. Fedorko}87_{, M. Fehling-Kaschek}47_{, L. Feligioni}82_{, D. Fellmann}5_{, C. Feng}32d_,

E.J. Feng5_{, A.B. Fenyuk}127_{, J. Ferencei}143b_{, W. Fernando}5_{, S. Ferrag}52_{, J. Ferrando}52_{, V. Ferrara}41_,

A. Ferrari165_{, P. Ferrari}104_{, R. Ferrari}118a_{, D.E. Ferreira de Lima}52_{, A. Ferrer}166_{, D. Ferrere}48_{, C. Ferretti}86_,

A. Ferretto Parodi49a,49b_{, M. Fiascaris}30_{, F. Fiedler}80_{, A. Filipˇciˇc}73_{, F. Filthaut}103_{, M. Fincke-Keeler}168_,

M.C.N. Fiolhais123a,h, L. Fiorini166, A. Firan39, G. Fischer41, M.J. Fisher108, M. Flechl47, I. Fleck140,

J. Fleckner80_{, P. Fleischmann}173_{, S. Fleischmann}174_{, T. Flick}174_{, A. Floderus}78_{, L.R. Flores Castillo}172_,

M.J. Flowerdew98_{, T. Fonseca Martin}16_{, A. Formica}135_{, A. Forti}81_{, D. Fortin}158a_{, D. Fournier}114_{, H. Fox}70_,

P. Francavilla11_{, M. Franchini}19a,19b_{, S. Franchino}118a,118b_{, D. Francis}29_{, T. Frank}171_{, S. Franz}29_,

M. Fraternali118a,118b_{, S. Fratina}119_{, S.T. French}27_{, C. Friedrich}41_{, F. Friedrich}43_{, R. Froeschl}29_{, D. Froidevaux}29_,

J.A. Frost27_{, C. Fukunaga}155_{, E. Fullana Torregrosa}29_{, B.G. Fulsom}142_{, J. Fuster}166_{, C. Gabaldon}29_,

O. Gabizon171_{, T. Gadfort}24_{, S. Gadomski}48_{, G. Gagliardi}49a,49b_{, P. Gagnon}59_{, C. Galea}97_{, E.J. Gallas}117_,

V. Gallo16_{, B.J. Gallop}128_{, P. Gallus}124_{, K.K. Gan}108_{, Y.S. Gao}142,e_{, A. Gaponenko}14_{, F. Garberson}175_,

M. Garcia-Sciveres14_{, C. Garc´ıa}166_{, J.E. Garc´ıa Navarro}166_{, R.W. Gardner}30_{, N. Garelli}29_{, H. Garitaonandia}104_,

V. Garonne29_{, C. Gatti}46_{, G. Gaudio}118a_{, B. Gaur}140_{, L. Gauthier}135_{, P. Gauzzi}131a,131b_{, I.L. Gavrilenko}93_,

C. Gay167_{, G. Gaycken}20_{, E.N. Gazis}9_{, P. Ge}32d_{, Z. Gecse}167_{, C.N.P. Gee}128_{, D.A.A. Geerts}104_,

Ch. Geich-Gimbel20_{, K. Gellerstedt}145a,145b_{, C. Gemme}49a_{, A. Gemmell}52_{, M.H. Genest}54_{, S. Gentile}131a,131b_,

M. George53_{, S. George}75_{, P. Gerlach}174_{, A. Gershon}152_{, C. Geweniger}57a_{, H. Ghazlane}134b_{, N. Ghodbane}33_,

B. Giacobbe19a_{, S. Giagu}131a,131b_{, V. Giakoumopoulou}8_{, V. Giangiobbe}11_{, F. Gianotti}29_{, B. Gibbard}24_,

A. Gibson157_{, S.M. Gibson}29_{, D. Gillberg}28_{, A.R. Gillman}128_{, D.M. Gingrich}2,d_{, J. Ginzburg}152_{, N. Giokaris}8_,

M.P. Giordani163c_{, R. Giordano}101a,101b_{, F.M. Giorgi}15_{, P. Giovannini}98_{, P.F. Giraud}135_{, D. Giugni}88a_,

M. Giunta92, P. Giusti19a, B.K. Gjelsten116, L.K. Gladilin96, C. Glasman79, J. Glatzer47, A. Glazov41,

K.W. Glitza174_{, G.L. Glonti}63_{, J.R. Goddard}74_{, J. Godfrey}141_{, J. Godlewski}29_{, M. Goebel}41_{, T. G¨opfert}43_,

C. Goeringer80_{, C. G¨ossling}42_{, S. Goldfarb}86_{, T. Golling}175_{, A. Gomes}123a,b_{, L.S. Gomez Fajardo}41_,

R. Gon¸calo75_{, J. Goncalves Pinto Firmino Da Costa}41_{, L. Gonella}20_{, S. Gonzalez}172_{, S. Gonz´alez de la Hoz}166_,

G. Gonzalez Parra11_{, M.L. Gonzalez Silva}26_{, S. Gonzalez-Sevilla}48_{, J.J. Goodson}147_{, L. Goossens}29_,

P.A. Gorbounov94_{, H.A. Gordon}24_{, I. Gorelov}102_{, G. Gorfine}174_{, B. Gorini}29_{, E. Gorini}71a,71b_{, A. Goriˇsek}73_,

E. Gornicki38_{, B. Gosdzik}41_{, A.T. Goshaw}5_{, M. Gosselink}104_{, M.I. Gostkin}63_{, I. Gough Eschrich}162_,

M. Gouighri134a_{, D. Goujdami}134c_{, M.P. Goulette}48_{, A.G. Goussiou}137_{, C. Goy}4_{, S. Gozpinar}22_,

I. Grabowska-Bold37_{, P. Grafstr¨om}19a,19b_{, K-J. Grahn}41_{, F. Grancagnolo}71a_{, S. Grancagnolo}15_{, V. Grassi}147_,

V. Gratchev120_{, N. Grau}34_{, H.M. Gray}29_{, J.A. Gray}147_{, E. Graziani}133a_{, O.G. Grebenyuk}120_{, T. Greenshaw}72_,

Z.D. Greenwood24,m_{, K. Gregersen}35_{, I.M. Gregor}41_{, P. Grenier}142_{, J. Griffiths}137_{, N. Grigalashvili}63_,

A.A. Grillo136_{, S. Grinstein}11_{, Y.V. Grishkevich}96_{, J.-F. Grivaz}114_{, E. Gross}171_{, J. Grosse-Knetter}53_,

J. Groth-Jensen171_{, K. Grybel}140_{, D. Guest}175_{, C. Guicheney}33_{, S. Guindon}53_{, U. Gul}52_{, H. Guler}84,p_,

J. Gunther124_{, B. Guo}157_{, J. Guo}34_{, P. Gutierrez}110_{, N. Guttman}152_{, O. Gutzwiller}172_{, C. Guyot}135_,

C. Gwenlan117_{, C.B. Gwilliam}72_{, A. Haas}142_{, S. Haas}29_{, C. Haber}14_{, H.K. Hadavand}39_{, D.R. Hadley}17_,

P. Haefner20_{, F. Hahn}29_{, S. Haider}29_{, Z. Hajduk}38_{, H. Hakobyan}176_{, D. Hall}117_{, J. Haller}53_{, K. Hamacher}174_,

P. Hamal112_{, M. Hamer}53_{, A. Hamilton}144b,q_{, S. Hamilton}160_{, L. Han}32b_{, K. Hanagaki}115_{, K. Hanawa}159_,

M. Hance14_{, C. Handel}80_{, P. Hanke}57a_{, J.R. Hansen}35_{, J.B. Hansen}35_{, J.D. Hansen}35_{, P.H. Hansen}35_,

P. Hansson142_{, K. Hara}159_{, G.A. Hare}136_{, T. Harenberg}174_{, S. Harkusha}89_{, D. Harper}86_{, R.D. Harrington}45_,

O.M. Harris137_{, J. Hartert}47_{, F. Hartjes}104_{, T. Haruyama}64_{, A. Harvey}55_{, S. Hasegawa}100_{, Y. Hasegawa}139_,

S. Hassani135_{, S. Haug}16_{, M. Hauschild}29_{, R. Hauser}87_{, M. Havranek}20_{, C.M. Hawkes}17_{, R.J. Hawkings}29_,

A.D. Hawkins78_{, D. Hawkins}162_{, T. Hayakawa}65_{, T. Hayashi}159_{, D. Hayden}75_{, C.P. Hays}117_{, H.S. Hayward}72_,

S. Heisterkamp35_{, L. Helary}21_{, C. Heller}97_{, M. Heller}29_{, S. Hellman}145a,145b_{, D. Hellmich}20_{, C. Helsens}11_,

R.C.W. Henderson70_{, M. Henke}57a_{, A. Henrichs}53_{, A.M. Henriques Correia}29_{, S. Henrot-Versille}114_{, C. Hensel}53_,

T. Henß174_{, C.M. Hernandez}7_{, Y. Hern´andez Jim´enez}166_{, R. Herrberg}15_{, G. Herten}47_{, R. Hertenberger}97_,

L. Hervas29_{, G.G. Hesketh}76_{, N.P. Hessey}104_{, E. Hig´on-Rodriguez}166_{, J.C. Hill}27_{, K.H. Hiller}41_{, S. Hillert}20_,

S.J. Hillier17_{, I. Hinchliffe}14_{, E. Hines}119_{, M. Hirose}115_{, F. Hirsch}42_{, D. Hirschbuehl}174_{, J. Hobbs}147_{, N. Hod}152_,

M.C. Hodgkinson138_{, P. Hodgson}138_{, A. Hoecker}29_{, M.R. Hoeferkamp}102_{, J. Hoffman}39_{, D. Hoffmann}82_,

M. Hohlfeld80_{, M. Holder}140_{, S.O. Holmgren}145a_{, T. Holy}126_{, J.L. Holzbauer}87_{, T.M. Hong}119_,

L. Hooft van Huysduynen107_{, C. Horn}142_{, S. Horner}47_{, J-Y. Hostachy}54_{, S. Hou}150_{, A. Hoummada}134a_,

J. Howard117_{, J. Howarth}81_{, I. Hristova}15_{, J. Hrivnac}114_{, T. Hryn’ova}4_{, P.J. Hsu}80_{, S.-C. Hsu}14_{, Z. Hubacek}126_,

F. Hubaut82_{, F. Huegging}20_{, A. Huettmann}41_{, T.B. Huffman}117_{, E.W. Hughes}34_{, G. Hughes}70_{, M. Huhtinen}29_,

M. Hurwitz14_{, U. Husemann}41_{, N. Huseynov}63,r_{, J. Huston}87_{, J. Huth}56_{, G. Iacobucci}48_{, G. Iakovidis}9_,

M. Ibbotson81_{, I. Ibragimov}140_{, L. Iconomidou-Fayard}114_{, J. Idarraga}114_{, P. Iengo}101a_{, O. Igonkina}104_,

Y. Ikegami64_{, M. Ikeno}64_{, D. Iliadis}153_{, N. Ilic}157_{, T. Ince}20_{, J. Inigo-Golfin}29_{, P. Ioannou}8_{, M. Iodice}133a_,

K. Iordanidou8_{, V. Ippolito}131a,131b_{, A. Irles Quiles}166_{, C. Isaksson}165_{, M. Ishino}66_{, M. Ishitsuka}156_,

R. Ishmukhametov39, C. Issever117, S. Istin18a, A.V. Ivashin127, W. Iwanski38, H. Iwasaki64, J.M. Izen40,

V. Izzo101a_{, B. Jackson}119_{, J.N. Jackson}72_{, P. Jackson}142_{, M.R. Jaekel}29_{, V. Jain}59_{, K. Jakobs}47_{, S. Jakobsen}35_,

T. Jakoubek124_{, J. Jakubek}126_{, D.K. Jana}110_{, E. Jansen}76_{, H. Jansen}29_{, A. Jantsch}98_{, M. Janus}47_{, G. Jarlskog}78_,

L. Jeanty56_{, I. Jen-La Plante}30_{, D. Jennens}85_{, P. Jenni}29_{, P. Jeˇz}35_{, S. J´ez´equel}4_{, M.K. Jha}19a_{, H. Ji}172_{, W. Ji}80_,

J. Jia147_{, Y. Jiang}32b_{, M. Jimenez Belenguer}41_{, S. Jin}32a_{, O. Jinnouchi}156_{, M.D. Joergensen}35_{, D. Joffe}39_,

M. Johansen145a,145b_{, K.E. Johansson}145a_{, P. Johansson}138_{, S. Johnert}41_{, K.A. Johns}6_{, K. Jon-And}145a,145b_,

G. Jones169_{, R.W.L. Jones}70_{, T.J. Jones}72_{, C. Joram}29_{, P.M. Jorge}123a_{, K.D. Joshi}81_{, J. Jovicevic}146_{, T. Jovin}12b_,

X. Ju172_{, C.A. Jung}42_{, R.M. Jungst}29_{, V. Juranek}124_{, P. Jussel}60_{, A. Juste Rozas}11_{, S. Kabana}16_{, M. Kaci}166_,

A. Kaczmarska38_{, P. Kadlecik}35_{, M. Kado}114_{, H. Kagan}108_{, M. Kagan}56_{, E. Kajomovitz}151_{, S. Kalinin}174_,

L.V. Kalinovskaya63_{, S. Kama}39_{, N. Kanaya}154_{, M. Kaneda}29_{, S. Kaneti}27_{, T. Kanno}156_{, V.A. Kantserov}95_,

J. Kanzaki64_{, B. Kaplan}175_{, A. Kapliy}30_{, J. Kaplon}29_{, D. Kar}52_{, M. Karagounis}20_{, K. Karakostas}9_,

M. Karnevskiy41_{, V. Kartvelishvili}70_{, A.N. Karyukhin}127_{, L. Kashif}172_{, G. Kasieczka}57b_{, R.D. Kass}108_,

A. Kastanas13_{, M. Kataoka}4_{, Y. Kataoka}154_{, E. Katsoufis}9_{, J. Katzy}41_{, V. Kaushik}6_{, K. Kawagoe}68_,

T. Kawamoto154_{, G. Kawamura}80_{, M.S. Kayl}104_{, V.A. Kazanin}106_{, M.Y. Kazarinov}63_{, R. Keeler}168_{, R. Kehoe}39_,

M. Keil53_{, G.D. Kekelidze}63_{, J.S. Keller}137_{, M. Kenyon}52_{, O. Kepka}124_{, N. Kerschen}29_{, B.P. Kerˇsevan}73_,

S. Kersten174_{, K. Kessoku}154_{, J. Keung}157_{, F. Khalil-zada}10_{, H. Khandanyan}164_{, A. Khanov}111_{, D. Kharchenko}63_,

A. Khodinov95, A. Khomich57a, T.J. Khoo27, G. Khoriauli20, A. Khoroshilov174, V. Khovanskiy94, E. Khramov63,

J. Khubua50b_{, H. Kim}145a,145b_{, S.H. Kim}159_{, N. Kimura}170_{, O. Kind}15_{, B.T. King}72_{, M. King}65_{, R.S.B. King}117_,

J. Kirk128_{, A.E. Kiryunin}98_{, T. Kishimoto}65_{, D. Kisielewska}37_{, T. Kitamura}65_{, T. Kittelmann}122_{, E. Kladiva}143b_,

M. Klein72_{, U. Klein}72_{, K. Kleinknecht}80_{, M. Klemetti}84_{, A. Klier}171_{, P. Klimek}145a,145b_{, A. Klimentov}24_,

R. Klingenberg42_{, J.A. Klinger}81_{, E.B. Klinkby}35_{, T. Klioutchnikova}29_{, P.F. Klok}103_{, S. Klous}104_{, E.-E. Kluge}57a_,

T. Kluge72_{, P. Kluit}104_{, S. Kluth}98_{, N.S. Knecht}157_{, E. Kneringer}60_{, E.B.F.G. Knoops}82_{, A. Knue}53_{, B.R. Ko}44_,

T. Kobayashi154_{, M. Kobel}43_{, M. Kocian}142_{, P. Kodys}125_{, K. K¨oneke}29_{, A.C. K¨onig}103_{, S. Koenig}80_{, L. K¨opke}80_,

F. Koetsveld103_{, P. Koevesarki}20_{, T. Koffas}28_{, E. Koffeman}104_{, L.A. Kogan}117_{, S. Kohlmann}174_{, F. Kohn}53_,

Z. Kohout126_{, T. Kohriki}64_{, T. Koi}142_{, G.M. Kolachev}106,∗_{, H. Kolanoski}15_{, V. Kolesnikov}63_{, I. Koletsou}88a_,

J. Koll87_{, M. Kollefrath}47_{, A.A. Komar}93_{, Y. Komori}154_{, T. Kondo}64_{, T. Kono}41,s_{, A.I. Kononov}47_,

R. Konoplich107,t_{, N. Konstantinidis}76_{, S. Koperny}37_{, K. Korcyl}38_{, K. Kordas}153_{, A. Korn}117_{, A. Korol}106_,

I. Korolkov11_{, E.V. Korolkova}138_{, V.A. Korotkov}127_{, O. Kortner}98_{, S. Kortner}98_{, V.V. Kostyukhin}20_{, S. Kotov}98_,

V.M. Kotov63_{, A. Kotwal}44_{, C. Kourkoumelis}8_{, V. Kouskoura}153_{, A. Koutsman}158a_{, R. Kowalewski}168_,

T.Z. Kowalski37_{, W. Kozanecki}135_{, A.S. Kozhin}127_{, V. Kral}126_{, V.A. Kramarenko}96_{, G. Kramberger}73_,

M.W. Krasny77_{, A. Krasznahorkay}107_{, J.K. Kraus}20_{, S. Kreiss}107_{, F. Krejci}126_{, J. Kretzschmar}72_{, N. Krieger}53_,

P. Krieger157_{, K. Kroeninger}53_{, H. Kroha}98_{, J. Kroll}119_{, J. Kroseberg}20_{, J. Krstic}12a_{, U. Kruchonak}63_,

H. Kr¨uger20_{, T. Kruker}16_{, N. Krumnack}62_{, Z.V. Krumshteyn}63_{, T. Kubota}85_{, S. Kuday}3a_{, S. Kuehn}47_,

A. Kugel57c_{, T. Kuhl}41_{, D. Kuhn}60_{, V. Kukhtin}63_{, Y. Kulchitsky}89_{, S. Kuleshov}31b_{, C. Kummer}97_{, M. Kuna}77_,

J. Kunkle119_{, A. Kupco}124_{, H. Kurashige}65_{, M. Kurata}159_{, Y.A. Kurochkin}89_{, V. Kus}124_{, E.S. Kuwertz}146_,

M. Kuze156_{, J. Kvita}141_{, R. Kwee}15_{, A. La Rosa}48_{, L. La Rotonda}36a,36b_{, L. Labarga}79_{, J. Labbe}4_{, S. Lablak}134a_,

C. Lacasta166_{, F. Lacava}131a,131b_{, H. Lacker}15_{, D. Lacour}77_{, V.R. Lacuesta}166_{, E. Ladygin}63_{, R. Lafaye}4_,

B. Laforge77_{, T. Lagouri}79_{, S. Lai}47_{, E. Laisne}54_{, M. Lamanna}29_{, L. Lambourne}76_{, C.L. Lampen}6_{, W. Lampl}6_,