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Journal of High Energy Physics. 2024 Aug 20;2024(8):153
The Author(s)
ATLAS Collaboration
A combination of searches for Higgs boson decays into a visible photon and a massless dark photon (H → γγd) is presented using 139 fb−1 of proton-proton collision data at a centre-of-mass energy of √ s = 13 TeV recorded by the ATLAS detector at the Large Hadron Collider. The observed (expected) 95% confdence level upper limit on the Standard Model Higgs boson decay branching ratio is determined to be B(H → γγd) < 1.3% (1.5)%. The search is also sensitive to higher-mass Higgs bosons decaying into the same fnal state. The observed (expected) 95% confdence level limit on the cross-section times branching ratio ranges from 16 fb (20 fb) for mH = 400 GeV to 1.0 fb (1.5 fb) for mH = 3 TeV. Results are also interpreted in the context of a minimal simplifed model.
JHEP08(2024)153PuAlished for SISS Ay SpringerReceived: June 5, 2024Accepted: July 22, 2024Published: August 20, 2024Combination of searches for Higgs boson decays into aphoton and a massless dark photon using pp collisionsat √s = 13TeV with the ATLAS detectorThe ATLAS collaborationE-mail: atlas.publications@cern.chAbstract: A combination of searches for Higgs boson decays into a visible photon and amassless dark photon (H → γγd) is presented using 139 fb−1 of proton-proton collision dataat a centre-of-mass energy of√s = 13TeV recorded by the ATLAS detector at the LargeHadron Collider. The observed (expected) 95% confidence level upper limit on the StandardModel Higgs boson decay branching ratio is determined to be B(H → γγd) < 1.3% (1.5)%.The search is also sensitive to higher-mass Higgs bosons decaying into the same final state.The observed (expected) 95% confidence level limit on the cross-section times branching ratioranges from 16 fb (20 fb) for mH = 400GeV to 1.0 fb (1.5 fb) for mH = 3TeV. Results arealso interpreted in the context of a minimal simplified model.Keywords: Hadron-Hadron Scattering , Higgs PhysicsArXiv ePrint: 2406.01656Open Access, Copyright CERN,for the benefit of the ATLAS Collaboration.Article funded by SCOAP3.https://doi.org/10.1007/JHEP08(2024)153JHEP08(2024)153Contents1 Introduction 12 Description of the input analyses 33 Statistical combination 64 Results and interpretation 75 Conclusion 9The ATLAS collaboration 161 IntroductionThe existence of dark matter is supported by a series of astrophysical observations [1–8], butits unknown fundamental nature remains one of the central questions in particle physics. Thediscovery of a Higgs boson (H ) [9, 10] with a mass of 125GeV at the Large Hadron Collider(LHC) [11] has initiated an extensive effort aimed at investigating its possible connectionwith physics beyond the Standard Model (BSM). In particular, an upper limit of the orderof 10% on the undetected Higgs boson decay branching ratio [12, 13] motivates searchesfor elusive BSM dark sector particles coupled to the Higgs boson. One example of suchparticles is an undetectable, massless dark photon (γd), which acts as the force carrier ofan extra U(1)d gauge group of the dark sector. Dark photons may introduce dark matterself-interactions that can potentially solve the small-scale structure formation problem [14]and the PAMELA-Fermi-AMS2 anomaly [15]. They may also play a role in enhancingthe light dark matter annihilation rate to reach the required phenomenological threshold,thereby making asymmetric dark matter scenarios phenomenologically viable [16]. A potentialapproach to search for this particle is through the Higgs boson decaying into a visible photonand a massless dark photon (H → γγd) [17–23]. This scenario can involve either the StandardModel (SM) Higgs boson (H 125) or additional high-mass Higgs bosons predicted in someBSM theories (HBSM). As the produced γd is invisible to the detector, its signature ischaracterised by missing transverse momentum, whose magnitude is denoted EmissT . The samebehaviour is also exhibited by ultra-light dark photons with masses below the threshold todecay into SM particles or by the lightest supersymmetry particles in a cascaded Higgs-bosondecay [24, 25]. In this paper, the Higgs boson is assumed to be produced via three differentprocesses, including gluon-gluon fusion (ggF), vector-boson fusion (VBF), and in associationwith a Z boson (ZH), with the SM-like production cross-sections [26]. Their leading-orderFeynman diagrams, including the Higgs boson decay, are shown in figure 1.The CMS experiment reported searches for such Higgs boson decays exploiting the ZHproduction mechanism, with an integrated luminosity of 137 fb−1 [27], or via VBF production– 1 –JHEP08(2024)153(a) (b)(c) (d) (e)Figure 1. Leading-order Feynman diagrams for Higgs boson production decaying into a visiblephoton and a massless dark photon. The Higgs boson is produced via different processes: (a) ggF,(b) VBF, (c) qq¯ → ZH and (d) and (e) gg → ZH.with an integrated luminosity of 130 fb−1 [28], where a combination of the two searches isalso performed. Using the 8TeV collision data, the ATLAS and CMS collaborations alsoreported various searches targeting the same γ + EmissT final states [29–31].This paper presents a combined search for H → γγd produced in three distinct final-statesignatures: γ+EmissT +VBF jets (VBF channel1), γ+EmissT +Z(→ ℓℓ, ℓ = e, µ) (ZH channel)and γ + EmissT (ggF channel). The searches under consideration use the full LHC Run 2 datasample corresponding to an integrated luminosity of 139 fb−1 [32, 33] of proton-proton (pp)collision data recorded with the ATLAS detector at a centre-of-mass energy of√s = 13TeV.The results from the VBF channel are derived based on the analysis described in ref. [34], withan extension to higher-mass Higgs bosons and the inclusion of the ggF process contributions.The results for the ZH channel are taken from ref. [35]. The results for the ggF channelare based on the reinterpretation of the mono-γ results in ref. [36] using the RECASTtechnique [37]. Using the available results in the individual publications, the VBF and ZHchannels are combined under the SM Higgs boson assumption, and the VBF and ggF channelsare combined under the additional high-mass Higgs boson hypothesis in the narrow widthapproximation. The range of the HBSM masses probed starts at 400GeV, as the sensitivityof the ggF channel decreases for lower masses, and goes up to 3TeV.The ATLAS detector [38] is a multipurpose particle detector with cylindrical geometry.It consists of an inner tracking detector surrounded by a thin superconducting solenoidproviding a 2T axial magnetic field, electromagnetic and hadronic sampling calorimeters,and a muon spectrometer with three toroidal superconducting magnets, providing a near1In this paper, the term ‘channel’ is used to refer to the final-state signature that defines the event selections.The term ‘process’ refers to the production mode of the Higgs boson. Events from multiple processes cancontribute to a given channel and they are all treated as signal events.– 2 –JHEP08(2024)1534π coverage in solid angle.2 An extensive software suite [39] is used in data simulation, inthe reconstruction and analysis of real and simulated data, in detector operations, and inthe trigger [40] and data acquisition systems of the experiment.Monte Carlo (MC) samples of simulated signal events for the ggF, VBF, and ZH viaboth the qq¯ → ZH and gg → ZH processes were generated at next-to-next-to-leading order(NNLO) for ggF, next-to-leading order (NLO) for VBF and qq¯ → ZH or leading order (LO)for gg → ZH in quantum chromodynamics (QCD) using Powheg v2 [41–44], interfaced toPythia 8 [45] for parton showering, hadronisation, and underlying event modelling, with theAZNLO set of tuned parameters [46]. The signal predictions from these MC samples werenormalised to the NNLO (VBF and ZH) or next-to-NNLO (ggF) cross-section in QCD pluselectroweak corrections at NLO [26, 47–56]. The Higgs boson mass was set to 125GeV forthe SM scenario. For the additional higher-mass Higgs boson scenarios, the mass takes valuesin the 400GeV–1000GeV range, in steps of 200GeV, and in the 1000GeV–3000GeV range,in steps of 500GeV. For the BSM Higgs boson samples, the detector response was simulatedusing a fast parameterised simulation of the ATLAS calorimeters and the full Geant4 [57, 58]simulation was used for the SM Higgs boson samples. Additional pp collisions simulatedusing Pythia 8 [59] with the A3 set of tuned parameters [60] were overlaid to simulate theeffect of multiple interactions in the same and neighbouring bunch crossings (pile-up). Thesimulated events are weighted to reproduce the distribution of the pile-up observed in thedata. These samples are used to check the orthogonality of the channels and produce thefinal results. Descriptions of the data and simulation samples used to model backgroundsfrom SM processes can be found in refs. [34–36].2 Description of the input analysesThe detailed information about the reconstruction, identification and calibration of physicsobjects used for analysis selections described below is given in refs. [34–36, 61–69]. A briefoverview of the already published Run 2 searches relevant to the combination performed hereis given below. The H 125 → γγd search is performed in the VBF and ZH channels whileHBSM → γγd is probed in the VBF and ggF channels. No significant deviation from the SMprediction is observed in any of these studies. All searches utilise the signature of an isolatedphoton and EmissT , with variations on the number of selected leptons and jets.Events in the VBF channel were selected with the EmissT trigger algorithm [70]. They arefurther required to have EmissT > 150GeV and two VBF jets. The VBF jets are the leadingand subleading transverse momentum (pT) jets, denoted j1 and j2, satisfying pj1T > 60GeVand pj2T > 50GeV, respectively. In addition, they are required to have a large pseudorapidityseparation (|∆ηj1j2 | > 3, ηj1 · ηj2 < 0), a large invariant mass (mj1j2 > 250GeV) and not beback-to-back in azimuthal angle (∆ϕj1j2 < 2). An additional jet is allowed with pj3T > 25GeV2ATLAS uses a right-handed coordinate system with its origin at the nominal interaction point (IP) in thecentre of the detector and the z-axis along the beam pipe. The x-axis points from the IP to the centre ofthe LHC ring, and the y-axis points upwards. Polar coordinates (r, ϕ) are used in the transverse plane, ϕbeing the azimuthal angle around the z-axis. The pseudorapidity is defined in terms of the polar angle θ asη = − ln tan(θ/2) and is equal to the rapidity y = 12 ln(E+pzcE−pzc)in the relativistic limit. Angular distance ismeasured in units of ∆R ≡√(∆y)2 + (∆ϕ)2.– 3 –JHEP08(2024)153and a centrality3 of Cj3 < 0.7. Events with a reconstructed lepton (ℓ = e, µ) are rejected.The photon must be isolated and lie in the electromagnetic calorimeter acceptance |ηγ | < 2.37but not in the transition region (1.37 < |ηγ | < 1.52) between the barrel and endcap. Theseisolation and η requirements on the photon are used in all three analyses in addition to energy-related criteria specific to the different analyses. In the VBF analysis discussed here, thephoton is required to have 15GeV < EγT < max(110GeV, 0.733×mT), where the transversemass mT is defined as mT(γ,EmissT ) =√2EγTEmissT[1− cos(ϕγ − ϕEmissT )], bounded above bythe Higgs boson mass. The centrality of the photon is required to be Cγ > 0.4. To increasethe sensitivity of the search, events are categorised in ten signal regions (SRs) based on mjjand mT. The dominant backgrounds are W (→ ℓν)γ+ jets events, in which the lepton fromthe W boson decay is lost if it falls outside of the acceptance, and Z(→ νν)γ+ jets events.Four dedicated control regions (CRs) are designed to capture the background contributionsfrom W (→ eν)γ+ jets, W (→ µν)γ+ jets, Z(→ νν)γ+ jets and processes where electronsare misidentified as fake photons. Backgrounds due to jets misidentified as fake photonsare estimated by using a data-driven method. Contribution from the ggF process was notconsidered in the original analysis [34] but is included for this combination. All SRs and CRsare simultaneously fitted using the profile likelihood fit method to constrain the backgroundcontributions and to extract the signal contribution.In the ZH channel, Z → ℓ+ℓ− events were selected with single-lepton and dileptontriggers [71, 72]. Events are required to contain two same-flavour, oppositely charged (SFOC)leptons with invariant mass 76GeV < mℓℓ < 116GeV. Furthermore, they are required to haveEmissT > 60GeV and a photon with EγT > 25GeV satisfying the isolation and η selections. Theselected objects are required to satisfy ∆ϕ(EmissT , pℓℓγT ) > 2.4 and mℓℓγ > 100GeV. Eventswith a third lepton with pT > 10GeV or any b-tagged jet (77% working point [73]) are rejected.To enhance the sensitivity of the search, a boosted decision tree (BDT) algorithm is applied toseparate the signal from the backgrounds. The dominant background contribution comes fromEmissT mismeasurement in mainly Zγ+ jets and Z + jets processes due to undetected particlesor hadronic jets not fully contained in the detector acceptance. Another major backgroundis from electrons misidentified as photons in the SM diboson processes. Both of thesebackgrounds are estimated with data-driven techniques. The irreducible V V γ (V = W,Z)background with both V decaying leptonically is constrained in the fit by a dedicated CR.Backgrounds from top quark and Higgs boson production are found to be minor and estimatedfrom MC simulations. Contributions from ggF and VBF produced Higgs boson processes tothe ZH channel are assumed to be negligible and therefore not considered. A simultaneous fitexploiting the distribution of the BDT discriminant and the single bin V V γ CR is performed.Events in the ggF channel were selected with a single photon trigger with a threshold ofEγT > 140GeV [71]. Events are required to have EmissT > 200GeV and at least one photonsatisfying the isolation and η selections. The leading photon in the events is required tofulfil the following criteria: the transverse energy EγT > 150GeV, the separation between its3The centrality of an object i in this channel is defined as Ci = exp[− 4(ηj1−ηj2 )2(ηi−ηj1+ηj22)2]. Whenthe object i is centred between the two jets, Ci reaches the maximum value of 1. When the object i is alignedwith one of the two jets, Ci decreases to 1/e.– 4 –JHEP08(2024)1532−101−10110210310410510610710810Eventsγ)ννZ( (e)γFake (jet)γFake γ)νW(l+jetγ γZ(ll)SM Total Data:dγγ→Signal (ggF+VBF) H = 400 GeVHm = 800 GeVHm = 1.5 TeVHm = 3.0 TeVHmATLAS-1 = 13 TeV, 139 fbsPost-fit, SR200 250 300 350 400 450 [GeV]missTE0.80.911.11.2Data / Bkg Figure 2. Number of events in each EmissT bin in the SR of the ggF channel after a background-only fit.The signals HBSM → γγd are superimposed onto the observed data and the expected SM background.The ggF and VBF processes are considered, assuming B(HBSM → γγd) = 5% and the productioncross-sections from ref. [26]. The error bars on data represent the statistical uncertainty, and theshaded band includes statistical and systematic uncertainties determined from the fit. The lowerpanel shows the ratio of observed data to expected SM background yields. The last bin includes theoverflow. This analysis is reinterpreted from the mono-γ results in ref. [36].extrapolated origin and primary vertex of the event along the beam axis |∆zγ | < 250mmand ∆ϕ(γ,EmissT ) > 0.4. At most one jet is allowed in the selection if pjT > 30GeV, |ηj | < 4.5and ∆ϕ(j, EmissT ) > 0.4. Events that contain leptons (ℓ = e, µ, hadronically decaying τ) arerejected. To improve the sensitivity, four SRs are defined corresponding to different EmissTranges. The SM background arises from several processes with either true photons or fakephotons from misidentified electrons or jets. The background with true photons is dominatedby the SM Z(→ νν)γ process. Secondary contributions come from γ + jets events and fromW (→ ℓν)γ and Z(→ ℓℓ)γ production with unidentified electrons, muons or with hadronicallydecaying τ -leptons. Four CRs are defined to estimate the contributions of these true-photonprocesses in the SRs through the profile likelihood fit. The fake photon backgrounds areestimated with control samples that contain electrons or jets, scaled by misidentificationrates determined from data. Signal contributions from both the ggF and VBF Higgs bosonprocesses are considered. Figure 2 shows the EmissT distribution in the SR after a background-only fit to data. Signals with higher mass tend to have larger EmissT . The highest EmissT SRcaptures about 30% of the events for signal benchmarks with mH ≥ 1.0TeV.Theoretical uncertainties due to the QCD factorisation and renormalisation scales, andthe choice of parton distribution functions are included. Uncertainties in initial- and final-stateradiation due to the choice of parton shower parameters are estimated through simulationswith alternative sets of tuned parameters.The event selections for the input channels are summarised in table 1. To perform thecombination, a few adjustments are made. In the VBF channel, the contribution of the ggF– 5 –JHEP08(2024)153Channels VBF ZH ggFTrigger EmissT Lepton(s) PhotonPhotons = 1, Cγ > 0.4 = 1 ≥ 1EγT [GeV] ∈ (15,max(110, 0.733×mT)) > 25 > 150EmissT [GeV] > 150 > 60 > 200Jets 2 or 3, mj1j2 > 250GeV, |∆ηj1j2 | > 3 ≤ 2 ≤ 1ηj1 · ηj2 < 0, ∆ϕj1j2 < 2, Cj3 < 0.7Leptons = 0 (e, µ) = 2, SFOC = 0 (e, µ, τ)mℓℓ ∈ (76, 116) GeVDisc. variables mjj and mT in SR and 4 CRs BDT score and 1 CR EmissTReference [34] [35] [36]Processes consideredin the combination VBF, ggF ZH ggF, VBFCombination scenario SM, BSM SM BSMTable 1. Summary of the main event selections, discriminating variables and processes considered inthe input channels. The definition of the variables is provided in the text.process to the BSM Higgs boson decay search is included using the RECAST technique. Thecontribution to the signal yields is up to 30% for the low masses and decreases to 1% forthe high masses. Additional BSM Higgs boson signal samples are generated to align withthe masses probed in the ggF analysis. The fit regions used in the three analyses are eitherorthogonal due to variations in the number and type of physics objects required in their finalstates or have a negligible number of overlapping events due to different jet algorithms beingused. They are therefore treated as statistically independent.3 Statistical combinationThe results of the combination presented in this paper are obtained from a likelihood functionL(µ, θ⃗ ), where µ denotes the parameter of interest (POI) of the model, and θ⃗ constitutes a setof nuisance parameters, encoding the systematic uncertainty contributions and backgroundnormalisation factors that are constrained by CRs in data. The final likelihood functionL(µ, θ⃗ ) is the product of the likelihoods from individual channels within the combination,which are themselves products of likelihoods computed from the final observables in variouscategories in a single analysis. To derive upper limits on the POI, the profile-likelihood-ratiotest statistic is used with the CLs method [74] following the asymptotic formulae [75].All systematic uncertainties that are considered in the individual analyses are included inthe combination and those that stem from common sources are treated as correlated among theinput searches. A complete discussion of their sources can be found in the individual channel– 6 –JHEP08(2024)153publications [34–36]. Systematic uncertainties related to the data-taking conditions, such asthose associated with the integrated luminosity and the modelling of pile-up, are treated ascorrelated. Experimental uncertainties related to physics objects used by multiple searchesare treated as correlated where appropriate, with the following exceptions. Uncertaintiesrelated to the same object but implemented with different reduced uncertainty schemes aretreated as uncorrelated. In addition, uncertainties that were heavily constrained or pulledin the original input channel are treated as uncorrelated, and the impact on the final upperlimits would be ≤ 3% if they were correlated. These constraining powers come from thespecial phase space probed in certain channels and therefore passing these constraints tothe other channels should be avoided. Uncertainties related to background modelling areconsidered as uncorrelated since the composition and phase space of the backgrounds aredifferent. Uncertainties related to signal modelling, stemming from the choice of partondistribution functions and QCD calculations, have minor impact on the final results and aretreated as uncorrelated. Ignoring correlations of the systematic uncertainties between theinput channels is found to impact the upper limits by ≤ 2%. The H 125 → γγd search hassimilar impacts from the data statistical (66%) and systematic (75%) uncertainties, wherethe values are relative to the total uncertainty. The dominant contributions to the systematicuncertainties stem from the background modelling (47%), jet and EmissT calibration (40%),followed by the MC statistical uncertainty (36%) and fake-background estimate (35%). All ofthese impacts are evaluated from the quadratic differences of the fitted errors in the POIbefore and after fixing the considered nuisance parameters to their best-fit values. In theHBSM → γγd search, the statistical uncertainty increases from 75% to 86% for the higherHiggs boson mass assumptions. The dominant contributions come from the fake-backgroundestimate, which decreases from 52% to 29% depending on the mass, and background modellinguncertainty, ranging from 27%–38%. The uncertainties related to jet and EmissT , leptons, andMC sample size share a similar ∼ 20% impact each.4 Results and interpretationThis combination yields an observed (expected) 95% confidence level (CL) upper limit on thebranching ratio B(H 125 → γγd) is 1.3% (1.5%). Relative to the most stringent result fromthe VBF analysis, this combination brings an improvement of 29% (14%) in the sensitivity.The limits are displayed in figure 3(a). The observed (expected) 95% CL upper limits onthe BSM Higgs boson production cross-section times B(HBSM → γγd) as a function of theBSM Higgs boson mass mH , obtained from this combination, are shown in figure 3(b). Theobserved (expected) limit ranges from 16 fb (26 fb) for mH = 400GeV to 1.0 fb (1.5 fb) formH = 3000GeV. Assuming a branching ratio B(HBSM → γγd) of 5% and theoreticallypredicted cross-sections for HBSM production from ref. [26], masses of HBSM below around1600GeV (1500GeV) are excluded. Relative to the leading ggF channel, the combinationwith the VBF channel yields an improvement of 33% (14%) on the cross-section timesB(HBSM → γγd) at mH = 1500GeV.Additionally, the results on B(H 125 → γγd) are interpreted under a minimal simplifiedmodel described in refs. [17, 76]. The model assumes the SM prediction for the cross-sectionand its systematic uncertainties for all Higgs boson production modes. It introduces a generic– 7 –JHEP08(2024)1530 1 2 3 4 5 6 7 895% CL upper limit on (Hd) [%]CombinedVBF channelZH channelATLAS s = 13 TeV, 139 fb1SM Hd1.3 1.51.8 1.72.3 2.8Obs. Exp.Observed limit (95% CL)Expected limit (95% CL)Expected limit ±1Expected limit ±2(a)500 1000 1500 2000 2500 3000mH [GeV]10310210110095% CL upper limit on ×ggF+VBF [pb]ATLAS s= 13 TeV, 139 fb1BSM HdObserved limit (95% CL)Expected limit (95% CL)Expected limit ±1Expected limit ±2( = 0.05) ×theoryVBF channelggF channelCombined(b)Figure 3. Observed and expected 95% CL upper limits on (a) the branching ratio B(H 125 → γγd)and (b) B(HBSM → γγd) times the BSM Higgs boson ggF + VBF production cross-section σggF+VBFas a function of the Higgs boson mass mH . Results obtained from the input channels are overlaid. Theexpected limit and the corresponding error bands are derived assuming the absence of the H → γγdprocess and with all nuisance parameters profiled to the observed data. The theory predictions andtheir error band are taken from ref. [26] assuming a branching ratio B(HBSM → γγd) = 5%.messenger sector consisting of one left-doublet and one right-singlet of the SU(2)L gaugegroup connecting the dark and the observable sectors. A minimal scenario can be realisedunder mass universality in the left and right messenger sector with a mixing parameterξ. Under this scenario, the messenger sector couples to both U(1) and U(1)d gauge fields,allowing three Higgs boson decay modes: γγd, γdγd and γγ. Their branching ratios are allinterconnected and can be expressed using two free, dimensionless parameters: ξ and thefine structure constant αd associated with the U(1)d gauge group [76], whose values are zeroin the SM. Hence, setting upper limits on, or measuring the value of the branching ratioof the Higgs boson decaying into γγ, γγd, and γdγd can be translated into restrictions onthe allowed parameter space in the (αd, ξ) plane. The range 0 < αd < 1 and 0 ≤ ξ < 1 isexplored in this study. An extra parameter χ = ±1 accounts for the relative sign of the newphysics and SM contributions in the amplitudes of the H 125 → γγ and H 125 → gg decays. Itprovides two scenarios with either constructive (χ = +1) or destructive (χ = −1) interferencebetween the messenger sector and the SM particles affecting the B(H 125 → γγ).Figure 4 shows the observed exclusion limits derived from the combination of the VBF andZH channels for H 125 → γγd and from the reinterpretation of the ATLAS search for H 125 →invisible [77]. In addition, the ATLAS measurement of B(H 125 → γγ) = 0.247+0.022−0.020% [12]provides a one standard deviation (σ) upper bound. The SM predicted B(H 125 → γγ) definesa region in the (αd, ξ) parameter space of the minimal model that is not allowed whenassuming a positive interference from the messenger sector in the γγ final state (χ = +1).From the reinterpretation of the B(H 125 → invisible) result in terms of a H 125 → γdγdsignal, values down to about ξ ≃ 0.7 at αd = 1 are excluded for χ = +1. The H 125 → γγdcombination presented here provides additional sensitivity in the low αd region, which isalso disfavoured by the B(H 125 → γγ) measurement. The χ = −1 scenario has also beeninvestigated but no constraints can be placed in this case.– 8 –JHEP08(2024)1530 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1dα0.60.650.70.750.80.850.90.951ξ Observed 95% CLdγγ→H combinationZHVBF-inv Observed 95% CL→HPLB 842 (2023) 137963% -0.020+0.022) = 0.247γγ→125HBR( ATLAS measurementγγ→HNature 607 (2022) 52) = 0.227%γγ→125HBR( SM predictionγγ→HarXiv:1610.07922ATLAS-1 = 13 TeV, 139 fbsDark Photon Minimal Model = +1χ = 125 GeV, HmSM pred.σATLAS meas. + 1ATLAS meas.Figure 4. Observed 95% CL exclusion regions in the (αd, ξ) parameter space from the VBF-ZHcombination of H 125 → γγd searches (dark coloured area) and the reinterpretation of the ATLASmeasured limit of B(H 125 → invisible) as H 125 → γdγd (light coloured area). Both the central value(dashed line) and the +1σ upper bound (dashed-hashed line) show the less favoured (αd, ξ) planeobtained from the current ATLAS measurement of B(H 125 → γγ). The dash-dotted line and theassociated dashed area show the parameter space that is not allowed by the SM B(H 125 → γγ)predictions assuming positive interference with the minimal messenger sector. The parameter χ = +1parameterises the relative sign of the new physics and SM contributions in the amplitudes of theH 125 → γγ and H 125 → gg decays.5 ConclusionIn conclusion, this paper reports a combined search for H → γγd produced in ggF, VBF, andZH processes using 139 fb−1 of pp collision data at√s = 13TeV collected by the ATLASdetector at the LHC. Various Higgs boson mass assumptions are probed including the SMvalue of 125GeV and higher values ranging from 400GeV to 3TeV. The combined analysis setsan observed (expected) 95% CL upper limit on B(H 125 → γγd) at 1.3 (1.5)%. The observed(expected) 95% confidence level limit on the cross-section times branching ratio ranges from16 fb (26 fb) formH = 400GeV to 1.0 fb (1.5 fb) formH = 3TeV. This study provides the moststringent constraints on Higgs bosons decaying into a photon and a massless dark photon todate. The results are also interpreted in the context of a minimal simplified model, providingcomplementary exclusion in the parameter space obtained from other searches for this model.AcknowledgmentsWe thank CERN for the very successful operation of the LHC and its injectors, as wellas the support staff at CERN and at our institutions worldwide without whom ATLAScould not be operated efficiently.The crucial computing support from all WLCG partners is acknowledged gratefully, inparticular from CERN, the ATLAS Tier-1 facilities at TRIUMF/SFU (Canada), NDGF– 9 –JHEP08(2024)153(Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF(Italy), NL-T1 (The Netherlands), PIC (Spain), RAL (U.K.) and BNL (U.S.A.), the Tier-2facilities worldwide and large non-WLCG resource providers. Major contributors of computingresources are listed in ref. [78].We gratefully acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC,Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; CNPq and FAPESP, Brazil;NSERC, NRC and CFI, Canada; CERN; ANID, Chile; CAS, MOST and NSFC, China;Minciencias, Colombia; MEYS CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS and CEA-DRF/IRFU, France; SRNSFG, Georgia; BMBF, HGF and MPG, Germany;GSRI, Greece; RGC and Hong Kong SAR, China; ISF and Benoziyo Center, Israel; INFN,Italy; MEXT and JSPS, Japan; CNRST, Morocco; NWO, The Netherlands; RCN, Norway;MNiSW, Poland; FCT, Portugal; MNE/IFA, Romania; MESTD, Serbia; MSSR, Slovakia;ARRS and MIZŠ, Slovenia; DSI/NRF, South Africa; MICINN, Spain; SRC and WallenbergFoundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST,Taipei; TENMAK, Türkiye; STFC, United Kingdom; DOE and NSF, United States ofAmerica.Individual groups and members have received support from BCKDF, CANARIE, CRCand DRAC, Canada; CERN-CZ, FORTE and PRIMUS, Czech Republic; COST, ERC, ERDF,Horizon 2020, ICSC-NextGenerationEU and Marie Skłodowska-Curie Actions, EuropeanUnion; Investissements d’Avenir Labex, Investissements d’Avenir Idex and ANR, France; DFGand AvH Foundation, Germany; Herakleitos, Thales and Aristeia programmes co-financed byEU-ESF and the Greek NSRF, Greece; BSF-NSF and MINERVA, Israel; NCN and NAWA,Poland; La Caixa Banking Foundation, CERCA Programme Generalitat de Catalunya andPROMETEO and GenT Programmes Generalitat Valenciana, Spain; Göran GustafssonsStiftelse, Sweden; The Royal Society and Leverhulme Trust, United Kingdom.In addition, individual members wish to acknowledge support from Armenia: YerevanPhysics Institute (FAPERJ); CERN: European Organization for Nuclear Research (CERNPJAS); Chile: Agencia Nacional de Investigación y Desarrollo (FONDECYT 1230812, FONDE-CYT 1230987, FONDECYT 1240864); China: Chinese Ministry of Science and Technology(MOST-2023YFA1605700), National Natural Science Foundation of China (NSFC - 12175119,NSFC 12275265, NSFC-12075060); Czech Republic: Czech Science Foundation (GACR - 24-11373S), Ministry of Education Youth and Sports (FORTE CZ.02.01.01/00/22_008/0004632),PRIMUS Research Programme (PRIMUS/21/SCI/017); EU: H2020 European ResearchCouncil (ERC — 101002463); European Union: European Research Council (ERC — 948254,ERC 101089007), Horizon 2020 Framework Programme (MUCCA — CHIST-ERA-19-XAI-00), European Union, Future Artificial Intelligence Research (FAIR-NextGenerationEUPE00000013), Italian Center for High Performance Computing, Big Data and QuantumComputing (ICSC, NextGenerationEU); France: Agence Nationale de la Recherche (ANR-20-CE31-0013, ANR-21-CE31-0013, ANR-21-CE31-0022), Investissements d’Avenir Labex (ANR-11-LABX-0012); Germany: Baden-Württemberg Stiftung (BW Stiftung-Postdoc Elitepro-gramme), Deutsche Forschungsgemeinschaft (DFG — 469666862, DFG — CR 312/5-2);Italy: Istituto Nazionale di Fisica Nucleare (ICSC, NextGenerationEU); Japan: JapanSociety for the Promotion of Science (JSPS KAKENHI JP22H01227, JSPS KAKENHIJP22H04944, JSPS KAKENHI JP22KK0227, JSPS KAKENHI JP23KK0245); The Nether-– 10 –JHEP08(2024)153lands: Netherlands Organisation for Scientific Research (NWO Veni 2020 — VI.Veni.202.179);Norway: Research Council of Norway (RCN-314472); Poland: Polish National Agency forAcademic Exchange (PPN/PPO/2020/1/00002/U/00001), Polish National Science Cen-tre (NCN 2021/42/E/ST2/00350, NCN OPUS nr 2022/47/B/ST2/03059, NCN UMO-2019/34/E/ST2/00393, UMO-2020/37/B/ST2/01043, UMO-2021/40/C/ST2/00187, UMO-2022/47/O/ST2/00148, UMO-2023/49/B/ST2/04085); Slovenia: Slovenian Research Agency(ARIS grant J1-3010); Spain: Generalitat Valenciana (Artemisa, FEDER, IDIFEDER/2018/048), Ministry of Science and Innovation (MCIN & NextGenEU PCI2022-135018-2, MICIN& FEDER PID2021-125273NB, RYC2019-028510-I, RYC2020-030254-I, RYC2021-031273-I,RYC2022-038164-I), PROMETEO and GenT Programmes Generalitat Valenciana (CIDE-GENT/2019/027); Sweden: Swedish Research Council (Swedish Research Council 2023-04654,VR 2018-00482, VR 2022-03845, VR 2022-04683, VR 2023-03403, VR grant 2021-03651), Knutand Alice Wallenberg Foundation (KAW 2018.0157, KAW 2018.0458, KAW 2019.0447, KAW2022.0358); Switzerland: Swiss National Science Foundation (SNSF — PCEFP2_194658);United Kingdom: Leverhulme Trust (Leverhulme Trust RPG-2020-004), Royal Society(NIF-R1-231091); United States of America: U.S. Department of Energy (ECA DE-AC02-76SF00515), Neubauer Family Foundation.Open Access. 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Augsten 135, S. Auricchio 73a,73b, A.D. Auriol 21, V.A. Austrup 103,G. Avolio 37, K. Axiotis 57, G. Azuelos 110,ac, D. Babal 29b, H. Bachacou 138, K. Bachas 155,o,A. Bachiu 35, F. Backman 48a,48b, A. Badea 40, T.M. Baer 108, P. Bagnaia 76a,76b,M. Bahmani 19, D. Bahner 55, K. Bai 126, J.T. Baines 137, L. Baines 96, O.K. Baker 175,E. Bakos 16, D. Bakshi Gupta 8, L.E. Balabram Filho 84b, V. Balakrishnan 123,R. Balasubramanian 4, E.M. Baldin 38, P. Balek 87a, E. Ballabene 24b,24a, F. Balli 138,L.M. Baltes 64a, W.K. Balunas 33, J. Balz 102, I. Bamwidhi 119b, E. Banas 88,M. Bandieramonte 132, A. Bandyopadhyay 25, S. Bansal 25, L. Barak 154, M. Barakat 49,E.L. Barberio 107, D. Barberis 58b,58a, M. Barbero 104, M.Z. Barel 117, T. Barillari 112,M-S. Barisits 37, T. Barklow 146, P. Baron 125, D.A. Baron Moreno 103, A. Baroncelli 63a,A.J. Barr 129, J.D. Barr 98, F. Barreiro 101, J. Barreiro Guimarães da Costa 14, U. Barron 154,M.G. Barros Teixeira 133a, S. Barsov 38, F. Bartels 64a, R. Bartoldus 146, A.E. Barton 93,P. Bartos 29a, A. Basan 102, M. Baselga 50, A. Bassalat 67,b, M.J. Basso 159a, S. Bataju 45,R. Bate 167, R.L. Bates 60, S. Batlamous101, B. Batool 144, M. Battaglia 139, D. Battulga 19,M. Bauce 76a,76b, M. Bauer 80, P. Bauer 25, L.T. Bazzano Hurrell 31, J.B. Beacham 52,T. Beau 130, J.Y. Beaucamp 92, P.H. Beauchemin 161, P. Bechtle 25, H.P. Beck 20,n,– 16 –JHEP08(2024)153K. Becker 170, A.J. Beddall 83, V.A. Bednyakov 39, C.P. Bee 148, L.J. Beemster 16,T.A. Beermann 37, M. Begalli 84d, M. Begel 30, A. Behera 148, J.K. Behr 49, J.F. Beirer 37,F. Beisiegel 25, M. Belfkir 119b, G. Bella 154, L. Bellagamba 24b, A. Bellerive 35, P. Bellos 21,K. Beloborodov 38, D. Benchekroun 36a, F. Bendebba 36a, Y. Benhammou 154,K.C. Benkendorfer 62, L. Beresford 49, M. Beretta 54, E. Bergeaas Kuutmann 164, N. Berger 4,B. Bergmann 135, J. Beringer 18a, G. Bernardi 5, C. Bernius 146, F.U. Bernlochner 25,F. Bernon 37,104, A. Berrocal Guardia 13, T. Berry 97, P. Berta 136, A. Berthold 51,S. Bethke 112, A. Betti 76a,76b, A.J. Bevan 96, N.K. Bhalla 55, S. Bhatta 148,D.S. Bhattacharya 169, P. Bhattarai 146, K.D. Bhide 55, V.S. Bhopatkar 124, R.M. Bianchi 132,G. Bianco 24b,24a, O. Biebel 111, R. Bielski 126, M. Biglietti 78a, C.S. Billingsley45,Y. Bimgdi 36f , M. Bindi 56, A. Bingul 22b, C. Bini 76a,76b, G.A. Bird 33, M. Birman 172,M. Biros 136, S. Biryukov 149, T. Bisanz 50, E. Bisceglie 44b,44a, J.P. Biswal 137,D. Biswas 144, I. Bloch 49, A. Blue 60, U. Blumenschein 96, J. Blumenthal 102,V.S. Bobrovnikov 38, M. Boehler 55, B. Boehm 169, D. Bogavac 37, A.G. Bogdanchikov 38,L.S. Boggia 130, C. Bohm 48a, V. Boisvert 97, P. Bokan 37, T. Bold 87a, M. Bomben 5,M. Bona 96, M. Boonekamp 138, C.D. Booth 97, A.G. Borbély 60, I.S. Bordulev 38,G. Borissov 93, D. Bortoletto 129, D. Boscherini 24b, M. Bosman 13, J.D. Bossio Sola 37,K. Bouaouda 36a, N. Bouchhar 166, L. Boudet 4, J. Boudreau 132, E.V. Bouhova-Thacker 93,D. Boumediene 41, R. Bouquet 58b,58a, A. Boveia 122, J. Boyd 37, D. Boye 30, I.R. Boyko 39,L. Bozianu 57, J. Bracinik 21, N. Brahimi 4, G. Brandt 174, O. Brandt 33, F. Braren 49,B. Brau 105, J.E. Brau 126, R. Brener 172, L. Brenner 117, R. Brenner 164, S. Bressler 172,G. Brianti 79a,79b, D. Britton 60, D. Britzger 112, I. Brock 25, G. Brooijmans 42,E.M. Brooks 159b, E. Brost 30, L.M. Brown 168, L.E. Bruce 62, T.L. Bruckler 129,P.A. Bruckman de Renstrom 88, B. Brüers 49, A. Bruni 24b, G. Bruni 24b, M. Bruschi 24b,N. Bruscino 76a,76b, T. Buanes 17, Q. Buat 141, D. Buchin 112, A.G. Buckley 60,O. Bulekov 38, B.A. Bullard 146, S. Burdin 94, C.D. Burgard 50, A.M. Burger 37,B. Burghgrave 8, O. Burlayenko 55, J. Burleson 165, J.T.P. Burr 33, J.C. Burzynski 145,E.L. Busch 42, V. Büscher 102, P.J. Bussey 60, J.M. Butler 26, C.M. Buttar 60,J.M. Butterworth 98, W. Buttinger 137, C.J. Buxo Vazquez 109, A.R. Buzykaev 38,S. Cabrera Urbán 166, L. Cadamuro 67, D. Caforio 59, H. Cai 132, Y. Cai 14,114c, Y. Cai 114a,V.M.M. Cairo 37, O. Cakir 3a, N. Calace 37, P. Calafiura 18a, G. Calderini 130,P. Calfayan 69, G. Callea 60, L.P. Caloba84b, D. Calvet 41, S. Calvet 41, M. Calvetti 75a,75b,R. Camacho Toro 130, S. Camarda 37, D. Camarero Munoz 27, P. Camarri 77a,77b,M.T. Camerlingo 73a,73b, D. Cameron 37, C. Camincher 168, M. Campanelli 98,A. Camplani 43, V. Canale 73a,73b, A.C. Canbay 3a, E. Canonero 97, J. Cantero 166,Y. Cao 165, F. Capocasa 27, M. Capua 44b,44a, A. Carbone 72a,72b, R. Cardarelli 77a,J.C.J. Cardenas 8, G. Carducci 44b,44a, T. Carli 37, G. Carlino 73a, J.I. Carlotto 13,B.T. Carlson 132,p, E.M. Carlson 168,159a, J. Carmignani 94, L. Carminati 72a,72b,A. Carnelli 138, M. Carnesale 76a,76b, S. Caron 116, E. Carquin 140f , I.B. Carr 107,S. Carrá 72a, G. Carratta 24b,24a, A.M. Carroll 126, T.M. Carter 53, M.P. Casado 13,h,M. Caspar 49, F.L. Castillo 4, L. Castillo Garcia 13, V. Castillo Gimenez 166,N.F. Castro 133a,133e, A. Catinaccio 37, J.R. Catmore 128, T. Cavaliere 4, V. Cavaliere 30,N. Cavalli 24b,24a, L.J. Caviedes Betancourt23b, Y.C. Cekmecelioglu 49, E. Celebi 83, S. Cella 37,– 17 –JHEP08(2024)153F. Celli 129, M.S. Centonze 71a,71b, V. Cepaitis 57, K. Cerny 125, A.S. Cerqueira 84a,A. Cerri 149, L. Cerrito 77a,77b, F. Cerutti 18a, B. Cervato 144, A. Cervelli 24b, G. Cesarini 54,S.A. Cetin 83, D. Chakraborty 118, J. Chan 18a, W.Y. Chan 156, J.D. Chapman 33,E. Chapon 138, B. Chargeishvili 152b, D.G. Charlton 21, M. Chatterjee 20, C. Chauhan 136,Y. Che 114a, S. Chekanov 6, S.V. Chekulaev 159a, G.A. Chelkov 39,a, A. Chen 108,B. Chen 154, B. Chen 168, H. Chen 114a, H. Chen 30, J. Chen 63c, J. Chen 145, M. Chen 129,S. Chen 89, S.J. Chen 114a, X. Chen 63c, X. Chen 15,ab, Y. Chen 63a, C.L. Cheng 173,H.C. Cheng 65a, S. Cheong 146, A. Cheplakov 39, E. Cheremushkina 49, E. Cherepanova 117,R. Cherkaoui El Moursli 36e, E. Cheu 7, K. Cheung 66, L. Chevalier 138, V. Chiarella 54,G. Chiarelli 75a, N. Chiedde 104, G. Chiodini 71a, A.S. Chisholm 21, A. Chitan 28b,M. Chitishvili 166, M.V. Chizhov 39, K. Choi 11, Y. Chou 141, E.Y.S. Chow 116, K.L. Chu 172,M.C. Chu 65a, X. Chu 14,114c, Z. Chubinidze 54, J. Chudoba 134, J.J. Chwastowski 88,D. Cieri 112, K.M. Ciesla 87a, V. Cindro 95, A. Ciocio 18a, F. Cirotto 73a,73b, Z.H. Citron 172,M. Citterio 72a, D.A. Ciubotaru28b, A. Clark 57, P.J. Clark 53, N. Clarke Hall 98,C. Clarry 158, J.M. Clavijo Columbie 49, S.E. Clawson 49, C. Clement 48a,48b, Y. Coadou 104,M. Cobal 70a,70c, A. Coccaro 58b, R.F. Coelho Barrue 133a, R. Coelho Lopes De Sa 105,S. Coelli 72a, B. Cole 42, J. Collot 61, P. Conde Muiño 133a,133g, M.P. Connell 34c,S.H. Connell 34c, E.I. Conroy 129, F. Conventi 73a,ad, H.G. Cooke 21, A.M. Cooper-Sarkar 129,F.A. Corchia 24b,24a, A. Cordeiro Oudot Choi 130, L.D. Corpe 41, M. Corradi 76a,76b,F. Corriveau 106,w, A. Cortes-Gonzalez 19, M.J. Costa 166, F. Costanza 4, D. Costanzo 142,B.M. Cote 122, J. Couthures 4, G. Cowan 97, K. Cranmer 173, L. Cremer 50,D. Cremonini 24b,24a, S. Crépé-Renaudin 61, F. Crescioli 130, M. Cristinziani 144,M. Cristoforetti 79a,79b, V. Croft 117, J.E. Crosby 124, G. Crosetti 44b,44a, A. Cueto 101,H. Cui 98, Z. Cui 7, W.R. Cunningham 60, F. Curcio 166, J.R. Curran 53, P. Czodrowski 37,M.J. Da Cunha Sargedas De Sousa 58b,58a, J.V. Da Fonseca Pinto 84b, C. Da Via 103,W. Dabrowski 87a, T. Dado 37, S. Dahbi 151, T. Dai 108, D. Dal Santo 20, C. Dallapiccola 105,M. Dam 43, G. D’amen 30, V. D’Amico 111, J. Damp 102, J.R. Dandoy 35, D. Dannheim 37,M. Danninger 145, V. Dao 148, G. Darbo 58b, S.J. Das 30,ae, F. Dattola 49, S. D’Auria 72a,72b,A. D’avanzo 73a,73b, C. David 34a, T. Davidek 136, I. Dawson 96, H.A. Day-hall 135, K. De 8,R. De Asmundis 73a, N. De Biase 49, S. De Castro 24b,24a, N. De Groot 116, P. de Jong 117,H. De la Torre 118, A. De Maria 114a, A. De Salvo 76a, U. De Sanctis 77a,77b,F. De Santis 71a,71b, A. De Santo 149, J.B. De Vivie De Regie 61, J. Debevc 95, D.V. Dedovich39,J. Degens 94, A.M. Deiana 45, F. Del Corso 24b,24a, J. Del Peso 101, L. Delagrange 130,F. Deliot 138, C.M. Delitzsch 50, M. Della Pietra 73a,73b, D. Della Volpe 57, A. Dell’Acqua 37,L. Dell’Asta 72a,72b, M. Delmastro 4, P.A. Delsart 61, S. Demers 175, M. Demichev 39,S.P. Denisov 38, L. D’Eramo 41, D. Derendarz 88, F. Derue 130, P. Dervan 94, K. Desch 25,C. Deutsch 25, F.A. Di Bello 58b,58a, A. Di Ciaccio 77a,77b, L. Di Ciaccio 4,A. Di Domenico 76a,76b, C. Di Donato 73a,73b, A. Di Girolamo 37, G. Di Gregorio 37,A. Di Luca 79a,79b, B. Di Micco 78a,78b, R. Di Nardo 78a,78b, K.F. Di Petrillo 40,M. Diamantopoulou 35, F.A. Dias 117, T. Dias Do Vale 145, M.A. Diaz 140a,140b,F.G. Diaz Capriles 25, A.R. Didenko39, M. Didenko 166, E.B. Diehl 108, S. Díez Cornell 49,C. Diez Pardos 144, C. Dimitriadi 164, A. Dimitrievska 21, J. Dingfelder 25, T. Dingley 129,I-M. Dinu 28b, S.J. Dittmeier 64b, F. Dittus 37, M. Divisek 136, B. Dixit 94, F. Djama 104,– 18 –JHEP08(2024)153T. Djobava 152b, C. Doglioni 103,100, A. Dohnalova 29a, J. Dolejsi 136, Z. Dolezal 136,K. Domijan 87a, K.M. Dona 40, M. Donadelli 84d, B. Dong 109, J. Donini 41,A. D’Onofrio 73a,73b, M. D’Onofrio 94, J. Dopke 137, A. Doria 73a,N. Dos Santos Fernandes 133a, P. Dougan 103, M.T. Dova 92, A.T. Doyle 60, M.A. Draguet 129,E. Dreyer 172, I. Drivas-koulouris 10, M. Drnevich 120, M. Drozdova 57, D. Du 63a,T.A. du Pree 117, F. Dubinin 38, M. Dubovsky 29a, E. Duchovni 172, G. Duckeck 111,O.A. Ducu 28b, D. Duda 53, A. Dudarev 37, E.R. Duden 27, M. D’uffizi 103, L. Duflot 67,M. Dührssen 37, I. Duminica 28g, A.E. Dumitriu 28b, M. Dunford 64a, S. Dungs 50,K. Dunne 48a,48b, A. Duperrin 104, H. Duran Yildiz 3a, M. Düren 59, A. Durglishvili 152b,B.L. Dwyer 118, G.I. Dyckes 18a, M. Dyndal 87a, B.S. Dziedzic 37, Z.O. Earnshaw 149,G.H. Eberwein 129, B. Eckerova 29a, S. Eggebrecht 56, E. Egidio Purcino De Souza 84e,L.F. Ehrke 57, G. Eigen 17, K. Einsweiler 18a, T. Ekelof 164, P.A. Ekman 100, S. El Farkh 36b,Y. El Ghazali 63a, H. El Jarrari 37, A. El Moussaouy 36a, V. Ellajosyula 164, M. Ellert 164,F. Ellinghaus 174, N. Ellis 37, J. Elmsheuser 30, M. Elsawy 119a, M. Elsing 37,D. Emeliyanov 137, Y. Enari 85, I. Ene 18a, S. Epari 13, P.A. Erland 88,D. Ernani Martins Neto 88, M. Errenst 174, M. Escalier 67, C. Escobar 166, E. Etzion 154,G. Evans 133a, H. Evans 69, L.S. Evans 97, A. Ezhilov 38, S. Ezzarqtouni 36a,F. Fabbri 24b,24a, L. Fabbri 24b,24a, G. Facini 98, V. Fadeyev 139, R.M. Fakhrutdinov 38,D. Fakoudis 102, S. Falciano 76a, L.F. Falda Ulhoa Coelho 37, F. Fallavollita 112,G. Falsetti 44b,44a, J. Faltova 136, C. Fan 165, K.Y. Fan 65b, Y. Fan 14, Y. Fang 14,114c,M. Fanti 72a,72b, M. Faraj 70a,70b, Z. Farazpay 99, A. Farbin 8, A. Farilla 78a,T. Farooque 109, S.M. Farrington 53, F. Fassi 36e, D. Fassouliotis 9, M. Faucci Giannelli 77a,77b,W.J. Fawcett 33, L. Fayard 67, P. Federic 136, P. Federicova 134, O.L. Fedin 38,a,M. Feickert 173, L. Feligioni 104, D.E. Fellers 126, C. Feng 63b, Z. Feng 117, M.J. Fenton 162,L. Ferencz 49, R.A.M. Ferguson 93, S.I. Fernandez Luengo 140f , P. Fernandez Martinez 13,M.J.V. Fernoux 104, J. Ferrando 93, A. Ferrari 164, P. Ferrari 117,116, R. Ferrari 74a,D. Ferrere 57, C. Ferretti 108, D. Fiacco 76a,76b, F. Fiedler 102, P. Fiedler 135, S. Filimonov38,A. Filipčič 95, E.K. Filmer 1, F. Filthaut 116, M.C.N. Fiolhais 133a,133c,c, L. Fiorini 166,W.C. Fisher 109, T. Fitschen 103, P.M. Fitzhugh138, I. Fleck 144, P. Fleischmann 108,T. Flick 174, M. Flores 34d,z, L.R. Flores Castillo 65a, L. Flores Sanz De Acedo 37,F.M. Follega 79a,79b, N. Fomin 33, J.H. Foo 158, A. Formica 138, A.C. Forti 103, E. Fortin 37,A.W. Fortman 18a, M.G. Foti 18a, L. Fountas 9,i, D. Fournier 67, H. Fox 93,P. Francavilla 75a,75b, S. Francescato 62, S. Franchellucci 57, M. Franchini 24b,24a,S. Franchino 64a, D. Francis37, L. Franco 116, V. Franco Lima 37, L. Franconi 49,M. Franklin 62, G. Frattari 27, Y.Y. Frid 154, J. Friend 60, N. Fritzsche 37, A. Froch 55,D. Froidevaux 37, J.A. Frost 129, Y. Fu 63a, S. Fuenzalida Garrido 140f , M. Fujimoto 104,K.Y. Fung 65a, E. Furtado De Simas Filho 84e, M. Furukawa 156, J. Fuster 166, A. Gaa 56,A. Gabrielli 24b,24a, A. Gabrielli 158, P. Gadow 37, G. Gagliardi 58b,58a, L.G. Gagnon 18a,S. Gaid 163, S. Galantzan 154, J. Gallagher 1, E.J. Gallas 129, B.J. Gallop 137, K.K. Gan 122,S. Ganguly 156, Y. Gao 53, F.M. Garay Walls 140a,140b, B. Garcia30, C. García 166,A. Garcia Alonso 117, A.G. Garcia Caffaro 175, J.E. García Navarro 166, M. Garcia-Sciveres 18a,G.L. Gardner 131, R.W. Gardner 40, N. Garelli 161, D. Garg 81, R.B. Garg 146, J.M. Gargan53,C.A. Garner158, C.M. Garvey 34a, V.K. Gassmann161, G. Gaudio 74a, V. Gautam13,– 19 –JHEP08(2024)153P. Gauzzi 76a,76b, J. Gavranovic 95, I.L. Gavrilenko 38, A. Gavrilyuk 38, C. Gay 167,G. Gaycken 126, E.N. Gazis 10, A.A. Geanta 28b, C.M. Gee 139, A. Gekow122, C. Gemme 58b,M.H. Genest 61, A.D. Gentry 115, S. George 97, W.F. George 21, T. Geralis 47,P. Gessinger-Befurt 37, M.E. Geyik 174, M. Ghani 170, K. Ghorbanian 96, A. Ghosal 144,A. Ghosh 162, A. Ghosh 7, B. Giacobbe 24b, S. Giagu 76a,76b, T. Giani 117, A. Giannini 63a,S.M. Gibson 97, M. Gignac 139, D.T. Gil 87b, A.K. Gilbert 87a, B.J. Gilbert 42,D. Gillberg 35, G. Gilles 117, L. Ginabat 130, D.M. Gingrich 2,ac, M.P. Giordani 70a,70c,P.F. Giraud 138, G. Giugliarelli 70a,70c, D. Giugni 72a, F. Giuli 37, I. Gkialas 9,i,L.K. Gladilin 38, C. Glasman 101, G.R. Gledhill 126, G. Glemža 49, M. Glisic126, I. Gnesi 44b,Y. Go 30, M. Goblirsch-Kolb 37, B. Gocke 50, D. Godin110, B. Gokturk 22a, S. Goldfarb 107,T. Golling 57, M.G.D. Gololo 34g, D. Golubkov 38, J.P. Gombas 109, A. Gomes 133a,133b,G. Gomes Da Silva 144, A.J. Gomez Delegido 166, R. Gonçalo 133a, L. Gonella 21,A. Gongadze 152c, F. Gonnella 21, J.L. Gonski 146, R.Y. González Andana 53,S. González de la Hoz 166, R. Gonzalez Lopez 94, C. Gonzalez Renteria 18a,M.V. Gonzalez Rodrigues 49, R. Gonzalez Suarez 164, S. Gonzalez-Sevilla 57, L. Goossens 37,B. Gorini 37, E. Gorini 71a,71b, A. Gorišek 95, T.C. Gosart 131, A.T. Goshaw 52,M.I. Gostkin 39, S. Goswami 124, C.A. Gottardo 37, S.A. Gotz 111, M. Gouighri 36b,V. Goumarre 49, A.G. Goussiou 141, N. Govender 34c, R.P. Grabarczyk 129,I. Grabowska-Bold 87a, K. Graham 35, E. Gramstad 128, S. Grancagnolo 71a,71b,C.M. Grant1,138, P.M. Gravila 28f , F.G. Gravili 71a,71b, H.M. Gray 18a, M. Greco 71a,71b,M.J. Green 1, C. Grefe 25, A.S. Grefsrud 17, I.M. Gregor 49, K.T. Greif 162, P. Grenier 146,S.G. Grewe112, A.A. Grillo 139, K. Grimm 32, S. Grinstein 13,s, J.-F. Grivaz 67, E. Gross 172,J. Grosse-Knetter 56, L. Guan 108, J.G.R. Guerrero Rojas 166, G. Guerrieri 37, R. Gugel 102,J.A.M. Guhit 108, A. Guida 19, E. Guilloton 170, S. Guindon 37, F. Guo 14,114c, J. Guo 63c,L. Guo 49, Y. Guo 108, R. Gupta 132, S. Gurbuz 25, S.S. Gurdasani 55, G. Gustavino 76a,76b,P. Gutierrez 123, L.F. Gutierrez Zagazeta 131, M. Gutsche 51, C. Gutschow 98, C. Gwenlan 129,C.B. Gwilliam 94, E.S. Haaland 128, A. Haas 120, M. Habedank 49, C. Haber 18a,H.K. Hadavand 8, A. Hadef 51, S. Hadzic 112, A.I. Hagan 93, J.J. Hahn 144, E.H. Haines 98,M. Haleem 169, J. Haley 124, J.J. Hall 142, G.D. Hallewell 104, L. Halser 20, K. Hamano 168,M. Hamer 25, G.N. Hamity 53, E.J. Hampshire 97, J. Han 63b, K. Han 63a, L. Han 114a,L. Han 63a, S. Han 18a, Y.F. Han 158, K. Hanagaki 85, M. Hance 139, D.A. Hangal 42,H. Hanif 145, M.D. Hank 131, J.B. Hansen 43, P.H. Hansen 43, D. Harada 57,T. Harenberg 174, S. Harkusha 38, M.L. Harris 105, Y.T. Harris 25, J. Harrison 13,N.M. Harrison 122, P.F. Harrison170, N.M. Hartman 112, N.M. Hartmann 111, R.Z. Hasan 97,137,Y. Hasegawa 143, F. Haslbeck 129, S. Hassan 17, R. Hauser 109, C.M. Hawkes 21,R.J. Hawkings 37, Y. Hayashi 156, D. Hayden 109, C. Hayes 108, R.L. Hayes 117,C.P. Hays 129, J.M. Hays 96, H.S. Hayward 94, F. He 63a, M. He 14,114c, Y. He 49, Y. He 98,N.B. Heatley 96, V. Hedberg 100, A.L. Heggelund 128, N.D. Hehir 96,∗, C. Heidegger 55,K.K. Heidegger 55, J. Heilman 35, S. Heim 49, T. Heim 18a, J.G. Heinlein 131,J.J. Heinrich 126, L. Heinrich 112,aa, J. Hejbal 134, A. Held 173, S. Hellesund 17,C.M. Helling 167, S. Hellman 48a,48b, R.C.W. Henderson93, L. Henkelmann 33,A.M. Henriques Correia37, H. Herde 100, Y. Hernández Jiménez 148, L.M. Herrmann 25,T. Herrmann 51, G. Herten 55, R. Hertenberger 111, L. Hervas 37, M.E. Hesping 102,– 20 –JHEP08(2024)153N.P. Hessey 159a, M. Hidaoui 36b, N. Hidic 136, E. Hill 158, S.J. Hillier 21, J.R. Hinds 109,F. Hinterkeuser 25, M. Hirose 127, S. Hirose 160, D. Hirschbuehl 174, T.G. Hitchings 103,B. Hiti 95, J. Hobbs 148, R. Hobincu 28e, N. Hod 172, M.C. Hodgkinson 142,B.H. Hodkinson 129, A. Hoecker 37, D.D. Hofer 108, J. Hofer 166, T. Holm 25, M. Holzbock 37,L.B.A.H. Hommels 33, B.P. Honan 103, J.J. Hong 69, J. Hong 63c, T.M. Hong 132,B.H. Hooberman 165, W.H. Hopkins 6, M.C. Hoppesch 165, Y. Horii 113, M.E. Horstmann 112,S. Hou 151, A.S. Howard 95, J. Howarth 60, J. Hoya 6, M. Hrabovsky 125, A. Hrynevich 49,T. Hryn’ova 4, P.J. Hsu 66, S.-C. Hsu 141, T. Hsu 67, M. Hu 18a, Q. Hu 63a, S. Huang 65b,X. Huang 14,114c, Y. Huang 142, Y. Huang 102, Y. Huang 14, Z. Huang 103, Z. Hubacek 135,M. Huebner 25, F. Huegging 25, T.B. Huffman 129, C.A. Hugli 49, M. Huhtinen 37,S.K. Huiberts 17, R. Hulsken 106, N. Huseynov 12,f , J. Huston 109, J. Huth 62,R. Hyneman 146, G. Iacobucci 57, G. Iakovidis 30, L. Iconomidou-Fayard 67, J.P. Iddon 37,P. Iengo 73a,73b, R. Iguchi 156, Y. Iiyama 156, T. Iizawa 129, Y. Ikegami 85, N. Ilic 158,H. Imam 84c, G. Inacio Goncalves 84d, M. Ince Lezki 57, T. Ingebretsen Carlson 48a,48b,J.M. Inglis 96, G. Introzzi 74a,74b, M. Iodice 78a, V. Ippolito 76a,76b, R.K. Irwin 94,M. Ishino 156, W. Islam 173, C. Issever 19,49, S. Istin 22a,ag, H. Ito 171, R. Iuppa 79a,79b,A. Ivina 172, J.M. Izen 46, V. Izzo 73a, P. Jacka 134, P. Jackson 1, C.S. Jagfeld 111,G. Jain 159a, P. Jain 49, K. Jakobs 55, T. Jakoubek 172, J. Jamieson 60, W. Jang 156,M. Javurkova 105, P. Jawahar 103, L. Jeanty 126, J. Jejelava 152a,y, P. Jenni 55,e,C.E. Jessiman 35, C. Jia63b, J. Jia 148, X. Jia 14,114c, Z. Jia 114a, C. Jiang 53, S. Jiggins 49,J. Jimenez Pena 13, S. Jin 114a, A. Jinaru 28b, O. Jinnouchi 157, P. Johansson 142,K.A. Johns 7, J.W. Johnson 139, F.A. Jolly 49, D.M. Jones 149, E. Jones 49, K.S. Jones8,P. Jones 33, R.W.L. Jones 93, T.J. Jones 94, H.L. Joos 56,37, R. Joshi 122, J. Jovicevic 16,X. Ju 18a, J.J. Junggeburth 105, T. Junkermann 64a, A. Juste Rozas 13,s, M.K. Juzek 88,S. Kabana 140e, A. Kaczmarska 88, M. Kado 112, H. Kagan 122, M. Kagan 146, A. Kahn 131,C. Kahra 102, T. Kaji 156, E. Kajomovitz 153, N. Kakati 172, I. Kalaitzidou 55,C.W. Kalderon 30, N.J. Kang 139, D. Kar 34g, K. Karava 129, M.J. Kareem 159b,E. Karentzos 55, O. Karkout 117, S.N. Karpov 39, Z.M. Karpova 39, V. Kartvelishvili 93,A.N. Karyukhin 38, E. Kasimi 155, J. Katzy 49, S. Kaur 35, K. Kawade 143, M.P. Kawale 123,C. Kawamoto 89, T. Kawamoto 63a, E.F. Kay 37, F.I. Kaya 161, S. Kazakos 109,V.F. Kazanin 38, Y. Ke 148, J.M. Keaveney 34a, R. Keeler 168, G.V. Kehris 62, J.S. Keller 35,A.S. Kelly98, J.J. Kempster 149, P.D. Kennedy 102, O. Kepka 134, B.P. Kerridge 137,S. Kersten 174, B.P. Kerševan 95, L. Keszeghova 29a, S. Ketabchi Haghighat 158,R.A. Khan 132, A. Khanov 124, A.G. Kharlamov 38, T. Kharlamova 38, E.E. Khoda 141,M. Kholodenko 133a, T.J. Khoo 19, G. Khoriauli 169, J. Khubua 152b,∗, Y.A.R. Khwaira 130,B. Kibirige34g, D. Kim 6, D.W. Kim 48a,48b, Y.K. Kim 40, N. Kimura 98, M.K. Kingston 56,A. Kirchhoff 56, C. Kirfel 25, F. Kirfel 25, J. Kirk 137, A.E. Kiryunin 112, S. Kita 160,C. Kitsaki 10, O. Kivernyk 25, M. Klassen 161, C. Klein 35, L. Klein 169, M.H. Klein 45,S.B. Klein 57, U. Klein 94, P. Klimek 37, A. Klimentov 30, T. Klioutchnikova 37, P. Kluit 117,S. Kluth 112, E. Kneringer 80, T.M. Knight 158, A. Knue 50, D. Kobylianskii 172,S.F. Koch 129, M. Kocian 146, P. Kodyš 136, D.M. Koeck 126, P.T. Koenig 25, T. Koffas 35,O. Kolay 51, I. Koletsou 4, T. Komarek 88, K. Köneke 55, A.X.Y. Kong 1, T. Kono 121,N. Konstantinidis 98, P. Kontaxakis 57, B. Konya 100, R. Kopeliansky 42, S. Koperny 87a,– 21 –JHEP08(2024)153K. Korcyl 88, K. Kordas 155,d, A. Korn 98, S. Korn 56, I. Korolkov 13, N. Korotkova 38,B. Kortman 117, O. Kortner 112, S. Kortner 112, W.H. Kostecka 118, V.V. Kostyukhin 144,A. Kotsokechagia 37, A. Kotwal 52, A. Koulouris 37, A. Kourkoumeli-Charalampidi 74a,74b,C. Kourkoumelis 9, E. Kourlitis 112,aa, O. Kovanda 126, R. Kowalewski 168, W. Kozanecki 126,A.S. Kozhin 38, V.A. Kramarenko 38, G. Kramberger 95, P. Kramer 102, M.W. Krasny 130,A. Krasznahorkay 37, A.C. Kraus 118, J.W. Kraus 174, J.A. Kremer 49, T. Kresse 51,L. Kretschmann 174, J. Kretzschmar 94, K. Kreul 19, P. Krieger 158, M. Krivos 136,K. Krizka 21, K. Kroeninger 50, H. Kroha 112, J. Kroll 134, J. Kroll 131, K.S. Krowpman 109,U. Kruchonak 39, H. Krüger 25, N. Krumnack82, M.C. Kruse 52, O. Kuchinskaia 38,S. Kuday 3a, S. Kuehn 37, R. Kuesters 55, T. Kuhl 49, V. Kukhtin 39, Y. Kulchitsky 38,a,S. Kuleshov 140d,140b, M. Kumar 34g, N. Kumari 49, P. Kumari 159b, A. Kupco 134,T. Kupfer50, A. Kupich 38, O. Kuprash 55, H. Kurashige 86, L.L. Kurchaninov 159a,O. Kurdysh 67, Y.A. Kurochkin 38, A. Kurova 38, M. Kuze 157, A.K. Kvam 105, J. Kvita 125,T. Kwan 106, N.G. Kyriacou 108, L.A.O. Laatu 104, C. Lacasta 166, F. Lacava 76a,76b,H. Lacker 19, D. Lacour 130, N.N. Lad 98, E. Ladygin 39, A. Lafarge 41, B. Laforge 130,T. Lagouri 175, F.Z. Lahbabi 36a, S. Lai 56, J.E. Lambert 168, S. Lammers 69, W. Lampl 7,C. Lampoudis 155,d, G. Lamprinoudis102, A.N. Lancaster 118, E. Lançon 30, U. Landgraf 55,M.P.J. Landon 96, V.S. Lang 55, O.K.B. Langrekken 128, A.J. Lankford 162, F. Lanni 37,K. Lantzsch 25, A. Lanza 74a, M. Lanzac Berrocal 166, J.F. Laporte 138, T. Lari 72a,F. Lasagni Manghi 24b, M. Lassnig 37, V. Latonova 134, A. Laurier 153, S.D. Lawlor 142,Z. Lawrence 103, R. Lazaridou170, M. Lazzaroni 72a,72b, B. Le103, H.D.M. Le 109,E.M. Le Boulicaut 175, L.T. Le Pottier 18a, B. Leban 24b,24a, A. Lebedev 82, M. LeBlanc 103,F. Ledroit-Guillon 61, S.C. Lee 151, S. Lee 48a,48b, T.F. Lee 94, L.L. Leeuw 34c,H.P. Lefebvre 97, M. Lefebvre 168, C. Leggett 18a, G. Lehmann Miotto 37, M. Leigh 57,W.A. Leight 105, W. Leinonen 116, A. Leisos 155,q, M.A.L. Leite 84c, C.E. Leitgeb 19,R. Leitner 136, K.J.C. Leney 45, T. Lenz 25, S. Leone 75a, C. Leonidopoulos 53,A. Leopold 147, R. Les 109, C.G. Lester 33, M. Levchenko 38, J. Levêque 4, L.J. Levinson 172,G. Levrini 24b,24a, M.P. Lewicki 88, C. Lewis 141, D.J. Lewis 4, L. Lewitt 142, A. Li 30,B. Li 63b, C. Li63a, C-Q. Li 112, H. Li 63a, H. Li 63b, H. Li 114a, H. Li 15, H. Li 63b,J. Li 63c, K. Li 14, L. Li 63c, M. Li 14,114c, S. Li 14,114c, S. Li 63d,63c, T. Li 5, X. Li 106,Z. Li 129, Z. Li 156, Z. Li 14,114c, Z. Li 63a, S. Liang 14,114c, Z. Liang 14, M. Liberatore 138,B. Liberti 77a, K. Lie 65c, J. Lieber Marin 84e, H. Lien 69, H. Lin 108, K. Lin 109,R.E. Lindley 7, J.H. Lindon 2, J. Ling 62, E. Lipeles 131, A. Lipniacka 17, A. Lister 167,J.D. Little 69, B. Liu 14, B.X. Liu 114b, D. Liu 63d,63c, E.H.L. Liu 21, J.B. Liu 63a,J.K.K. Liu 33, K. Liu 63d, K. Liu 63d,63c, M. Liu 63a, M.Y. Liu 63a, P. Liu 14,Q. Liu 63d,141,63c, X. Liu 63a, X. Liu 63b, Y. Liu 114b,114c, Y.L. Liu 63b, Y.W. Liu 63a,S.L. Lloyd 96, E.M. Lobodzinska 49, P. Loch 7, T. Lohse 19, K. Lohwasser 142,E. Loiacono 49, M. Lokajicek 134,∗, J.D. Lomas 21, J.D. Long 165, I. Longarini 162,R. Longo 165, I. Lopez Paz 68, A. Lopez Solis 49, N.A. Lopez-canelas 7, N. Lorenzo Martinez 4,A.M. Lory 111, M. Losada 119a, G. Löschcke Centeno 149, O. Loseva 38, X. Lou 48a,48b,X. Lou 14,114c, A. Lounis 67, P.A. Love 93, G. Lu 14,114c, M. Lu 67, S. Lu 131, Y.J. Lu 66,H.J. Lubatti 141, C. Luci 76a,76b, F.L. Lucio Alves 114a, F. Luehring 69, O. Lukianchuk 67,B.S. Lunday 131, O. Lundberg 147, B. Lund-Jensen 147,∗, N.A. Luongo 6, M.S. Lutz 37,– 22 –JHEP08(2024)153A.B. Lux 26, D. Lynn 30, R. Lysak 134, E. Lytken 100, V. Lyubushkin 39, T. Lyubushkina 39,M.M. Lyukova 148, M.Firdaus M. Soberi 53, H. Ma 30, K. Ma 63a, L.L. Ma 63b, W. Ma 63a,Y. Ma 124, J.C. MacDonald 102, P.C. Machado De Abreu Farias 84e, R. Madar 41,T. Madula 98, J. Maeda 86, T. Maeno 30, H. Maguire 142, V. Maiboroda 138,A. Maio 133a,133b,133d, K. Maj 87a, O. Majersky 49, S. Majewski 126, N. Makovec 67,V. Maksimovic 16, B. Malaescu 130, Pa. Malecki 88, V.P. Maleev 38, F. Malek 61,m,M. Mali 95, D. Malito 97, U. Mallik 81, S. Maltezos10, S. Malyukov39, J. Mamuzic 13,G. Mancini 54, M.N. Mancini 27, G. Manco 74a,74b, J.P. Mandalia 96, S.S. Mandarry 149,I. Mandić 95, L. Manhaes de Andrade Filho 84a, I.M. Maniatis 172, J. Manjarres Ramos 91,D.C. Mankad 172, A. Mann 111, S. Manzoni 37, L. Mao 63c, X. Mapekula 34c,A. Marantis 155,q, G. Marchiori 5, M. Marcisovsky 134, C. Marcon 72a, M. Marinescu 21,S. Marium 49, M. Marjanovic 123, A. Markhoos 55, M. Markovitch 67, E.J. Marshall 93,Z. Marshall 18a, S. Marti-Garcia 166, J. Martin 98, T.A. Martin 137, V.J. Martin 53,B. Martin dit Latour 17, L. Martinelli 76a,76b, M. Martinez 13,s, P. Martinez Agullo 166,V.I. Martinez Outschoorn 105, P. Martinez Suarez 13, S. Martin-Haugh 137,G. Martinovicova 136, V.S. Martoiu 28b, A.C. Martyniuk 98, A. Marzin 37, D. Mascione 79a,79b,L. Masetti 102, J. Masik 103, A.L. Maslennikov 38, P. Massarotti 73a,73b, P. Mastrandrea 75a,75b,A. Mastroberardino 44b,44a, T. Masubuchi 127, T.T. Mathew 126, T. Mathisen 164,J. Matousek 136, J. Maurer 28b, T. Maurin 60, A.J. Maury 67, B. Maček 95, D.A. Maximov 38,A.E. May 103, R. Mazini 151, I. Maznas 118, M. Mazza 109, S.M. Mazza 139,E. Mazzeo 72a,72b, C. Mc Ginn 30, J.P. Mc Gowan 168, S.P. Mc Kee 108, C.C. McCracken 167,E.F. McDonald 107, A.E. McDougall 117, J.A. Mcfayden 149, R.P. McGovern 131,R.P. Mckenzie 34g, T.C. Mclachlan 49, D.J. Mclaughlin 98, S.J. McMahon 137,C.M. Mcpartland 94, R.A. McPherson 168,w, S. Mehlhase 111, A. Mehta 94, D. Melini 166,B.R. Mellado Garcia 34g, A.H. Melo 56, F. Meloni 49, A.M. Mendes Jacques Da Costa 103,H.Y. Meng 158, L. Meng 93, S. Menke 112, M. Mentink 37, E. Meoni 44b,44a, G. Mercado 118,S. Merianos 155, C. Merlassino 70a,70c, L. Merola 73a,73b, C. Meroni 72a,72b, J. Metcalfe 6,A.S. Mete 6, E. Meuser 102, C. Meyer 69, J-P. Meyer 138, R.P. Middleton 137, L. Mijović 53,G. Mikenberg 172, M. Mikestikova 134, M. Mikuž 95, H. Mildner 102, A. Milic 37,D.W. Miller 40, E.H. Miller 146, L.S. Miller 35, A. Milov 172, D.A. Milstead48a,48b, T. Min114a,A.A. Minaenko 38, I.A. Minashvili 152b, L. Mince 60, A.I. Mincer 120, B. Mindur 87a,M. Mineev 39, Y. Mino 89, L.M. Mir 13, M. Miralles Lopez 60, M. Mironova 18a,M.C. Missio 116, A. Mitra 170, V.A. Mitsou 166, Y. Mitsumori 113, O. Miu 158,P.S. Miyagawa 96, T. Mkrtchyan 64a, M. Mlinarevic 98, T. Mlinarevic 98, M. Mlynarikova 37,S. Mobius 20, P. Mogg 111, M.H. Mohamed Farook 115, A.F. Mohammed 14,114c,S. Mohapatra 42, G. Mokgatitswane 34g, L. Moleri 172, B. Mondal 144, S. Mondal 135,K. Mönig 49, E. Monnier 104, L. Monsonis Romero166, J. Montejo Berlingen 13,A. Montella 48a,48b, M. Montella 122, F. Montereali 78a,78b, F. Monticelli 92, S. Monzani 70a,70c,A. Morancho Tarda 43, N. Morange 67, A.L. Moreira De Carvalho 49, M. Moreno Llácer 166,C. Moreno Martinez 57, J.M. Moreno Perez23b, P. Morettini 58b, S. Morgenstern 37, M. Morii 62,M. Morinaga 156, F. Morodei 76a,76b, L. Morvaj 37, P. Moschovakos 37, B. Moser 129,M. Mosidze 152b, T. Moskalets 45, P. Moskvitina 116, J. Moss 32,j , P. Moszkowicz 87a,A. Moussa 36d, E.J.W. Moyse 105, O. Mtintsilana 34g, S. Muanza 104, J. Mueller 132,– 23 –JHEP08(2024)153D. Muenstermann 93, R. Müller 37, G.A. Mullier 164, A.J. Mullin33, J.J. Mullin131,D.P. Mungo 158, D. Munoz Perez 166, F.J. Munoz Sanchez 103, M. Murin 103,W.J. Murray 170,137, M. Muškinja 95, C. Mwewa 30, A.G. Myagkov 38,a, A.J. Myers 8,G. Myers 108, M. Myska 135, B.P. Nachman 18a, O. Nackenhorst 50, K. Nagai 129,K. Nagano 85, J.L. Nagle 30,ae, E. Nagy 104, A.M. Nairz 37, Y. Nakahama 85,K. Nakamura 85, K. Nakkalil 5, H. Nanjo 127, E.A. Narayanan 115, I. Naryshkin 38,L. Nasella 72a,72b, M. Naseri 35, S. 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Paredes Hernandez 65b, A. Pareti 74a,74b, K.R. Park 42,T.H. Park 158, M.A. Parker 33, F. Parodi 58b,58a, E.W. Parrish 118, V.A. Parrish 53,J.A. Parsons 42, U. Parzefall 55, B. Pascual Dias 110, L. Pascual Dominguez 101,E. Pasqualucci 76a, S. Passaggio 58b, F. Pastore 97, P. Patel 88, U.M. Patel 52, J.R. Pater 103,T. Pauly 37, C.I. Pazos 161, J. Pearkes 146, M. Pedersen 128, R. Pedro 133a,S.V. Peleganchuk 38, O. Penc 37, E.A. Pender 53, S. Peng15, G.D. Penn 175, K.E. Penski 111,M. Penzin 38, B.S. Peralva 84d, A.P. Pereira Peixoto 141, L. Pereira Sanchez 146,D.V. Perepelitsa 30,ae, G. Perera 105, E. Perez Codina 159a, M. Perganti 10, H. Pernegger 37,S. Perrella 76a,76b, O. Perrin 41, K. Peters 49, R.F.Y. Peters 103, B.A. Petersen 37,T.C. Petersen 43, E. Petit 104, V. Petousis 135, C. Petridou 155,d, T. Petru 136,A. Petrukhin 144, M. Pettee 18a, A. Petukhov 38, K. Petukhova 37, R. Pezoa 140f ,L. Pezzotti 37, G. Pezzullo 175, A.J. Pfleger 37, T.M. Pham 173, T. Pham 107,P.W. Phillips 137, G. Piacquadio 148, E. Pianori 18a, F. Piazza 126, R. Piegaia 31,D. Pietreanu 28b, A.D. Pilkington 103, M. Pinamonti 70a,70c, J.L. Pinfold 2,– 24 –JHEP08(2024)153B.C. Pinheiro Pereira 133a, J. Pinol Bel 13, A.E. Pinto Pinoargote 138,138, L. Pintucci 70a,70c,K.M. Piper 149, A. Pirttikoski 57, D.A. Pizzi 35, L. Pizzimento 65b, A. Pizzini 117,M.-A. Pleier 30, V. Pleskot 136, E. Plotnikova39, G. Poddar 96, R. Poettgen 100,L. Poggioli 130, I. Pokharel 56, S. Polacek 136, G. Polesello 74a, A. Poley 145,159a,A. Polini 24b, C.S. Pollard 170, Z.B. Pollock 122, E. Pompa Pacchi 76a,76b, N.I. Pond 98,D. Ponomarenko 69, L. Pontecorvo 37, S. Popa 28a, G.A. Popeneciu 28d, A. Poreba 37,D.M. Portillo Quintero 159a, S. Pospisil 135, M.A. Postill 142, P. Postolache 28c,K. Potamianos 170, P.A. Potepa 87a, I.N. Potrap 39, C.J. Potter 33, H. Potti 150,J. Poveda 166, M.E. Pozo Astigarraga 37, A. Prades Ibanez 77a,77b, J. Pretel 168, D. Price 103,M. Primavera 71a, L. Primomo 70a,70c, M.A. Principe Martin 101, R. Privara 125,T. Procter 60, M.L. Proffitt 141, N. Proklova 131, K. Prokofiev 65c, G. Proto 112,J. Proudfoot 6, M. Przybycien 87a, W.W. Przygoda 87b, A. Psallidas 47, J.E. Puddefoot 142,D. Pudzha 55, D. Pyatiizbyantseva 38, J. Qian 108, D. Qichen 103, Y. Qin 13, T. Qiu 53,A. Quadt 56, M. Queitsch-Maitland 103, G. Quetant 57, R.P. Quinn 167,G. Rabanal Bolanos 62, D. Rafanoharana 55, F. Raffaeli 77a,77b, F. Ragusa 72a,72b,J.L. Rainbolt 40, J.A. Raine 57, S. Rajagopalan 30, E. Ramakoti 38, L. Rambelli 58b,58a,I.A. Ramirez-Berend 35, K. Ran 49,114c, D.S. Rankin 131, N.P. Rapheeha 34g, H. Rasheed 28b,V. Raskina 130, D.F. Rassloff 64a, A. Rastogi 18a, S. Rave 102, S. Ravera 58b,58a, B. Ravina 56,I. Ravinovich 172, M. Raymond 37, A.L. Read 128, N.P. Readioff 142, D.M. Rebuzzi 74a,74b,G. Redlinger 30, A.S. Reed 112, K. Reeves 27, J.A. Reidelsturz 174, D. Reikher 126, A. Rej 50,C. Rembser 37, M. Renda 28b, F. Renner 49, A.G. Rennie 162, A.L. Rescia 49, S. Resconi 72a,M. Ressegotti 58b,58a, S. Rettie 37, J.G. Reyes Rivera 109, E. Reynolds 18a, O.L. Rezanova 38,P. Reznicek 136, H. Riani 36d, N. Ribaric 52, E. Ricci 79a,79b, R. Richter 112, S. Richter 48a,48b,E. Richter-Was 87b, M. Ridel 130, S. Ridouani 36d, P. Rieck 120, P. Riedler 37,E.M. Riefel 48a,48b, J.O. Rieger 117, M. Rijssenbeek 148, M. Rimoldi 37, L. Rinaldi 24b,24a,P. Rincke 56,164, T.T. Rinn 30, M.P. Rinnagel 111, G. Ripellino 164, I. Riu 13,J.C. Rivera Vergara 168, F. Rizatdinova 124, E. Rizvi 96, B.R. Roberts 18a, S.S. Roberts 139,S.H. Robertson 106,w, D. Robinson 33, M. Robles Manzano 102, A. Robson 60,A. Rocchi 77a,77b, C. Roda 75a,75b, S. Rodriguez Bosca 37, Y. Rodriguez Garcia 23a,A. Rodriguez Rodriguez 55, A.M. Rodríguez Vera 118, S. Roe37, J.T. Roemer 37,A.R. Roepe-Gier 139, O. Røhne 128, R.A. Rojas 105, C.P.A. Roland 130, J. Roloff 30,A. Romaniouk 38, E. Romano 74a,74b, M. Romano 24b, A.C. Romero Hernandez 165,N. Rompotis 94, L. Roos 130, S. Rosati 76a, B.J. Rosser 40, E. Rossi 129, E. Rossi 73a,73b,L.P. Rossi 62, L. Rossini 55, R. Rosten 122, M. Rotaru 28b, B. Rottler 55, C. Rougier 91,D. Rousseau 67, D. Rousso 49, A. Roy 165, S. Roy-Garand 158, A. Rozanov 104,Z.M.A. Rozario 60, Y. Rozen 153, A. Rubio Jimenez 166, A.J. Ruby 94, V.H. Ruelas Rivera 19,T.A. Ruggeri 1, A. Ruggiero 129, A. Ruiz-Martinez 166, A. Rummler 37, Z. Rurikova 55,N.A. Rusakovich 39, H.L. Russell 168, G. Russo 76a,76b, J.P. Rutherfoord 7,S. Rutherford Colmenares 33, M. Rybar 136, E.B. Rye 128, A. Ryzhov 45,J.A. Sabater Iglesias 57, H.F-W. Sadrozinski 139, F. Safai Tehrani 76a,B. Safarzadeh Samani 137, S. Saha 1, M. Sahinsoy 83, A. Saibel 166, M. Saimpert 138,M. Saito 156, T. Saito 156, A. Sala 72a,72b, D. Salamani 37, A. Salnikov 146, J. Salt 166,A. Salvador Salas 154, D. Salvatore 44b,44a, F. Salvatore 149, A. Salzburger 37, D. Sammel 55,– 25 –JHEP08(2024)153E. Sampson 93, D. Sampsonidis 155,d, D. Sampsonidou 126, J. Sánchez 166,V. Sanchez Sebastian 166, H. Sandaker 128, C.O. Sander 49, J.A. Sandesara 105,M. Sandhoff 174, C. Sandoval 23b, L. Sanfilippo 64a, D.P.C. Sankey 137, T. Sano 89,A. Sansoni 54, L. Santi 37,76b, C. Santoni 41, H. Santos 133a,133b, A. Santra 172,E. Sanzani 24b,24a, K.A. Saoucha 163, J.G. Saraiva 133a,133d, J. Sardain 7, O. Sasaki 85,K. Sato 160, C. Sauer64b, E. Sauvan 4, P. Savard 158,ac, R. Sawada 156, C. Sawyer 137,L. Sawyer 99, C. Sbarra 24b, A. Sbrizzi 24b,24a, T. Scanlon 98, J. Schaarschmidt 141,U. Schäfer 102, A.C. Schaffer 67,45, D. Schaile 111, R.D. Schamberger 148, C. Scharf 19,M.M. Schefer 20, V.A. Schegelsky 38, D. Scheirich 136, M. Schernau 162, C. Scheulen 56,C. Schiavi 58b,58a, M. Schioppa 44b,44a, B. Schlag 146,l, K.E. Schleicher 55, S. Schlenker 37,J. Schmeing 174, M.A. Schmidt 174, K. Schmieden 102, C. Schmitt 102, N. Schmitt 102,S. Schmitt 49, L. Schoeffel 138, A. Schoening 64b, P.G. Scholer 35, E. Schopf 129, M. Schott 25,J. Schovancova 37, S. Schramm 57, T. Schroer 57, H-C. Schultz-Coulon 64a, M. Schumacher 55,B.A. Schumm 139, Ph. Schune 138, A.J. Schuy 141, H.R. Schwartz 139, A. Schwartzman 146,T.A. Schwarz 108, Ph. Schwemling 138, R. Schwienhorst 109, F.G. Sciacca 20, A. Sciandra 30,G. Sciolla 27, F. Scuri 75a, C.D. Sebastiani 94, K. Sedlaczek 118, S.C. Seidel 115,A. Seiden 139, B.D. Seidlitz 42, C. Seitz 49, J.M. Seixas 84b, G. Sekhniaidze 73a, L. Selem 61,N. Semprini-Cesari 24b,24a, D. Sengupta 57, V. Senthilkumar 166, L. Serin 67, M. Sessa 77a,77b,H. Severini 123, F. Sforza 58b,58a, A. Sfyrla 57, Q. Sha 14, E. Shabalina 56, A.H. Shah 33,R. Shaheen 147, J.D. Shahinian 131, D. Shaked Renous 172, L.Y. Shan 14, M. Shapiro 18a,A. Sharma 37, A.S. Sharma 167, P. Sharma 81, P.B. Shatalov 38, K. Shaw 149, S.M. Shaw 103,Q. Shen 63c, D.J. Sheppard 145, P. Sherwood 98, L. Shi 98, X. Shi 14, S. Shimizu 85,C.O. Shimmin 175, J.D. Shinner 97, I.P.J. Shipsey 129, S. Shirabe 90, M. Shiyakova 39,u,M.J. Shochet 40, D.R. Shope 128, B. Shrestha 123, S. Shrestha 122,af , I. Shreyber 38,M.J. Shroff 168, P. Sicho 134, A.M. Sickles 165, E. Sideras Haddad 34g, A.C. Sidley 117,A. Sidoti 24b, F. Siegert 51, Dj. Sijacki 16, F. Sili 92, J.M. Silva 53, I. Silva Ferreira 84b,M.V. Silva Oliveira 30, S.B. Silverstein 48a, S. Simion67, R. Simoniello 37, E.L. Simpson 103,H. Simpson 149, L.R. Simpson 108, N.D. Simpson100, S. Simsek 83, S. Sindhu 56, P. Sinervo 158,S. Singh 158, S. Sinha 49, S. Sinha 103, M. Sioli 24b,24a, I. Siral 37, E. Sitnikova 49,J. Sjölin 48a,48b, A. Skaf 56, E. Skorda 21, P. Skubic 123, M. Slawinska 88, V. Smakhtin172,B.H. Smart 137, S.Yu. Smirnov 38, Y. Smirnov 38, L.N. Smirnova 38,a, O. Smirnova 100,A.C. Smith 42, D.R. Smith162, E.A. Smith 40, J.L. Smith 103, R. Smith146, M. Smizanska 93,K. Smolek 135, A.A. Snesarev 38, H.L. Snoek 117, S. Snyder 30, R. Sobie 168,w, A. Soffer 154,C.A. Solans Sanchez 37, E.Yu. Soldatov 38, U. Soldevila 166, A.A. Solodkov 38, S. Solomon 27,A. Soloshenko 39, K. Solovieva 55, O.V. Solovyanov 41, P. Sommer 51, A. Sonay 13,W.Y. Song 159b, A. Sopczak 135, A.L. Sopio 98, F. Sopkova 29b, J.D. Sorenson 115,I.R. Sotarriva Alvarez 157, V. Sothilingam64a, O.J. Soto Sandoval 140c,140b, S. Sottocornola 69,R. Soualah 163, Z. Soumaimi 36e, D. South 49, N. Soybelman 172, S. Spagnolo 71a,71b,M. Spalla 112, D. Sperlich 55, G. Spigo 37, B. Spisso 73a,73b, D.P. Spiteri 60, M. Spousta 136,E.J. Staats 35, R. Stamen 64a, A. Stampekis 21, E. Stanecka 88, W. Stanek-Maslouska 49,M.V. Stange 51, B. Stanislaus 18a, M.M. Stanitzki 49, B. Stapf 49, E.A. Starchenko 38,G.H. Stark 139, J. Stark 91, P. Staroba 134, P. Starovoitov 64a, S. Stärz 106, R. Staszewski 88,G. Stavropoulos 47, P. Steinberg 30, B. Stelzer 145,159a, H.J. Stelzer 132,– 26 –JHEP08(2024)153O. Stelzer-Chilton 159a, H. Stenzel 59, T.J. Stevenson 149, G.A. Stewart 37, J.R. Stewart 124,M.C. Stockton 37, G. Stoicea 28b, M. Stolarski 133a, S. Stonjek 112, A. Straessner 51,J. Strandberg 147, S. Strandberg 48a,48b, M. Stratmann 174, M. Strauss 123, T. Strebler 104,P. Strizenec 29b, R. Ströhmer 169, D.M. Strom 126, R. Stroynowski 45, A. Strubig 48a,48b,S.A. Stucci 30, B. Stugu 17, J. Stupak 123, N.A. Styles 49, D. Su 146, S. Su 63a, W. Su 63d,X. Su 63a, D. Suchy 29a, K. Sugizaki 156, V.V. Sulin 38, M.J. Sullivan 94, D.M.S. Sultan 129,L. Sultanaliyeva 38, S. Sultansoy 3b, T. Sumida 89, S. Sun 173, O. Sunneborn Gudnadottir 164,N. Sur 104, M.R. Sutton 149, H. Suzuki 160, M. Svatos 134, M. Swiatlowski 159a,T. Swirski 169, I. Sykora 29a, M. Sykora 136, T. Sykora 136, D. Ta 102, K. Tackmann 49,t,A. Taffard 162, R. Tafirout 159a, J.S. Tafoya Vargas 67, Y. Takubo 85, M. Talby 104,A.A. Talyshev 38, K.C. Tam 65b, N.M. Tamir154, A. Tanaka 156, J. Tanaka 156, R. Tanaka 67,M. Tanasini 148, Z. Tao 167, S. Tapia Araya 140f , S. Tapprogge 102,A. Tarek Abouelfadl Mohamed 109, S. Tarem 153, K. Tariq 14, G. Tarna 28b, G.F. Tartarelli 72a,M.J. Tartarin 91, P. Tas 136, M. Tasevsky 134, E. Tassi 44b,44a, A.C. Tate 165, G. Tateno 156,Y. Tayalati 36e,v, G.N. Taylor 107, W. Taylor 159b, R. Teixeira De Lima 146,P. Teixeira-Dias 97, J.J. Teoh 158, K. Terashi 156, J. Terron 101, S. Terzo 13, M. Testa 54,R.J. Teuscher 158,w, A. Thaler 80, O. Theiner 57, T. Theveneaux-Pelzer 104, O. Thielmann 174,D.W. Thomas97, J.P. Thomas 21, E.A. Thompson 18a, P.D. Thompson 21, E. Thomson 131,R.E. Thornberry 45, C. Tian 63a, Y. Tian 56, V. Tikhomirov 38,a, Yu.A. Tikhonov 38,S. Timoshenko38, D. Timoshyn 136, E.X.L. Ting 1, P. Tipton 175, A. Tishelman-Charny 30,S.H. Tlou 34g, K. Todome 157, S. Todorova-Nova 136, S. Todt51, L. Toffolin 70a,70c,M. Togawa 85, J. Tojo 90, S. Tokár 29a, K. Tokushuku 85, O. Toldaiev 69, M. Tomoto 85,113,L. Tompkins 146,l, K.W. Topolnicki 87b, E. Torrence 126, H. Torres 91, E. Torró Pastor 166,M. Toscani 31, C. Tosciri 40, M. Tost 11, D.R. Tovey 142, I.S. Trandafir 28b, T. Trefzger 169,A. Tricoli 30, I.M. Trigger 159a, S. Trincaz-Duvoid 130, D.A. Trischuk 27, B. Trocmé 61,A. Tropina39, L. Truong 34c, M. Trzebinski 88, A. Trzupek 88, F. Tsai 148, M. Tsai 108,A. Tsiamis 155, P.V. Tsiareshka38, S. Tsigaridas 159a, A. Tsirigotis 155,q, V. Tsiskaridze 158,E.G. Tskhadadze 152a, M. Tsopoulou 155, Y. Tsujikawa 89, I.I. Tsukerman 38, V. Tsulaia 18a,S. Tsuno 85, K. Tsuri 121, D. Tsybychev 148, Y. Tu 65b, A. Tudorache 28b, V. Tudorache 28b,A.N. Tuna 62, S. Turchikhin 58b,58a, I. Turk Cakir 3a, R. Turra 72a, T. Turtuvshin 39,P.M. Tuts 42, S. Tzamarias 155,d, E. Tzovara 102, F. Ukegawa 160, P.A. Ulloa Poblete 140c,140b,E.N. Umaka 30, G. Unal 37, A. Undrus 30, G. Unel 162, J. Urban 29b, P. Urrejola 140a,G. Usai 8, R. Ushioda 157, M. Usman 110, F. Ustuner 53, Z. Uysal 83, V. Vacek 135,B. Vachon 106, T. Vafeiadis 37, A. Vaitkus 98, C. Valderanis 111, E. Valdes Santurio 48a,48b,M. Valente 159a, S. Valentinetti 24b,24a, A. Valero 166, E. Valiente Moreno 166, A. Vallier 91,J.A. Valls Ferrer 166, D.R. Van Arneman 117, T.R. Van Daalen 141, A. Van Der Graaf 50,P. Van Gemmeren 6, M. Van Rijnbach 37, S. Van Stroud 98, I. Van Vulpen 117, P. Vana 136,M. Vanadia 77a,77b, W. Vandelli 37, E.R. Vandewall 124, D. Vannicola 154, L. Vannoli 54,R. Vari 76a, E.W. Varnes 7, C. Varni 18b, T. Varol 151, D. Varouchas 67, L. Varriale 166,K.E. Varvell 150, M.E. Vasile 28b, L. Vaslin85, G.A. Vasquez 168, A. Vasyukov 39,L.M. Vaughan 124, R. Vavricka102, T. Vazquez Schroeder 37, J. Veatch 32, V. Vecchio 103,M.J. Veen 105, I. Veliscek 30, L.M. Veloce 158, F. Veloso 133a,133c, S. Veneziano 76a,A. Ventura 71a,71b, S. Ventura Gonzalez 138, A. Verbytskyi 112, M. Verducci 75a,75b,– 27 –JHEP08(2024)153C. Vergis 96, M. Verissimo De Araujo 84b, W. Verkerke 117, J.C. Vermeulen 117,C. Vernieri 146, M. Vessella 105, M.C. Vetterli 145,ac, A. Vgenopoulos 102, N. Viaux Maira 140f ,T. Vickey 142, O.E. Vickey Boeriu 142, G.H.A. Viehhauser 129, L. Vigani 64b, M. Vigl 112,M. Villa 24b,24a, M. Villaplana Perez 166, E.M. Villhauer53, E. Vilucchi 54, M.G. Vincter 35,A. Visibile117, C. Vittori 37, I. Vivarelli 24b,24a, E. Voevodina 112, F. Vogel 111, J.C. Voigt 51,P. Vokac 135, Yu. Volkotrub 87b, J. Von Ahnen 49, E. Von Toerne 25, B. Vormwald 37,V. Vorobel 136, K. Vorobev 38, M. Vos 166, K. Voss 144, M. Vozak 117, L. Vozdecky 123,N. Vranjes 16, M. Vranjes Milosavljevic 16, M. Vreeswijk 117, N.K. Vu 63d,63c, R. Vuillermet 37,O. Vujinovic 102, I. Vukotic 40, I.K. Vyas 35, S. Wada 160, C. Wagner105, J.M. Wagner 18a,W. Wagner 174, S. Wahdan 174, H. Wahlberg 92, J. Walder 137, R. Walker 111,W. Walkowiak 144, A. Wall 131, E.J. Wallin 100, T. Wamorkar 6, A.Z. Wang 139,C. Wang 102, C. Wang 11, H. Wang 18a, J. Wang 65c, P. Wang 98, R. Wang 62, R. Wang 6,S.M. Wang 151, S. Wang 63b, S. Wang 14, T. Wang 63a, W.T. Wang 81, W. Wang 14,X. Wang 114a, X. Wang 165, X. Wang 63c, Y. Wang 63d, Y. Wang 114a, Y. Wang 63a,Z. Wang 108, Z. Wang 63d,52,63c, Z. Wang 108, A. Warburton 106, R.J. Ward 21,N. Warrack 60, S. Waterhouse 97, A.T. Watson 21, H. Watson 53, M.F. Watson 21,E. Watton 60,137, G. Watts 141, B.M. Waugh 98, J.M. Webb 55, C. Weber 30, H.A. Weber 19,M.S. Weber 20, S.M. Weber 64a, C. Wei 63a, Y. Wei 55, A.R. Weidberg 129, E.J. Weik 120,J. Weingarten 50, C. Weiser 55, C.J. Wells 49, T. Wenaus 30, B. Wendland 50, T. Wengler 37,N.S. Wenke112, N. Wermes 25, M. Wessels 64a, A.M. Wharton 93, A.S. White 62, A. White 8,M.J. White 1, D. Whiteson 162, L. Wickremasinghe 127, W. Wiedenmann 173, M. Wielers 137,C. Wiglesworth 43, D.J. Wilbern123, H.G. Wilkens 37, J.J.H. Wilkinson 33, D.M. Williams 42,H.H. Williams131, S. Williams 33, S. Willocq 105, B.J. Wilson 103, P.J. Windischhofer 40,F.I. Winkel 31, F. Winklmeier 126, B.T. Winter 55, J.K. Winter 103, M. Wittgen146,M. Wobisch 99, T. Wojtkowski61, Z. Wolffs 117, J. Wollrath162, M.W. Wolter 88,H. Wolters 133a,133c, M.C. Wong139, E.L. Woodward 42, S.D. Worm 49, B.K. Wosiek 88,K.W. Woźniak 88, S. Wozniewski 56, K. Wraight 60, C. Wu 21, M. Wu 114b, M. Wu 116,S.L. Wu 173, X. Wu 57, Y. Wu 63a, Z. Wu 4, J. Wuerzinger 112,aa, T.R. Wyatt 103,B.M. Wynne 53, S. Xella 43, L. Xia 114a, M. Xia 15, M. Xie 63a, S. Xin 14,114c, A. Xiong 126,J. Xiong 18a, D. Xu 14, H. Xu 63a, L. Xu 63a, R. Xu 131, T. Xu 108, Y. Xu 15, Z. Xu 53,Z. Xu114a, B. Yabsley 150, S. Yacoob 34a, Y. Yamaguchi 85, E. Yamashita 156,H. Yamauchi 160, T. Yamazaki 18a, Y. Yamazaki 86, J. Yan63c, S. Yan 60, Z. Yan 105,H.J. Yang 63c,63d, H.T. Yang 63a, S. Yang 63a, T. Yang 65c, X. Yang 37, X. Yang 14,Y. Yang 45, Y. Yang63a, Z. Yang 63a, W-M. Yao 18a, H. Ye 114a, H. Ye 56, J. Ye 14, S. Ye 30,X. Ye 63a, Y. Yeh 98, I. Yeletskikh 39, B.K. Yeo 18b, M.R. Yexley 98, T.P. Yildirim 129,P. Yin 42, K. Yorita 171, S. Younas 28b, C.J.S. Young 37, C. Young 146, C. Yu 14,114c,Y. Yu 63a, J. Yuan 14,114c, M. Yuan 108, R. Yuan 63d,63c, L. Yue 98, M. Zaazoua 63a,B. Zabinski 88, E. Zaid53, Z.K. Zak 88, T. Zakareishvili 166, S. Zambito 57,J.A. Zamora Saa 140d,140b, J. Zang 156, D. Zanzi 55, O. Zaplatilek 135, C. Zeitnitz 174,H. Zeng 14, J.C. Zeng 165, D.T. Zenger Jr 27, O. Zenin 38, T. Ženiš 29a, S. Zenz 96,S. Zerradi 36a, D. Zerwas 67, M. Zhai 14,114c, D.F. Zhang 142, J. Zhang 63b, J. Zhang 6,K. Zhang 14,114c, L. Zhang 63a, L. Zhang 114a, P. Zhang 14,114c, R. Zhang 173, S. Zhang 108,S. Zhang 91, T. Zhang 156, X. Zhang 63c, X. Zhang 63b, Y. Zhang 63c, Y. Zhang 98,– 28 –JHEP08(2024)153Y. Zhang 114a, Z. Zhang 18a, Z. Zhang 63b, Z. Zhang 67, H. Zhao 141, T. Zhao 63b,Y. Zhao 139, Z. Zhao 63a, Z. Zhao 63a, A. Zhemchugov 39, J. Zheng 114a, K. Zheng 165,X. Zheng 63a, Z. Zheng 146, D. Zhong 165, B. Zhou 108, H. Zhou 7, N. Zhou 63c, Y. Zhou15,Y. Zhou 114a, Y. Zhou7, C.G. Zhu 63b, J. Zhu 108, X. Zhu63d, Y. Zhu 63c, Y. Zhu 63a,X. Zhuang 14, K. Zhukov 69, N.I. Zimine 39, J. Zinsser 64b, M. Ziolkowski 144, L. Živković 16,A. Zoccoli 24b,24a, K. Zoch 62, T.G. Zorbas 142, O. Zormpa 47, W. Zou 42, L. Zwalinski 371Department of Physics, University of Adelaide, Adelaide, Australia2Department of Physics, University of Alberta, Edmonton AB, Canada3 (a)Department of Physics, Ankara University, Ankara; (b)Division of Physics, TOBB University ofEconomics and Technology, Ankara, Türkiye4 LAPP, Université Savoie Mont Blanc, CNRS/IN2P3, Annecy, France5APC, Université Paris Cité, CNRS/IN2P3, Paris, France6High Energy Physics Division, Argonne National Laboratory, Argonne IL, United States of America7Department of Physics, University of Arizona, Tucson AZ, United States of America8Department of Physics, University of Texas at Arlington, Arlington TX, United States of America9 Physics Department, National and Kapodistrian University of Athens, Athens, Greece10 Physics Department, National Technical University of Athens, Zografou, Greece11Department of Physics, University of Texas at Austin, Austin TX, United States of America12 Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan13 Institut de Física d’Altes Energies (IFAE), Barcelona Institute of Science and Technology, Barcelona,Spain14 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China15 Physics Department, Tsinghua University, Beijing, China16 Institute of Physics, University of Belgrade, Belgrade, Serbia17Department for Physics and Technology, University of Bergen, Bergen, Norway18 (a)Physics Division, Lawrence Berkeley National Laboratory, Berkeley CA; (b)University of California,Berkeley CA, United States of America19 Institut für Physik, Humboldt Universität zu Berlin, Berlin, Germany20Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University ofBern, Bern, Switzerland21 School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom22 (a)Department of Physics, Bogazici University, Istanbul; (b)Department of Physics Engineering, GaziantepUniversity, Gaziantep; (c)Department of Physics, Istanbul University, Istanbul, Türkiye23 (a)Facultad de Ciencias y Centro de Investigaciónes, Universidad Antonio Nariño, Bogotá;(b)Departamento de Física, Universidad Nacional de Colombia, Bogotá, Colombia24 (a)Dipartimento di Fisica e Astronomia A. Righi, Università di Bologna, Bologna; (b)INFN Sezione diBologna, Italy25 Physikalisches Institut, Universität Bonn, Bonn, Germany26Department of Physics, Boston University, Boston MA, United States of America27Department of Physics, Brandeis University, Waltham MA, United States of America28 (a)Transilvania University of Brasov, Brasov; (b)Horia Hulubei National Institute of Physics and NuclearEngineering, Bucharest; (c)Department of Physics, Alexandru Ioan Cuza University of Iasi, Iasi;(d)National Institute for Research and Development of Isotopic and Molecular Technologies, PhysicsDepartment, Cluj-Napoca; (e)National University of Science and Technology Politechnica, Bucharest;(f)West University in Timisoara, Timisoara; (g)Faculty of Physics, University of Bucharest, Bucharest,Romania29 (a)Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava; (b)Department ofSubnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, SlovakRepublic30 Physics Department, Brookhaven National Laboratory, Upton NY, United States of America31Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales, Departamento de Física, yCONICET, Instituto de Física de Buenos Aires (IFIBA), Buenos Aires, Argentina– 29 –JHEP08(2024)15332California State University, CA, United States of America33Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom34 (a)Department of Physics, University of Cape Town, Cape Town; (b)iThemba Labs, Western Cape;(c)Department of Mechanical Engineering Science, University of Johannesburg, Johannesburg; (d)NationalInstitute of Physics, University of the Philippines Diliman (Philippines); (e)University of South Africa,Department of Physics, Pretoria; (f)University of Zululand, KwaDlangezwa; (g)School of Physics,University of the Witwatersrand, Johannesburg, South Africa35Department of Physics, Carleton University, Ottawa ON, Canada36 (a)Faculté des Sciences Ain Chock, Réseau Universitaire de Physique des Hautes Energies - UniversitéHassan II, Casablanca; (b)Faculté des Sciences, Université Ibn-Tofail, Kénitra; (c)Faculté des SciencesSemlalia, Université Cadi Ayyad, LPHEA-Marrakech; (d)LPMR, Faculté des Sciences, UniversitéMohamed Premier, Oujda; (e)Faculté des sciences, Université Mohammed V, Rabat; (f)Institute ofApplied Physics, Mohammed VI Polytechnic University, Ben Guerir, Morocco37CERN, Geneva, Switzerland38Affiliated with an institute covered by a cooperation agreement with CERN39Affiliated with an international laboratory covered by a cooperation agreement with CERN40 Enrico Fermi Institute, University of Chicago, Chicago IL, United States of America41 LPC, Université Clermont Auvergne, CNRS/IN2P3, Clermont-Ferrand, France42Nevis Laboratory, Columbia University, Irvington NY, United States of America43Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark44 (a)Dipartimento di Fisica, Università della Calabria, Rende; (b)INFN Gruppo Collegato di Cosenza,Laboratori Nazionali di Frascati, Italy45 Physics Department, Southern Methodist University, Dallas TX, United States of America46 Physics Department, University of Texas at Dallas, Richardson TX, United States of America47National Centre for Scientific Research “Demokritos”, Agia Paraskevi, Greece48 (a)Department of Physics, Stockholm University; (b)Oskar Klein Centre, Stockholm, Sweden49Deutsches Elektronen-Synchrotron DESY, Hamburg and Zeuthen, Germany50 Fakultät Physik, Technische Universität Dortmund, Dortmund, Germany51 Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany52Department of Physics, Duke University, Durham NC, United States of America53 SUPA - School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom54 INFN e Laboratori Nazionali di Frascati, Frascati, Italy55 Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg, Germany56 II. Physikalisches Institut, Georg-August-Universität Göttingen, Göttingen, Germany57Département de Physique Nucléaire et Corpusculaire, Université de Genève, Genève, Switzerland58 (a)Dipartimento di Fisica, Università di Genova, Genova; (b)INFN Sezione di Genova, Italy59 II. Physikalisches Institut, Justus-Liebig-Universität Giessen, Giessen, Germany60 SUPA - School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom61 LPSC, Université Grenoble Alpes, CNRS/IN2P3, Grenoble INP, Grenoble, France62 Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge MA,United States of America63 (a)Department of Modern Physics and State Key Laboratory of Particle Detection and Electronics,University of Science and Technology of China, Hefei; (b)Institute of Frontier and InterdisciplinaryScience and Key Laboratory of Particle Physics and Particle Irradiation (MOE), Shandong University,Qingdao; (c)School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory forParticle Astrophysics and Cosmology (MOE), SKLPPC, Shanghai; (d)Tsung-Dao Lee Institute, Shanghai;(e)School of Physics and Microelectronics, Zhengzhou University, China64 (a)Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg; (b)PhysikalischesInstitut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany65 (a)Department of Physics, Chinese University of Hong Kong, Shatin, N.T., Hong Kong; (b)Department ofPhysics, University of Hong Kong, Hong Kong; (c)Department of Physics and Institute for AdvancedStudy, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, China66Department of Physics, National Tsing Hua University, Hsinchu, Taiwan– 30 –JHEP08(2024)15367 IJCLab, Université Paris-Saclay, CNRS/IN2P3, 91405, Orsay, France68Centro Nacional de Microelectrónica (IMB-CNM-CSIC), Barcelona, Spain69Department of Physics, Indiana University, Bloomington IN, United States of America70 (a)INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine; (b)ICTP, Trieste; (c)DipartimentoPolitecnico di Ingegneria e Architettura, Università di Udine, Udine, Italy71 (a)INFN Sezione di Lecce; (b)Dipartimento di Matematica e Fisica, Università del Salento, Lecce, Italy72 (a)INFN Sezione di Milano; (b)Dipartimento di Fisica, Università di Milano, Milano, Italy73 (a)INFN Sezione di Napoli; (b)Dipartimento di Fisica, Università di Napoli, Napoli, Italy74 (a)INFN Sezione di Pavia; (b)Dipartimento di Fisica, Università di Pavia, Pavia, Italy75 (a)INFN Sezione di Pisa; (b)Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy76 (a)INFN Sezione di Roma; (b)Dipartimento di Fisica, Sapienza Università di Roma, Roma, Italy77 (a)INFN Sezione di Roma Tor Vergata; (b)Dipartimento di Fisica, Università di Roma Tor Vergata,Roma, Italy78 (a)INFN Sezione di Roma Tre; (b)Dipartimento di Matematica e Fisica, Università Roma Tre, Roma, Italy79 (a)INFN-TIFPA; (b)Università degli Studi di Trento, Trento, Italy80Universität Innsbruck, Department of Astro and Particle Physics, Innsbruck, Austria81University of Iowa, Iowa City IA, United States of America82Department of Physics and Astronomy, Iowa State University, Ames IA, United States of America83 Istinye University, Sariyer, Istanbul, Türkiye84 (a)Departamento de Engenharia Elétrica, Universidade Federal de Juiz de Fora (UFJF), Juiz de Fora;(b)Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro; (c)Instituto de Física,Universidade de São Paulo, São Paulo; (d)Rio de Janeiro State University, Rio de Janeiro; (e)FederalUniversity of Bahia, Bahia, Brazil85KEK, High Energy Accelerator Research Organization, Tsukuba, Japan86Graduate School of Science, Kobe University, Kobe, Japan87 (a)AGH University of Krakow, Faculty of Physics and Applied Computer Science, Krakow; (b)MarianSmoluchowski Institute of Physics, Jagiellonian University, Krakow, Poland88 Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland89 Faculty of Science, Kyoto University, Kyoto, Japan90Research Center for Advanced Particle Physics and Department of Physics, Kyushu University, Fukuoka,Japan91 L2IT, Université de Toulouse, CNRS/IN2P3, UPS, Toulouse, France92 Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina93 Physics Department, Lancaster University, Lancaster, United Kingdom94Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom95Department of Experimental Particle Physics, Jožef Stefan Institute and Department of Physics,University of Ljubljana, Ljubljana, Slovenia96 School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom97Department of Physics, Royal Holloway University of London, Egham, United Kingdom98Department of Physics and Astronomy, University College London, London, United Kingdom99 Louisiana Tech University, Ruston LA, United States of America100 Fysiska institutionen, Lunds universitet, Lund, Sweden101Departamento de Física Teorica C-15 and CIAFF, Universidad Autónoma de Madrid, Madrid, Spain102 Institut für Physik, Universität Mainz, Mainz, Germany103 School of Physics and Astronomy, University of Manchester, Manchester, United Kingdom104CPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille, France105Department of Physics, University of Massachusetts, Amherst MA, United States of America106Department of Physics, McGill University, Montreal QC, Canada107 School of Physics, University of Melbourne, Victoria, Australia108Department of Physics, University of Michigan, Ann Arbor MI, United States of America109Department of Physics and Astronomy, Michigan State University, East Lansing MI,United States of America110Group of Particle Physics, University of Montreal, Montreal QC, Canada– 31 –JHEP08(2024)153111 Fakultät für Physik, Ludwig-Maximilians-Universität München, München, Germany112Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), München, Germany113Graduate School of Science and Kobayashi-Maskawa Institute, Nagoya University, Nagoya, Japan114 (a)Department of Physics, Nanjing University, Nanjing; (b)School of Science, Shenzhen Campus of SunYat-sen University; (c)University of Chinese Academy of Science (UCAS), Beijing, China115Department of Physics and Astronomy, University of New Mexico, Albuquerque NM,United States of America116 Institute for Mathematics, Astrophysics and Particle Physics, Radboud University/Nikhef, Nijmegen,The Netherlands117Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam,The Netherlands118Department of Physics, Northern Illinois University, DeKalb IL, United States of America119 (a)New York University Abu Dhabi, Abu Dhabi; (b)United Arab Emirates University, Al Ain,United Arab Emirates120Department of Physics, New York University, New York NY, United States of America121Ochanomizu University, Otsuka, Bunkyo-ku, Tokyo, Japan122Ohio State University, Columbus OH, United States of America123Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman OK,United States of America124Department of Physics, Oklahoma State University, Stillwater OK, United States of America125 Palacký University, Joint Laboratory of Optics, Olomouc, Czech Republic126 Institute for Fundamental Science, University of Oregon, Eugene, OR, United States of America127Graduate School of Science, Osaka University, Osaka, Japan128Department of Physics, University of Oslo, Oslo, Norway129Department of Physics, Oxford University, Oxford, United Kingdom130 LPNHE, Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris, France131Department of Physics, University of Pennsylvania, Philadelphia PA, United States of America132Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh PA, United States of America133 (a)Laboratório de Instrumentação e Física Experimental de Partículas - LIP, Lisboa; (b)Departamento deFísica, Faculdade de Ciências, Universidade de Lisboa, Lisboa; (c)Departamento de Física, Universidadede Coimbra, Coimbra; (d)Centro de Física Nuclear da Universidade de Lisboa, Lisboa; (e)Departamento deFísica, Universidade do Minho, Braga; (f)Departamento de Física Teórica y del Cosmos, Universidad deGranada, Granada (Spain); (g)Departamento de Física, Instituto Superior Técnico, Universidade deLisboa, Lisboa, Portugal134 Institute of Physics of the Czech Academy of Sciences, Prague, Czech Republic135Czech Technical University in Prague, Prague, Czech Republic136Charles University, Faculty of Mathematics and Physics, Prague, Czech Republic137 Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom138 IRFU, CEA, Université Paris-Saclay, Gif-sur-Yvette, France139 Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz CA,United States of America140 (a)Departamento de Física, Pontificia Universidad Católica de Chile, Santiago; (b)Millennium Institutefor Subatomic physics at high energy frontier (SAPHIR), Santiago; (c)Instituto de InvestigaciónMultidisciplinario en Ciencia y Tecnología, y Departamento de Física, Universidad de La Serena;(d)Universidad Andres Bello, Department of Physics, Santiago; (e)Instituto de Alta Investigación,Universidad de Tarapacá, Arica; (f)Departamento de Física, Universidad Técnica Federico Santa María,Valparaíso, Chile141Department of Physics, University of Washington, Seattle WA, United States of America142Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom143Department of Physics, Shinshu University, Nagano, Japan144Department Physik, Universität Siegen, Siegen, Germany145Department of Physics, Simon Fraser University, Burnaby BC, Canada146 SLAC National Accelerator Laboratory, Stanford CA, United States of America– 32 –JHEP08(2024)153147Department of Physics, Royal Institute of Technology, Stockholm, Sweden148Departments of Physics and Astronomy, Stony Brook University, Stony Brook NY,United States of America149Department of Physics and Astronomy, University of Sussex, Brighton, United Kingdom150 School of Physics, University of Sydney, Sydney, Australia151 Institute of Physics, Academia Sinica, Taipei, Taiwan152 (a)E. Andronikashvili Institute of Physics, Iv. Javakhishvili Tbilisi State University, Tbilisi; (b)HighEnergy Physics Institute, Tbilisi State University, Tbilisi; (c)University of Georgia, Tbilisi, Georgia153Department of Physics, Technion, Israel Institute of Technology, Haifa, Israel154Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel155Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece156 International Center for Elementary Particle Physics and Department of Physics, University of Tokyo,Tokyo, Japan157Department of Physics, Tokyo Institute of Technology, Tokyo, Japan158Department of Physics, University of Toronto, Toronto ON, Canada159 (a)TRIUMF, Vancouver BC; (b)Department of Physics and Astronomy, York University, Toronto ON,Canada160Division of Physics and Tomonaga Center for the History of the Universe, Faculty of Pure and AppliedSciences, University of Tsukuba, Tsukuba, Japan161Department of Physics and Astronomy, Tufts University, Medford MA, United States of America162Department of Physics and Astronomy, University of California Irvine, Irvine CA, United States ofAmerica163University of Sharjah, Sharjah, United Arab Emirates164Department of Physics and Astronomy, University of Uppsala, Uppsala, Sweden165Department of Physics, University of Illinois, Urbana IL, United States of America166 Instituto de Física Corpuscular (IFIC), Centro Mixto Universidad de Valencia - CSIC, Valencia, Spain167Department of Physics, University of British Columbia, Vancouver BC, Canada168Department of Physics and Astronomy, University of Victoria, Victoria BC, Canada169 Fakultät für Physik und Astronomie, Julius-Maximilians-Universität Würzburg, Würzburg, Germany170Department of Physics, University of Warwick, Coventry, United Kingdom171Waseda University, Tokyo, Japan172Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel173Department of Physics, University of Wisconsin, Madison WI, United States of America174 Fakultät für Mathematik und Naturwissenschaften, Fachgruppe Physik, Bergische Universität Wuppertal,Wuppertal, Germany175Department of Physics, Yale University, New Haven CT, United States of AmericaaAlso Affiliated with an institute covered by a cooperation agreement with CERNbAlso at An-Najah National University, Nablus, PalestinecAlso at Borough of Manhattan Community College, City University of New York, New York NY,United States of AmericadAlso at Center for Interdisciplinary Research and Innovation (CIRI-AUTH), Thessaloniki, GreeceeAlso at CERN, Geneva, Switzerlandf Also at CMD-AC UNEC Research Center, Azerbaijan State University of Economics (UNEC), AzerbaijangAlso at Département de Physique Nucléaire et Corpusculaire, Université de Genève, Genève, SwitzerlandhAlso at Departament de Fisica de la Universitat Autonoma de Barcelona, Barcelona, SpainiAlso at Department of Financial and Management Engineering, University of the Aegean, Chios, Greecej Also at Department of Physics, California State University, Sacramento, United States of AmericakAlso at Department of Physics, King’s College London, London, United KingdomlAlso at Department of Physics, Stanford University, Stanford CA, United States of AmericamAlso at Department of Physics, Stellenbosch University, South AfricanAlso at Department of Physics, University of Fribourg, Fribourg, SwitzerlandoAlso at Department of Physics, University of Thessaly, GreecepAlso at Department of Physics, Westmont College, Santa Barbara, United States of America– 33 –JHEP08(2024)153qAlso at Hellenic Open University, Patras, GreecerAlso at Imam Mohammad Ibn Saud Islamic University, Saudi ArabiasAlso at Institucio Catalana de Recerca i Estudis Avancats, ICREA, Barcelona, SpaintAlso at Institut für Experimentalphysik, Universität Hamburg, Hamburg, GermanyuAlso at Institute for Nuclear Research and Nuclear Energy (INRNE) of the Bulgarian Academy ofSciences, Sofia, BulgariavAlso at Institute of Applied Physics, Mohammed VI Polytechnic University, Ben Guerir, MoroccowAlso at Institute of Particle Physics (IPP), CanadaxAlso at Institute of Physics, Azerbaijan Academy of Sciences, Baku, AzerbaijanyAlso at Institute of Theoretical Physics, Ilia State University, Tbilisi, GeorgiazAlso at National Institute of Physics, University of the Philippines Diliman (Philippines), PhilippinesaaAlso at Technical University of Munich, Munich, GermanyabAlso at The Collaborative Innovation Center of Quantum Matter (CICQM), Beijing, ChinaacAlso at TRIUMF, Vancouver BC, CanadaadAlso at Università di Napoli Parthenope, Napoli, ItalyaeAlso at University of Colorado Boulder, Department of Physics, Colorado, United States of Americaaf Also at Washington College, Chestertown, MD, United States of AmericaagAlso at Yeditepe University, Physics Department, Istanbul, Türkiye∗Deceased– 34 –
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Hadron-Hadron Scattering
Higgs Physics
Combination of searches for Higgs boson decays into a photon and a massless dark photon using pp collisions at √s = 13 TeV with the ATLAS detector
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