This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

Discriminating between Higgs Production Mechanisms via Jet Charge at the LHC

Hai Tao Li [email protected] School of Physics, Shandong University, Jinan, Shandong 250100, China    Bin Yan [email protected] (corresponding author) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China    C.-P. Yuan [email protected] Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
Abstract

Discriminating the Higgs production mechanisms plays a crucial role in directly measuring the couplings of Higgs to gauge bosons for probing the nature of the electroweak symmetry breaking. We propose a novel method to distinguish the Higgs production mechanisms at the LHC by utilizing the jet charge asymmetry of the two leading forward jets in Higgs plus two jets production. This novel observable provides a way to disentangle the WW-fusion from the ZZ-fusion and gluon fusion processes for the first time, due to the electric charge correlation of the two leading jets in the events. We show that the Higgs couplings to gauge bosons can be well constrained and its conclusion does not depend on the other possible new physics effects which modify the Higgs total or partial width. We also discuss the complementary roles between the proposed jet charge asymmetry measurement and the Higgs signal strength measurements at the HL-LHC in determining the Higgs couplings.

preprint: MSUHEP-23-001

Introduction: Precisely measuring the interactions between the Higgs boson and the weak gauge bosons (WW and ZZ) plays a crucial role to verify the electroweak symmetry breaking (EWSB) mechanism of the Standard Model (SM) and beyond. These couplings have been widely discussed under the framework of κ\kappa scheme or the Standard Model effective field theory (SMEFT) at the Large Hadron Collider (LHC) and future colliders [1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18]. From the recent global analysis of the ATLAS [19] and CMS [20] Collaborations at the 13 TeV LHC, the magnitudes of these couplings have been severely constrained by the Higgs data within an uncertainty about 𝒪(10%)\mathcal{O}(10\%), i.e. κW=1.05±0.06\kappa_{W}=1.05\pm 0.06, κZ=0.99±0.06\kappa_{Z}=0.99\pm 0.06 (ATLAS) and κW=1.02±0.08\kappa_{W}=1.02\pm 0.08, κZ=1.04±0.07\kappa_{Z}=1.04\pm 0.07 (CMS), where κW,Z\kappa_{W,Z} are the effective gauge coupling strengths between the Higgs boson and the WW and ZZ bosons, respectively,

hVV=κWghWWSMhWμ+Wμ+κZ2ghZZSMhZμZμ,\mathcal{L}_{hVV}=\kappa_{W}g_{hWW}^{\rm SM}hW_{\mu}^{+}W^{-\mu}+\frac{\kappa_{Z}}{2}g_{hZZ}^{\rm SM}hZ_{\mu}Z^{\mu}, (1)

where ghVVSM=2mV2/vg_{hVV}^{\rm SM}=2m_{V}^{2}/v, with V=W,ZV=W,Z, are the Higgs couplings to gauge boson VV in the SM, and v=246GeVv=246~{}{\rm GeV} is the vacuum expectation value.

However, to date, all the knowledge of the Higgs couplings is inferred from the global analysis of the Higgs data under the narrow width approximation for the Higgs production and decay. As a result, the measurements of the Higgs properties are strongly depending on the assumption of the Higgs width, which is difficult to be directly measured at the LHC [19, 20]. Therefore, probing the Higgs couplings with the fewest possible theoretical assumptions (e.g., Higgs width) plays a crucial role to verify the nature of the EWSB. One of the approaches to overcome the shortness of the current global analysis is to measure the off-shell Higgs signal strengths [21, 22, 23, 24]. Unfortunately, the Higgs cross sections decrease so fast in off-shell Higgs phase space region that it would be a challenge to measure the Higgs couplings with a high accuracy [25, 26]. Moreover, generally, the determination of the Higgs couplings also depends on other theoretical assumptions made in the analysis [23, 27, 28, 29, 30, 31, 32].

Refer to caption
Figure 1: Illustrative Feynman diagrams of VBF and GGF Higgs+2 jets production at the LHC. The black dots denote the effective Higgs couplings to gauge bosons.

For the purpose of determining the hVVhVV couplings, the mechanism of Higgs production via vector boson fusion (VBF) plays an essential role at the LHC. The representative Feynman diagrams at the leading order are shown in Fig. 1. Since the Higgs+2 jets production through the gluon-gluon fusion (GGF) process is the dominant background for the VBF Higgs production at the LHC, the attempt of separating the VBF from the GGF production has been widely discussed [33, 34, 35, 36, 37, 38, 39, 40, 41]. It shows that the contribution from the GGF process can be largely suppressed by requiring a large rapidity gap and a large invariant mass of the two hardest jets in the Higgs+2 jets events [33, 34, 35]. We can also utilize the different features of soft gluon radiations between the VBF and GGF processes to suppress the contribution from the GGF, e.g., the difference in the jet energy profiles [36] and the azimuthal angle correlation between the Higgs and two-jet system [37, 40]. But, none of them could distinguish WWWW and ZZZZ-boson fusion processes. Separating the WW boson’s contribution from the VBF Higgs production is an important task for determining κW\kappa_{W} and κZ\kappa_{Z}, separately, at the LHC.

To suppress the contributions from the ZZ-boson fusion and the GGF processes, we define a novel observable called jet charge asymmetry between the two leading jets in the Higgs+2 jets production. For the first time, we demonstrate that the jet charge correlations in Higgs+2 jets production can be used to separate the WW-boson fusion from the ZZ-boson fusion and GGF processes; the electric charges of the two leading jets in WW-boson fusion are opposite, while they could be the same or opposite for the ZZ-boson fusion and the GGF processes. We argue that one could determine the κW,Z\kappa_{W,Z} without making an assumption on the Higgs width and the other possible new physics effects from Higgs decay. Moreover, the correlation between κW\kappa_{W} and κZ\kappa_{Z}, obtained from the jet charges measurement, would be different from other experimental observable (e.g., the Higgs signal strength measurement) in the VBF processes. Therefore, the jet charge correlation in the production of Higgs+2 jets could play an important, and complementary, role in determining the hVVhVV couplings.

Jet charge: Jet charge can be used to mimic the electric charge of the parent parton which evolves into a collimated spray of particles. It is defined as a weighted sum of the electric charge of the jet constituents [42, 43, 44],

QJ=1(pTJ)κijetQi(pTi)κ,κ>0,Q_{J}=\frac{1}{(p_{T}^{J})^{\kappa}}\sum_{i\in{\rm jet}}Q_{i}(p_{T}^{i})^{\kappa},\quad\kappa>0, (2)

with pTJp_{T}^{J} the transverse momentum of the jet, pTip_{T}^{i} and QiQ_{i} are the transverse momentum and electric charge of particle ii inside the jet. And κ\kappa is a free parameter which suppresses the contribution from soft radiations. The theoretical framework to calculate jet charge in QCD was proposed in Refs. [43, 44]. As one of the jet substructure techniques, jet charge has been used for quark/gluon jet discrimination [45, 46, 47]. There are many efforts using jet charge as a tool to tag the hard process [48] and to search for new physics signals [49, 50]. Jet charge has also been applied to probe nuclear medium effects in heavy-ion and electron-ion collisions [51, 52, 53], as well as quark flavor structure of the nucleon [54, 55, 56]. Experimentally, jet charge has been recently measured by ATLAS and CMS Collaborations [57, 58, 59, 60]. The theoretical and experimental efforts show that the jet charge serves well for identifying the charge of the primordial parton of the hard scattering. In this letter, we will apply the jet charge observable in the production of Higgs+2 jets to discriminate the Higgs production mechanisms at the LHC and to further constrain the Higgs couplings to gauge bosons.

Collider simulation: We perform a detailed Monte Carlo simulation to explore the potential of the LHC for discriminating Higgs production mechanisms and probing the hVVhVV couplings via jet charge correlations. We generate both the W/ZW/Z fusion and GGF Higgs production processes at the 14 TeV LHC by MadGraph5 [61] at the parton-level with the CT14LO parton distribution functions (PDFs) [62]. The following basic cuts for the jets are required in the partonic final state: pTj>20GeVp_{T}^{j}>20~{}{\rm GeV} with |ηj|<5|\eta_{j}|<5, where pTjp_{T}^{j} and ηj\eta_{j} denotes the transverse momentum and rapidity of jet, respectively. The GGF process was generated under the heavy top quark limit, i.e., the EFT operator αs/(12πv)hGμνaGμν,a\alpha_{s}/(12\pi v)hG_{\mu\nu}^{a}G^{\mu\nu,a}, which provides a good approximation when the top quarks inside the loop are off-shell. To get the isolated jets, we require the cone distance between the two jets ΔR>0.4\Delta R>0.4. To suppress the contribution from the GGF process, we further require the invariant mass of jet pair mjj>110GeVm_{jj}>110~{}{\rm GeV} and rapidity gap between the two jets |Δηjj|>2.5|\Delta\eta_{jj}|>2.5. The jet is defined based on the anti-kTk_{T} algorithm [63] with the radius parameter R=0.4R=0.4. Then we pass the events to PYTHIA [64, 65] for parton showering and hadronization. At the analysis level, all the events are required to pass a set of selection cuts following the settings from Ref. [19],

pTj>30GeV,\displaystyle p_{T}^{j}>30~{}{\rm GeV}, 1<|ηj|<4.5,\displaystyle 1<|\eta_{j}|<4.5,
mjj>120GeV,\displaystyle m_{jj}>120~{}{\rm GeV}, |Δηjj|>3.5,\displaystyle|\Delta\eta_{jj}|>3.5, |ηh|<2.5,\displaystyle|\eta_{h}|<2.5\,, (3)

where ηh\eta_{h} is the pseudorapidity of the Higgs boson.

Refer to caption
Refer to caption
Refer to caption
Figure 2: The jet charge correlations between the leading and subleading jets from WW-fusion, ZZ-fusion, and GGF processes with jet charge parameter κ=0.3\kappa=0.3.
Refer to caption
Figure 3: The jet charge asymmetry A¯Q\overline{A}_{Q} distributions as a function of the average transverse momentum of the two leading jets p¯T\overline{p}_{T} at the 14 TeV LHC with the integrated luminosity =300fb1\mathcal{L}=300~{}{\rm fb}^{-1}. Its systematic uncertainties are assumed to cancel out.

On average the sign of the jet charge is consistent with the charge of the parton which evolves into the jet from the measurements at the LHC [58, 59]. Therefore, the charge correlations for different VBF channels indicate the charge correlations of the parton in the hard process. Figure 2 shows the jet charge correlations between the leading and subleading jets from the WW-fusion, ZZ-fusion and GGF processes after the kinematic cuts (see Eq. (3)) with the benchmark jet charge parameter κ=0.3\kappa=0.3. It clearly shows that the opposite sign of the two leading jet charges is favored in WW-fusion process due to the partonic nature of the hard scattering at the leading order. However, this feature is disappeared in ZZ-fusion and GGF processes. It arises from the fact that both the opposite and same sign electric charges of the two leading jets in ZZ-fusion could be generated with a comparable production rate, while the sign of the jet charges in the GGF process is arbitrary. Motivated by this, we define the jet charge asymmetry of the two leading jets in Higgs+2 jets production by

AQ=|QJ1QJ2QJ1+QJ2|,A_{Q}=\left|\frac{Q_{J}^{1}-Q_{J}^{2}}{Q_{J}^{1}+Q_{J}^{2}}\right|, (4)

where QJ1,2Q_{J}^{1,2} is the jet charge of the leading and subleading jets, respectively. The advantage of this observable is that the systematic uncertainties, which are the dominant errors in jet charge measurements at the ATLAS and CMS Collaborations [58, 59], are expected to be canceled. This conclusion has been verified by the previous studies of other track-based observable in the HERA measurement [66]. On the other hand, the jet charge distributions are sensitive only to the weight of the jet flavor of final states in the hard scattering but not to the Higgs decay information (i.e., the Higgs width and the other possible new physics effects in Higgs decay). However, the jet charge asymmetry in Eq. (4) may be unstable since it can be much enhanced for the events with QJ1+QJ20Q_{J}^{1}+Q_{J}^{2}\sim 0, therefore, we will utilize the average values of the jet charges to define this asymmetry in this paper, i.e.,

A¯Q|QJ1QJ2||QJ1+QJ2|Q()Q(+),\overline{A}_{Q}\equiv\frac{\langle\left|Q_{J}^{1}-Q_{J}^{2}\right|\rangle}{\langle\left|Q_{J}^{1}+Q_{J}^{2}\right|\rangle}\equiv\frac{\langle Q^{(-)}\rangle}{\langle Q^{(+)}\rangle}, (5)

where Q\langle Q\rangle denotes the average value of the quantity QQ and Q(±)=|QJ1±QJ2|Q^{(\pm)}=|Q_{J}^{1}\pm Q_{J}^{2}|. From the definition, if the charges have the opposite sign such as the partonic process for WW-fusion case, the asymmetry is expected to be A¯Q>1\overline{A}_{Q}>1. However, if the charges have the same sign, e.g., the ZZ-fusion process uuuuhuu\to uuh, A¯Q<1\overline{A}_{Q}<1. For the GGF process the charges are fully uncorrelated so that A¯Q1\overline{A}_{Q}\sim 1.

Figure 3 shows the jet charge asymmetry A¯Q\overline{A}_{Q} as a function of the average transverse momentum of the two leading jets (p¯T(pT1+pT2)/2\overline{p}_{T}\equiv(p_{T}^{1}+p_{T}^{2})/2) in Higgs+2 jets production at the 14 TeV LHC with the integrated luminosity =300fb1\mathcal{L}=300~{}{\rm fb}^{-1}. The statistical uncertainties are estimated from the Pythia simulation by generating a large number of pseudo experiments. We assume that the statistical errors follow the Gaussian distribution and could be rescaled to any integrated luminosity by the event numbers. We have checked that A¯Q\overline{A}_{Q} does not noticeably depend on the choice of κ\kappa value, when varying from 0.3 to 0.7. As expected we find A¯Q>1\overline{A}_{Q}>1 for the WW-fusion (black points) since the sign of the jet charges are opposite. However, the asymmetry is close to one for the ZZ-fusion as shown with blue points in Fig. 3. To further understand the behavior of the ZZ-fusion, we also show A¯Q\overline{A}_{Q} for the ZZ-fusion with opposite (red points) and same sign jet charges (cyan points) in the same figure and the results are consistent with the argument before. When we combine all possible channels, this asymmetry would be close to one for the ZZ-fusion process since the opposite and same sign jet charge configurations could give a comparable contribution. The dominant contributions for the GGF process come from the qgqg and gggg initial states, in result, we could expect that A¯Q1\overline{A}_{Q}\sim 1 due to the uncorrelated nature of the jet charges in this process.

We also notice that the jet charge asymmetry is not very sensitive to p¯T\overline{p}_{T} for the ZZ-fusion and the GGF processes. In particular, it exhibits a weak p¯T\overline{p}_{T} dependence for the WW-fusion and the ZZ-fusion with opposite or same sign jet charges. To be clear about the p¯T\overline{p}_{T} dependence for the WW and the ZZ-fusion processes, we calculate various initial state (qqqq^{\prime}) fraction distributions fqqf_{qq^{\prime}} for the WW-fusion and the ZZ-fusion after the kinematic cuts in Eq. (3) at the leading order; see Fig. 4. It shows that the dudu quark initial state dominates the cross section in WW-fusion (see Fig. 4(a)) and it will induce a weak p¯T\overline{p}_{T} dependence for the charge asymmetry in Fig. 3 (black points). For the ZZ-fusion process, we only show the fractions of the dominated channels in Fig. 4(b). The weak p¯T\overline{p}_{T} dependence for the charge asymmetry of the ZZ-fusion with opposite (red points in Fig. 3) and same sign (cyan points in Fig. 3) jet charges can also be understood from the behavior of the dominated fractions fudf_{ud} and fuuf_{uu}. As a consequence, the jet charge asymmetry of the ZZ-fusion will not be sensitive to the p¯T\overline{p}_{T} after we combine all the subprocesses.

Refer to caption
Refer to caption
Figure 4: Various initial state (qqqq^{\prime}) fraction distributions fqqf_{qq^{\prime}} for Higgs+2 jets production via WW-fusion and ZZ-fusion at the 14 TeV LHC, as a function of the average jet p¯T\overline{p}_{T}.

Next, we utilize the A¯Q\overline{A}_{Q} information to constrain the hVVhVV couplings. After combing the WW-fusion, ZZ-fusion and GGF cross sections, the jet charge asymmetry in Higgs+2 jets process reads as

A¯Qtot=\displaystyle\overline{A}_{Q}^{\rm tot}= fWQ()W+fZQ()Z+fGQ()GfWQ(+)W+fZQ(+)Z+fGQ(+)G,\displaystyle\frac{f_{W}\langle Q^{(-)}\rangle_{W}+f_{Z}\langle Q^{(-)}\rangle_{Z}+f_{G}\langle Q^{(-)}\rangle_{G}}{f_{W}\langle Q^{(+)}\rangle_{W}+f_{Z}\langle Q^{(+)}\rangle_{Z}+f_{G}\langle Q^{(+)}\rangle_{G}}\;, (6)

where the subscripts WW, ZZ and GG represent the contribution from different channels accordingly. The fractions fi(p¯T,κW/Z)f_{i}(\overline{p}_{T},\kappa_{W/Z}) is defined as σi/(σW+σZ+σG)\sigma_{i}/(\sigma_{W}+\sigma_{Z}+\sigma_{G}) with i=W,Z,Gi=W,Z,G. It shows that the WW-boson fusion dominates the cross section after applying the kinematic cuts in Eq. (3). The contamination from GGF can be further suppressed with boosted decision trees analysis, as shown in Fig. 2 of Ref. [67]. To estimate the impact of the jet charge asymmetry on constraining the hVVhVV couplings, we consider hWW(22ν)andZZ(4)h\to WW^{*}(\to 2\ell 2\nu_{\ell}){\,\rm and\,}ZZ^{*}(\to 4\ell), with =e,μ,τ\ell=e,\mu,\tau, as our benchmark decay processes in this work. The dominant background with these decay products is the GGF process [68]. But we emphasize that the correlations between κW\kappa_{W} and κZ\kappa_{Z} measured from jet charges would not be sensitive to the Higgs decay information, which has been canceled in the definition of fractions. It can only change the statistical uncertainties in each p¯T\overline{p}_{T} bin through the event numbers. The result could potentially be improved if we combine more decay modes of the Higgs boson, which is however beyond the scope of this work. Performing the pseudo experiments, we conduct a combined χ2\chi^{2} analysis as

χ2=i[A¯Qi,totA¯Qi,tot,0δA¯Qi,tot]2,\chi^{2}=\sum_{i}\left[\frac{\overline{A}_{Q}^{i,\rm tot}-\overline{A}_{Q}^{i,\rm tot,0}}{\delta\overline{A}_{Q}^{i,\rm tot}}\right]^{2}, (7)

where A¯Qi,tot,0\overline{A}_{Q}^{i,\rm tot,0} and δA¯Qi,tot\delta\overline{A}_{Q}^{i,\rm tot} are the jet charge asymmetry in the SM (i.e., κW=κZ=1\kappa_{W}=\kappa_{Z}=1) and the statistical uncertainty of the ii-th bin, respectively. For simplicity, we have assumed that the experimental values of jet charges agree with the SM predictions. Note that we have rescaled the statistical uncertainties to include the branching ratio BR(h22ν/4){\rm BR}(h\to 2\ell 2\nu_{\ell}/4\ell) in each bin in our χ2\chi^{2} analysis. The kinematic cuts for the decay products of Higgs boson can also change the total event numbers. However, such effects should not significantly change the conclusions of this paper and will be ignored in the following analysis. It shows that the typical error of A¯Qtot\overline{A}_{Q}^{\rm tot} is around 𝒪(1%)\mathcal{O}(1\%), which strongly depends on the average jet p¯T\overline{p}_{T}.

Refer to caption
Figure 5: The expected constraints at the HL-LHC on κW,Z\kappa_{W,Z} from the jet charge asymmetry A¯Q\overline{A}_{Q} (red). The blue region is bounded by the RhR_{h} in gghgg\to h production. The gray and brown regions represent the constraints from the VBF Higgs signal strength measurements via the decay modes hZZh\to ZZ^{*} and hWWh\to WW^{*}, respectively, and they depend on the assumption of the Higgs boson width Γh\Gamma_{h}.

In Fig. 5, we show the expected limits on the hVVhVV couplings at the 68% confidence level (C.L.) for the integrated luminosity 3000fb13000~{}{\rm fb}^{-1}, obtained from the jet charge asymmetries (red band) at the 14 TeV LHC (HL-LHC). It is evident that κW\kappa_{W} and κZ\kappa_{Z} cannot be uniquely determined by the measurement of jet charge asymmetry alone. In order to further reduce the error band in the parameter space of κW\kappa_{W} and κZ\kappa_{Z}, without making any assumption on the total decay width (Γh\Gamma_{h}) of the Higgs boson, we consider the following ratio of the Higgs signal strength measurements,

Rhμ(gghWW)μ(gghZZ)=κW2κZ2,R_{h}\equiv\frac{\mu(gg\to h\to WW^{*})}{\mu(gg\to h\to ZZ^{*})}=\frac{\kappa_{W}^{2}}{\kappa_{Z}^{2}}\,, (8)

where the signal strength modifier μ(gghVV)\mu(gg\to h\to VV^{*}) is defined as the measured cross section relative to the SM expectation. Hence, any new physics contributions to gghgg\to h production cross section would cancel in RhR_{h}. Its constraint on κW\kappa_{W} and κZ\kappa_{Z} at the HL-LHC is shown as the blue band in Fig. 5, where the error of RhR_{h} is taken to be 5.7% [69]. It is evident that the combined analysis of the A¯Qtot\overline{A}_{Q}^{\rm tot} and RhR_{h} data can further constrain the allowed κW\kappa_{W} and κZ\kappa_{Z} values at the HL-LHC. We note that the correlation between κW\kappa_{W} and κZ\kappa_{Z}, extracted from A¯Qtot\overline{A}_{Q}^{\rm tot}, is dependent of the fraction (fW,Zf_{W,Z}) of production cross section contributed by various subprocesses, which is sensitive to the kinematic selection of the VBF events. Hence, it is possible to apply some advanced technologies, such as Boosted Decision Tree or Machine Learning, to further improve the constraints on κW\kappa_{W} and κZ\kappa_{Z}, which is however beyond the scope of this work.

For completeness, we also show in Fig. 5 the expected limits from the Higgs signal strength measurements of the VBF Higgs production with hWWh\to WW^{*} (denoted by μVBFWW\mu_{\rm VBF}^{WW} in the figure, brown region) and hZZh\to ZZ^{*} (denoted by μVBFZZ\mu_{\rm VBF}^{ZZ} in the figure, gray region) at the HL-LHC [69]. Here, the error of the signal strength of the VBF production with hWWh\to WW^{*} and hZZh\to ZZ^{*} is taken to be 5.5% and 9.5%, respectively [69]. We note that while the constraints imposed by the A¯Qtot\overline{A}_{Q}^{\rm tot} and RhR_{h} data are independent of Γh\Gamma_{h}, those imposed by μVBFWW\mu_{\rm VBF}^{WW} and μVBFZZ\mu_{\rm VBF}^{ZZ} are dependent of the assumption made in the calculation of Γh\Gamma_{h}. Here, we assumed that Γh\Gamma_{h} is only modified by the values of κW\kappa_{W} and κZ\kappa_{Z}.

Conclusions: In this Letter, we propose a novel and feasible method to separate the WW-fusion from the ZZ-fusion and the gluon-fusion (GGF) processes by utilizing the jet charge asymmetry A¯Q\overline{A}_{Q} of the two leading jets in Higgs+2 jets production at the HL-LHC. This is crucial for separately measuring the couplings of Higgs boson to W+WW^{+}W^{-} and ZZZZ gauge bosons, without the need of making any assumption about the decay width of Higgs boson. Owing to the partonic nature of the hard scattering, we demonstrate that the asymmetry A¯Q>1\overline{A}_{Q}>1 for WW-fusion, while it is always close to one for the ZZ-fusion and the GGF processes. Such a different feature can be used to discriminate the Higgs production mechanisms and to determine the Higgs couplings to the gauge bosons κV\kappa_{V}. While the usual methods of determining κV\kappa_{V} from the Higgs signal strength measurement depends on the assumption of Γh\Gamma_{h}, the proposed measurement of A¯Qtot\overline{A}_{Q}^{\rm tot} does not rely on such an assumption.

Acknowledgments. HTL is supported by the National Science Foundation of China under grant No. 12275156. BY is supported by the IHEP under Contract No. E25153U1. CPY is supported by the U.S. National Science Foundation under Grant No. PHY-2013791 and is grateful for the support from the Wu-Ki Tung endowed chair in particle physics.

References

  • Englert et al. [2014] C. Englert, A. Freitas, M. M. Mühlleitner, T. Plehn, M. Rauch, M. Spira, and K. Walz, J. Phys. G 41, 113001 (2014), eprint 1403.7191.
  • Cheung et al. [2014] K. Cheung, J. S. Lee, and P.-Y. Tseng, Phys. Rev. D 90, 095009 (2014), eprint 1407.8236.
  • Bergstrom and Riad [2015] J. Bergstrom and S. Riad, Phys. Rev. D 91, 075008 (2015), eprint 1411.4876.
  • Falkowski [2016] A. Falkowski, Pramana 87, 39 (2016), eprint 1505.00046.
  • Craig et al. [2016] N. Craig, J. Gu, Z. Liu, and K. Wang, JHEP 03, 050 (2016), eprint 1512.06877.
  • Corbett et al. [2015] T. Corbett, O. J. P. Eboli, D. Goncalves, J. Gonzalez-Fraile, T. Plehn, and M. Rauch, JHEP 08, 156 (2015), eprint 1505.05516.
  • Durieux et al. [2017] G. Durieux, C. Grojean, J. Gu, and K. Wang, JHEP 09, 014 (2017), eprint 1704.02333.
  • De Blas et al. [2019] J. De Blas, G. Durieux, C. Grojean, J. Gu, and A. Paul, JHEP 12, 117 (2019), eprint 1907.04311.
  • Cao et al. [2019] Q.-H. Cao, L.-X. Xu, B. Yan, and S.-H. Zhu, Phys. Lett. B 789, 233 (2019), eprint 1810.07661.
  • Chiang et al. [2018] C.-W. Chiang, X.-G. He, and G. Li, JHEP 08, 126 (2018), eprint 1805.01689.
  • Ellis et al. [2021] J. Ellis, M. Madigan, K. Mimasu, V. Sanz, and T. You, JHEP 04, 279 (2021), eprint 2012.02779.
  • Araz et al. [2021] J. Y. Araz, S. Banerjee, R. S. Gupta, and M. Spannowsky, JHEP 04, 125 (2021), eprint 2011.03555.
  • Yan [2021] B. Yan, Phys. Lett. B 822, 136709 (2021), eprint 2105.04530.
  • Xie and Yan [2021] K.-P. Xie and B. Yan, Phys. Lett. B 820, 136515 (2021), eprint 2104.12689.
  • Bizoń et al. [2022] W. Bizoń, F. Caola, K. Melnikov, and R. Röntsch, Phys. Rev. D 105, 014023 (2022), eprint 2106.06328.
  • Banerjee et al. [2022] S. Banerjee, R. S. Gupta, O. Ochoa-Valeriano, and M. Spannowsky, JHEP 02, 176 (2022), eprint 2109.14634.
  • Sharma and Shivaji [2022] P. Sharma and A. Shivaji (2022), eprint 2207.03862.
  • Asteriadis et al. [2022] K. Asteriadis, F. Caola, K. Melnikov, and R. Röntsch (2022), eprint 2206.14630.
  • ATL [2022a] Nature 607, 52 (2022a), eprint 2207.00092.
  • CMS [2022] Nature 607, 60 (2022), eprint 2207.00043.
  • Caola and Melnikov [2013] F. Caola and K. Melnikov, Phys. Rev. D 88, 054024 (2013), eprint 1307.4935.
  • Campbell et al. [2014] J. M. Campbell, R. K. Ellis, and C. Williams, Phys. Rev. D 89, 053011 (2014), eprint 1312.1628.
  • Gainer et al. [2015] J. S. Gainer, J. Lykken, K. T. Matchev, S. Mrenna, and M. Park, Phys. Rev. D 91, 035011 (2015), eprint 1403.4951.
  • Li et al. [2015] C. S. Li, H. T. Li, D. Y. Shao, and J. Wang, JHEP 08, 065 (2015), eprint 1504.02388.
  • Sirunyan et al. [2019] A. M. Sirunyan et al. (CMS), Phys. Rev. D 99, 112003 (2019), eprint 1901.00174.
  • Tumasyan et al. [2022] A. Tumasyan et al. (CMS) (2022), eprint 2202.06923.
  • Englert and Spannowsky [2014] C. Englert and M. Spannowsky, Phys. Rev. D 90, 053003 (2014), eprint 1405.0285.
  • Cacciapaglia et al. [2014] G. Cacciapaglia, A. Deandrea, G. Drieu La Rochelle, and J.-B. Flament, Phys. Rev. Lett. 113, 201802 (2014), eprint 1406.1757.
  • Englert et al. [2015] C. Englert, Y. Soreq, and M. Spannowsky, JHEP 05, 145 (2015), eprint 1410.5440.
  • Lee et al. [2019] S. J. Lee, M. Park, and Z. Qian, Phys. Rev. D 100, 011702 (2019), eprint 1812.02679.
  • Cao et al. [2020] Q.-H. Cao, B. Yan, C. P. Yuan, and Y. Zhang, Phys. Rev. D 102, 055010 (2020), eprint 2004.02031.
  • Azatov et al. [2022] A. Azatov et al. (2022), eprint 2203.02418.
  • Barger et al. [1991a] V. D. Barger, K.-m. Cheung, T. Han, J. Ohnemus, and D. Zeppenfeld, Phys. Rev. D 44, 1426 (1991a).
  • Barger et al. [1991b] V. D. Barger, K.-m. Cheung, T. Han, and D. Zeppenfeld, Phys. Rev. D 44, 2701 (1991b), [Erratum: Phys.Rev.D 48, 5444 (1993)].
  • Kauer et al. [2001] N. Kauer, T. Plehn, D. L. Rainwater, and D. Zeppenfeld, Phys. Lett. B 503, 113 (2001), eprint hep-ph/0012351.
  • Rentala et al. [2013] V. Rentala, N. Vignaroli, H.-n. Li, Z. Li, and C. P. Yuan, Phys. Rev. D 88, 073007 (2013), eprint 1306.0899.
  • Sun et al. [2016] P. Sun, C. P. Yuan, and F. Yuan, Phys. Lett. B 762, 47 (2016), eprint 1605.00063.
  • Chan et al. [2017] C.-H. Chan, K. Cheung, Y.-L. Chung, and P.-H. Hsu, Phys. Rev. D 96, 096009 (2017), eprint 1706.02864.
  • Liu et al. [2019] T. Liu, K. Melnikov, and A. A. Penin, Phys. Rev. Lett. 123, 122002 (2019), eprint 1906.10899.
  • Sun et al. [2019] P. Sun, C. P. Yuan, and F. Yuan, Phys. Lett. B 797, 134852 (2019), eprint 1802.02980.
  • Chiang et al. [2022] C.-W. Chiang, D. Shih, and S.-F. Wei (2022), eprint 2209.05518.
  • Field and Feynman [1978] R. D. Field and R. P. Feynman, Nucl. Phys. B 136, 1 (1978).
  • Krohn et al. [2013] D. Krohn, M. D. Schwartz, T. Lin, and W. J. Waalewijn, Phys. Rev. Lett. 110, 212001 (2013), eprint 1209.2421.
  • Waalewijn [2012] W. J. Waalewijn, Phys. Rev. D 86, 094030 (2012), eprint 1209.3019.
  • Fraser and Schwartz [2018] K. Fraser and M. D. Schwartz, JHEP 10, 093 (2018), eprint 1803.08066.
  • Larkoski and Metodiev [2019] A. J. Larkoski and E. M. Metodiev, JHEP 10, 014 (2019), eprint 1906.01639.
  • Gianelle et al. [2022] A. Gianelle, P. Koppenburg, D. Lucchesi, D. Nicotra, E. Rodrigues, L. Sestini, J. de Vries, and D. Zuliani, JHEP 08, 014 (2022), eprint 2202.13943.
  • Chen et al. [2020a] Y.-C. J. Chen, C.-W. Chiang, G. Cottin, and D. Shih, Phys. Rev. D 101, 053001 (2020a), eprint 1908.08256.
  • Li et al. [2021] H. T. Li, B. Yan, and C. P. Yuan (2021), eprint 2112.07747.
  • Wong and Yan [2023] X. Wong and B. Yan (2023), eprint 2302.02084.
  • Chen et al. [2020b] S.-Y. Chen, B.-W. Zhang, and E.-K. Wang, Chin. Phys. C 44, 024103 (2020b), eprint 1908.01518.
  • Li and Vitev [2020] H. T. Li and I. Vitev, Phys. Rev. D 101, 076020 (2020), eprint 1908.06979.
  • Li and Vitev [2021] H. T. Li and I. Vitev, Phys. Rev. Lett. 126, 252001 (2021), eprint 2010.05912.
  • Kang et al. [2020] Z.-B. Kang, X. Liu, S. Mantry, and D. Y. Shao, Phys. Rev. Lett. 125, 242003 (2020), eprint 2008.00655.
  • Kang et al. [2021] Z.-B. Kang, X. Liu, S. Mantry, M. C. Spraker, and T. Wilson, Phys. Rev. D 103, 074028 (2021), eprint 2101.04304.
  • Lee et al. [2022] K. Lee, J. Mulligan, M. Płoskoń, F. Ringer, and F. Yuan (2022), eprint 2210.06450.
  • Khachatryan et al. [2014] V. Khachatryan et al. (CMS), JHEP 12, 017 (2014), eprint 1410.4227.
  • Aad et al. [2016] G. Aad et al. (ATLAS), Phys. Rev. D 93, 052003 (2016), eprint 1509.05190.
  • Sirunyan et al. [2017] A. M. Sirunyan et al. (CMS), JHEP 10, 131 (2017), eprint 1706.05868.
  • Sirunyan et al. [2020] A. M. Sirunyan et al. (CMS), JHEP 07, 115 (2020), eprint 2004.00602.
  • Alwall et al. [2014] J. Alwall, R. Frederix, S. Frixione, V. Hirschi, F. Maltoni, O. Mattelaer, H. S. Shao, T. Stelzer, P. Torrielli, and M. Zaro, JHEP 07, 079 (2014), eprint 1405.0301.
  • Dulat et al. [2016] S. Dulat, T.-J. Hou, J. Gao, M. Guzzi, J. Huston, P. Nadolsky, J. Pumplin, C. Schmidt, D. Stump, and C. P. Yuan, Phys. Rev. D 93, 033006 (2016), eprint 1506.07443.
  • Cacciari et al. [2008] M. Cacciari, G. P. Salam, and G. Soyez, JHEP 04, 063 (2008), eprint 0802.1189.
  • Sjöstrand et al. [2015] T. Sjöstrand, S. Ask, J. R. Christiansen, R. Corke, N. Desai, P. Ilten, S. Mrenna, S. Prestel, C. O. Rasmussen, and P. Z. Skands, Comput. Phys. Commun. 191, 159 (2015), eprint 1410.3012.
  • Bierlich et al. [2022] C. Bierlich et al. (2022), eprint 2203.11601.
  • Aaron et al. [2009] F. D. Aaron et al. (H1), Phys. Lett. B 681, 125 (2009), eprint 0907.2666.
  • ATL [2022b] (2022b), eprint 2208.02338.
  • ATL [2016] Tech. Rep., CERN, Geneva (2016), URL https://cds.cern.ch/record/2145377.
  • Cepeda et al. [2019] M. Cepeda et al., CERN Yellow Rep. Monogr. 7, 221 (2019), eprint 1902.00134.