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Detecting Heavy Higgs Bosons from Natural SUSY
at a 100 TeV Hadron Collider

Howard Baer [email protected] Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA    Vernon Barger [email protected] Department of Physics, University of Wisconsin, Madison, WI 53706, USA    Rishabh Jain [email protected] Department of Physics, National Taiwan University, Taipei, Taiwan 10617, R.O.C    Chung Kao [email protected] Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA    Dibyashree Sengupta [email protected] Department of Physics, National Taiwan University, Taipei, Taiwan 10617, R.O.C    Xerxes Tata [email protected] Department of Physics, University of Hawaii, Honolulu, HI 96822, USA
Abstract

Supersymmetric models with radiatively-driven naturalness (RNS) enjoy low electroweak fine-tuning whilst respecting LHC search limits on gluinos and top squarks and allowing for mh125m_{h}\simeq 125 GeV. While the heavier Higgs bosons H,AH,\ A may have TeV-scale masses, the SUSY conserving μ\mu parameter must lie in the few hundred GeV range. Thus, in natural SUSY models there should occur large heavy Higgs boson branching fractions to electroweakinos, with Higgs boson decays to higgsino plus gaugino dominating when they are kinematically accessible. These SUSY decays can open up new avenues for discovery. We investigate the prospects of discovering heavy neutral Higgs bosons HH and AA decaying into light plus heavy chargino pairs which can yield a four isolated lepton plus missing transverse energy signature at the LHC and at a future 100 TeV pppp collider. We find that discovery of heavy Higgs decay to electroweakinos via its 44\ell decay mode is very difficult at HL-LHC. For FCC-hh or SPPC, we study the H,AH,\ A\rightarrow SUSY reaction along with dominant physics backgrounds from the Standard Model and devise suitable selection requirements to extract a clean signal for FCC-hh or SPPC with s=100\sqrt{s}=100 TeV, assuming an integrated luminosity of 15 ab1ab^{-1}. We find that while a conventional cut-and-count analysis yields a signal statistical significance greater than 5σ5\sigma for mA,H1.11.65m_{A,H}\sim 1.1-1.65 TeV, a boosted-decision-tree analysis allows for heavy Higgs signal discovery at FCC-hh or SPPC for mA,H12m_{A,H}\sim 1-2 TeV.

preprint:                                                                                    OU-HEP-211202 December 2021

I Introduction

With the discovery of the 125 GeV Standard Model-like Higgs boson at LHC higgs , all the particle states required by the Standard Model (SM) have been confirmed. And yet, many mysteries of nature still remain unsolved. Supersymmetric extensions of the SM are highly motivated in that they offer a solution to the gauge hierarchy problem (GHP) ghp which arises from the quadratic sensitivity of the Higgs boson mass to high scale physics. SUSY models are also supported indirectly by various precision measurements within the SM: 1. the weak scale gauge couplings nearly unify under renormalization group evolution at energy scale mGUT2×1016m_{GUT}\simeq 2\times 10^{16} GeV in the MSSM, but not the SM gcu , 2. the measured value of top quark mass falls within the range needed to initiate a radiative breakdown of electroweak symmetry in the MSSM top , 3. the measured value of the Higgs boson mass mh125m_{h}\simeq 125 GeV falls within the narrow range of MSSM predicted values mhiggs , and 4. precision electroweak measurements actually favor heavy SUSY over the SM sven .

Recent LHC searches with s=\sqrt{s}= 13 TeV and integrated luminosity L=139fb1L=139\;{\rm fb}^{-1} have put lower bounds on the mass of the gluino of about 2.2 TeV atlasg ; cmsg and on the mass of top squark of about 1.1 TeV atlast ; cmst . These limits, which have been obtained using simplified model analyses assuming that the sparticle spectrum is not compressed, fall well above upper bounds derived from early naturalness considerations bg ; dg ; ac ; unn1 ; unn . However, the naturalness estimates from the log-derivative measure are highly dependent on what one regards as independent parameters of the theory dew .111The various soft SUSY breaking terms which are adopted for the log-derivative measure are introduced to parameterize one’s ignorance of how soft terms arise. In more UV-complete models such as string theory, then the various soft terms are all calculable and not independent. Ignoring this could result in an over-estimate of the UV sensitivity of the theory by orders of magnitude. We adopt the more conservative quantity ΔEW\Delta_{EW}, that allows for the possibility of correlations among model parameters, as a measure of naturalness rns . ΔEW\Delta_{EW} can be extracted from Eq. (1),

mZ22=mHd2+Σdd(mHu2+Σuu)tan2βtan2β1μ2,\frac{m_{Z}^{2}}{2}=\frac{m_{H_{d}}^{2}+\Sigma_{d}^{d}-(m_{H_{u}}^{2}+\Sigma_{u}^{u})\tan^{2}\beta}{\tan^{2}\beta-1}-\mu^{2}\;, (1)

which relates the mass of Standard Model ZZ boson to SUSY Lagrangian parameters at the weak scale and is obtained from the minimization conditions of the MSSM scalar potential baerbook . The electroweak fine-tuning parameter ΔEW\Delta_{EW} is defined by,

ΔEW(max|termonRHSofEq.1|)/(mZ2/2).\Delta_{EW}\equiv\mathrm{(}\rm{max|term\ on\ RHS\ of\ Eq.~{}\ref{eq:mzs}}|)/(m_{Z}^{2}/2). (2)

The condition for naturalness is that the maximal contribution to the ZZ mass should be within a factor of several of its measured value. We consider spectra that yield ΔEW>ΔEW(max)=30\Delta_{EW}>\Delta_{EW}(\rm max)=30 as fine-tuned upper .

This condition then requires :

  • the SUSY-conserving μ\mu parameter \approx 110-350 GeV;

  • the up-Higgs soft mass term mHu2m_{H_{u}}^{2} may be large at high scales but can be radiatively-driven to (negative) natural values mweak2\sim-m_{weak}^{2} at the weak scale;

  • The finite radiative correction Σuu(t~1,2)\Sigma_{u}^{u}(\tilde{t}_{1,2}) has an upper bound of (350(350 GeV)2 which is possible even for mt~m_{\tilde{t}} up to 3 TeV and mg~m_{\tilde{g}} \approx 6 TeV bounds , compatible with LHC constraints;

  • the heavy Higgs masses mA,H,H±|mHd|m_{A,H,H^{\pm}}\sim|m_{H_{d}}|, with |mHd|/tanβmZ2ΔEW|m_{H_{d}}|/\tan\beta\sim{m_{Z}\over\sqrt{2}}\sqrt{\Delta_{EW}}.

We thus see that naturalness requires bbbms

mA<mZtanβΔEW(max)2,m_{A}~{}\mbox{\raisebox{-2.58334pt}{$\stackrel{{\scriptstyle<}}{{\sim}}$}}~{}\frac{m_{Z}\tan\beta\sqrt{\Delta_{EW}(\rm max)}}{\sqrt{2}}, (3)

and further, that for tanβ550\tan\beta\sim 5-50, the heavy Higgs boson masses may be expected to lie in the (multi)-TeV range for an electroweak fine-tuning of up to a part in thirty.

The conditions mentioned above are satisfied in radiatively-driven natural supersymmetric (RNS) models. One of the features of RNS models is that the heavier Higgs bosons may lie in the multi-TeV range while at least some of the electroweakinos (EWinos) are below a few hundred GeV. This means that generically we expect that in natural SUSY models the supersymmetric decay modes of the heavy Higgs bosons should be kinematically accessible, and often with branching fractions comparable to SM decay modes. If SUSY decay modes of the heavy Higgs bosons are allowed, then 1. SM search modes will be suppressed due to the presence of the SUSY decay modes and 2. potentially new avenues for heavy Higgs discovery may open up. This situation was investigated long ago under the supposition that the lightest EWinos were predominantly gaugino-like bbdkt . In Ref. bbkt , a lucrative A,Hχ~20χ~204+TA,H\rightarrow\tilde{\chi}_{2}^{0}\tilde{\chi}^{0}_{2}\rightarrow 4\ell+\not{E}_{T} search mode was identified for LHC. However, in RNS models, we expect instead that the lightest EWinos to be dominantly higgsino-like.

Thus, we explore here a new possible heavy Higgs discovery channel for SUSY models with light higgsinos. We identify the dominant new SUSY decay mode for heavy neutral Higgs in natural SUSY models as H,Aχ~1±χ~2H,\ A\rightarrow\tilde{\chi}_{1}^{\pm}\tilde{\chi}_{2}^{\mp} that proceeds with full gauge strength222By full gauge strength, we only mean that the Higgs scalar-higgsino-gaugino vertex is unsuppressed. We recognize, of course, that the overall coupling of the heavy Higgs sector to the gauge boson sector is suppressed by mixing angles in the scalar Higgs sector. (provided that the decay is kinematically allowed). Allowing for chargino cascade decays, then an analogous clean 4+T4\ell+\not{E}_{T} signature can be found. It includes leptons from the lighter chargino decay χ~1ν¯χ~10\tilde{\chi}_{1}^{-}\rightarrow\ell^{-}\bar{\nu}_{\ell}\tilde{\chi}_{1}^{0} where the final state leptons are expected to be quite soft in the chargino rest frame due to the expected small mass gap mχ~1mχ~10m_{\tilde{\chi}_{1}^{-}}-m_{\tilde{\chi}_{1}^{0}}. However, due to mH,Am_{H,A} lying in the TeV-range, these final state leptons may be strongly boosted and thus can potentially contribute to the signal. In this paper, we examine the particular reaction ppH,Aχ~1±χ~24+Tpp\rightarrow H,\ A\rightarrow\tilde{\chi}_{1}^{\pm}\tilde{\chi}_{2}^{\mp}\rightarrow 4\ell+\not{E}_{T} where due to the heavy Higgs resonance, we expect MT(4,T)M_{T}(4\ell,\not{E}_{T}) to be kinematically bounded by mH,Am_{H,A} (see Fig. 1). While this reaction will prove difficult to extract at HL-LHC – due in part to the several leptonic branching fractions which are required – we find that discovery in this channel should be possible at the FCC-hhBordry:2018gri or SPPCCEPC-SPPCStudyGroup:2015csa pppp collider with s100\sqrt{s}\sim 100 TeV and 15 ab-1 of integrated luminosity. The FCC-hh or SPPC collider has emerged as the next target hadron collider for CERN after HL-LHC in the updated European strategy report euro .

Refer to caption
Figure 1: Feynman diagram for ggH,A(χ~2±χ~14+T)+Xgg\rightarrow H,\ A(\rightarrow\tilde{\chi}_{2}^{\pm}\tilde{\chi}_{1}^{\mp}\rightarrow 4\ell+\not{E}_{T})+X production; there is a similar diagram for H,AH,\ A production via bb¯b\bar{b} fusion.

To be specific, we will adopt a RNS benchmark (BM) point as listed in Table 1, as generated using Isajet 7.88 isajet . This BM comes from the two-extra-parameter non-universal Higgs model NUHM2 nuhm2 . The NUHM2 model parameter space is given by m0,m1/2,A0,tanβm_{0},m_{1/2},A_{0},\tan\beta along with non-universal Higgs mass soft terms mHumHdm0m_{H_{u}}\neq m_{H_{d}}\neq m_{0}. Using the EW minimization conditions, it is convenient to trade the high scale soft terms mHu,mHdm_{H_{u}},\ m_{H_{d}} for the weak scale parameters μ\mu and mAm_{A}. This BM point yields mg~2.4m_{\tilde{g}}\simeq 2.4 TeV, somewhat beyond the LHC lower limit of 2.2 TeV obtained from a simplified model analysis. The heavy neutral Higgs scalars have mass mH,A1.2m_{H,A}\sim 1.2 TeV which is somewhat beyond the recent ATLAS limitATLAS-H that requires mH,A>1m_{H,A}~{}\mbox{\raisebox{-2.58334pt}{$\stackrel{{\scriptstyle>}}{{\sim}}$}}~{}1 TeV for tanβ=10\tan\beta=10 via an H,Aτ+τH,\ A\rightarrow\tau^{+}\tau^{-} search at s=13\sqrt{s}=13 TeV and 139 fb-1 of integrated luminosity (while assuming no SUSY decay modes of the heavy Higgs bosons). Also, the SUSY μ\mu parameter is taken to be μ=200\mu=200 GeV so that the BM point lies just beyond the recent analyses of the soft dilepton plus monojet higgsino signallhcsoftdilep . For the listed BM point, the lighter EWinos χ~1,20\tilde{\chi}_{1,2}^{0} and χ~1±\tilde{\chi}_{1}^{\pm} are higgsino-like while χ~30\tilde{\chi}_{3}^{0} is bino-like and χ~40\tilde{\chi}_{4}^{0} and χ~2±\tilde{\chi}_{2}^{\pm} are wino-like.

parameter NUHM2
m0m_{0} 5 TeV
m1/2m_{1/2} 1.0 TeV
A0A_{0} -8.3 TeV
tanβ\tan\beta 10
μ\mu 200 GeV
mAm_{A} 1.2 TeV
mg~m_{\tilde{g}} 2423 GeV
mu~Lm_{\tilde{u}_{L}} 5293 GeV
mu~Rm_{\tilde{u}_{R}} 5439 GeV
me~Rm_{\tilde{e}_{R}} 4804 GeV
mt~1m_{\tilde{t}_{1}} 1388 GeV
mt~2m_{\tilde{t}_{2}} 3722 GeV
mb~1m_{\tilde{b}_{1}} 3756 GeV
mb~2m_{\tilde{b}_{2}} 5150 GeV
mτ~1m_{\tilde{\tau}_{1}} 4727 GeV
mτ~2m_{\tilde{\tau}_{2}} 5097 GeV
mν~τm_{\tilde{\nu}_{\tau}} 5094 GeV
mχ~1±m_{\tilde{\chi}_{1}^{\pm}} 208.4 GeV
mχ~2±m_{\tilde{\chi}_{2}^{\pm}} 856.7 GeV
mχ~10m_{\tilde{\chi}_{1}^{0}} 195.4 GeV
mχ~20m_{\tilde{\chi}_{2}^{0}} 208.5 GeV
mχ~30m_{\tilde{\chi}_{3}^{0}} 451.7 GeV
mχ~40m_{\tilde{\chi}_{4}^{0}} 867.9 GeV
mhm_{h} 125.0 GeV
Ωz~1stdh2\Omega_{\tilde{z}_{1}}^{std}h^{2} 0.011
BF(bsγ)×104BF(b\rightarrow s\gamma)\times 10^{4} 3.23.2
BF(Bsμ+μ)×109BF(B_{s}\rightarrow\mu^{+}\mu^{-})\times 10^{9} 3.83.8
σSI(χ~10,p)\sigma^{SI}(\tilde{\chi}_{1}^{0},p) (pb) 3.1×1093.1\times 10^{-9}
σSD(χ~10,p)\sigma^{SD}(\tilde{\chi}_{1}^{0},p) (pb) 6.1×1056.1\times 10^{-5}
σv|v0\langle\sigma v\rangle|_{v\rightarrow 0} (cm3/sec) 2.0×10252.0\times 10^{-25}
ΔEW\Delta_{\rm EW} 25.5
Table 1: Input parameters (TeV) and masses (GeV) for a SUSY benchmark point from the NUHM2 model with mt=173.2m_{t}=173.2 GeV using Isajet 7.88 isajet .

I.1 Review of some previous related work and plan for this work

SUSY Higgs boson decays to EWinos were first calculated in Baer et al. Ref. bddt . A more comprehensive treatment was given in Gunion et al. ssc1 and Gunion and Haber gh3 . Griest and Haber ghaber considered the effect of invisible Higgs decays Hχ~10χ~10H\rightarrow\tilde{\chi}^{0}_{1}\tilde{\chi}^{0}_{1}. In Kunszt and Zwirner Ref. kz , the phenomenology of SUSY Higgs bosons in the mAm_{A} vs. tanβ\tan\beta plane with just SM decay modes was considered in light of the important radiative corrections to mhm_{h}. The mAm_{A} vs. tanβ\tan\beta plane was mapped including the effects of Higgs to SUSY decays in Baer et al. Ref. bbdkt where diminution of SM Higgs decay channels due to SUSY modes was considered along with the potential for new discovery channels arising from the SUSY decay modes. In Ref. bbkt , the discovery channel H,Aχ~20χ~204+TH,\ A\rightarrow\tilde{\chi}^{0}_{2}\tilde{\chi}^{0}_{2}\rightarrow 4\ell+\not{E}_{T} was examined. In Djouadi et al. djkz , SUSY decays of heavy Higgs bosons at e+ee^{+}e^{-} colliders were considered. Barger et al. in Ref. bbgh examined ss-channel production of SM and SUSY Higgs bosons at muon colliders. In Belanger et al. belanger , SUSY decays of Higgs bosons at LHC were examined. Choi et al.cdls examined the effects of CP violating phases on Higgs to SUSY decays. In Ref. css , a CMS study of H,Aχ~20χ~204+TH,\ A\rightarrow\tilde{\chi}^{0}_{2}\tilde{\chi}^{0}_{2}\rightarrow 4\ell+\not{E}_{T} was performed. In Ref. bisset , signals from H,A4+TH,\ A\rightarrow 4\ell+\not{E}_{T} were examined including all SUSY cascade decays of heavy Higgs bosons in scenarios where the χ~10\tilde{\chi}_{1}^{0} was bino-like. In Bae et al.bbbms , the impact of natural SUSY with light higgsinos on SUSY Higgs phenomenology was examined and natural regions of the mAm_{A} vs. tanβ\tan\beta plane were displayed along with relevant SUSY Higgs branching fractions. The LHC SUSY Higgs signatures H,AmonoX+TH,A\rightarrow mono-X+\not{E}_{T} (where X=W,Z,hX=W,\ Z,\ h) were examined against huge SM backgrounds. In Bae et al. Ref. bbns , the effect of natural SUSY on Higgs coupling measurements κi\kappa_{i} was examined. In Barman et al. bbcc , SUSY Higgs branching fractions and monoX+Tmono-X+\not{E}_{T} signatures were examined at LHC for several benchmark points along with a Higgs to SUSY trilepton signature. In Ref. bagnaschi , six MSSM SUSY Higgs benchmark points were proposed for LHC search studies, including one with a low, natural value of μ\mu (which seems now to be LHC-excluded). Gori, Liu and Shakya examined SUSY Higgs decays to EWinos and to stau pairs in Ref. gls . In Adhikary et al. abgkk , Higgs decay to EWinos at LHC were examined, especially the Z+TZ+\not{E}_{T} and h+Th+\not{E}_{T} signatures along with the possibility of Higgs decays to long-lived charged particles (LLCPs).

I.2 Plan for this paper

In the present paper, we examine Higgs decays to SUSY particles in natural SUSY models with light higgsinos. In particular, in light of the large SM backgrounds for monoX+Tmono-X+\not{E}_{T} searches, we examine the viability of resurrecting the H,A4+TH,\ A\rightarrow 4\ell+\not{E}_{T} signature. In the natural SUSY case, this signature could arise from H,Aχ~1±χ~2H,\ A\rightarrow\tilde{\chi}_{1}^{\pm}\tilde{\chi}_{2}^{\mp} followed by χ~2±Zχ~1±\tilde{\chi}_{2}^{\pm}\rightarrow Z\tilde{\chi}_{1}^{\pm}. The Z+Z\rightarrow\ell^{+}\ell^{-} decay should be easily visible but the leptons from χ~1νχ~10\tilde{\chi}_{1}^{-}\rightarrow\ell\nu_{\ell}\tilde{\chi}_{1}^{0} are typically very soft in the χ~1±\tilde{\chi}_{1}^{\pm} rest frame. Owing to the TeV scale values of mH,Am_{H,A}, these otherwise soft leptons may be boosted to detectable levels. While such a complicated decay channel appears intractable at HL-LHC, the FCC-hh or SPPC operating at s100\sqrt{s}\sim 100 TeV and 15 ab-1 should allow for discovery for mH,A12m_{H,A}\sim 1-2 TeV with advanced machine learning (ML) techniques; here we have used boosted decision trees as an illustration.333Since one of our goals is to illustrate how ML techniques may help to eke out a signal that lies below the discovery limit using standard cut-and-count analyses if the Higgs boson is very massive, we have confined our study to the signal in this single channel, and for simplicity carried out our calculations using parton level simulations.

The remainder of this paper is organized as follows. In Sec. II, we present ss-channel production rates for heavy Higgs bosons at LHC14 and at FCC-hh or SPPC. In Sec. III, we discuss the heavy Higgs branching fractions that are expected in natural SUSY models and we motivate our particular four lepton SUSY Higgs discovery channel. In Sec. IV, we discuss leading SM backgrounds to the H,A4+TH,\ A\rightarrow 4\ell+\not{E}_{T} signal channel. In Sec. V, we perform a cut-based analysis while in Sec. VI we show one can do much better by invoking a boosted-decision-tree (BDT) analysis. In Sec. VII, we summarize our main conclusions.

II Heavy Higgs production at LHC and FCC-hh or SPPC

Here, we will focus on the ss-channel heavy neutral Higgs boson production reactions ppH,App\rightarrow H,\ A which occurs via the gluon-gluon and bb¯b\bar{b} fusion subprocesses. Other reactions such as ppqqHpp\rightarrow qqH (VV fusion reactions) WHWH, ZHZH and tt¯Ht\bar{t}H all occur at lower rates higgspro and also lead to different final state topologies. Hence, we will not include these in our analysis.

In Fig. 2, we show the heavy neutral Higgs production cross sections at next-to-next-to-leading order (NNLO) in QCD. We adopt the SusHi program Harlander:2012pb ; Harlander:2016hcx ; Harlander:2002wh ; Harlander:2003ai ; Aglietti:2004nj ; Bonciani:2010ms ; Degrassi:2010eu ; Degrassi:2011vq ; Degrassi:2012vt ; Harlander:2005rq ; Chetyrkin:2000yt to generate these results, which include QCD corrections and effects from top and bottom squark loops. Higher order QCD corrections typically boost these cross sections above their leading order estimates. Frame (a) shows results for s=14\sqrt{s}=14 TeV while frame (b) shows results for s=100\sqrt{s}=100 TeV. We see that even for tanβ=10\tan\beta=10, heavy Higgs boson production via bb¯b\bar{b} fusion dominates that from gluon fusion. From frame (a), we see that for mA800m_{A}\sim 800 GeV, the total production cross sections occur for both HH and AA production at the 40\sim 40 fb level. As mAm_{A} increases, the rates fall and are already below the 0.2 fb level for mA>2m_{A}~{}\mbox{\raisebox{-2.58334pt}{$\stackrel{{\scriptstyle>}}{{\sim}}$}}~{}2 TeV. We can anticipate that once we fold in various leptonic branching fractions and include detector acceptances, we will not expect very high rates for multi-lepton signals from heavy neutral SUSY Higgs bosons at LHC14. In frame (b), we show the results for s=100\sqrt{s}=100 TeV. Here, the cross sections are increased by factors of 70-500 as mAm_{A} varies from 800-2000 GeV.

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Figure 2: σNNLO(ppH,A+X)\sigma_{NNLO}(pp\rightarrow H,\ A+X) for ss-channel heavy neutral Higgs boson production reactions via gggg and bb¯b\bar{b} fusion versus mAm_{A} for (a) s=\sqrt{s}= 14 and (b) s=\sqrt{s}= 100 TeV. We take tanβ=10\tan\beta=10. Results are from SusHi Harlander:2012pb ; Harlander:2016hcx .

III Heavy Higgs and sparticle branching fractions

In this Section, we present some updated heavy neutral and charged Higgs branching fractions which we extract from the Isajet 7.88 code isajet . We adopt the benchmark point from Table 1 except now we allow the heavy Higgs mass mAm_{A} to vary. In frame (a), we show branching fractions for the heavy neutral scalar HH. At low mHm_{H}, the SM modes Hbb¯H\rightarrow b\bar{b}, ττ¯\tau\bar{\tau} and tt¯t\bar{t} are dominant, with their exact values depending on tanβ\tan\beta (large tanβ\tan\beta enhances the bb¯b\bar{b} and ττ¯\tau\bar{\tau} modes). For mH400650m_{H}\sim 400-650 GeV, the SM modes are still dominant even though the light electroweakino modes are open. We can understand this by examining the Higgs sector Lagrangian in the notation of Ref. baerbook , Sec. 8.4:

2i,A𝒮igtAλ¯A1γ52ψi+h.c.{\cal L}\ni-\sqrt{2}\sum_{i,A}{\cal S}_{i}^{\dagger}gt_{A}\bar{\lambda}_{A}\frac{1-\gamma_{5}}{2}\psi_{i}+h.c. (4)

where 𝒮i{\cal S}_{i} labels various matter and Higgs scalars (labeled by ii), ψi\psi_{i} is the fermionic superpartner of 𝒮i{\cal S}_{i}, and λA\lambda_{A} is the gaugino with gauge index AA. Also, gg is the gauge coupling for the gauge group and tAt_{A} are the corresponding gauge group generator matrices. Letting 𝒮i{\cal S}_{i} be the Higgs scalar fields, then we see that the Higgs-EWino coupling is maximal when there is little mixing in that the Higgs fields couple directly to gaugino plus higgsino. Back in Fig. 3(a), for mHm_{H} small, then the only open decay modes are HH to higgsino plus higgsino, and so the coupling must be dynamically suppressed because the gaugino component of the lightest EWinos is very small. Thus the SM modes are still dominant. As mHm_{H} increases, then the decay to gaugino plus higgsino turns on and the above coupling is unsuppressed (as has also been noted in footnote 2, above). For our choice of SUSY parameters, this happens around mH650m_{H}\sim 650 GeV for HH decay to higgsino plus bino and around mH1050m_{H}\sim 1050 GeV for HH decay to wino plus higgsino. Since the latter coupling involves the larger SU(2)LSU(2)_{L} gauge coupling, the decay HH\rightarrow wino plus higgsino ultimately dominates the branching fraction once it is kinematically allowed. Thus, for mH>1250m_{H}~{}\mbox{\raisebox{-2.58334pt}{$\stackrel{{\scriptstyle>}}{{\sim}}$}}~{}1250 GeV, Hχ~1±χ~2H\rightarrow\tilde{\chi}_{1}^{\pm}\tilde{\chi}_{2}^{\mp} dominates the branching fraction (blue curve), while decays of HH to the lighter neutral higgsino-like neutralino plus the heavier neutral wino or bino-like neutralino (green curve) have a branching fraction about half as large. In this range of mHm_{H}, the SM HH decay modes are severely depressed from their two-Higgs doublet (non-SUSY) expectation. This will make heavy Higgs detection via tt¯t\bar{t}, bb¯b\bar{b} and ττ¯\tau\bar{\tau} much more difficult. On the other hand, it opens up new discovery channels by searching for the dominant HH\rightarrow EWino modes.

Refer to caption
Refer to caption
Refer to caption
Figure 3: Branching fractions versus heavy Higgs mass for a) HH, b) AA and c) H+H^{+} into SM and SUSY particles in the NUHM2 model with μ=200\mu=200 GeV and m0=5m_{0}=5 TeV, m1/2=1m_{1/2}=1 TeV, A0=8.3A_{0}=-8.3 TeV and tanβ=10\tan\beta=10.

In Fig. 3(b), we show the same branching fractions except now for the pseudoscalar AA. The branching fractions look qualitatively similar to those in frame (a) since the same reasoning applies. Thus, the AA will decay mainly to SM modes for smaller values of mAm_{A} even though decays to higgsino-like pairs are available. It is only when decays to gaugino plus higgsino open up that the branching fractions to SUSY modes begin to dominate.

For completeness, we also show in Fig. 3(c) the branching fractions for charged Higgs decays H+H^{+}. As in the previous cases, H+H^{+} decay to SM modes tb¯t\bar{b} and τ+ντ\tau^{+}\nu_{\tau} dominate at low values of mH+m_{H^{+}} even though decay to χ~1+χ~1,20\tilde{\chi}_{1}^{+}\tilde{\chi}^{0}_{1,2} modes are kinematically allowed. As mH+m_{H^{+}} increases, then decays to χ~1+χ~30\tilde{\chi}_{1}^{+}\tilde{\chi}^{0}_{3} (higgsino-bino) followed by χ~2+χ~1,20\tilde{\chi}_{2}^{+}\tilde{\chi}^{0}_{1,2} and χ~40χ~1+\tilde{\chi}^{0}_{4}\tilde{\chi}_{1}^{+} (higgsino-wino) turn on and rapidly dominate the decays.

Some dominant heavy neutral Higgs decay branching fractions are shown in Table 2 for the benchmark point shown in Table 1. We see again that for the benchmark point the H,AH,\ A decays to SM modes are suppressed compared to decay rates into gaugino plus higgsino.

decay mode BF
Hbb¯H\rightarrow b\bar{b} 22.5%
Hχ~1±χ~2H\rightarrow\tilde{\chi}_{1}^{\pm}\tilde{\chi}_{2}^{\mp} 31.2%
Hχ~20χ~40H\rightarrow\tilde{\chi}_{2}^{0}\tilde{\chi}_{4}^{0} 12.2%
Abb¯A\rightarrow b\bar{b} 22.9%
Aχ~1±χ~2A\rightarrow\tilde{\chi}_{1}^{\pm}\tilde{\chi}_{2}^{\mp} 30.0%
Aχ~10χ~40A\rightarrow\tilde{\chi}_{1}^{0}\tilde{\chi}_{4}^{0} 12.2%
Table 2: Dominant branching fractions for heavy Higgs H,AH,\ A for the benchmark point with mA=1200m_{A}=1200 GeV.

In Fig. 4, we combine the H,AH,\ A production rates from Fig. 2 with the Higgs boson and sparticle branching fractions to the 4+T4\ell+\not{E}_{T} final state depicted in Fig. 1. We see from Fig. 4(a) that, for tanβ=10\tan\beta=10, even without cuts we expect at most 7\sim 7 signal events at HL-LHC, assuming an integrated luminosity of 3000 fb-1. Moreover, we expect that this will be reduced considerably once detector efficiency and analysis cuts are folded in. However, as we can see from frame (b), the raw signal cross section is larger at the higher energy FCC-hh or SPPC by a factor 150-500 (compared to LHC14), so that with the projected 15 ab-1 of integrated luminosity, we may hope to be able to extract an observable signal even after cuts. We will, therefore, mostly focus our attention on a 100 TeV pppp collider in the remainder of this paper.

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Figure 4: NNLO Cross sections from SusHi σ(A)\sigma(A), σ(H)\sigma(H), and σ(A)+σ(H)\sigma(A)+\sigma(H) times the cascade decay branching fractions into the 4+T4\ell+\not{E}_{T} final state in fb vs. mAm_{A} for (a) 14 TeV and (b) 100 TeV without any cuts.

The reader may be concerned that our dismissal of the possibility of a signal in the 4+T4\ell+\not{E}_{T} channel at LHC14 was based on the event rate for tanβ=10\tan\beta=10 when it is well-known that the couplings of the AA and HH both increase with tanβ\tan\beta, resulting in an increased rate for H/AH/A production from bottom quark fusion. It should, however, be remembered that the range of mAm_{A} excluded by the current upper limit on the cross section times branching ratio for the decay ϕττ¯\phi\rightarrow\tau\bar{\tau} (ϕ=A,H\phi=A,H) also increases with tanβ\tan\beta for this same reason. This is illustrated in Fig. 5 where we show the expectations for the resonant production of tau pairs from the decay of H/Aττ¯H/A\rightarrow\tau\bar{\tau} versus mAm_{A} for several values of tanβtan\beta. Other parameters are taken to be the same as for the model-line introduced earlier. The horizontal black line is the current ATLAS upper bound on this rate ATLAS-H . We see that while mA>1.1m_{A}>1.1 TeV for tanβ=10\tan\beta=10, for tanβ=50\tan\beta=50, mA>2m_{A}>2 TeV. Scaling the cross section in the left frame of Fig. 4 by the ratio of the corresponding values of tan2β\tan^{2}\beta still leaves us with just a handful of events before cuts at the HL-LHC for currently allowed values of mAm_{A}.

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Figure 5: The summed cross section times branching ratio for A/Hττ¯A/H\rightarrow\tau\bar{\tau} versus mAm_{A} at LHC14 for several values of tanβ\tan\beta. Other parameters are fixed at their values for the model line introduced in the text. The horizontal black line shows the current upper limit on the cross section obtained by ATLAS.

IV SM Backgrounds and Analysis Cuts

Our signal ppH,Aχ1±χ24+Tpp\rightarrow H,A\rightarrow\chi_{1}^{\pm}\chi_{2}^{\mp}\rightarrow 4\ell+\not{E}_{T} contains 4 leptons and missing energy in the final states, where one pair of leptons comes from the decay of a ZZ-boson. Since, as just mentioned, the signal rate is too small at the HL-LHC, we will from now on mostly focus our attention on a 100 TeV pppp collider.

Our simplified study has been carried out at parton level. The dominant SM background to the 4+T4\ell+\not{E}_{T} events comes from W±WVW^{\pm}W^{\mp}V, tt¯Vt\bar{t}V, ZhZh and ZZVZZV (V=W±,Z,γV=W^{\pm},Z,\gamma). Notice that the partonic final states from the signal, as well as from all the backgrounds other than tt¯Vt\bar{t}V production, are free of any hadronic activity. We use tree-level matrix elements from the HELAS library in Madgraph to evaluate the backgrounds, and then scale our cross section to NLO with KK-Factors calculated using MCFM  mcfm .444The KK-factors that we use are, KWWV=1.36K_{WWV}=1.36, Ktt¯V=1.30K_{t\bar{t}V}=1.30, KZh=1.40K_{Zh}=1.40 and KZZV=1.40K_{ZZV}=1.40. For the tt¯Vt\bar{t}V background we veto events which contain any bb-jets (i.e. bb-quarks) with pT>20p_{T}>20 GeV and |η(b)|<2.5|\eta(b)|<2.5. This serves as a powerful cut in reducing this background. However, with PDF enhancements, we find that this background becomes the second most dominant background at s=\sqrt{s}= 100 TeV. W±WVW^{\pm}W^{\mp}V proves to be the most dominant background at all energies.

To select events, we identify the isolated leptons if they satisfy

  • pTp_{T} (1\ell_{1}, 2\ell_{2}, 3\ell_{3}, 4\ell_{4}) >> 20 GeV, 10 GeV, 10 GeV, 10 GeV;

  • |η||\eta| (1\ell_{1}, 2\ell_{2}, 3\ell_{3}, 4\ell_{4}) << 2.5.

We model experimental errors in the measurement of lepton energies by Gaussian smearing electron and muon energies using ATLAS:2013-004 ,

ΔEE=0.25E(GeV)0.01,\frac{\Delta E}{E}=\frac{0.25}{\sqrt{\rm E(GeV)}}\oplus 0.01, (5)

where \oplus denotes addition in quadrature.

Since the signal of interest has a final state of 4+T4\ell+\not{E}_{T}, we started with a set of minimal cuts, labeled as Cuts A, which include :

  • Veto events with bb-jets pTp_{T} (jet) >> 20 GeV and |η||\eta| (jet) << 2.5 as already mentioned;

  • ΔR(j,)>\Delta_{R}(j,\ell)> 0.4, where jj denotes a bb-quark with pT<20p_{T}<20 GeV or with |ηb|>0.4|\eta_{b}|>0.4, to mimic lepton isolation;

  • Invariant mass for two opposite sign same flavor leptons M+M_{\ell^{+}\ell^{-}} >> 10 GeV, to reduce the background from γ¯\gamma^{*}\rightarrow\ell\bar{\ell};

  • T>125\not{E}_{T}>125 GeV.

After applying cut A, the mass distributions and T\not{E}_{T} distribution obtained (upon summing bb¯b\bar{b} and gggg initiated processes) are shown in Fig 6 and 7, respectively.

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Figure 6: Plots of the (a) invariant mass distribution M(12)M(\ell_{1}\ell_{2}) of the two leptons that form an invariant mass closest to mZm_{Z},(b) invariant mass distribution of the remaining two leptons, M(3,4)M(\ell_{3},\ell_{4}), (c) invariant mass of the 44\ell system, and (d) cluster transverse mass distribution of the 4+T4\ell+\not{E}_{T} system, for the Higgs signal (ppH,A4+T+X)(pp\rightarrow H,\ A\rightarrow 4\ell+\not{E}_{T}+X), after the cut set A defined in the text. The corresponding contributions from the dominant physics backgrounds are also shown.
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Figure 7: The missing transverse energy T\not{E}_{T} distribution for the Higgs signal (ppH,A4+T+X)(pp\rightarrow H,\ A\rightarrow 4\ell+\not{E}_{T}+X) after the cuts set A. The corresponding contributions from the dominant physics backgrounds are also shown.

Since neutralinos and neutrinos escape detection (and so serve as sources of missing energy) it is not possible to reconstruct the invariant mass of HH or AA as a bump in the invariant mass of the final state. We can, however, sharpen the signal by additional cuts. Motivated by Aaboud:2018xdl , we apply T275\not{E}_{T}\geq 275 GeV cut, since we have two neutralinos of mass \sim 100 GeV in the final state. As can be seen from Figs 6 and 7, the following mass cuts and T\not{E}_{T} cuts can reduce the SM background very efficiently. Further cuts applied are :

  • We define 1\ell_{1} and 2\ell_{2} as the two leptons whose invariant mass is closest to mZm_{Z} and require |M(1,2)mZ|<10|M(\ell_{1},\ell_{2})-m_{Z}|<10 GeV since the signal includes one ZZ boson;555Although we do not explicitly require it, for the most part, 1\ell_{1} and 2\ell_{2} have opposite sign and same flavour.

  • 10<M(3,4)<7510<M(\ell_{3},\ell_{4})<75 GeV, where 3\ell_{3} and 4\ell_{4} denotes the remaining leptons.

  • 0.14mA<M(4)<0.34mA0.14\ m_{A}<M(4\ell)<0.34\ m_{A}

  • T>275\not{E}_{T}>275 GeV.

Of course, since mAm_{A} is not a priori known, the cut on M(4)M(4\ell) needs further explanation. Unless mAm_{A} has already been measured from studies of AA or HH decays via SM channels, operationally, mAm_{A} here refers to the upper end point of the signal MT(4,T)M_{T}(4\ell,\not{E}_{T}) distribution shown in frame (d) of Fig. 6, assuming that it can be experimentally extracted.666We appreciate that the extraction of this end point may be very difficult. Since this is a first exploration of the 4+T4\ell+\not{E}_{T} signal from the decay of heavy Higgs bosons in natural SUSY models, we do not attempt to explore the details of the end point determination, but simply assume that it can be extracted from the data. We note that the optimal choice of the M(4)M(4\ell) cut would only be weakly sensitive to the lightest neutralino mass for mA,Hmχ~10m_{A,H}\gg m_{\tilde{\chi}^{0}_{1}}. The cut set A, augmented by the cuts listed above, is labeled as cut set B.

In Fig. 8, we show the signal cross section versus mAm_{A} after cuts B at (a) the HL-LHC, and (b) a 100 TeV pppp collider. We indeed see from frame (a) that for all values of mAm_{A} the signal lies well below the one event level. Although perhaps only of academic interest, it is worth noting that a comparison of this figure with Fig. 4(a) shows that the signal efficiency is \sim 5-10% despite the requirement all four leptons are required to have a pTp_{T} of at least 10 GeV. This is a reflection of the boost the electroweakinos, and concomitantly the leptons, gain when they originate in the decays of the heavy Higgs bosons. From Fig. 8(b), we project that at the FCC or at the SPPC with an integrated luminosity of 15 ab-1, several tens of signal events may be expected after cuts B over most of the range of mAm_{A} in the figure.

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Figure 8: NNLO Cross sections, σ(A)\sigma(A), σ(H)\sigma(H), and σ(A)+σ(H)\sigma(A)+\sigma(H) times the cascade decay branching fractions into the 4+T4\ell+\not{E}_{T} final state in fb vs. mAm_{A} for (a) 14 TeV and (b) 100 TeV, after the cut set B defined in the text.

V Discovery Potential with Cut-and-Count Analysis

In this section, we study the discovery potential of the 4+T4\ell+\not{E}_{T} signal for heavy Higgs bosons at a 100 TeV pppp collider using a traditional cut-and-count analysis. To this end, we show in Table 3 our results for the signal after the cut set B for three benchmark points (BPs) with varying mAm_{A} (with other parameters fixed to their values in Table 1), along with the main sources of SM backgrounds. The subdominant background listed in the fourth-last row is the combined background resulting from SM ZhZh and from ZZVZZV production.

BP1 BP2 BP3
mAm_{A}  =  1200GeV1200\ \rm GeV mAm_{A}  =  1400GeV1400\ \rm GeV mAm_{A}  =  1600GeV1600\ \rm GeV
ppHpp\rightarrow H 4.12 ×103\times 10^{-3} 3.45×103\times 10^{-3} 2.17 ×103\times 10^{-3}
ppApp\rightarrow A 4.38 ×103\times 10^{-3} 3.73 ×103\times 10^{-3} 2.35 ×103\times 10^{-3}
W+W+W^{+}W^{-}\ell^{+}\ell^{-} 7.13 ×103\times 10^{-3} 7.23 ×103\times 10^{-3} 6.18 ×103\times 10^{-3}
tt¯+t\bar{t}\ell^{+}\ell^{-} 1.83 ×103\times 10^{-3} 1.58 ×103\times 10^{-3} 1.17 ×103\times 10^{-3}
Z++\ell^{+}\ell^{-}\ell^{+}\ell^{-} 1.38×103\times 10^{-3} 1.41 ×103\times 10^{-3} 1.24×103\times 10^{-3}
NSN_{S} 127 108 68
NBN_{B} 155 153 129
NssN_{ss} 9.1 7.9 5.5
Table 3: The signal and SM backgrounds at a 100 TeV pppp collider for three benchmark points after the cut set B defined in the text. All the cross sections are in fb. Here, NSN_{S} is the total number signal events, combining both scalar and pseudo scalar and NBN_{B} is the total number of background events and NssN_{ss} is the statistical significance of the signal, all for an integrated luminosity of 15 ab1\rm ab^{-1}. We have all flavours of leptons (ee and μ\mu).

In Fig. 9, we present our estimates of statistical significance stat ,

Nss(2×(NS+NB)ln(1+NS/NB)2×NS),N_{ss}\equiv\sqrt{(2\times(N_{S}+N_{B})\ln(1+N_{S}/N_{B})-2\times N_{S})},

for 1100 GeV mA2000\leq m_{A}\leq 2000 GeV. Our selection cuts work well in removing a large part of the background. We see that with a center of mass energy of 100 TeV and integrated luminosity of \mathcal{L} = 15 ab1\rm ab^{-1}, we have enough events to claim a 5σ5\sigma discovery for mA1.11.65m_{A}\sim 1.1-1.65 TeV. We also obtain a 95% CL exclusion limit for the H,A4+TH,\ A\rightarrow 4\ell+\not{E}_{T} signal for values of mAm_{A} extending out as far as 2 TeV.

We now turn to an examination of whether we can use machine learning techniques to suppress the background further and concomitantly increase the reach. In the next section, we study the use of boosted decision trees to further enhance the signal.

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Figure 9: The signal significance NssN_{ss} vs mAm_{A} using a traditional cut-based analysis for ppH+A4+Tpp\rightarrow H+A\rightarrow 4\ell+\not{E}_{T} events at a 100 TeV pppp collider.

VI Improvement with Boosted Decision Trees

We have just seen that the cut-based signal from heavy Higgs boson decays via the 4+T4\ell+\not{E}_{T} channel yields a statistically significant discovery level over a limited range of mAm_{A} values even at a 100 TeV pppp collider. Of course, it is possible that this signal may be combined with a signal from other channels to claim discovery over a wider range. The point of this study, however, is to examine how much improvement may be possible without combining other channels if we go beyond the traditional cut-based analysis which as we saw yields a discovery significance of Nss>5N_{ss}>5 for mA1.11.65m_{A}\sim 1.1-1.65 TeV for s\sqrt{s} = 100 TeV and 15 ab-1 of integrated luminosity.

It has been found that ML techniques can greatly improve the signal-to-background discrimination and they are widely used by experimental analyses. In this section we use boosted decision trees (BDT) for which algorithms are included in the ToolKit for MultiVariate Analysis (TMVA) TMVA , a multivariate analysis package included with ROOT. For this study, we have used the following variables for training and testing,

  • The invariant mass M(4)M(4\ell).

  • The invariant masses M(1,2)M(\ell_{1},\ell_{2}) and M(3,4)M(\ell_{3},\ell_{4})

  • T\not{E}_{T}, missing transverse energy.

We have generated signal files for each value of mAm_{A} along with the backgrounds at 100 TeV after applying the cut set B, except that we have now relaxed the cut on T\not{E}_{T} to be T>200\not{E}_{T}>200 GeV before passing the samples for training and testing. We train 400,000 signal events and 400,000 background events for each channel. We used the same number of events for testing. Figure 10 shows the BDT response for three BPs with different mAm_{A} values.

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Figure 10: The BDT response for mAm_{A} = (a) 1200, (b) 1400 and (c) 1600 GeV. The BDT response of test points (solid) and training points (with error bar) is superposed in the figure.

In Table 4, we present our estimate of NssN_{ss} from the BDT analysis for the same BP points as in Table 3. We see that there is, indeed, a significant improvement over the previous cut-based analysis.

Number of Events pp ϕ0\rightarrow\phi^{0} Total Background NssN_{ss}
BP1, mA=1200GeVm_{A}=1200\ \rm GeV
All mass cuts 127 155 9.1
BDT cut 132 58 13.7
BP2, mA=1400GeVm_{A}=1400\ \rm GeV
All mass cuts 107 153 7.9
BDT cut 133 46 14.9
BP3, mA=1600GeVm_{A}=1600\ \rm GeV
All mass cuts 68 129 5.5
BDT cut 72 25 11.0
Table 4: A comparison between the cut based and BDT analyses for the three benchmark points introduced in the text.

Fig. 11 shows the individual contributions from each of HH and AA for the BDT analysis along with the significance from the combined HH and AA signal. This may be compared to the significance shown in Fig. 9 for the traditional cut-and-count analysis. We see that, by using the BDT analysis, we would be able to discover HH and AA at the 5σ5\sigma level via H,A4+TH,\ A\rightarrow 4\ell+\not{E}_{T} channel for mA12m_{A}\sim 1-2 TeV – a considerable improvement in range of mAm_{A} over the usual cut-based method!

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Figure 11: Statistical significance plots for the H,A4+TH,\ A\rightarrow 4\ell+\not{E}_{T} signal at a 100 TeV hadron collider after the BDT analysis.

VII Conclusions

In this paper, we have examined heavy neutral Higgs boson discovery as motivated by natural SUSY models with light higgsinos. In such models, the heavy Higgs H,AH,\ A decays to electroweakinos are almost always open since the lightest higgsinos are expected to have masses below 350\sim 350 GeV range whilst the HH and AA bosons can have TeV-scale masses. Since decays to pairs of higgsino-like states are dynamically suppressed, our channel of primary interest is H,Aχ~1±χ~2H,\ A\rightarrow\tilde{\chi}_{1}^{\pm}\tilde{\chi}_{2}^{\mp} decay, followed by χ~2±Zχ~1±\tilde{\chi}_{2}^{\pm}\rightarrow Z\tilde{\chi}_{1}^{\pm} followed by Z+Z\rightarrow\ell^{+}\ell^{-} and then each χ~1±±νχ~10\tilde{\chi}_{1}^{\pm}\rightarrow\ell^{\pm}\nu_{\ell}\tilde{\chi}_{1}^{0}. Combining all flavours of decays to ee and μ\mu leads to a distinctive H,A4+TH,\ A\rightarrow 4\ell+\not{E}_{T} signature for heavy Higgs boson decay to SUSY particles. The leptons from χ~1±\tilde{\chi}_{1}^{\pm} decay are soft in the χ~1±\tilde{\chi}_{1}^{\pm} rest frame but are boosted to higher energies due to the large mH,Am_{H,A} masses. Thus, we evaluated this signal channel against dominant SM backgrounds for both HL-LHC and for FCC-hh or SPPC with s=100\sqrt{s}=100 TeV, applying judicious cuts on various combinations of invariant masses of the leptons, and also requiring T>275\not{E}_{T}>275 GeV. Our selection requirements retain much of the signal while removing the physics background efficiently.

In our analysis we have focused on production of the heavy Higgs bosons with a mass (mHmAm_{H}\simeq m_{A}) between 1 TeV and 2 TeV. While a signal (in the 4+T4\ell+\not{E}_{T} channel) is not likely to be observable at HL-LHC, prospects are much better at FCC-hh or SPPC. The best case for discovery is near mA1.21.3m_{A}\simeq 1.2-1.3 TeV that has a balance between kinematics of leptons in the final state and production cross sections. We note the following:

  • A 100 TeV hadron collider offers promise to discover a heavy neutral Higgs boson via one of its dominant SUSY decay modes in natural SUSY models with a mass 12\sim 1-2 TeV. With a conventional cut-based analysis, we are able to obtain a Nss>5N_{ss}>5 statistical significance over a range mA1.11.65m_{A}\sim 1.1-1.65 TeV. We find though that a BDT analysis of the same signal can potentially improve the significance greatly giving NssN_{ss} as high as 16 for mA1.3m_{A}\simeq~{}1.3 TeV, and Nss>5N_{ss}>5 over a range mA12m_{A}\sim 1-2 TeV even via our proposed very difficult discovery channel.

  • For somewhat smaller values of heavy Higgs boson masses characterized by mA<1m_{A}~{}\mbox{\raisebox{-2.58334pt}{$\stackrel{{\scriptstyle<}}{{\sim}}$}}~{}1 TeV, the signal cross section is suppressed both by smaller branching ratio into the SUSY mode, and also by a smaller boost of the daughter EWinos which, in turn, reduces the efficiency with which the softer leptons pass the cuts. Nonetheless, the heavy neutral SUSY Higgs bosons should be detectable in this range via SM decay modes such as H,Aττ¯H,\ A\rightarrow\tau\bar{\tau}.

  • For increasing mAm_{A} values beyond 1.3\sim 1.3 TeV, the Higgs production cross section becomes much smaller since the gggg and bb¯b\bar{b} fusion production cross sections are increasingly suppressed.

  • We stress that we have focused only on the signal from a difficult SUSY decay mode of the heavy Higgs boson with an eye to assessing how ML techniques could serve to enhance difficult-to-see signals. Hence we have not examined the possibility of combining SUSY modes or whether the discovery of a heavy Higgs boson might be possible from a study of its SM decays.

For mAmHm_{A}\simeq m_{H} significantly beyond 1 TeV and tanβ1050\tan\beta\sim 10-50, it may become increasingly challenging to search for heavy Higgs bosons via their decays into SM particles due to the diminished branching fractions to bb¯b\bar{b} and ττ¯\tau\bar{\tau}, once the dominant SUSY decay channels become allowed. The chargino and neutralino discovery channel for heavy Higgs bosons at high energy hadron colliders offers an important opportunity to discover the heavy neutral Higgs bosons via their decay into EWinos. An upgrade to a 100 TeV hadron collider seems essential for heavy Higgs HH and AA discovery via the natural SUSY 4+T4\ell+\not{E}_{T} channel.

Acknowledgement

We thank an anonymous referee for useful suggestions. This work was supported in part by the US Department of Energy, Office of High Energy Physics Grant No. DE-SC-0009956 and DE-SC-0017647. The work of DS was supported in part by the Ministry of Science and Technology (MOST) of Taiwan under Grant No. 110-2811-M-002-574, and work of RJ is supported by MOST 110-2639-M-002-002-ASP.

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