Pith. sign in

REVIEW 2 major objections 4 minor 103 references

A first dedicated search for dark matter produced with bottom quarks and a Z boson at a hadron collider finds no signal and sets cross-section limits down to 10^-3 pb.

Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →

T0 review · deepseek-v4-flash

2026-08-04 09:55 UTC pith:WQ6IXJHK

load-bearing objection First dedicated CMS probe of the bb+Z(ll)+MET channel: a solid, careful search whose main soft spot is a validation gap in the DY pTmiss correction. the 2 major comments →

arxiv 2510.12396 v2 pith:WQ6IXJHK submitted 2025-10-14 hep-ex

Search for dark matter production in association with bottom quarks and a lepton pair in proton-proton collisions at sqrt{s} = 13 TeV

classification hep-ex
keywords dark matterpseudoscalar mediator2HDM+amissing transverse momentumbottom-quark jetsZ bosonHiggs bosoncollider search
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper argues that a new dark-matter production channel—bottom-quark pairs recoiling against a leptonically decaying Z boson and large missing transverse momentum, with the missing momentum originating from a pseudoscalar mediator decaying into dark matter—can be isolated from standard model backgrounds, and that no excess is observed in the full 138 fb^-1 dataset. The channel matters because it reaches a region of the 2HDM+a parameter space, especially large tan-beta, that other dark-matter and flavor searches cannot reach, including the region favored by a dark-matter interpretation of the galactic-center gamma-ray excess. The paper's central result is the first experimental constraint on the product sigma(pp->bbH) x B(H->Za) x B(Z->ll) x B(a->chi chi), with observed 95% confidence-level upper limits falling from about 10^-2 pb for a 400 GeV heavy scalar to about 10^-3 pb for a 2000 GeV heavy scalar. These limits exclude heavy-scalar masses up to roughly 900 GeV for small mediator masses in the benchmark model, and they exclude a substantial part of the parameter space preferred by the observed dark-matter relic density.

Core claim

The discovery claim is a null result: in proton-proton collisions at 13 TeV, events with an opposite-sign same-flavor lepton pair near the Z mass, at least one b-tagged jet, and large missing transverse momentum agree with standard model predictions. The paper establishes the first dedicated collider search for this final state and reports observed 95% CL upper limits on sigma(pp->bbH) B(H->Za) B(Z->ll) B(a->chi chi) ranging from about 10^-2 pb at mH = 400 GeV to about 10^-3 pb at mH = 2000 GeV. In the benchmark 2HDM+a interpretation, the results exclude heavy scalar masses up to about 900 GeV for small pseudoscalar masses, and up to about 1.1 TeV for tan-beta near 25, covering a meaningful

What carries the argument

The central machinery is the event-selection plus multivariate discriminant: a loose requirement of at least one b-tagged jet is combined with a Z-mass window on an opposite-sign same-flavor dilepton pair and a missing-transverse-momentum threshold, and then a fully connected neural network (the MLP, binned into 17 MLP4 score intervals) combines kinematic variables such as pT^miss, the transverse mass mT, and mT2 to separate signal from background. Backgrounds are controlled with four single-bin control regions for Drell-Yan, top-quark pair, WZ, and ZZ production, an analytical kinematic solver vetoes dileptonic top-quark events, and the Drell-Yan missing-momentum scale and resolution are co

Load-bearing premise

The analysis assumes that the data-driven correction to the Drell-Yan missing-momentum scale and resolution, derived at low missing momentum and checked in a region without b jets, remains valid in the signal region where missing momentum is large and at least one b jet is present.

What would settle it

The central null result would be weakened if, in a dedicated validation region requiring at least one b-tagged jet, a Z-like dilepton pair, no extra leptons, and 300 < pT^miss < 500 GeV, the ratio of observed events to the corrected prediction deviated from unity by more than the quoted uncertainty.

Watch this falsifier — get emailed when new claim-graph text bears on it.

If this is right

  • The quoted upper limits provide the first model-independent cross-section bounds for the bb + Z + missing-momentum final state, applicable to any model with a heavy scalar decaying to Z plus invisible particles in association with bottom quarks.
  • In the benchmark 2HDM+a scenario, heavy scalar masses up to about 900 GeV are excluded for small pseudoscalar masses, closing part of the parameter space favored by dark-matter relic-density calculations.
  • The analysis excludes low mediator masses over a broad range of the mixing angle sin(theta), leaving only very small and very large values of sin(theta) uncovered.
  • The search is most sensitive to semi-boosted topologies with mH - ma near 1 TeV, while compressed mass configurations and configurations with very large mass splittings remain less constrained.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • An extension the paper leaves implicit is that including final states where the Z decays to tau leptons, or where the dilepton pair arises from a non-resonant spectrum, could cover configurations where the present lepton selection loses efficiency.
  • Because the dominant limitations come from the normalization uncertainties of the WZ and ZZ backgrounds, a future analysis could improve sensitivity with a dedicated diboson-enriched control region or by exploiting jet substructure for more boosted topologies.
  • The tabulated model-independent results allow reinterpretation in other pseudoscalar-mediator or two-Higgs-doublet scenarios beyond the benchmark, which is a natural follow-up given the cosmological motivation.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

2 major / 4 minor

Summary. This paper presents a search for dark matter produced in association with b quarks and a lepton pair in 138 fb^-1 of 13 TeV CMS data, using the 2HDM+a model with the process pp -> bbH, H -> Za, Z -> ll, a -> chichi. A multivariate MLP discriminant is trained on simulated signal and background events, and a profile-likelihood fit combines a 17-bin signal region with four control regions (DY, tt, WZ, ZZ) to constrain background normalizations. A data-driven correction to the DY pTmiss scale and resolution is derived in a low-pTmiss sideband and applied to the signal region. The observations are consistent with the standard-model expectation, and 95% CL upper limits are set on sigma(pp->bbH) B(H->Za) B(Z->ll) B(a->chichi) in the range 10^-2 to 10^-3 pb for mH = 400-2000 GeV. The results are interpreted as constraints on the 2HDM+a parameter space and compared with the region favored by the relic-density calculation.

Significance. If the result holds, this is the first dedicated experimental search for this specific bbZ(ll)+pTmiss signature, and it probes regions of the 2HDM+a parameter space (in particular high tan(beta)) that are motivated by the gamma-ray galactic center excess and are not directly covered by earlier mono-Z or mono-H searches. The analysis is careful and thorough: it uses the full Run 2 dataset, applies a multivariate discriminant, enumerates systematic uncertainties in detail, provides control-region validation plots, and makes tabulated results available in HEPData. The main strengths are the explicit signal model, the use of data-driven background normalizations with cross-checked control regions, and the public record of the results.

major comments (2)
  1. [Section 6] The data-driven correction to the DY pTmiss scale and resolution is derived in a sideband with pTmiss < 65 GeV and then extrapolated to the signal region. The only stated verification is in a region with no b jets and pTmiss < 300 GeV (Section 6). This does not directly validate the correction in the SR phase space, which requires Nb >= 1 and extends to pTmiss values well above 300 GeV. Because the MLP discriminant uses pTmiss and mT(ell,ell,pTmiss) as leading inputs (Section 5.3), a miscalibration of the DY tail would directly reshape the SR templates and thereby shift the derived limits, especially for low-mH signals that populate the lower MLP4 bins. Please either provide a validation in a b-enriched region with higher pTmiss, or quantify the uncertainty from this extrapolation and show its effect on the final limits.
  2. [Section 8] The background-only fit changes the WZ and ZZ normalizations by +101% and +113%, respectively. These processes populate the high-MLP4 (signal-like) bins, and the paper states that their normalization uncertainties are among the most important systematics. The WZ and ZZ control regions are single-bin, so they constrain the overall normalization but not the shape of the MLP4 distribution in the SR. Given the very large correction factors, additional validation is needed to demonstrate that the shape modeling in the b-enriched phase space is reliable. Please show pre-fit and post-fit comparisons in finer-grained b-enriched CRs, or otherwise discuss how the large k-factors are constrained by the data.
minor comments (4)
  1. [Section 5.3] The definition of the MLP4 score in Eq. (4) appears to contain a typographical issue: the floor function is not explicitly written. Please clarify the transformation.
  2. [Section 8.1 / Figure 7] The y-axis of Figure 7 is described as the upper limit on sigmaB but the scaling by arbitrary factors (x10^-n) is only noted in the caption. It would be clearer to label each panel with the absolute scale or indicate the scaling directly on the axis.
  3. [References] The benchmark parameters in Eq. (1) are cited to Refs. [3,52], but readers may benefit from a direct reference to the specific 2HDM+a parameter scan in which this benchmark was first used. Please check whether a more precise citation is available.
  4. [Section 6] The validation of the DY Nb=0/Nb>=1 normalization consistency is described only in words. A figure or table showing the compatibility of the ratios in the two categories would strengthen this cross-check.

Circularity Check

0 steps flagged

No circularity found: the search derives limits from an externally defined 2HDM+a model, with backgrounds normalized in disjoint control regions and the only data-driven correction being a standard auxiliary measurement.

full rationale

The analysis is a search for a BSM signal in an externally defined 2HDM+a model. The benchmark signal parameters (Eq. 1) are taken from prior literature (Refs. [3], [51], [52]), not fitted to the data; the signal is simulated with MG5 at fixed masses and couplings. Background normalizations are fitted in control regions that are disjoint from the signal region (DY CR requires Nb=0 and pTmiss<140 GeV; tt, WZ, ZZ CRs have different final-state requirements), so the SR counts are not equal to the fit by construction. The one data-driven calibration, the DY pTmiss recoil correction, is derived in a sideband with pTmiss<65 GeV and propagated to the SR; this is a standard auxiliary measurement and the SR is not used to derive it, so it is not a fitted-input-called-prediction step. The paper explicitly notes the extrapolation is verified only in a region with no b jets and pTmiss<300 GeV; this is a validation gap (a robustness risk), not a circularity, because the correction is not an ansatz that already contains the SR result. The relic-density comparison uses an independent MadDM calculation. No uniqueness theorem or load-bearing self-citation is invoked: the only comparison to a prior CMS search [28] is an external cross-check of the excluded mass range. Therefore the derivation chain is self-contained with respect to the final limits.

Axiom & Free-Parameter Ledger

3 free parameters · 6 axioms · 0 invented entities

The paper introduces no new physical entities; it searches for the established H, a, and chi fields of the 2HDM+a model. The free parameters are benchmark-model choices and fit nuisance parameters, not new physical constants fitted to the target result. No independent falsifiable handle is created beyond the search limits themselves.

free parameters (3)
  • 2HDM+a benchmark parameters = m_chi=45 GeV, tan(beta)=11, sin(theta)=0.35, lambda_3=lambda_P1=lambda_P2=0.25, y_chi=1
    Benchmark scenario in Eq. (1), taken from prior literature (Refs. [3,14,51,52]). Not fitted to this data, but all signal simulations and model exclusions are conditional on these choices.
  • Background normalization parameters (DY, tt, WZ, ZZ) = DY +10%, tt +8%, WZ +101%, ZZ +113% relative to pre-fit predictions
    Unconstrained normalization parameters fitted to control regions in the maximum-likelihood fit (Section 8). They affect the background model used to derive limits.
  • DY pTmiss correction parameters (double Gaussian) = not public; derived in sideband with pTmiss<65 GeV
    Parameterized double-Gaussian correction to DY pTmiss scale/resolution fitted in a sideband and extrapolated to the signal region (Section 6).
axioms (6)
  • domain assumption The Standard Model is the correct low-energy description of background processes.
    All backgrounds are generated with standard SM MC samples (DY, tt, single top, diboson, minor processes), and the fit assumes these are the only background sources.
  • domain assumption The 2HDM+a model correctly describes signal production and decay kinematics.
    Signal samples are generated with MG5 using a dedicated 2HDM+a model (Ref. [51]); the interpretation layer assumes this model and the benchmark parameter choices.
  • domain assumption The GEANT4-based CMS detector simulation, after data-to-simulation corrections, accurately models the detector response.
    All MC samples are passed through full CMS simulation; corrections are applied for trigger, lepton, jet, b-tag, and pTmiss response. The analysis relies on this simulation for signal shapes and part of the background prediction.
  • domain assumption The narrow-width approximation for the H and a resonances is valid in the considered parameter space.
    Explicitly assumed in Section 8.1 when converting limits to the (mH, ma) plane; the paper states the widths were checked to validate this approximation.
  • standard math The asymptotic CLs method yields valid 95% confidence intervals.
    Upper limits are computed with the asymptotic approximation of CLs (Refs. [98,99]), a standard statistical procedure.
  • domain assumption NNPDF3.1 NNLO PDFs and the PYTHIA CP5 tune adequately model initial-state partons and hadronization.
    Used for all signal and background simulations; PDF and scale uncertainties are estimated but the central predictions rely on these choices.

pith-pipeline@v1.3.0-alltime-deepseek · 46501 in / 10585 out tokens · 93719 ms · 2026-08-04T09:55:21.497519+00:00 · methodology

0 comments
read the original abstract

A search is performed for dark matter produced in association with bottom quarks and a pair of electrons or muons in data collected with the CMS detector at the LHC, corresponding to 138 fb$^{-1}$ of integrated luminosity of proton-proton collisions at a center-of-mass energy of 13 TeV. For the first time at the LHC, the associated production of a bottom quark-antiquark pair and a new heavy neutral Higgs boson (H) that subsequently decays into a leptonically decaying Z boson and a pseudoscalar (a) is explored. The latter acts as a dark matter mediator in the context of the two Higgs doublet model plus a pseudoscalar (2HDM+a). Multivariate techniques that target a wide range of mass configurations for the H and a particles are used. The observations are consistent with the expectations from standard model processes. Upper limits at 95% confidence level are set on the product of cross section and branching fraction of the new particles, ranging from 10$^{-2}$ pb for an H mass of 400 GeV to 10$^{-3}$ pb for an H mass of 2000 GeV. Constraints on the parameter space of a benchmark 2HDM+a model are derived and compared with expectations in the context of cosmological predictions.

Figures

Figures reproduced from arXiv: 2510.12396 by CMS Collaboration.

Figure 1
Figure 1. Figure 1: Example diagram at leading order for the production of a heavy pseudoscalar medi [PITH_FULL_IMAGE:figures/full_fig_p004_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: Normalized distributions in p miss T (upper left), m ℓℓ,p miss T T (upper right), m ℓℓ T2 (lower left), and ∆R ℓℓ (lower right) in the SR for the main background processes (solid lines) and signals with high (dark gray dashed line) and low (light gray dashed line) mH values. The vertical bars at the center of the bins represent the statistical uncertainty in the predictions [PITH_FULL_IMAGE:figures/full_f… view at source ↗
Figure 3
Figure 3. Figure 3: Illustration of the requirements on the SR and CRs. All requirements are applied on [PITH_FULL_IMAGE:figures/full_fig_p013_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: Distributions in p miss T for the DY (upper left), tt (upper right), WZ (lower left), and ZZ (lower right) CRs. In the WZ and ZZ CRs, p miss T is obtained by removing the additional leptons from the calculation. The distributions are shown after performing a background-only fit in the p miss T distributions of all CRs. The last bin includes the overflow, except for the DY CR where p miss T < 140 GeV. The l… view at source ↗
Figure 5
Figure 5. Figure 5: Distributions in the MLP4 score for the DY (upper left), t [PITH_FULL_IMAGE:figures/full_fig_p016_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: Main statistical discriminant of the analysis used to extract the signal after having [PITH_FULL_IMAGE:figures/full_fig_p019_6.png] view at source ↗
Figure 7
Figure 7. Figure 7: Observed and expected upper limits at 95% CL on the product of the signal cross sec [PITH_FULL_IMAGE:figures/full_fig_p020_7.png] view at source ↗
Figure 8
Figure 8. Figure 8: Excluded regions in the parameter space of the 2HDM+a. The solid lines encompass [PITH_FULL_IMAGE:figures/full_fig_p022_8.png] view at source ↗

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

103 extracted references · 1 canonical work pages

  1. [1]

    Cosmological constraints on the properties of weakly interacting massive particles

    G. Steigman and M. S. Turner, “Cosmological constraints on the properties of weakly interacting massive particles”,Nucl. Phys. B253(1985) 375, doi:10.1016/0550-3213(85)90537-1

  2. [2]

    WIMP dark matter candidates and searches — current status and future prospects

    L. Roszkowski, E. M. Sessolo, and S. Trojanowski, “WIMP dark matter candidates and searches — current status and future prospects”,Rept. Prog. Phys.81(2018) 066201, doi:10.1088/1361-6633/aab913,arXiv:1707.06277

  3. [3]

    Probing the pseudoscalar portal to dark matter via ¯bbZ(→ℓℓ)+̸E T : From the LHC to the galactic center excess

    P . Tunney, J. M. No, and M. Fairbairn, “Probing the pseudoscalar portal to dark matter via ¯bbZ(→ℓℓ)+̸E T : From the LHC to the galactic center excess”,Phys. Rev. D96(2017) 095020,doi:10.1103/PhysRevD.96.095020,arXiv:1705.09670

  4. [4]

    Particle dark matter: Evidence, candidates and constraints

    G. Bertone, D. Hooper, and J. Silk, “Particle dark matter: Evidence, candidates and constraints”,Phys. Rept.405(2005) 279,doi:10.1016/j.physrep.2004.08.031, arXiv:hep-ph/0404175

  5. [5]

    Dark sector searches with the CMS experiment

    CMS Collaboration, “Dark sector searches with the CMS experiment”,Phys. Rep.(2024) 448,doi:10.1016/j.physrep.2024.09.013,arXiv:2405.13778. References 23

  6. [6]

    Dark matter searches at accelerators

    A. De Roeck, “Dark matter searches at accelerators”,Nucl. Phys. B1003(2024) 116480, doi:10.1016/j.nuclphysb.2024.116480

  7. [7]

    Constraints on simplified dark matter models involving an s-channel mediator with the ATLAS detector in pp collisions at √s=13 TeV

    ATLAS Collaboration, “Constraints on simplified dark matter models involving an s-channel mediator with the ATLAS detector in pp collisions at √s=13 TeV”,Eur. Phys. J. C84(2024) 1102,doi:10.1140/epjc/s10052-024-13215-5, arXiv:2404.15930

  8. [8]

    Combination and summary of ATLAS dark matter searches interpreted in a 2HDM with a pseudo-scalar mediator using 139 fb−1 of √s=13 TeV pp collision data

    ATLAS Collaboration, “Combination and summary of ATLAS dark matter searches interpreted in a 2HDM with a pseudo-scalar mediator using 139 fb−1 of √s=13 TeV pp collision data”,Sci. Bull.69(2024) 3005,doi:10.1016/j.scib.2024.06.003, arXiv:2306.00641

  9. [9]

    FERMI-LAT observations of high-energyγ-ray emission toward the galatic center

    Fermi-LAT Collaboration, “FERMI-LAT observations of high-energyγ-ray emission toward the galatic center”,Astrophys. J.819(2016) 44, doi:10.3847/0004-637X/819/1/44,arXiv:1511.02938

  10. [10]

    Limits to dark matter annihilation cross-section from a combined analysis of MAGIC and Fermi-LAT observations of dwarf satellite galaxies

    MAGIC Collaboration, “Limits to dark matter annihilation cross-section from a combined analysis of MAGIC and Fermi-LAT observations of dwarf satellite galaxies”, JCAP02(2016) 039,doi:10.1088/1475-7516/2016/02/039, arXiv:1601.06590

  11. [11]

    Dark matter annihilation in the galactic center as seen by the Fermi gamma ray space telescope

    D. Hooper and L. Goodenough, “Dark matter annihilation in the galactic center as seen by the Fermi gamma ray space telescope”,Phys. Lett. B697(2011) 412, doi:10.1016/j.physletb.2011.02.029,arXiv:1010.2752

  12. [12]

    Origin of the gamma rays from the galactic center

    D. Hooper and T. Linden, “Origin of the gamma rays from the galactic center”,Phys. Rev. D84(2011) 123005,doi:10.1103/PhysRevD.84.123005,arXiv:1110.0006

  13. [13]

    Detection of a gamma-ray source in the galactic center consistent with extended emission from dark matter annihilation and concentrated astrophysical emission

    K. N. Abazajian and M. Kaplinghat, “Detection of a gamma-ray source in the galactic center consistent with extended emission from dark matter annihilation and concentrated astrophysical emission”,Phys. Rev. D86(2012) 083511, doi:10.1103/PhysRevD.86.083511,arXiv:1207.6047. [Erratum: doi:10.1103/PhysRevD.87.129902]

  14. [14]

    Dark matter interpretation of the Fermi-LAT observation toward the galactic center

    C. Karwin et al., “Dark matter interpretation of the Fermi-LAT observation toward the galactic center”,Phys. Rev. D95(2017) 103005, doi:10.1103/PhysRevD.95.103005,arXiv:1612.05687

  15. [15]

    Extended gamma-ray emission from coy dark matter

    C. Boehm et al., “Extended gamma-ray emission from coy dark matter”,JCAP05 (2014) 009,doi:10.1088/1475-7516/2014/05/009,arXiv:1401.6458

  16. [16]

    Bottom-up approach to the galactic center excess

    E. Izaguirre, G. Krnjaic, and B. Shuve, “Bottom-up approach to the galactic center excess”,Phys. Rev. D90(2014) 055002,doi:10.1103/PhysRevD.90.055002, arXiv:1404.2018

  17. [17]

    Renormalizable model for the galactic center gamma-ray excess from dark matter annihilation

    S. Ipek, D. McKeen, and A. E. Nelson, “Renormalizable model for the galactic center gamma-ray excess from dark matter annihilation”,Phys. Rev. D90(2014) 055021, doi:10.1103/PhysRevD.90.055021,arXiv:1404.3716

  18. [18]

    Simplified dark matter models for the galactic center gamma-ray excess

    A. Berlin, D. Hooper, and S. D. McDermott, “Simplified dark matter models for the galactic center gamma-ray excess”,Phys. Rev. D89(2014) 115022, doi:10.1103/PhysRevD.89.115022,arXiv:1404.0022. 24

  19. [19]

    Dark matter with pseudoscalar-mediated interactions explains the DAMA Signal and the galactic center excess

    C. Arina, E. Del Nobile, and P . Panci, “Dark matter with pseudoscalar-mediated interactions explains the DAMA Signal and the galactic center excess”,Phys. Rev. Lett. 114(2015) 011301,doi:10.1103/PhysRevLett.114.011301,arXiv:1406.5542

  20. [20]

    Constraining the spin-dependent WIMP-nucleon cross sections with XENON1T

    XENON Collaboration, “Constraining the spin-dependent WIMP-nucleon cross sections with XENON1T”,Phys. Rev. Lett.122(2019) 141301, doi:10.1103/PhysRevLett.122.141301,arXiv:1902.03234

  21. [21]

    Recommendations on presenting LHC searches for missing transverse energy signals using simplifieds-channel models of dark matter

    A. Boveia et al., “Recommendations on presenting LHC searches for missing transverse energy signals using simplifieds-channel models of dark matter”,Phys. Dark Univ.27 (2020) 100365,doi:10.1016/j.dark.2019.100365,arXiv:1603.04156

  22. [22]

    Pseudoscalar portal dark matter

    A. Berlin, S. Gori, T. Lin, and L.-T. Wang, “Pseudoscalar portal dark matter”,Phys. Rev. D92(2015) 015005,doi:10.1103/PhysRevD.92.015005,arXiv:1502.06000

  23. [23]

    Search for new phenomena in events with an energetic jet and missing transverse momentum in pp collisions at √s=13 TeV with the ATLAS detector

    ATLAS Collaboration, “Search for new phenomena in events with an energetic jet and missing transverse momentum in pp collisions at √s=13 TeV with the ATLAS detector”,Phys. Rev. D103(2021) 112006,doi:10.1103/PhysRevD.103.112006, arXiv:2102.10874

  24. [24]

    Search for new particles in events with energetic jets and large missing transverse momentum in proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Search for new particles in events with energetic jets and large missing transverse momentum in proton-proton collisions at √s=13 TeV”,JHEP11 (2021) 153,doi:10.1007/JHEP11(2021)153,arXiv:2107.13021

  25. [25]

    Search for dark matter in association with an energetic photon in pp collisions at √s=13 TeV with the ATLAS detector

    ATLAS Collaboration, “Search for dark matter in association with an energetic photon in pp collisions at √s=13 TeV with the ATLAS detector”,JHEP02(2021) 226, doi:10.1007/JHEP02(2021)226,arXiv:2011.05259

  26. [26]

    Search for new physics in final states with a single photon and missing transverse momentum in proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Search for new physics in final states with a single photon and missing transverse momentum in proton-proton collisions at √s=13 TeV”,JHEP02 (2019) 074,doi:10.1007/JHEP02(2019)074,arXiv:1810.00196

  27. [27]

    Search for associated production of aZboson with an invisibly decaying Higgs boson or dark matter candidates at √s=13 TeV with the ATLAS detector

    ATLAS Collaboration, “Search for associated production of aZboson with an invisibly decaying Higgs boson or dark matter candidates at √s=13 TeV with the ATLAS detector”,Phys. Lett. B829(2022) 137066, doi:10.1016/j.physletb.2022.137066,arXiv:2111.08372

  28. [28]

    Search for dark matter produced in association with a leptonically decaying Z boson in proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Search for dark matter produced in association with a leptonically decaying Z boson in proton-proton collisions at √s=13 TeV”,Eur. Phys. J. C81(2021) 13,doi:10.1140/epjc/s10052-020-08739-5,arXiv:2008.04735. [Erratum: doi:10.1140/epjc/s10052-021-08959-3]

  29. [29]

    Search for dark matter produced in association with a standard model Higgs boson decaying into b-quarks using the full run 2 dataset from the ATLAS detector

    ATLAS Collaboration, “Search for dark matter produced in association with a standard model Higgs boson decaying into b-quarks using the full run 2 dataset from the ATLAS detector”,JHEP11(2021) 209,doi:10.1007/JHEP11(2021)209, arXiv:2108.13391

  30. [30]

    Search for dark matter in events with missing transverse momentum and a Higgs boson decaying into two photons in pp collisions at√s=13 TeV with the ATLAS detector

    ATLAS Collaboration, “Search for dark matter in events with missing transverse momentum and a Higgs boson decaying into two photons in pp collisions at√s=13 TeV with the ATLAS detector”,JHEP10(2021) 013, doi:10.1007/JHEP10(2021)013,arXiv:2104.13240

  31. [31]

    Search for dark matter particles produced in association with a Higgs boson in proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Search for dark matter particles produced in association with a Higgs boson in proton-proton collisions at √s=13 TeV”,JHEP03(2020) 025, doi:10.1007/JHEP03(2020)025,arXiv:1908.01713. References 25

  32. [32]

    Search for dark matter produced in association with a Higgs boson decaying to a pair of bottom quarks in proton–proton collisions at √s=13 TeV

    CMS Collaboration, “Search for dark matter produced in association with a Higgs boson decaying to a pair of bottom quarks in proton–proton collisions at √s=13 TeV”,Eur. Phys. J. C79(2019) 280,doi:10.1140/epjc/s10052-019-6730-7, arXiv:1811.06562

  33. [33]

    Search for dark matter produced in association with a Higgs boson decaying toγγorτ +τ− at √s=13 TeV

    CMS Collaboration, “Search for dark matter produced in association with a Higgs boson decaying toγγorτ +τ− at √s=13 TeV”,JHEP09(2018) 046, doi:10.1007/JHEP09(2018)046,arXiv:1806.04771

  34. [34]

    ATLAS Collaboration, “Search for dark matter produced in association with a dark Higgs boson decaying into W+W− in the one-lepton final state at √s=13 TeV using 139 fb−1 of pp collisions recorded with the ATLAS detector”,JHEP07(2023) 116, doi:10.1007/JHEP07(2023)116,arXiv:2211.07175

  35. [35]

    ATLAS Collaboration, “Search for dark matter produced in association with a dark Higgs boson decaying into W±W∓ or ZZ in fully hadronic final states from√s=13 TeV pp collisions recorded with the ATLAS detector”,Phys. Rev. Lett.126 (2021) 121802,doi:10.1103/PhysRevLett.126.121802,arXiv:2010.06548

  36. [36]

    Search for dark matter produced in association with a single top quark and an energetic W boson in √s=13 TeV pp collisions with the ATLAS detector

    ATLAS Collaboration, “Search for dark matter produced in association with a single top quark and an energetic W boson in √s=13 TeV pp collisions with the ATLAS detector”,Eur. Phys. J. C83(2023) 603,doi:10.1140/epjc/s10052-023-11582-z, arXiv:2211.13138

  37. [37]

    Search for dark matter produced in association with a single top quark in √s=13 TeV pp collisions with the ATLAS detector

    ATLAS Collaboration, “Search for dark matter produced in association with a single top quark in √s=13 TeV pp collisions with the ATLAS detector”,Eur. Phys. J. C81(2021) 860,doi:10.1140/epjc/s10052-021-09566-y,arXiv:2011.09308

  38. [38]

    Search for dark matter particles produced in association with a top quark pair at √s=13 TeV

    CMS Collaboration, “Search for dark matter particles produced in association with a top quark pair at √s=13 TeV”,Phys. Rev. Lett.122(2019) 011803, doi:10.1103/PhysRevLett.122.011803,arXiv:1807.06522

  39. [39]

    Search for dark matter produced in association with a single top quark or a top quark pair in proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Search for dark matter produced in association with a single top quark or a top quark pair in proton-proton collisions at √s=13 TeV”,JHEP03(2019) 141,doi:10.1007/JHEP03(2019)141,arXiv:1901.01553

  40. [40]

    Measurement of the B 0 S→µ+µ− decay properties and search for the B0→µ+µ− decay in proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Measurement of the B 0 S→µ+µ− decay properties and search for the B0→µ+µ− decay in proton-proton collisions at √s=13 TeV”,Phys. Lett. B842(2023) 137955,doi:10.1016/j.physletb.2023.137955,arXiv:2212.10311

  41. [41]

    Study of the rare decays ofB 0 s andB 0 mesons into muon pairs using data collected during 2015 and 2016 with the ATLAS detector

    ATLAS Collaboration, “Study of the rare decays ofB 0 s andB 0 mesons into muon pairs using data collected during 2015 and 2016 with the ATLAS detector”,JHEP04(2019) 098,doi:10.1007/JHEP04(2019)098,arXiv:1812.03017

  42. [42]

    Weak radiative decays of the B meson and bounds on MH± in the two-Higgs-doublet model

    M. Misiak and M. Steinhauser, “Weak radiative decays of the B meson and bounds on MH± in the two-Higgs-doublet model”,Eur. Phys. J. C77(2017) 201, doi:10.1140/epjc/s10052-017-4776-y,arXiv:1702.04571

  43. [43]

    Measurement of the inclusiveB→X s+d γ branching fraction, photon energy spectrum and HQE parameters

    Belle Collaboration, A. Abdesselam et al., “Measurement of the inclusiveB→X s+d γ branching fraction, photon energy spectrum and HQE parameters”, in38th International Conference on High Energy Physics. 8, 2016.arXiv:1608.02344

  44. [44]

    B s,d →ℓ +ℓ− in a two Higgs doublet model

    H. E. Logan and U. Nierste, “B s,d →ℓ +ℓ− in a two Higgs doublet model”,Nucl. Phys. B 586(2000) 39,doi:10.1016/S0550-3213(00)00417-X,arXiv:hep-ph/0004139. 26

  45. [45]

    Updated NNLO QCD predictions for the weak radiative B-meson decays

    M. Misiak et al., “Updated NNLO QCD predictions for the weak radiative B-meson decays”,Phys. Rev. Lett.114(2015) 221801, doi:10.1103/PhysRevLett.114.221801,arXiv:1503.01789

  46. [46]

    Measurement of theB 0 s →µ +µ− branching fraction and search for B0 →µ +µ− with the CMS experiment

    CMS Collaboration, “Measurement of theB 0 s →µ +µ− branching fraction and search for B0 →µ +µ− with the CMS experiment”,Phys. Rev. Lett.111(2013) 101804, doi:10.1103/PhysRevLett.111.101804,arXiv:1307.5025

  47. [47]

    Dark matter through the axion portal

    Y. Nomura and J. Thaler, “Dark matter through the axion portal”,Phys. Rev. D79(2009) 075008,doi:10.1103/PhysRevD.79.075008,arXiv:0810.5397

  48. [48]

    Simplified models for dark matter face their consistent completions

    D. Goncalves, P . A. N. Machado, and J. M. No, “Simplified models for dark matter face their consistent completions”,Phys. Rev. D95(2017) 055027, doi:10.1103/PhysRevD.95.055027,arXiv:1611.04593

  49. [49]

    Looking through the pseudoscalar portal into dark matter: Novel mono-Higgs and mono-Z signatures at the LHC

    J. M. No, “Looking through the pseudoscalar portal into dark matter: Novel mono-Higgs and mono-Z signatures at the LHC”,Phys. Rev. D93(2016) 031701, doi:10.1103/PhysRevD.93.031701,arXiv:1509.01110

  50. [50]

    Theory and phenomenology of two-Higgs-doublet models

    G. C. Branco et al., “Theory and phenomenology of two-Higgs-doublet models”,Phys. Rept.516(2012) 1,doi:10.1016/j.physrep.2012.02.002,arXiv:1106.0034

  51. [51]

    Simplified dark matter models with two Higgs doublets: I. Pseudoscalar mediators

    M. Bauer, U. Haisch, and F. Kahlhoefer, “Simplified dark matter models with two Higgs doublets: I. Pseudoscalar mediators”,JHEP05(2017) 138, doi:10.1007/JHEP05(2017)138,arXiv:1701.07427

  52. [52]

    Next-generation spin-0 dark matter models

    LHC Dark Matter Working Group, “Next-generation spin-0 dark matter models”,Phys. Dark Univ.27(2020) 100351,doi:10.1016/j.dark.2019.100351, arXiv:1810.09420

  53. [53]

    HEPData record for this analysis, 2025.doi:10.17182/hepdata.157541

  54. [54]

    The CMS experiment at the CERN LHC

    CMS Collaboration, “The CMS experiment at the CERN LHC”,JINST3(2008) S08004, doi:10.1088/1748-0221/3/08/S08004

  55. [55]

    Performance of the CMS level-1 trigger in proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Performance of the CMS level-1 trigger in proton-proton collisions at √s=13 TeV”,JINST15(2020) P10017, doi:10.1088/1748-0221/15/10/P10017,arXiv:2006.10165

  56. [56]

    The CMS trigger system

    CMS Collaboration, “The CMS trigger system”,JINST12(2017) P01020, doi:10.1088/1748-0221/12/01/P01020,arXiv:1609.02366

  57. [57]

    The automated computation of tree-level and next-to-leading order differential cross sections, and their matching to parton shower simulations

    J. Alwall et al., “The automated computation of tree-level and next-to-leading order differential cross sections, and their matching to parton shower simulations”,JHEP07 (2014) 079,doi:10.1007/JHEP07(2014)079,arXiv:1405.0301

  58. [58]

    Merging meets matching in MC@NLO

    R. Frederix and S. Frixione, “Merging meets matching in MC@NLO”,JHEP12(2012) 061,doi:10.1007/JHEP12(2012)061,arXiv:1209.6215

  59. [59]

    Matching NLO QCD computations with Parton Shower simulations: The POWHEG method

    S. Frixione, P . Nason, and C. Oleari, “Matching NLO QCD computations with Parton Shower simulations: The POWHEG method”,JHEP11(2007) 070, doi:10.1088/1126-6708/2007/11/070,arXiv:0709.2092

  60. [60]

    A general framework for implementing NLO calculations in shower Monte Carlo programs: The POWHEG BOX

    S. Alioli, P . Nason, C. Oleari, and E. Re, “A general framework for implementing NLO calculations in shower Monte Carlo programs: The POWHEG BOX”,JHEP06(2010) 043,doi:10.1007/JHEP06(2010)043,arXiv:1002.2581. References 27

  61. [61]

    Combining QCD and electroweak corrections to dilepton production in FEWZ

    Y. Li and F. Petriello, “Combining QCD and electroweak corrections to dilepton production in FEWZ”,Phys. Rev. D86(2012) 094034, doi:10.1103/PhysRevD.86.094034,arXiv:1208.5967

  62. [62]

    Top++: A program for the calculation of the top-pair cross-section at hadron colliders

    M. Czakon and A. Mitov, “Top++: A program for the calculation of the top-pair cross-section at hadron colliders”,Comput. Phys. Commun.185(2014) 2930, doi:10.1016/j.cpc.2014.06.021,arXiv:1112.5675

  63. [63]

    Two-loop soft anomalous dimensions for single top quark associated production with a W− or H−

    N. Kidonakis, “Two-loop soft anomalous dimensions for single top quark associated production with a W− or H−”,Phys. Rev. D82(2010) 054018, doi:10.1103/PhysRevD.82.054018,arXiv:1005.4451

  64. [64]

    Vector boson pair production at the LHC

    J. M. Campbell, R. K. Ellis, and C. Williams, “Vector boson pair production at the LHC”, JHEP07(2011) 018,doi:10.1007/JHEP07(2011)018,arXiv:1105.0020

  65. [65]

    Top-pair production at the LHC through NNLO QCD and NLO EW

    M. Czakon et al., “Top-pair production at the LHC through NNLO QCD and NLO EW”,JHEP10(2017) 186,doi:10.1007/JHEP10(2017)186,arXiv:1705.04105

  66. [66]

    Fully differential NNLO computations with MATRIX

    M. Grazzini, S. Kallweit, and M. Wiesemann, “Fully differential NNLO computations with MATRIX”,Eur. Phys. J. C78(2018) 537, doi:10.1140/epjc/s10052-018-5771-7,arXiv:1711.06631

  67. [67]

    Measurement of the inclusive and differential WZ production cross sections, polarization angles, and triple gauge couplings in pp collisions at√s=13 TeV

    CMS Collaboration, “Measurement of the inclusive and differential WZ production cross sections, polarization angles, and triple gauge couplings in pp collisions at√s=13 TeV”,JHEP07(2022) 032,doi:10.1007/JHEP07(2022)032, arXiv:2110.11231

  68. [68]

    Parton distributions from high-precision collider data

    NNPDF Collaboration, “Parton distributions from high-precision collider data”,Eur. Phys. J. C77(2017) 663,doi:10.1140/epjc/s10052-017-5199-5, arXiv:1706.00428

  69. [69]

    An introduction to pythia 8.2

    T. Sj ¨ostrand et al., “An introduction to pythia 8.2”,Comput. Phys. Commun.191(2015) 159,doi:10.1016/j.cpc.2015.01.024,arXiv:1410.3012

  70. [70]

    Extraction and validation of a new set of CMSPYTHIA8 tunes from underlying-event measurements

    CMS Collaboration, “Extraction and validation of a new set of CMSPYTHIA8 tunes from underlying-event measurements”,Eur. Phys. J. C80(2020) 4, doi:10.1140/epjc/s10052-019-7499-4,arXiv:1903.12179

  71. [71]

    GEANT4–a simulation toolkit

    GEANT4 Collaboration, “GEANT4–a simulation toolkit”,Nucl. Instrum. Meth. A506 (2003) 250,doi:10.1016/S0168-9002(03)01368-8

  72. [72]

    Particle-flow reconstruction and global event description with the CMS detector

    CMS Collaboration, “Particle-flow reconstruction and global event description with the CMS detector”,JINST12(2017) P10003,doi:10.1088/1748-0221/12/10/P10003, arXiv:1706.04965

  73. [73]

    Technical proposal for the phase-II upgrade of the CMS detector

    CMS Collaboration, “Technical proposal for the phase-II upgrade of the CMS detector”, technical report, 2015.doi:10.17181/CERN.VU8I.D59J

  74. [74]

    Electron and photon reconstruction and identification with the CMS experiment at the CERN LHC

    CMS Collaboration, “Electron and photon reconstruction and identification with the CMS experiment at the CERN LHC”,JINST16(2021) P05014, doi:10.1088/1748-0221/16/05/P05014,arXiv:2012.06888

  75. [75]

    Performance of the CMS muon detector and muon reconstruction with proton-proton collisions at √s=13 TeV

    CMS Collaboration, “Performance of the CMS muon detector and muon reconstruction with proton-proton collisions at √s=13 TeV”,JINST13(2018) P06015, doi:10.1088/1748-0221/13/06/P06015,arXiv:1804.04528. 28

  76. [76]

    The anti-kT jet clustering algorithm

    M. Cacciari, G. P . Salam, and G. Soyez, “The anti-kT jet clustering algorithm”,JHEP04 (2008) 063,doi:10.1088/1126-6708/2008/04/063,arXiv:0802.1189

  77. [77]

    FastJet user manual

    M. Cacciari, G. P . Salam, and G. Soyez, “FastJet user manual”,Eur. Phys. J. C72(2012) 1896,doi:10.1140/epjc/s10052-012-1896-2,arXiv:1111.6097

  78. [78]

    Dispelling theN 3 myth for thek T jet-finder

    M. Cacciari and G. P . Salam, “Dispelling theN 3 myth for thek T jet-finder”,Phys. Lett. B 641(2006) 57,doi:10.1016/j.physletb.2006.08.037, arXiv:hep-ph/0512210

  79. [79]

    Jet energy scale and resolution in the CMS experiment in pp collisions at 8 TeV

    CMS Collaboration, “Jet energy scale and resolution in the CMS experiment in pp collisions at 8 TeV”,JINST12(2017) P02014, doi:10.1088/1748-0221/12/02/P02014,arXiv:1607.03663

  80. [80]

    Pileup mitigation at CMS in 13 TeV data

    CMS Collaboration, “Pileup mitigation at CMS in 13 TeV data”,JINST15(2020) P09018, doi:10.1088/1748-0221/15/09/P09018,arXiv:2003.00503

Showing first 80 references.