Pith.

High Energy Physics - Phenomenology · arXiv:1309.3561 v2 · submitted 13 Sep 2013 · 64 references

Constraining Higgs mediated dark matter interactions

Admir Greljo, J. Julio, Jernej F. Kamenik, Christopher Smith, Jure Zupan

The paper says

“We perform an analysis of Higgs portal models of dark matter (DM), where DM is light enough to contribute to invisible Higgs decays.”

more of the abstract

Using effective field theory we show that DM can be a thermal relic only if there are additional light particles present with masses below a few 100 GeV. We give three concrete examples of viable Higgs portal models of light DM: (i) the SM extended by DM scalar along with an electroweak triplet and a singlet, (ii) a Two Higgs Doublet Model of type II with additional scalar DM, (iii) SM with DM and an extra scalar singlet that is lighter than DM. In all three examples the Br(h to invisible) constraint is not too restrictive, because it is governed by different parameters than the relic abundance. Additional light particles can have implications for flavor violation and collider searches.

from the abstract

Pith says

Machine review · deepseek-v4.1-flash · 14 Nov 2026 · what was read was not recorded · not checked by a person

Reviewed in 2026 with later literature in view.

It can be wrong. Challenge this review or reply to it.

Holds up, with conditions. A careful, correct power-counting argument plus three worked models; the abstract's 'only if' is a touch stronger than the derivation, but nothing load-bearing is wrong. This line is wrong

This review says the paper's mathematics is wrong. Pith did not check that against the paper's source.

7 minor

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Not checked: figures, code, what the 64 references say.

7 minor objections

The paper says, at Abstract (s1) and Section V

Pith says: minor objection 1 of 7

The abstract states without qualification that DM can be a thermal relic 'only if' additional light particles are present, whereas the derivation in Section II assumes O(1) Wilson coefficients and no cancellations, and the conclusions qualify the result as holding 'barring fine-tuned situations'. Since the three models of Section IV are precisely realizations of the loophole (small gSSh in model (ii), a light h2 in model (iii)), the abstract would be more accurate if it carried the O(1)-coupling qualifier explicitly.

The paper says, at Section IV C, Fig. 8

Pith says: minor objection 2 of 7

The text assumes mh1/2 > mS > mh2 with mh1 = 125 GeV, i.e. mS < 62.5 GeV, but Fig. 8 plots the relic-density coupling λp for mDM up to 80 GeV. If the curve is shown beyond the region where h1→SS is kinematically open, the text should say so and state that the invisible-width discussion applies only for mS < 62.5 GeV; otherwise the figure range contradicts the stated assumption.

show 5 more

The paper says, at Section IV C, Eq. (44)

Pith says: minor objection 3 of 7

The factor cos²α multiplying B(h1→SS) in the invisible-width χ² is not explained and appears inconsistent with Eq. (43), where B(h1→SS) already enters the physical branching ratio through ΔB̂. The authors should clarify whether B(h1→SS) is defined before or after the h–φ mixing, and make Eqs. (43) and (44) consistent.

The paper says, at Section III, Eq. (8)

Pith says: minor objection 4 of 7

The statement that the operators in Eq. (8) are excluded by the combination of Z→invisible and direct detection is somewhat trivially true for mDM > 17 GeV, where the three-body decay h→DM DM Z is kinematically forbidden and B(h→invisible) vanishes identically.

more of objection 4

The logic would be clearer if the authors separated the two regimes explicitly: for mDM < 17 GeV the LEP Z→invisible bound applies, while for mDM > 17 GeV the invisible Higgs width is zero by kinematics and only direct detection is relevant.

The paper says, at Section IV A, Table I

Pith says: minor objection 5 of 7

The choice fττ = 1, fee = fμμ = 0 is made to satisfy the CMS bound mΔ > 204 GeV while still obtaining the correct relic density. This is a choice rather than a prediction, and the paper could state more explicitly that the flavor pattern is selected to evade the flavor-degenerate collider bound, and how much of the parameter space survives once the off-diagonal LFV bounds of Table I are imposed.

The paper says, at Section IV B, Eq. (31)–(32)

Pith says: minor objection 6 of 7

The tuning of tanβ to make σSIp vanish is acknowledged as an ad-hoc feature, but the paper could quantify how much tuning is required, for example the range of tanβ around 0.61 that keeps σSIp below the XENON100 bound for the benchmark mH = 200 GeV and mS = 40 GeV.

The paper says, at Notation

Pith says: minor objection 7 of 7

The manuscript uses both B(h→invisible) and Br(h→invisible) for the same quantity; standardizing the notation would improve readability.

What would settle it

Recompute the relic density and invisible width for model (i) with the flavor pattern f_ττ = 1, f_ee = f_μμ = 0, and verify that the CMS bound mΔ > 204 GeV is satisfied for the mΔ range required by the relic density. If the required mΔ falls below 204 GeV, the model is excluded and the 'viable example' claim weakens.

from the skeptic's reading

How the review went

4 readings by deepseek-v4.1-flash · 14 Nov 2026

  1. Reader holds up, with conditions confidence high
  2. Skeptic partly agrees 8 min 34 s · 24,217 tokens read, 21,564 written
  3. Editor wrote the verdict above 15 s · 25,016 tokens read, 713 written
  4. Referee minor revision: 7 minor 6 min 9 s · 24,306 tokens read, 15,160 written

Not run on this paper: the simulated authors' defence.

Pith did not check this review's objections against the paper.

The review in full

The review in brief, machine-written

The thing to know: this is the paper that closes the loophole in light Higgs-portal dark matter. Djouadi et al. had already shown the minimal portal is excluded; Greljo et al. ask whether raising the operator dimension or forbidding the two-body Higgs decay reopens it, and answer no. The key step is Section II, Eq. (6): the invisible width and the annihilation rate scale identically with the cutoff, so higher-dimensional operators make the tension worse, not better. That is a clean, correct piece of power counting, and it is the most useful result here. Section III then walks through the three-body and four-body operators, with relic-density and direct-detection numbers attached, and shows the required cutoff lands at a few hundred GeV, i.e. right where the EFT stops making sense. That is the argument, and it holds within its stated assumptions. The three models in Section IV are real work, not hand-waving: Table I's lepton-flavour bounds, the CMS triplet mass limit, the LEP mixing limit, and the global fit to the 2013 Higgs data in Appendix B are all genuine constraints, and the authors are upfront about the tuned cancellation in model (ii) and the tiny mu in model (i). Where I would push back is small. The abstract's 'only if' reads stronger than what Sections II and III deliver, since the derivation assumes order-one Wilson coefficients and no cancellations; the conclusions say 'barring fine-tuned situations', the abstract does not. That is a presentation fix, not a correctness problem. Model (i)'s flavour pattern (f_tau-tau = 1, f_ee = f_mumu = 0) is chosen to satisfy the CMS bound rather than shown to be natural, which is a fair thing for a referee to ask about but does not threaten the central message. The stress-test note is right that there is no load-bearing error here. This is for anyone working on Higgs-portal or light thermal relics, and it deserves a serious referee.

The strongest objection

The paper's central claim is conditional: it holds under the stated assumption of O(1) Wilson coefficients and no cancellations. The authors acknowledge this explicitly in the conclusions ('barring fine-tuned situations'), and the three models are presented as realizations of the loophole. The abstract's 'only if' is slightly stronger than the derivation, but the body is careful. I do not find a load-bearing error in the power-counting argument of Sections II and III, the relic-density calculations of Appendix A, or the model constructions of Section IV. The reader's concern about model (i)'s flavor pattern is a naturalness issue, not a viability issue: the paper explicitly chooses f_ττ = 1, f_ee = f_μμ = 0 to satisfy the CMS bound mΔ > 204 GeV while obtaining the correct relic density. The reader's concern about the abstract's phrasing is a presentation issue, not a correctness issue.

The paper's main technical point—that higher-dimensional operators do not relieve the tension because B_inv and <σv> scale identically with Λ—is correct as a power-counting statement. The three models are worked through with real constraints: lepton-flavour-violating bounds in Table I, CMS triplet mass limits, LEP mixing limits, and a global fit to the 2013 LHC Higgs data in Appendix B. The reader's concern about the O(1) assumption is valid but acknowledged; the abstract's 'only if' is slightly overstated, but the body is careful. The reader's concern about model (i)'s flavor pattern is a naturalness issue, not a viability issue. I do not find a load-bearing error.

The referee's report

The paper makes a useful and clearly organized contribution to the Higgs portal literature. The scaling argument of Eq. (6), showing that higher-dimensional operators cannot reconcile a thermal relic with the invisible-width bound when all coefficients are O(1), is a clean way to organize the problem, and the three worked models are well motivated and demonstrate the loophole concretely. The paper is explicit about its assumptions and about the tuning required in models (i) and (ii), and it identifies falsifiable signatures (lepton-flavor-violating decays in model (i), invisible heavy-Higgs decays and mono-jet signatures in model (ii), and four-b final states in model (iii)). The relic-density and direct-detection calculations in Appendix A use standard machinery and appear correctly implemented.

Pith's reading of the paper (a machine's summary, not the authors')

The paper asks whether dark matter lighter than half the Higgs mass can still be a thermal relic while respecting the bound on invisible Higgs decays, $B(hto text{invisible})<0.19$ at 95% CL. The naive answer is no: reproducing the observed relic density needs an order-one Higgs–dark-matter coupling, while the invisible width needs a coupling below the bottom Yukawa, roughly $0.02$. The authors test whether that verdict survives leaving the minimal renormalizable portal, checking higher-dimensional operators, three-body decays $hto text{DM},text{DM},Z$ built from the Higgs vector current, four-body decays through scalar and tensor fermion currents, and a neutrino-mass-like Weinberg operator. In every case the invisible width and the annihilation rate scale with the same power of the effective cutoff, so the relic density pushes that cutoff down to a few hundred GeV, precisely where the effective description stops making sense. The conclusion is that viable light Higgs-portal dark matter requires additional particles below a few hundred GeV, and the authors exhibit three models in which the parameter controlling the relic abundance is not the one controlling the invisible width.

What carries the argument. The load-bearing device is a scaling comparison. Writing the dark-matter–Higgs interaction as an operator of dimension $4+n$ suppressed by $Lambda^n$, the authors show that the invisible branching ratio scales as $10^3 (m_h/Lambda)^{2n}$ while the annihilation cross section scales as $y_f^2 (m_h/Lambda)^{2n} (m_{text{DM}}/m_h)^k / m_h^2$, with the same power of $Lambda$ in both. Dividing the two, the relic-density requirement fixes the ratio of the two observables up to mass-suppression factors that only make the Higgs constraint stronger, so no choice of operator dimension reconciles them. The second device is model construction: in each of the three examples the coupling that enters $B(h to text{invisible})$ differs from the combination that enters $langle sigma v rangle$ — for instance $lambda_S1 sin alpha cos beta - lambda_S2 cos alpha sin beta$ versus $-lambda_S1 cos alpha cos beta - lambda_S2 sin alpha sin beta$ in the two-Higgs-doublet case, and $lambda_6 cos^2alpha + lambda_5 sin^2alpha$ versus $lambda_5 cos alpha - lambda_6 sin alpha$ in the two-singlet case — so the invisible width can be dialled below the bound while the relic abundance stays fixed.

Core claim. Within an effective field theory containing only the Standard Model and a single dark-matter field, light dark matter cannot be a thermal relic: the coupling needed for the correct relic density inevitably produces an invisible Higgs branching ratio above the experimental bound, and raising the operator dimension does not help because $B(h to text{invisible})$ and $langle sigma_{text{ann}} v rangle$ carry the same suppression in the cutoff $Lambda$. The authors show the same obstruction applies when two-body $h to text{DM},text{DM}$ is forbidden and decays proceed through the Higgs vector current (three-body, excluded by $Z$ invisible width and direct detection), through scalar or tensor fermion currents (four-body, requiring $Lambda lesssim 600$ GeV), or through the Weinberg-like leptonic operator (requiring $Lambda simeq 300$ GeV for $m_{text{DM}}=40$ GeV). The escape is a dark sector with extra light states, which the paper demonstrates with three explicit models: the Standard Model plus a Dirac dark fermion, an electroweak triplet and a singlet; a type-II two-Higgs-doublet model with a singlet scalar dark matter candidate; and the Standard Model plus dark matter and a singlet scalar lighter than the dark matter.

The premise it rests on. The exclusion rests on every dimensionless coupling being of order one and on no accidental cancellations between contributions, a premise the authors state themselves and then deliberately circumvent in their own three viable models by arranging a hierarchy or a cancellation.

If the paper is right (Pith's inferences, not the authors')

If an invisible Higgs branching ratio at the few-tens-of-percent level is established, the dark matter cannot be a thermal relic unless its abundance is set by interactions that do not involve the Higgs field.

Any viable Higgs-portal thermal relic lighter than $m_h/2$ implies additional states with masses of a few hundred GeV or below, which places them within reach of the LHC rather than beyond it.

In the triplet-plus-singlet model the same couplings that fix the relic density induce charged-scalar exchange, so lepton-flavour-violating processes such as $mu^- to e^+e^-e^-$ and $mu to e gamma$ are predicted at rates the current bounds already constrain tightly.

In the two-Higgs-doublet variant the heavy CP-even scalar decays almost entirely invisibly, giving $tbar t$ plus missing energy and mono-jet signatures that can be searched for at the LHC.

In the two-singlet model the 125 GeV Higgs can decay into two light scalars at the level of about twenty percent, producing four $b$-jets that may originate from displaced vertices.

The abstract's 'only if' is more precisely 'only if, unless couplings are tuned small or two contributions cancel'; since the paper's own three examples are exactly such tunings, the result reads as a naturalness statement about the Higgs portal rather than a theorem about all possible portals.

Because the extra light states are what makes the portal work, an eventual invisible Higgs signal would point to a multi-state dark sector rather than a single dark particle, which changes what collider searches should be looking for.

If no invisible Higgs decay appears and direct detection remains null, the surviving corner is the tuned-cancellation region, where the heavy-scalar mixing angle and the dark-matter mass are the only handles — a target for precision Higgs coupling fits rather than for direct searches.

The leptophilic route ties Higgs-portal dark matter to neutrino mass generation, and the extremely small lepton-number-breaking parameter it requires, $mu lesssim 1$ eV, is itself a structural feature that future neutrino and flavour experiments could test.

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The paper

Abstract

We perform an analysis of Higgs portal models of dark matter (DM), where DM is light enough to contribute to invisible Higgs decays. Using effective field theory we show that DM can be a thermal relic only if there are additional light particles present with masses below a few 100 GeV. We give three concrete examples of viable Higgs portal models of light DM: (i) the SM extended by DM scalar along with an electroweak triplet and a singlet, (ii) a Two Higgs Doublet Model of type II with additional scalar DM, (iii) SM with DM and an extra scalar singlet that is lighter than DM. In all three examples the Br(h to invisible) constraint is not too restrictive, because it is governed by different parameters than the relic abundance. Additional light particles can have implications for flavor violation and collider searches.

The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. No sentence in this record was written by a model.

abstract compiled · 2026-09-23

The authors' main claim, as the classifier picked it out 1.00

“Using effective field theory we show that DM can be a thermal relic only if there are additional light particles present with masses below a few 100 GeV.”

How the main claim is stated: asserted 0.96

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.44 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.79 · compares with prior results 0.08 · mentions code or data availability 0.02

The abstract, sentence by sentence

This table labels the abstract only (arXiv listing abstract v2). The number is the probability the classifier gave the label.

SentenceRoleThe authors' own workStates the main conclusionStrength
We perform an analysis of Higgs portal models of dark matter (DM), where DM is light enough to contribute to invisible Higgs decays. contribution 0.94 0.86 0.04 asserted 0.96
Using effective field theory we show that DM can be a thermal relic only if there are additional light particles present with masses below a few 100 GeV. result 0.99 0.90 0.61 asserted 0.96
We give three concrete examples of viable Higgs portal models of light DM: (i) the SM extended by DM scalar along with an electroweak triplet and a singlet, (ii) a Two Higgs Doublet Model of type II with additional scalar DM, (iii) SM with DM and an extra scalar singlet that is lighter than DM. contribution 0.79 0.82 0.15 asserted 1.00
In all three examples the Br(h to invisible) constraint is not too restrictive, because it is governed by different parameters than the relic abundance. result 0.58 0.79 0.30 asserted 0.99
Additional light particles can have implications for flavor violation and collider searches. interpretation 0.98 0.23 0.06 hedged possibility 0.91

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.85

What was examined, and what was not

Sources read

  • arXiv listing abstract v2

Not examined

  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers

Levels run

  • P abstract

Not run

  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

How the labels were made

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,333 input tokens, $0.0002 reported.

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. This record as JSON

Figures (9)
Figure 1 of the paper
Figure 1. The spin independent DM-nucleon cross sections (dashed-blue) induced by Higgs vector current
Figure 2 of the paper
Figure 2. The DM-nucleon cross sections (dashed-blue) induced by operators (
Figure 3 of the paper
Figure 3. The b ¯b (blue) and τ +τ − (red) annihilation cross-sections (hσvi) for the fermionic operators in (10) (upper two panels) and for fermionic DM with axial vector coupling to Higgs vector current in (8) (c V ψ = 0). The continuous (dashed) lines indicate the present experimental upper bounds [26, 27] (predicted values assuming correct DM relic density) on hσvi. which is not excluded by direct detection. It demonstrates that for Z mediated channels, the constraints from indirect detection are not as significant. The reason lies in the assumed flavor structure. This is fixed for opera
Figure 4 of the paper
Figure 4. The dependence of the EFT cut-off scale Λ for scalar (blued dashed line) and tensor (green dotted
Figure 5 of the paper
Figure 5. The dependence on mDM of the parameter m∆ (red solid line) in the SM + DM model with an extra triplet and a singlet Lagrangian (17) for which proper relic density is obtained. The masses of physical φ − ∆0 mixed states, m1,2 are shown as blue dashed and green dotted lines. Other inputs in (17) are set to fab = y = λ = 1 with mφ = m∆. by either ∆+ or ∆++ particles, with the rate Γ(`a → `bγ) = m5 `a αem (24π 2) 2 (f † f) 2 ab  1 8m2 ∆+ + 1 m2 ∆++ 2 , (20) where αem is the QED fine-structure constant. The ` − a → ` + b ` − c ` − d decay can proceed through tree-level ∆++ exchange,…
Figure 6 of the paper
Figure 6. The value of gSSH that gives the observed DM relic density in 2HDM-II models with extra singlet, as function of DM mass, mDM, for the case where the invisible decay width of the Higgs and the DM-proton scattering cross section both vanish. Two choices of the heavy CP-even Higgs mass, mH = 200, 300 GeV are shown. where cu,c,t = gSSh(mH/mh) 2 cos α csc β + gSSH sin α csc β, cd,s,b = −gSSh(mH/mh) 2 sin α sec β + gSSH cos α sec β , (30) while the relevant nuclear form factors f p q are listed in Eq. (A7) . The h and H contributions may interfere destructively. In fact, σ SI p vanishes…
Figure 7 of the paper
Figure 7. The 68.3% and 95.5% C.L. parameter regions in 2HDM-II with an extra singlet that are allowed by the Higgs signal strength data are shown in dark grey and light grey, respectively. Orange-dashed curve correspond to β − α = π/2. Black-dashed curve correspond to Eq. (32). The 95.5% C.L. region allowed by the Higgs data together with direct DM detection bound from XENON100 is shown in cyan. For definiteness we assume mH = 200 GeV, mS = 40 GeV and gSSH such that the proper DM thermal relic is obtained. Higgs boson masses, mH = 200, 300 GeV. We also set tan β = 0.61 such that σ SI p…
Figure 8 of the paper
Figure 8. Coupling λp for which the proper relic abundance is obtained in the model with an extra scalar singlet (37). sin α also has to be greater than 10−8 , otherwise h2 is sufficiently long lived that it escapes the detector. For sin α ∼ 10−4 the h2 particle travels less than a few µm before decaying and can be searched for using displaced vertices. Note that the branching ratios of h2 are not affected by sin α and are the same as they would be for the SM Higgs with mh2 mass. For instance, for mh2 = 20 GeV the dominant branching ratio is B(h2 → b ¯b) ∼ 85%. The relic abundance is set by…
Figure 9 of the paper
Figure 9. Constraints from Higgs signal strengths of the Higgs portal model of light DM with an extra

Figures are the authors', reproduced from the paper.

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Cited by 22 Pith papers

Reviewed papers on Pith that cite this one. The full citation record

  1. On the Direct Detection of Dark Matter Annihilation hep-ph · Jan 2015
  2. Self-Interacting Dark Matter through the Higgs Portal hep-ph · Nov 2014
  3. Connecting Dark Matter UV Complete Models to Direct Detection Rates via Effective Field Theory hep-ph · Nov 2014
  4. Benchmarks for Dark Matter Searches at the LHC hep-ph · Feb 2014
  5. New Constraints on Dark Matter Effective Theories from Standard Model Loops hep-ph · Feb 2014
  6. Direct Detection Portals for Self-interacting Dark Matter hep-ph · Oct 2013
  7. Combined analysis of effective Higgs portal dark matter models hep-ph · Dec 2015
  8. Asymmetric Dark Matter Stars hep-ph · Jul 2015
  9. Integrating in the Higgs Portal to Fermion Dark Matter hep-ph · Jun 2015
  10. Nonstandard Yukawa Couplings and Higgs Portal Dark Matter hep-ph · Apr 2015
  11. The Flavour Portal to Dark Matter hep-ph · Jan 2015
  12. Classification of effective operators for interactions between the Standard Model and dark matter hep-ph · Dec 2014
  13. Scalar Simplified Models for Dark Matter hep-ph · Oct 2014
  14. The Fermionic Dark Matter Higgs Portal: an effective field theory approach hep-ph · Apr 2014
  15. Mono-Higgs Detection of Dark Matter at the LHC hep-ph · Feb 2014
  16. Towards Completing the Standard Model: Vacuum Stability, EWSB and Dark Matter hep-ph · Sep 2013
  17. Self-interacting dark matter and cosmology of a light scalar mediator hep-ph · Jul 2015
  18. Searching for Vector Dark Matter by Higgs Portal at the LHC hep-ph · Jul 2015
  19. Pseudoscalar Portal Dark Matter hep-ph · Feb 2015
  20. A Possible Explanation of Low Energy $\gamma$-ray Excess from Galactic Centre and Fermi Bubble by a Dark Matter Model with Two Real Scalars hep-ph · Dec 2013
  21. The Waning of the WIMP? A Review of Models, Searches, and Constraints hep-ph · Mar 2017
  22. Simplified Models vs. Effective Field Theory Approaches in Dark Matter Searches hep-ph · Mar 2016

Topics: Dark Matter, Dark Matter

How the literature uses it

27 arXiv papers cite this in 35 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 23 sentences without a confident label

Cites it as background 11 papers

What it cites · 23 sentences without a confident label

Uses the method or tool of 4 papers
Uses data or values from 8 papers
Compares with 2 papers
Cites as background 4 papers

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