High Energy Physics - Phenomenology · arXiv:1608.05345 v1 · submitted 18 Aug 2016 · 71 references
Forbidden Dark Matter at the Weak Scale via the Top Portal
The paper says
“At the tail of its velocity distribution, cold dark matter (DM) can annihilate at finite temperature to states heavier than itself. We explore the possibility that DM freezeout is dictated by these "forbidden annihilations" at the electroweak scale.”
more of the abstract
Demanding that annihilation products be Standard Model particles, we find that for the forbidden mechanism to primarily set the DM relic abundance, DM must couple predominantly, if not solely, to top quarks. This can be arranged by invoking a non-trivial flavor structure such as Minimal Flavor Violation. We avail two avenues to achieve the correct thermal cross-section, requiring a mediator exchanged in the s- or t-channel. These simplified models submit easily to direct detection and collider searches, and necessarily hide from indirect detection signals. Viable supersymmetric spectra involving the forbidden mechanism may be found if combined with co-annihilation.
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, honest simplified-model study of weak-scale forbidden DM; the top-portal uniqueness claim is an elimination argument, and the bottom-portal paragraph has a real numerical error in the LEP reach. This line is wrong
1 major objection · 8 minor
How often objections from reviews like this one are right: not yet measured
Not checked: figures, code, what the 71 references say.
The paper says, at Sec. II.2 (light-fermions bullet) and Sec. III.2 (bottom-portal paragraph)
The review did not quote this passage.
Pith says: Objection 1 of 1 · major
The LEP reach on t-channel mediators is quoted as 10^4 GeV in two places: Sec. II.2 states that 't-channel mediators of mass ≤ 10^4 GeV would have been seen at LEP searches [29,30]', and Sec. III.2 sets m_~B = 10^4 GeV as 'the edge of the LEP limit'.
more of objection 1
The actual LEP reach on pair-produced colored or charged mediators is of order 10^2 GeV, not 10^4 GeV. This is not a cosmetic slip: the bottom-portal viability estimate (m_DM = 4.0 GeV for Majorana fermion DM, 3.95 GeV for real scalar DM) is derived with m_~B = 10^4 GeV, and the t-channel cross-section scales as 1/m_~B^4. With the correct LEP edge, the annihilation rate is many orders of magnitude larger, the required m_DM moves further from m_b, and the viable window is correspondingly wider. The statement that 'the range of parameters where this scenario is viable is very limited' is therefore not supported by the calculation as presented. Because the bottom portal is the one surviving exception to the paper's elimination argument, this error weakens the abstract's claim that DM 'must couple predominantly, if not solely, to top quarks'. The authors should redo the bottom-portal estimate with the correct LEP reach, or explicitly soften the universality claim.
8 minor objections
The paper says, at Sec. III.1
Pith says: minor objection 1 of 8
The perturbativity bound λ ≤ 1.12 is an estimate based on requiring v/Λ ≤ 1/10 in the UV operator c H φ Qbar_3 t^c/Λ, and the quoted allowed ranges (m_DM ∈ [145, 170] GeV, m_MED ∈ [175, 725] GeV) depend on this choice. The paper should show how the allowed region in Fig. 3 changes if v/Λ is varied, or state the ranges as indicative rather than definite.
The paper says, at Sec. III.3 and abstract
Pith says: minor objection 2 of 8
The abstract states that the models 'necessarily hide from indirect detection signals'. The argument in Sec. III.3 is qualitative: the loop-induced channels are asserted to be 'highly sub-dominant' without a calculation. The paper should quantify the dominant loop-induced channel (e.g. gg or γγ) at the relevant DM mass to support the 'necessarily' claim, or soften the wording.
show 6 more
The paper says, at Sec. III.2, Eq. (3) and the line preceding it
Pith says: minor objection 3 of 8
The formula for the scalar spin-independent cross-section is written as σ^scal_SI ∼ λ^4 m_N^4 m_DM^2/m_MED^4, which has the wrong mass dimension; it should be λ^4 m_N^4/(m_DM^2 m_MED^4) to match Eq. (3) and the derivation from Eq. (B13). The typo should be corrected.
The paper says, at Sec. III.1 and Fig. 3
Pith says: minor objection 4 of 8
The monojet limit is obtained by recasting an EFT analysis, and the authors acknowledge that the EFT is inaccurate for m_MED < 450 GeV because the /ET > 450 GeV cut sends the propagator off-shell. The blue curve in Fig. 3 lies in this region.
more of objection 4
The conclusion that the s-channel model is 'mostly unconstrained' is robust because the true limit is weaker, but the figure should state explicitly that the EFT curve is an upper bound on the reach rather than a true limit.
The paper says, at Sec. III.4 and Fig. 5
Pith says: minor objection 5 of 8
The three-body check is illustrated at a single parameter point (λ = 1, m_MED = 180 GeV), which lies in the region excluded by LHC stop searches. The statement that the two-body channel dominates 'for all combinations of λ, m_MED and models considered here' would be better supported by showing the ratio of three-body to two-body cross-sections across the allowed parameter space, or at least by stating the scaling with λ and m_MED.
The paper says, at Sec. II.2
Pith says: minor objection 6 of 8
The statement that 'no searches have substantially excluded a top portal DM and its mediators' is somewhat strong given that the paper itself finds significant exclusions in the t-channel models from stop searches and direct detection. The wording should be qualified.
The paper says, at Sec. IV
Pith says: minor objection 7 of 8
The phrase 'priorly' is not a word and should be replaced by 'previously'. The sentence 'Consider a bino LSP will all other electroweakinos decoupled' should read 'with' rather than 'will'. The closing metaphor 'a significant stone to turn in the WIMP paradigm' is awkward and could be simplified.
The paper says, at Table I
Pith says: minor objection 8 of 8
The column layout of Table I is difficult to parse: the spin entries for the t-channel and s-channel mediators are not clearly separated from the gauge and Z2 quantum numbers. A clearer column structure would help the reader.
What would settle it
Recompute the bottom-portal relic density using the t-channel scalar formula (B12) with m_t → m_b = 4.2 GeV, λ = 3, and (i) m_B = 10^2 GeV and (ii) m_B = 10^4 GeV. Determine which value reproduces the quoted m_DM = 3.95 GeV. Independently, check the LEP limit on a pair-produced b-squark-like colored scalar: if the limit is ~10^2 GeV, the text's '10^4 GeV is the edge of the LEP limit' is wrong and the viable window must be re-derived; if the quoted m_DM matches 10^2 GeV rather than 10^4 GeV, the text contains a typo but the physics stands.
from the skeptic's reading
How the review went
4 readings by deepseek-v4.1-flash · 14 Nov 2026
- Reader holds up, with conditions
- Skeptic partly agrees
- Editor wrote the verdict above
- Referee major revision: 1 major objection, 8 minor
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 worth knowing: this is a competent, well-executed simplified-model paper. Forbidden annihilation has been around since Griest–Seckel, and the detailed-balance relic calculation follows D'Agnolo–Ruderman, but nobody had done the weak-scale version with SM final states. The authors do that, argue by elimination that the top quark is the only portal, and build two explicit models (s-channel pseudoscalar, t-channel scalar or fermion mediator) with relic density, monojet, stop-search, and direct-detection constraints all mapped on the same mDM–mMED plane. Appendix B gives explicit a and b coefficients, which is what makes the paper reusable. The relic calculation is cross-checked against MicrOmegas. The observation that forbidden WIMPs are structurally the opposite of secluded WIMPs — colliders and direct detection instead of indirect detection — is a genuinely useful framing point, and the indirect-detection immunity argument holds up on reading it (abstract:s2 is the claim; Sec. III.3 is the support). The paper is also unusually candid about its own approximations, which I count in its favor rather than against it: the EFT monojet recasting is flagged as crude, the Taylor expansion near the pole is marked with dashed lines, and the perturbativity bound is presented as an estimate. Those are acknowledged limitations, not new findings, and I would not hold them against the paper beyond what the authors already say. Soft spots, in order of how much they matter. First, the bottom-portal paragraph at the end of Sec. III.2 has a real error: it sets m_~B = 104 GeV and calls it 'the edge of the LEP limit.' LEP's reach on pair-produced colored mediators in missing-energy is O(100 GeV), not 10 TeV, and the same 104 GeV number appears in Sec. II.2 as the reason light-fermion mediators are excluded. If the true edge is ~100 GeV, the bottom portal has a much wider window than the quoted m_DM ≈ 4.0 GeV, and the 'must couple to top' claim is correspondingly softer. One correction to the stress-test note: its second point — that 104 GeV minimizes rather than maximizes the cross-section — does not land, because given the paper's (wrong) LEP premise, 104 GeV is the smallest allowed mass and hence does maximize. The error is the LEP number, not the logic. Second, the λ ≤ 1.12 perturbativity bound rests on v/Λ ≤ 1/10; the authors say so, but it moves the boundary of Fig. 3 and the quoted allowed ranges, so it is worth a sentence of scrutiny. Who should read it: anyone working on non-standard freezeout or simplified DM models with top couplings. It is a solid reference point. Recommendation: send it out. The bottom-portal error needs fixing, but it is a paragraph the authors already say they do not pursue, and the core construction stands.
The strongest objection
The paper's headline claim (abstract:s2) is that forbidden annihilation 'requires' DM to couple predominantly to top quarks. This is an argument by elimination (Sec. II.2), and the one surviving exception is the bottom portal, discussed at the end of Sec. III.2. That discussion sets m_B = 10^4 GeV, calling it 'the edge of the LEP limit,' and states this choice 'maximizes the forbidden annihilation cross-section.' Both statements are suspect. LEP's reach on pair-produced colored mediators is ~10^2 GeV, not 10^4 GeV, so 10^4 GeV is far above the LEP edge, not at it. Moreover, since the t-channel cross-section scales as 1/m_B^4, a smaller m_B gives a larger cross-section; setting m_B = 10^4 GeV minimizes, not maximizes, the annihilation rate. The quoted viable point (m_DM = 3.95 GeV for scalar DM) should therefore be re-derived. If the correct LEP edge is ~10^2 GeV, the bottom-portal window is different from the one quoted, and the 'must couple to top' universality is correspondingly less secure. This is not merely a typo: the elimination argument in Sec. II.2 assumes light-fermion mediators are ≤ O(10 GeV), which the paper's own 10^4 GeV example contradicts, so the two sections are in tension about how heavy a light-fermion mediator can be.
The paper is a competent simplified-model study, and the reader's verdict (CONDITIONAL) is broadly appropriate. I agree with the reader that the perturbativity bound λ ≤ 1.12 in Sec. III.1 is an estimate, not a derivation, and that it shapes the claimed s-channel parameter space. But I think the more load-bearing concern for the headline claim is the treatment of the bottom portal, because that is the one explicit exception to 'DM must couple predominantly to top quarks.' The reader's concern affects the size of the viable region; the bottom-portal concern affects whether the universality claim holds at all. The paper does acknowledge the bottom portal as a special case, so I do not present it as a new finding; what I flag is the internal tension between Sec. II.2 (light-fermion mediators ≤ O(10 GeV)) and Sec. III.2 (m_B = 10^4 GeV), together with the apparent misidentification of 10^4 GeV as the LEP edge. These are concrete and checkable. If the bottom-portal window is larger than quoted, the 'must' in abstract:s2 weakens to 'typically'; if it is smaller, the paper's conclusion is strengthened. Either way, the top-portal models themselves (Figs. 3 and 4) are unaffected, so the verdict level does not change. I also note that the paper's own caveats — the EFT monojet recasting, the Taylor-expansion breakdown near the pole, and the overestimated scalar-DM direct-detection cross-section in Appendix B — are acknowledged and appropriately scoped, so I do not count them as new concerns. The relic-density calculation (Appendix A) is standard detailed-balance and cross-checked against MicrOmegas, so I see no issue there.
The referee's report
The paper addresses an under-explored freezeout mechanism with a clear and concrete simplified-model framework. The relic-density calculation is transparent, the detailed-balance derivation in Appendix A is a useful service to the community, and the explicit a and b coefficients in Appendix B make the results reproducible. The collider and direct-detection recasts are appropriate and the models are falsifiable. The central claim that the top quark is the only viable SM portal for a principally forbidden WIMP is interesting, but it rests on an elimination argument whose one acknowledged exception, the bottom portal, is dismissed using a collider reach that appears to be misquoted by two orders of magnitude. That issue is load-bearing for the abstract's 'must couple predominantly to top quarks' and should be corrected before the paper's conclusion can be regarded as established.
Pith's reading of the paper (a machine's summary, not the authors')
Most dark matter models assume the particle annihilates into lighter things, which is why the relic abundance is tied to a simple ratio of coupling squared over mass squared. This paper asks the opposite: what if the annihilation products are heavier than the dark matter itself, so that only the fast tail of the velocity distribution can supply the energy? That 'forbidden' annihilation is Boltzmann-suppressed, so the underlying cross-section must be large to compensate. Working through every massive Standard Model final state, the authors argue that the only viable option is the top quark, because electroweak bosons and the Higgs always drag along light-fermion channels, and light fermions require mediators already excluded by LEP and di-fermion resonance searches. The payoff is a dark matter candidate a few GeV below the top mass whose abundance is set by top-quark annihilation, which makes it essentially invisible to indirect detection while remaining squarely in range of LHC stop-like searches and nuclear recoil experiments.
What carries the argument. The load-bearing device is a detailed-balance identity that converts the forbidden cross-section into the cross-section of the reverse process. Because the top quarks in the bath are in equilibrium, one can write $⟨σv⟩_{χχ→t̄t} = (g_t/g_χ)^2 (1+δ)^3 e^{-2δx} ⟨σv⟩_{t̄t→χχ}$, with $δ = (m_t - m_{DM})/m_{DM}$ and $x = m_{DM}/T$. The exponential is the Boltzmann penalty for reaching a final state heavier than the initial one; the prefactor and the reverse cross-section, Taylor-expanded as $a + b v^2$ and integrated against the thermal history, are what must be made large enough. Two mechanisms supply that size: a pseudoscalar $s$-channel mediator tuned near the $2m_t$ resonance, and a $t$-channel mediator with a coupling that simplified-model logic permits to be order one or larger. The same identity explains why the models are blind to indirect detection: at $T = 2.7$ K the exponential is vanishingly small, so the present-day annihilation rate is many orders of magnitude below the Fermi-LAT dwarf-spheroidal bound.
Core claim. The paper's central claim is that forbidden annihilation can be the principal setter of the dark matter relic abundance at the electroweak scale, and that demanding Standard Model annihilation products forces the dark matter to couple predominantly, if not solely, to top quarks. The argument proceeds by elimination: $ZZ$ and $WW$ final states always come with an $s$-channel $Z$ that also yields light fermions; Higgs final states require $m_{DM}$ within a few percent of $125$ GeV, where Higgs-portal models without parity violation are already in tension with LUX and PandaX-II; and bottom or lighter fermion final states need mediators below roughly $10$ GeV or $10^4$ GeV that would have shown up as di-fermion resonances or missing-energy signals. The top quark is what remains. The authors then build two simplified models that reach the observed $Ω_χ h^2 = 0.1197$: an $s$-channel CP-odd singlet mediator, where the enhancement comes from annihilation near the $2m_t$ pole, and a $t$-channel mediator, where the coupling $λ$ itself is allowed to be larger than one. Flavor safety is handled by Minimal Flavor Violation, so the mediator couples to fermions in proportion to Higgs Yukawas and the light-quark channels stay negligible. The resulting viable windows are $m_{DM} ∈ [145, 170]$ GeV with $m_{MED} ∈ [175, 725]$ GeV in the $s$-channel, and $m_{DM} ∈ [150, 170]$ GeV with $m_{MED}$ up to about $1000$ GeV in the $t$-channel.
The premise it rests on. The size of the allowed parameter space rests on a perturbativity estimate rather than a derivation: the authors assume the top-mediator coupling descends from an operator suppressed by a scale at least ten times the Higgs vacuum expectation value, giving $λ_t ≤ 0.1$ and hence $λ ≤ 1.12$ in the $s$-channel, and a different ultraviolet completion would move that boundary and change which masses are claimed viable.
If the paper is right (Pith's inferences, not the authors')
The $s$-channel pseudoscalar model survives the 8 TeV monojet search almost entirely, and even the 14 TeV, $3000$ fb$^{-1}$ projection only grazes its parameter space, so a forbidden WIMP of this type could be sitting just under current LHC reach.
In the $t$-channel models the mediator is QCD-produced and decays to a top plus missing energy, so existing stop searches recast directly: $m_{MED} ∈ [380, 690]$ GeV is excluded for fermionic dark matter and $m_{MED} ∈ [310, 920]$ GeV for scalar dark matter.
The scalar-dark-matter version scatters off nuclei strongly enough that LUX and PandaX-II already cover a wide band, and the residual region has a spin-independent cross-section around $2 × 10^{-45}$ cm$^2$, within reach of XENON1T.
Because the abundance is fixed by forbidden top annihilation, any loop-induced light final states are automatically far below the thermal cross-section, so the models cannot produce a detectable indirect-detection signal.
Three-body final states such as $tWb$ are shown to contribute at the ten-percent level or less for $m_{DM} \gtrsim 150$ GeV, so the two-body treatment of freezeout is adequate wherever the coupling stays perturbative.
The spectral tuning that forbidden models require — dark matter sitting a few GeV below the top — is the same kind of coincidence that co-annihilation and resonance models need, which suggests a common ultraviolet origin; a flavor symmetry tying the dark sector to the top Yukawa would be the natural place to look.
If the $t$-channel mediator is really a top-flavored scalar, the compressed region $m_{MED} \approx m_{DM} + m_t$ is the sharpest place to test the idea, since the recoil-against-ISR strategy proposed for compressed stops applies unchanged and has not yet been run as a dedicated search.
The authors note that a bino just below the top mass annihilating only through forbidden channels would overclose the universe unless a gluino sits within about ten percent in mass; this makes the gluino-bino compressed spectrum a concrete supersymmetric target that existing jets-plus-missing-energy searches are poorly suited to cover.
A cleaner experimental discriminator between the $s$- and $t$-channel versions would be the shape of the missing-energy spectrum in monojet events: the $t$-channel mediator is QCD-produced and gives harder top-associated activity, while the pseudoscalar gives the contact-operator-like monojet shape the EFT recasts assume.
Check this review
Pith stored no record of this review's passes and took no fingerprint of it. Reviews made by code from 13 Nov 2026 on carry both.
How often reviews like this one are right
Reviews like this one: written by deepseek-v4.1-flash, where what was read was not recorded.
How often objections from reviews like this one are right: not yet measured
Reviews by people
This review was written by a machine. No person has reviewed this paper on Pith yet. A scientist listed on Pith can review it for a fee, and their review is published here whatever it concludes.
The paper
Abstract
At the tail of its velocity distribution, cold dark matter (DM) can annihilate at finite temperature to states heavier than itself. We explore the possibility that DM freezeout is dictated by these "forbidden annihilations" at the electroweak scale. Demanding that annihilation products be Standard Model particles, we find that for the forbidden mechanism to primarily set the DM relic abundance, DM must couple predominantly, if not solely, to top quarks. This can be arranged by invoking a non-trivial flavor structure such as Minimal Flavor Violation. We avail two avenues to achieve the correct thermal cross-section, requiring a mediator exchanged in the s- or t-channel. These simplified models submit easily to direct detection and collider searches, and necessarily hide from indirect detection signals. Viable supersymmetric spectra involving the forbidden mechanism may be found if combined with co-annihilation.
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 0.99
“Demanding that annihilation products be Standard Model particles, we find that for the forbidden mechanism to primarily set the DM relic abundance, DM must couple predominantly, if not solely, to top quarks.”
How the main claim is stated: asserted 1.00
What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.68 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.07 · compares with prior results 0.11 · mentions code or data availability 0.02
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v1). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| At the tail of its velocity distribution, cold dark matter (DM) can annihilate at finite temperature to states heavier than itself. | background 1.00 | 0.08 | 0.04 | asserted 0.71 |
| We explore the possibility that DM freezeout is dictated by these "forbidden annihilations" at the electroweak scale. | contribution 0.98 | 0.51 | 0.11 | hedged possibility 0.88 |
| Demanding that annihilation products be Standard Model particles, we find that for the forbidden mechanism to primarily set the DM relic abundance, DM must couple predominantly, if not solely, to top quarks. | result 1.00 | 0.92 | 0.62 | asserted 1.00 |
| This can be arranged by invoking a non-trivial flavor structure such as Minimal Flavor Violation. | method 0.81 | 0.29 | 0.06 | hedged possibility 0.55 |
| We avail two avenues to achieve the correct thermal cross-section, requiring a mediator exchanged in the $s$- or $t$-channel. | method 0.78 | 0.79 | 0.08 | asserted 0.94 |
| These simplified models submit easily to direct detection and collider searches, and necessarily hide from indirect detection signals. | result 0.54 | 0.74 | 0.16 | asserted 1.00 |
| Viable supersymmetric spectra involving the forbidden mechanism may be found if combined with co-annihilation. | result 0.58 | 0.44 | 0.08 | hedged possibility 1.00 |
What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from argument 0.54
What was examined, and what was not
Sources read
- arXiv listing abstract v1
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-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 5,525 input tokens.
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 (5)
Figures are the authors', reproduced from the paper.
References (71)
- [1] B. W. Lee and S. Weinberg, Phys. Rev. Lett. 39, 165 (1977) on Pith
- [2] P. A. R. Ade et al. [Planck Collaboration], arXiv:1502.01589 [astro-ph.CO] on PithPith's reviewarXiv
- [3] J. L. Feng and J. Kumar, Phys. Rev. Lett. 101, 231301 (2008) [arXiv:0803.4196 [hep-ph]] on PithPith's reviewarXiv
- [4] F. D’Eramo and J. Thaler, JHEP 1006, 109 (2010) [arXiv:1003.5912 [hep-ph]] on PithPith's reviewarXiv
- [5] Y. Hochberg, E. Kuflik, T. Volansky and J. G. Wacker, Phys. Rev. Lett. 113, 171301 (2014) [arXiv:1402.5143 [hep-ph]] on PithPith's reviewarXiv
- [6] Y. Hochberg, E. Kuflik, H. Murayama, T. Volansky and J. G. Wacker, Phys. Rev. Lett. 115 (2015) no.2, 021301 [arXiv:1411.3727 [hep-ph]] on PithPith's reviewarXiv
- [7] K. Griest and D. Seckel, Phys. Rev. D 43, 3191 (1991) on Pith
- [8] P. Gondolo and G. Gelmini, Nucl. Phys. B 360, 145 (1991) on Pith
- [9] C. B. Jackson, G. Servant, G. Shaughnessy, T. M. P. Tait and M. Taoso, JCAP 1004, 004 (2010) [arXiv:0912.0004 [hep-ph]] on PithPith's reviewarXiv
- [10] C. B. Jackson, G. Servant, G. Shaughnessy, T. M. P. Tait and M. Taoso, JCAP1307, 021 (2013) doi:10.1088/1475- 7516/2013/07/021 [arXiv:1302.1802 [hep-ph]] on PithPith's reviewarXiv
- [11] C. B. Jackson, G. Servant, G. Shaughnessy, T. M. P. Tait and M. Taoso, JCAP 1307, 006 (2013) [arXiv:1303.4717 [hep-ph]] on PithPith's reviewarXiv
- [12] S. Tulin, H. B. Yu and K. M. Zurek, Phys. Rev. D 87, no. 3, 036011 (2013) [arXiv:1208.0009 [hep-ph]] on PithPith's reviewarXiv
- [13] R. T. D’Agnolo and J. T. Ruderman, Phys. Rev. Lett. 115, no. 6, 061301 (2015) [arXiv:1505.07107 [hep-ph]] on PithPith's reviewarXiv
- [14] S. Chang, R. Edezhath, J. Hutchinson and M. Luty, Phys. Rev. D 89, 015011 (2014) [arXiv:1307.8120 [hep- ph]] on PithPith's reviewarXiv
- [15] H. An, L. T. Wang and H. Zhang, Phys. Rev. D 89, 115014 (2014) [arXiv:1308.0592 [hep-ph]] on PithPith's reviewarXiv
- [16] Y. Bai and J. Berger, JHEP 1311, 171 (2013) [arXiv:1308.0612 [hep-ph]] on PithPith's reviewarXiv
- [17] A. DiFranzo, K. I. Nagao, A. Rajaraman and T. M. P. Tait, JHEP 1311, 014 (2013) [arXiv:1308.2679 [hep-ph]] on PithPith's reviewarXiv
- [18] M. Papucci, A. Vichi and K. M. Zurek, JHEP 1411, 024 (2014) [arXiv:1402.2285 [hep-ph]] on PithPith's reviewarXiv
- [19] M. Garny, A. Ibarra, S. Rydbeck and S. Vogl, JHEP 1406, 169 (2014) [arXiv:1403.4634 [hep-ph]] on PithPith's reviewarXiv
- [20] J. Abdallah, A. Ashkenazi, A. Boveia, G. Busoni, A. De Simone, C. Doglioni, A. Efrati and E. Etzion et al. , arXiv:1409.2893 [hep-ph] on PithPith's reviewarXiv
show 51 more
- [21] M. R. Buckley, D. Feld and D. Goncalves, Phys. Rev. D 91, 015017 (2015) [arXiv:1410.6497 [hep-ph]] on PithPith's reviewarXiv
- [22] P. Harris, V. V. Khoze, M. Spannowsky and C. Williams, Phys. Rev. D 91, 055009 (2015) [arXiv:1411.0535 [hep- ph]] on PithPith's reviewarXiv
- [23] J. Abdallah et al. , Phys. Dark Univ. 9-10, 8 (2015) [arXiv:1506.03116 [hep-ph]] on PithPith's reviewarXiv
- [24] W. Altmannshofer, P. J. Fox, R. Harnik, G. D. Kribs and N. Raj, Phys. Rev. D 91, no. 11, 115006 (2015) [arXiv:1411.6743 [hep-ph]] on PithPith's reviewarXiv
- [25] M. J. Baker et al. , JHEP 1512, 120 (2015) [arXiv:1510.03434 [hep-ph]] on PithPith's reviewarXiv
- [26] T. Cohen, J. Kearney, A. Pierce and D. Tucker-Smith, Phys. Rev. D 85, 075003 (2012) [arXiv:1109.2604 [hep- ph]] on PithPith's reviewarXiv
- [27] L. Lopez-Honorez, T. Schwetz and J. Zupan, Phys. Lett. B 716, 179 (2012) [arXiv:1203.2064 [hep-ph]] on PithPith's reviewarXiv
- [28] N. Craig, H. K. Lou, M. McCullough and A. Thalapillil, JHEP 1602, 127 (2016) [arXiv:1412.0258 [hep-ph]] on PithPith's reviewarXiv
- [29] http://lepsusy.web.cern.ch/lepsusy/www/inos_ moriond01/charginos_pub.html on Pith
- [30] http://lepsusy.web.cern.ch/lepsusy/www/sleptons_ summer04/slep_final.html on Pith
- [31] X. l. Chen and M. Kamionkowski, JHEP 9807, 001 (1998) [hep-ph/9805383] on PithPith's reviewarXiv
- [32] Y. Hosotani, P. Ko and M. Tanaka, Phys. Lett. B 680, 179 (2009) [arXiv:0908.0212 [hep-ph]] on PithPith's reviewarXiv
- [33] C. E. Yaguna, Phys. Rev. D 81, 075024 (2010) [arXiv:1003.2730 [hep-ph]] on PithPith's reviewarXiv
- [34] L. J. Hall and L. Randall, Phys. Rev. Lett. 65, 2939 (1990) on Pith
- [35] R. S. Chivukula and H. Georgi, Phys. Lett. B 188, 99 (1987) on Pith
- [36] A. J. Buras, P. Gambino, M. Gorbahn, S. Jager and L. Silvestrini, Phys. Lett. B 500, 161 (2001) [hep- ph/0007085] on Pith
- [37] G. D’Ambrosio, G. F. Giudice, G. Isidori and A. Strumia, Nucl. Phys. B 645, 155 (2002) [hep-ph/0207036] on PithPith's reviewarXiv
- [38] M. J. Dolan, F. Kahlhoefer, C. McCabe and K. Schmidt- Hoberg, JHEP 1503, 171 (2015) Erratum: [JHEP 1507, 103 (2015)] [arXiv:1412.5174 [hep-ph]] on PithPith's reviewarXiv
- [39] C. Kilic, M. D. Klimek and J. H. Yu, Phys. Rev. D 91, no. 5, 054036 (2015) [arXiv:1501.02202 [hep-ph]] on PithPith's reviewarXiv
- [40] J. Kile and A. Soni, Phys. Rev. D 84, 035016 (2011) [arXiv:1104.5239 [hep-ph]]. 15 on PithPith's reviewarXiv
- [41] P. Agrawal, S. Blanchet, Z. Chacko and C. Kilic, Phys. Rev. D 86, 055002 (2012) doi:10.1103/PhysRevD.86.055002 [arXiv:1109.3516 [hep-ph]] on PithPith's reviewarXiv
- [42] G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, arXiv:1305.0237 [hep-ph] on PithPith's reviewarXiv
- [43] M. Freytsis and Z. Ligeti, Phys. Rev. D83, 115009 (2011) [arXiv:1012.5317 [hep-ph]] on PithPith's reviewarXiv
- [44] K. R. Dienes, J. Kumar, B. Thomas and D. Yaylali, Phys. Rev. D 90, no. 1, 015012 (2014) [arXiv:1312.7772 [hep- ph]] on PithPith's reviewarXiv
- [45] U. Haisch, F. Kahlhoefer and J. Unwin, JHEP 1307, 125 (2013) [arXiv:1208.4605 [hep-ph]] on PithPith's reviewarXiv
- [46] P. J. Fox and C. Williams, Phys. Rev. D87, no. 5, 054030 (2013) [arXiv:1211.6390 [hep-ph]] on PithPith's reviewarXiv
- [47] T. Lin, E. W. Kolb and L. T. Wang, Phys. Rev. D 88, no. 6, 063510 (2013) [arXiv:1303.6638 [hep-ph]] on PithPith's reviewarXiv
- [48] U. Haisch, A. Hibbs and E. Re, Phys. Rev. D 89, 034009 (2014) [arXiv:1311.7131 [hep-ph]] on PithPith's reviewarXiv
- [49] U. Haisch and E. Re, JHEP 1506, 078 (2015) [arXiv:1503.00691 [hep-ph]] on PithPith's reviewarXiv
- [50] C. Arina et al. , [arXiv:1605.09242 [hep-ph]] on PithPith's reviewarXiv
- [51] M. Czakon, P. Fiedler and A. Mitov, Phys. Rev. Lett. 110, 252004 (2013) [arXiv:1303.6254 [hep-ph]] on PithPith's reviewarXiv
- [52] M. J. Dolan, M. Spannowsky, Q. Wang and Z. H. Yu, Phys. Rev. D 94, no. 1, 015025 (2016) [arXiv:1606.00019 [hep-ph]] on PithPith's reviewarXiv
- [53] V. Khachatryan et al. [CMS Collaboration], Eur. Phys. J. C 75, no. 5, 235 (2015) on Pith
- [54] ATLAS publication, ATL-PHYS-PUB-2013-011 on Pith
- [55] J. Hisano, R. Nagai and N. Nagata, JHEP 1505, 037 (2015) [arXiv:1502.02244 [hep-ph]] on PithPith's reviewarXiv
- [56] G. Aad et al. [ATLAS Collaboration], Eur. Phys. J. C 75, no. 10, 510 (2015) Erratum: [Eur. Phys. J. C 76, no. 3, 153 (2016)] [arXiv:1506.08616 [hep-ex]] on PithPith's reviewarXiv
- [57] V. Khachatryan et al. [CMS Collaboration], JHEP 1506, 116 (2015) [arXiv:1503.08037 [hep-ex]] on PithPith's reviewarXiv
- [58] CMS Collaboration [CMS Collaboration], CMS-PAS- SUS-14-011 on Pith
- [59] J. Alwall et al., JHEP 1407, 079 (2014) [arXiv:1405.0301 [hep-ph]] on PithPith's reviewarXiv
- [60] ATL-PHYS-PUB-2013-011 on Pith
- [61] [CMS Collaboration], arXiv:1307.7135 on PithPith's reviewarXiv
- [62] K. Hagiwara and T. Yamada, Phys. Rev. D 91, no. 9, 094007 (2015) doi:10.1103/PhysRevD.91.094007 [arXiv:1307.1553 [hep-ph]] on PithPith's reviewarXiv
- [63] H. An and L. T. Wang, Phys. Rev. Lett. 115, 181602 (2015) [arXiv:1506.00653 [hep-ph]] on PithPith's reviewarXiv
- [64] D. S. Akerib et al. [LUX Collaboration], Phys. Rev. Lett. 112, 091303 (2014) [arXiv:1310.8214 [astro-ph.CO]] on PithPith's reviewarXiv
- [65] A. Tan et al. [PandaX-II Collaboration], arXiv:1607.07400 [hep-ex] on PithPith's reviewarXiv
- [66] XENON1T collaboration Collaboration, E. Aprile, The XENON1T Dark Matter Search Experiment, arXiv:1206.6288 on PithPith's reviewarXiv
- [67] A. Anandakrishnan, J. H. Collins, M. Farina, E. Kuflik and M. Perelstein, Phys. Rev. D 93, no. 7, 075009 (2016) [arXiv:1506.05130 [hep-ph]] on PithPith's reviewarXiv
- [68] M. Ackermann et al. [Fermi-LAT Collaboration], Phys. Rev. D 89, 042001 (2014) [arXiv:1310.0828 [astro- ph.HE]] on PithPith's reviewarXiv
- [69] J. Alwall, M. P. Le, M. Lisanti and J. G. Wacker, Phys. Lett. B 666, 34 (2008) [arXiv:0803.0019 [hep-ph]] on PithPith's reviewarXiv
- [70] M. Pospelov, A. Ritz and M. B. Voloshin, Phys. Lett. B 662, 53 (2008) [arXiv:0711.4866 [hep-ph]] on PithPith's reviewarXiv
- [71] J. Hisano, K. Ishiwata and N. Nagata, Phys. Rev. D 82, 115007 (2010) [arXiv:1007.2601 [hep-ph]]. 16 on PithPith's reviewarXiv
Cited by 8 Pith papers
Reviewed papers on Pith that cite this one. The full citation record
- A Fourth Exception in the Calculation of Relic Abundances hep-ph · May 2017
- Bound-state effects on dark matter coannihilation: Pushing the boundaries of conversion-driven freeze-out hep-ph · Dec 2021
- Forbidden Dark Matter Annihilations into Standard Model Particles hep-ph · Dec 2020
- Enabling Forbidden Dark Matter hep-ph · Feb 2017
- Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos hep-ph · Jul 2019
- Exponentially Light Dark Matter from Coannihilation hep-ph · Mar 2018
- Top-philic dark matter within and beyond the WIMP paradigm hep-ph · Feb 2018
- Impeded Dark Matter hep-ph · Sep 2016
Topics: Dark Matter, Dark Matter
How the literature uses it
25 arXiv papers cite this in 29 sentences
Papers citing it · 16 sentences without a confident label
Cites it as background 13 papers
-
Kinematically forbidden annihilations of DM were first discussed in [ref] , where they are referred to as “forbidden channels." They were subsequently studied as a mechanism for light DM with annihilations to new dark sector particles [ref] , and for weak scale DM with annihilations to top quarks [ref] .
Forbidden Dark Matter Annihilations into Standard Model Particles · Introduction · 0.85
-
If $m_ϕ> m_σ$ this is a secluded DM scenario [ref] , while if $m_ϕ< m_σ$ it is a forbidden DM scenario [ref] (see [ref] for other forbidden DM models).
Forbidden conformal dark matter at a GeV · Why forbidden DM? · 0.91
-
It has long been appreciated [ref] that at least three “exceptions" exist to the standard WIMP computation: (1) mutual annihilation of multiple species (coannihilation), (2) annihilations into heavier states (forbidden channels) [ref] , and (3) annihilations near a pole in the cross section [ref] .
Exponentially Light Dark Matter from Coannihilation · Introduction · 0.94
Challenges and discussion
Disagree with the review, or know something it missed? Leave a comment, or challenge this review formally: a challenge becomes a permanent entry in this paper's record, and its decision is published here.
Come back by email
A short list of the week's newly reviewed papers. Nothing is sent until you confirm from your inbox, and every email has a link that stops it. No account.
No comments yet.
Sign in to comment